View source for TRAPPIST-1

{{Short description|Ultra-cool red dwarf star in the constellation Aquarius}}
{{Featured article}}

{{EngvarB|date=June 2022}}
{{Use dmy dates|date=June 2023}}
{{Sky|23|06|29.383|-|05|02|28.59}}
{{Starbox begin
| name = TRAPPIST-1
}}
{{Starbox image
| image = [[File:The ultracool dwarf star TRAPPIST-1 in the constellation of Aquarius.tif|300px|alt=TRAPPIST-1 lies in the northwestern part of the constellation Aquarius, close to the [[ecliptic]].]]
| caption = TRAPPIST-1 is within the red circle in the [[constellation]] [[Aquarius (constellation)|Aquarius]].
| credit =
}}
{{Starbox observe
| epoch = J2000
| constell = [[Aquarius (constellation)|Aquarius]]
| ra = {{RA|23|06|29.368}}{{sfn|Gaia EDR3|2021}}
| dec = {{DEC|−05|02|29.04}}{{sfn|Gaia EDR3|2021}}
| appmag_v = {{val|18.798|0.082}}{{sfn|Costa|Méndez|Jao|Henry|2006|p=1240}}
}}
<!--{{Starbox character
| type = [[Main sequence]]
| class = M8V{{sfn|Costa|Méndez|Jao|Henry|2006|p=1234}}
| appmag_2_passband = R
| appmag_2 = {{val|16.466|0.065}}{{sfn|Costa|Méndez|Jao|Henry|2006|p=1240}}
| appmag_3_passband = I
| appmag_3 = {{val|14.024|0.115}}{{sfn|Costa|Méndez|Jao|Henry|2006|p=1240}}
| appmag_4_passband = J
| appmag_4 = {{val|11.354|0.022}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
| appmag_5_passband = H
| appmag_5 = {{val|10.718|0.021}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
| appmag_6_passband = K
| appmag_6 = {{val|10.296|0.023}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
| r-i = 2.442
| v-r = 2.332
| j-h = 0.636
| j-k = 1.058
| variable =
}}-->
|-
! style="background-color: #FFFFC0; text-align: center;" colspan="2"| Characteristics
|- style="vertical-align:top"
! style="text-align:left" | [[Stellar evolution|Evolutionary&nbsp;stage]]
| [[Main sequence]]
|- style="vertical-align:top"
! style="text-align:left" | [[Stellar classification|Spectral&nbsp;type]]
| M8V{{sfn|Costa|Méndez|Jao|Henry|2006|p=1234}}
|- style="vertical-align:top"
! style="text-align:left" | Apparent&nbsp;magnitude&nbsp;(R)
| {{val|16.466|0.065}}{{sfn|Costa|Méndez|Jao|Henry|2006|p=1240}}
|- style="vertical-align:top"
! style="text-align:left" | Apparent&nbsp;magnitude&nbsp;(I)
| {{val|14.024|0.115}}{{sfn|Costa|Méndez|Jao|Henry|2006|p=1240}}
|- style="vertical-align:top"
! style="text-align:left" | Apparent&nbsp;magnitude&nbsp;(J)
| {{val|11.354|0.022}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
|- style="vertical-align:top"
! style="text-align:left" | Apparent&nbsp;magnitude&nbsp;(H)
| {{val|10.718|0.021}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
|- style="vertical-align:top"
! style="text-align:left" | Apparent&nbsp;magnitude&nbsp;(K)
| {{val|10.296|0.023}}{{sfn|Cutri|Skrutskie|Van Dyk|Beichman|2003|p=II/246}}
|- style="vertical-align:top"
! style="text-align:left" | V−R {{engvar |defaultWord=color index |defaultLang=en-US |en-UK=colour index |engvar= }}
| 2.332
|- style="vertical-align:top"
! style="text-align:left" | R−I {{engvar |defaultWord=[[color index]] |defaultLang=en-US |en-UK=[[colour index]] |engvar= }}
| 2.442
|- style="vertical-align:top"
! style="text-align:left" | J−H {{engvar |defaultWord=color index |defaultLang=en-US |en-UK=colour index |engvar= }}
| 0.636
|- style="vertical-align:top"
! style="text-align:left" | J−K {{engvar |defaultWord=color index |defaultLang=en-US |en-UK=colour index |engvar= }}
| 1.058
|- style="vertical-align:top"
{{Starbox astrometry
| prop_mo_ra = {{val|930.788}}{{sfn|Gaia EDR3|2021}}
| prop_mo_dec = {{val|-479.038}}{{sfn|Gaia EDR3|2021}}
| parallax = 80.2123
| p_error = 0.0716
| parallax_footnote = {{sfn|Gaia EDR3|2021}}
}}
{{Starbox detail
| mass                   =   0.0898{{±|0.0023}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=1}}
| radius                 =   0.1192{{±|0.0013}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=1}}
| luminosity_bolometric  =   0.000566{{±|0.000022}}{{snf|Davoudi|Rackham|Gillon|Wit|2024|p=12}}
<!--| luminosity_visual      =   0.00000373{{efn|Taking the absolute visual magnitude of TRAPPIST-1 <math>M_{V_\ast} = 18.4</math> and the absolute visual magnitude of the Sun <math>M_{V_\odot} = 4.83</math>, the visual luminosity can be calculated by <math>\tfrac{L_{V_\ast}}{L_{V_\odot}} = 10^{0.4(M_{V_\odot} - M_{V_\ast})}.</math>{{sfn|Dinerstein|2014|p=1}}}}-->
| gravity                =   {{Val|5.2396|0.0056|0.0073}}{{efn|A {{nowrap|log(''g'')}} of 2.992 for the Earth indicates that TRAPPIST-1 has a surface gravity approximately 177 times stronger than Earth's.}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=1}}
| temperature            =   {{val|2566|26|fmt=commas}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=1}}
| metal_fe               =   {{val|0.04|0.08}}{{sfn|Delrez|Gillon|Triaud|Demory|2018|pp=3577–3597}}
| rotation               =   {{val|3.295|0.003|u=[[day]]s}}{{sfn|Vida|Kővári|Pál|Oláh|2017|p=7}}
| rotational_velocity    =   6{{sfn|Barnes|Jenkins|Jones|Jeffers|2014|pp=3094–3113}}
| age_gyr                =   {{val|7.6|2.2}}{{sfn|Burgasser|Mamajek|2017|p=7}}
}}
{{Starbox catalog
| names ={{abbr|2MUDC|2MASS UltraCool Dwarves catalog}} 12171,{{sfn|Martínez-Rodríguez|Caballero|Cifuentes|Piro|2019|p=3}} [[2MASS]] J23062928–0502285, [[Ecliptic Plane Input Catalog|EPIC]] 246199087,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=2}} [[Kepler space telescope#Second Light (K2)|K2]]-112,{{sfn|Meadows|Schmidt|2020|p=727}} SPECULOOS-1,{{efn|An internal name of the star used by the [[SPECULOOS]] project, as this planetary system was its first discovery.}}{{sfn|Delrez|Murray|Pozuelos|Narita|2022|p=2}} TRAPPIST-1a{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=3}}
}}
{{Starbox reference
| Simbad = 2MASS+J23062928-0502285
| NSTED = TRAPPIST-1
| EPE = TRAPPIST-1
}}
{{Starbox end}}

'''TRAPPIST-1''' is a [[ultra-cool dwarf|cool]] [[red dwarf star]]{{efn|A red dwarf is a very small and cold star. They are the most common type of star in the [[Milky Way]].{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Red Dwarf}}}} with seven known [[exoplanet]]s. It lies in the constellation [[Aquarius (constellation)|Aquarius]] about {{val|40.66}} [[light-year]]s away from [[Earth]], and has a surface temperature of about {{cvt|2566|K|C F|lk=on|round=10}}. Its radius is slightly larger than [[Jupiter]] and it has a mass of about 9% of [[solar mass|the Sun]]. It is estimated to be 7.6 billion years old, making it older than the [[Solar System]]. The discovery of the star was first published in 2000.

Observations in 2016 from the [[Transiting Planets and Planetesimals Small Telescope]] (TRAPPIST) at [[La Silla Observatory]] in [[Chile]] and other telescopes led to the discovery of two [[terrestrial planet]]s in orbit around TRAPPIST-1. In 2017, further analysis of the original observations identified five more terrestrial planets. It takes the seven planets between about 1.5 and 19 days to [[orbital period|orbit around the star]] in circular orbits. They are all likely [[tidally locked]] to TRAPPIST-1, such that one side of each planet always faces the star, leading to permanent day on one side and permanent night on the other. Their masses are comparable to that of Earth and they all lie in the same plane; from Earth they seem to move past the disk of the star.

Up to four of the planets—designated [[TRAPPIST-1d|''d'']], [[TRAPPIST-1e|''e'']], [[TRAPPIST-1f|''f'']] and [[TRAPPIST-1g|''g'']]—orbit at distances where temperatures are suitable for the existence of liquid water, and are thus potentially hospitable to life. There is no evidence of an atmosphere on any of the planets, and observations of [[TRAPPIST-1b]] have ruled out the existence of an atmosphere. It is unclear whether radiation emissions from TRAPPIST-1 would allow for such atmospheres. The planets have low densities; they may consist of large amounts of [[Volatile (astrogeology)|volatile materials]]. Due to the possibility of several of the planets being habitable, the system has drawn interest from researchers and has appeared in popular culture.

== Discovery ==
The star now known as TRAPPIST-1 was discovered in 1999 by astronomer John Gizis and colleagues{{sfn|Gizis|Monet|Reid|Kirkpatrick|2000|p=1088}} during a [[Two Micron All-Sky Survey|survey]] of close-by [[Ultra-cool dwarf|ultra-cool dwarf stars]].{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=225}}{{sfn|Gizis|Monet|Reid|Kirkpatrick|2000|p=1085}} It appeared in sample C{{sfn|Gizis|Monet|Reid|Kirkpatrick|2000|p=1088}}{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=225}} of the surveyed stars, which was obtained in June 1999. Publication of the discovery took place in 2000.{{sfn|Gizis|Monet|Reid|Kirkpatrick|2000|p=1086}} The name is a reference to the [[TRAPPIST|TRAnsiting Planets and PlanetesImals Small Telescope]] (TRAPPIST){{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=2}}{{efn|TRAPPIST is a {{convert|60|cm|abbr=out|adj=on}} telescope{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=2}} intended to be a prototype for the "Search for habitable Planets EClipsing ULtra-cOOl Stars" project ([[SPECULOOS]]), which aims to identify planets around close, cold stars.{{sfn|Barstow|Irwin|2016|p=95}}{{sfn|Gillon|Jehin|Delrez|Magain|2013|p=1}} TRAPPIST is used to find [[exoplanet]]s, and is preferentially employed on stars colder than {{cvt|3000|K}}.{{sfn|Shields|Ballard|Johnson|2016|p=7}} }} project that discovered the first two [[exoplanet]]s around the star.{{sfn|Goldsmith|2018|p=118}}

Its planetary system was discovered by a team led by [[Michaël Gillon]], a Belgian astronomer{{sfn|Rinaldi|Núñez Ferrer|2017|p=1}} at the [[University of Liege]],{{sfn|Angosto|Zaragoza|Melón|2017|p=85}} in 2016{{sfn|Angosto|Zaragoza|Melón|2017|p=86}} during observations made at the [[La Silla Observatory]], Chile,{{sfn|Marov|Shevchenko|2020|p=865}}{{sfn|Linsky|2019|p=105}} using the TRAPPIST telescope. The discovery was based on anomalies in the [[light curve]]s{{efn|When a planet moves in front of its star, it absorbs part of the star's radiation, which may be observed via telescopes.{{sfn|Cisewski|2017|p=23}}}} measured by the telescope in 2015. These were initially interpreted as indicating the existence of three planets. In 2016, separate discoveries revealed that the third planet was in fact multiple planets. The telescopes and observatories involved were{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=2}} the [[Spitzer Space Telescope]] and the ground-based TRAPPIST, TRAPPIST-North in [[Oukaïmeden Observatory]], Morocco, the [[South African Astronomical Observatory]], and the [[Liverpool Telescope]]s and [[William Herschel Telescope]]s in Spain.{{sfn|Gillon|Triaud|Demory|Jehin|2017|p=461}}

The observations of TRAPPIST-1 are considered among the most important research findings of the Spitzer Space Telescope.{{sfn|Ducrot|2021|p=4}} Complementing the findings were observations by the [[Himalayan Chandra Telescope]], the [[United Kingdom Infrared Telescope]], and the [[Very Large Telescope]].{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=221}} Since then, research has confirmed the existence of at least seven planets in the system,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=3}} the orbits of which have been calculated using measurements from the Spitzer and Kepler telescopes.{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=2}} <!-- Not necessarily "some" -->Some news reports incorrectly attributed the discovery of the TRAPPIST-1 planets to [[NASA]]; in fact the TRAPPIST project that led to their discovery received funding from both NASA and the [[European Research Council]] of the [[European Union]] (EU).{{sfn|Rinaldi|Núñez Ferrer|2017|pp=1–2}}

== Description ==
[[File:The Sun and TRAPPIST-1.jpg|thumb|upright=1.2|True-colour illustration of the [[Sun]] ''(left)'' next to TRAPPIST-1 ''(right)''. TRAPPIST-1 is darker, redder, and smaller than the Sun.|alt=see caption]]

TRAPPIST-1 is in the constellation [[Aquarius (constellation)|Aquarius]],{{sfn|Angosto|Zaragoza|Melón|2017|p=85}} five degrees south of the [[celestial equator]].{{efn|The celestial equator is the [[equator]]'s projection into the sky.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Celestial Equator}}}}{{sfn|Gaia EDR3|2021}}{{sfn|Barstow|Irwin|2016|p=93}} It is a relatively close star{{sfn|Howell|Everett|Horch|Winters|2016|p=1}} located {{val|40.66|0.04}} light-years from Earth,{{efn|Based on [[parallax]] measurements;{{sfn|Gaia EDR3|2021}} the parallax is the position of a celestial object with respect to other celestial objects for a given position of Earth. It can be used to infer the distance of the object from Earth.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Parallax}}}}{{sfn|Gaia EDR3|2021}} with a large [[proper motion]]{{efn|The movement of the star in the sky, relative to background stars.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Proper Motion}}}}{{sfn|Howell|Everett|Horch|Winters|2016|p=1}} and no [[companion star]]s.{{sfn|Howell|Everett|Horch|Winters|2016|pp=1,4}}

It is a [[red dwarf]] of [[spectral class]] M{{val|8.0|0.5}},{{efn|Red dwarfs include the spectral type M and K.{{sfn|The SAO Encyclopedia of Astronomy|2022|loc=Red Dwarf}} Spectral types are used to categorise stars by their temperature.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Spectral Type}}}}{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=221}}{{sfn|Cloutier|Triaud|2016|p=4019}} meaning it is relatively small and cold.{{sfn|Lienhard|Queloz|Gillon|Burdanov|2020|pp=3790–3808}} With a radius 12% of that of the Sun, TRAPPIST-1 is only slightly larger than the planet [[Jupiter]] (though much more massive).{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=221}} Its mass is approximately 9% of that of the Sun,{{sfn|Lienhard|Queloz|Gillon|Burdanov|2020|pp=3790–3808}} being just sufficient to allow [[nuclear fusion]] to take place.{{sfn|Goldsmith|2018|p=82}}{{sfn|Fischer|Saur|2019|p=2}} TRAPPIST-1's density is unusually low for a red dwarf.{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=10}} It has a low [[effective temperature]]{{efn|The effective temperature is the temperature a [[black body]] that emits the same amount of radiation would have.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Effective Temperature}}}} of {{cvt|2566|K|C}} making it, {{as of|2022|lc=y}}, the coldest-known star to host planets.{{sfn|Delrez|Murray|Pozuelos|Narita|2022|p=21}} TRAPPIST-1 is cold enough for condensates to form in its [[photosphere]];{{efn|The photosphere is a thin layer at the surface of a star, where most of its light is produced.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Photosphere}}}} these have been detected through the [[Polarization (physics)|polarisation]] they induce in its radiation during [[astronomical transit|transits]] of its planets.{{sfn|Miles-Páez|Zapatero Osorio|Pallé|Metchev|2019|p=38}} [[Metals (astronomy)|Elements heavier than helium]] form compounds in its atmosphere, which display as [[absorption line]]s in TRAPPIST-1's spectrum.{{snf|Davoudi|Rackham|Gillon|Wit|2024|p=3}}

There is no evidence that it has a [[solar cycle|stellar cycle]].{{efn|The solar cycle is the Sun's 11-year long period, during which solar output varies by about 0.1%.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Variability (Stellar)}}}}{{sfn|Glazier|Howard|Corbett|Law|2020|p=2}} Its [[luminosity]], emitted mostly as [[infrared|infrared radiation]], is about 0.055% that of the Sun.{{sfn|Lienhard|Queloz|Gillon|Burdanov|2020|pp=3790–3808}}{{sfn|Fabbian|Simoniello|Collet|Criscuoli|2017|p=770}} Low-precision{{sfn|Wilson|Froning|Duvvuri|France|2021|p=10}} measurements from the [[XMM-Newton]] satellite{{sfn|Wilson|Froning|Duvvuri|France|2021|p=1}} and other facilities{{sfn|Wilson|Froning|Duvvuri|France|2021|p=2}} show that the star emits faint radiation at short wavelengths such as [[x-rays]] and [[UV radiation]].{{efn|Including [[Lyman-alpha radiation]]{{sfn|Pineda|Hallinan|2018|p=2}}}}{{sfn|Wilson|Froning|Duvvuri|France|2021|p=1}} There are no detectable [[radio wave]] emissions.{{sfn|Pineda|Hallinan|2018|p=7}}

=== Rotation period and age ===
Measurements of TRAPPIST-1's [[Stellar rotation|rotation]] have yielded a period of 3.3 days; earlier measurements of 1.4 days appear to have been caused by changes in the distribution of its [[starspot]]s.{{sfn|Roettenbacher|Kane|2017|p=2}} Its [[rotational axis]] may be slightly offset from that of its planets.{{sfn|Günther|Berardo|Ducrot|Murray|2022|p=13}}

Using a combination of techniques, the age of TRAPPIST-1 has been estimated at about {{val|7.6|2.2}} billion years,{{sfn|Burgasser|Mamajek|2017|p=1}} making it older than the Solar System, which is about {{val|4.5|}} billion years old.{{sfn|Acton|Slavney|Arvidson|Gaddis|2017|p=32}} It is expected to shine for ten trillion years—about 700 times{{sfn|Snellen|2017|p=423}} longer than the present [[age of the Universe]]{{sfn|Acton|Slavney|Arvidson|Gaddis|2017|p=34}}—whereas the Sun will run out of [[hydrogen]] and leave the [[main sequence]]{{efn|The main sequence is the longest stage of a star's lifespan, when it is fusing [[hydrogen]].{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Main Sequence}}}} in a few billion years.{{sfn|Snellen|2017|p=423}}

=== Activity ===
Photospheric features have been detected on TRAPPIST-1.{{sfn|Morris|Agol|Hebb|Hawley|2018|p=1}} The [[Kepler Space Telescope|Kepler]] and Spitzer Space Telescopes have observed possible bright spots, which may be [[Solar facula|faculae]],{{efn|Faculae are bright spots on the photosphere.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Sun (and Young Sun)}}}}{{sfn|Morris|Agol|Davenport|Hawley|2018|p=5}}{{sfn|Linsky|2019|p=250}} although some of these may be too large to qualify as such.{{sfn|Morris|Agol|Davenport|Hawley|2018|p=6}} Bright spots are correlated to the occurrence of some [[stellar flare|stellar flares]].{{efn|Flares are presumably magnetic phenomena lasting for minutes or hours during which parts of the star emit more radiation than usual.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Sun (and Young Sun)}} In the case of TRAPPIST-1, flares reach temperatures of no more than {{cvt|9000|K}}.{{sfn|Howard|Kowalski|Flagg|MacGregor|2023|p=17}}}}{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=5}} Kepler K2 observations have shown that TRAPPIST-1 produces frequent flares (42 flares in 80 days), including large, complex flares{{sfn|Vida|Kővári|Pál|Oláh|2017|p=2}} that could alter nearby planetary atmospheres irreversibly and significantly, raising doubts of hosting life as we know it on Earth.{{sfn|Vida|Kővári|Pál|Oláh|2017|p=5}}

The star has a strong [[magnetic field]]{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} with a mean intensity of about 600 [[Gauss (unit)|gauss]]{{efn|For comparison, a strong fridge magnet has a strength of about 100 gauss and [[Earth's magnetic field]] about 0.5 gauss.{{sfn|MagLab|2022}}}}{{sfn|Kochukhov|2021|p=28}} which may be an underestimate.{{snf|Davoudi|Rackham|Gillon|Wit|2024|p=2}} The magnetic field drives high [[chromosphere|chromospheric]]{{efn|The chromosphere is an outer layer of a star.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Sun (and Young Sun)}}}}{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} activity, and may be capable of trapping [[coronal mass ejection]]s.{{efn|A coronal mass ejection is an eruption of coronal material to the outside of a star.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Sun (and Young Sun)}}{{sfn|Mullan|Paudel|2019|p=2}}}}{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Sun (and Young Sun)}}{{sfn|Mullan|Paudel|2019|p=2}}

According to Garraffo ''et al.'' (2017), TRAPPIST-1 loses about {{val|3e-14}} solar masses per year{{sfn|Sakaue|Shibata|2021|p=1}} to the [[stellar wind]], a rate which is about 1.5 times that of the Sun.{{sfn|Linsky|2019|pp=147–150}} Dong ''et al.'' (2018) simulated the observed properties of TRAPPIST-1 with a mass loss of {{val|4.1e-15}} solar masses per year.{{sfn|Sakaue|Shibata|2021|p=1}} Simulations to estimate mass loss are complicated because, as of 2019, most of the parameters that govern TRAPPIST-1's stellar wind are not known from direct observation.{{sfn|Fischer|Saur|2019|p=6}}

== Planetary system ==
[[File:Comparison of the TRAPPIST-1 system with the inner Solar System and the Galilean Moons of Jupiter.jpg|thumb|Comparison of the orbits of the TRAPPIST-1 planets with the Solar System and Jupiter's moons|alt=The TRAPPIST-1 system is about as compact as Jupiter's moons and much more than the Solar System|upright=1.3]]

TRAPPIST-1 is orbited by seven planets, designated [[TRAPPIST-1b]], [[TRAPPIST-1c|1c]], [[TRAPPIST-1d|1d]], [[TRAPPIST-1e|1e]], [[TRAPPIST-1f|1f]], [[TRAPPIST-1g|1g]] and [[TRAPPIST-1h|1h]]{{sfn|Gonzales|Faherty|Gagné|Teske|2019|p=2}} in alphabetic order going out from the star.{{efn|Exoplanets are named in order of discovery as "b", "c" and so on; if multiple planets are discovered at once they are named in order of increasing orbital period.{{sfn|Schneider|Dedieu|Sidaner|Savalle|2011|p=8}} The term "TRAPPIST-1a" is used to refer to the star itself.{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=2}}}}{{sfn|Veras|Breedt|2017|p=2677}} These planets have orbital periods ranging from 1.5 to 19 days,{{sfn|Delrez|Gillon|Triaud|Demory|2018|pp=3577–3597}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|loc=Tables}}{{sfn|Grimm|Demory|Gillon|Dorn|2018}} at distances of 0.011–0.059 astronomical units{{efn|One astronomical unit (AU) is the mean distance between the Earth and the Sun.{{sfn|Fraire|Feldmann|Walter|Fantino|2019|p=1657}}}} (1.7–8.9 million km).{{sfn|Goldsmith|2018|p=120}}

All the planets are much closer to their star than [[Mercury (planet)|Mercury]] is to the Sun,{{sfn|Angosto|Zaragoza|Melón|2017|p=86}} making the TRAPPIST-1 system very compact.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} Kral ''et al.'' (2018) did not detect any [[comet]]s around TRAPPIST-1,{{sfn|Kral|Wyatt|Triaud|Marino|2018|p=2650}} and Marino ''et al.'' (2020) found no evidence of a [[Kuiper belt]],{{sfn|Childs|Martin|Livio|2022|p=4}} although it is uncertain whether a Solar System-like belt around TRAPPIST-1 would be observable from Earth.{{sfn|Martin|Livio|2022|p=6}} Observations with the [[Atacama Large Millimeter Array]] found no evidence of a [[circumstellar dust]] disk.{{sfn|Marino|Wyatt|Kennedy|Kama|2020|p=6071}}

The inclinations of planetary orbits relative to the system's [[ecliptic]] are less than 0.1 degrees,{{efn|For comparison, Earth's orbit around the Sun is inclined by about 1.578 degrees.{{sfn|Handbook of Scientific Tables|2022|p=2}}}}{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=14}} making TRAPPIST-1 the flattest planetary system in the [[NASA Exoplanet Archive]].{{sfn|Heising|Sasselov|Hernquist|Luisa Tió Humphrey|2021|p=1}} The orbits are highly circular, with minimal [[Orbital eccentricity|eccentricities]]{{efn|The inner two planets' orbits may be circular; the others could have a small eccentricity.{{sfn|Brasser|Pichierri|Dobos|Barr|2022|p=2373}}}}{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} and are well-aligned with the spin axis of TRAPPIST-1.{{sfn|Demory|Pozuelos|Chew|Sabin|2020|p=19}} The planets orbit in the same plane and, from the perspective of the Solar System, transit TRAPPIST-1 during their orbit{{sfn|Maltagliati|2017|p=1}} and frequently pass in front of each other.{{sfn|Kane|Jansen|Fauchez|Selsis|2021|p=1}}

=== Size and composition ===
<!--[[File:Possible Interiors of the TRAPPIST-1 Exoplanets.jpg|thumb|Possible interiors of TRAPPIST-1 planets|upright=2|alt=see caption]]-->

The radii of the planets are estimated to range between 77.5{{±|1.4|1.4}}% and 112.9{{±|1.5|1.3}}% of Earth's radius.{{sfn|Srinivas|2017|p=17}} The planet/star mass ratio of the TRAPPIST-1 system resembles that of the moon/planet ratio of the Solar System's [[gas giant]]s.{{sfn|Madhusudhan|2020|loc=p.&nbsp;6-5}}

The TRAPPIST-1 planets are expected to have compositions that resemble each other{{sfn|McDonough|Yoshizaki|2021|p=9}} as well as that of Earth.{{sfn|Linsky|2019|p=198}} The estimated densities of the planets are lower than Earth's{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=2}} which may imply that they have large amounts of [[volatility (chemistry)|volatile chemicals]].{{efn|A volatile is an element or compound with a low boiling point, such as ammonia, carbon dioxide, methane, nitrogen, sulfur dioxide or water.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Volatile}}}} Alternatively, their cores may be smaller than that of Earth and therefore they may be rocky planets with less iron than that of Earth,{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=30}}{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=11}} include large amounts of elements other than iron,{{sfn|Schlichting|Young|2022|p=16}} or their iron may exist in an oxidised form rather than as a core.{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=11}} Their densities are too low for a pure [[magnesium silicate]] composition,{{efn|The composition of the mantle of rocky planets is typically approximated as a magnesium silicate.{{sfn|Hakim|Rivoldini|Van Hoolst|Cottenier|2018|p=3}}}} requiring the presence of lower-density compounds such as water.{{sfn|Hakim|Rivoldini|Van Hoolst|Cottenier|2018|p=70}}{{sfn|Barth|Carone|Barnes|Noack|2021|p=1326}} Planets b, d, f, g and h are expected to contain large quantities of volatile chemicals.{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=8}} The planets may have deep atmospheres and oceans, and contain vast amounts of ice.{{sfn|Lingam|Loeb|2021|p=594}} [[Subsurface ocean]]s, buried under icy shells, would form in the colder planets.{{sfn|Quick|Roberge|Mendoza|Quintana|2023}} Several compositions are possible considering the large uncertainties in their densities.{{sfn|Van Hoolst|Noack|Rivoldini|2019|p=598}} The photospheric features of the star may introduce inaccuracies in measurements of the properties of TRAPPIST-1's planets,{{sfn|Morris|Agol|Hebb|Hawley|2018|p=1}} including their densities being underestimated by 8{{su|b=&nbsp;&nbsp;&nbsp;-7|p=+20}} percent,{{sfn|Linsky|2019|p=253}} and incorrect estimates of their water content.{{sfn|Linsky|2019|p=254}}

=== Resonance and tides ===
[[File:PIA21427 - TRAPPIST-1 Planetary Orbits and Transits.ogg|thumb|Animation of TRAPPIST-1 exoplanets transiting their host star, with effects on the star's light curve.|upright=1.5]]

The planets are in [[orbital resonance]]s.{{sfn|Aschwanden|Scholkmann|Béthune|Schmutz|2018|p=6}} The durations of their orbits have ratios of 8:5, 5:3, 3:2, 3:2, 4:3 and 3:2 between neighbouring planet pairs,{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=3}} and each set of three is in a [[Laplace resonance]].{{efn|A Laplace resonance is an orbital resonance that consists of three bodies, similar to the [[Galilean moon]]s [[Europa (moon)|Europa]], [[Ganymede (moon)|Ganymede]] and [[Io (moon)|Io]] around Jupiter.{{sfn|Madhusudhan|2020|loc=p.&nbsp;11-2}}}}{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} [[N-body simulation|Simulations]] have shown such resonances can remain stable over billions of years but that their stability is strongly dependent on initial conditions. Many configurations become unstable after less than a million years. The resonances enhance the exchange of [[angular momentum]] between the planets, resulting in measurable variations—earlier or later—in their transit times in front of TRAPPIST-1. These variations yield information on the planetary system,{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=2}} such as the masses of the planets, when other techniques are not available.{{sfn|Ducrot|2021|p=5}} The resonances and the proximity to the host star have led to comparisons between the TRAPPIST-1 system and the [[Galilean moon]]s of Jupiter.{{sfn|Maltagliati|2017|p=1}} [[Kepler-223]] is another exoplanet system with a TRAPPIST-1-like long resonance.{{sfn|Meadows|Schmidt|2020|p=4}}

The closeness of the planets to TRAPPIST-1 results in [[tidal force|tidal]] interactions{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=12–13}} stronger than those on Earth.{{sfn|Lingam|Loeb|2021|p=144}}
All the planets have reached an equilibrium with slow planetary rotations and [[tidal locking]],{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=12–13}} which can lead to the synchronisation of a planet's rotation to its revolution around its star.{{efn|This causes one half of the planet to perpetually face the star in a permanent day and the other half perpetually face away from the star in a permanent night.{{sfn|Goldsmith|2018|p=123}}}}{{sfn|Wolf|2017|p=1}} However, the mutual interactions of the planets could prevent them from reaching full synchronisation, which would have important implications for the planets' climates. These interactions could force periodic or episodic full rotations of the planets' surfaces with respect to the star on timescales of several Earth years.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=13}} Vinson, Tamayo and Hansen (2019) found the planets TRAPPIST-1d, e and f likely have [[Chaos theory|chaotic]] rotations due to mutual interactions, preventing them from becoming synchronised to their star. Lack of synchronisation potentially makes the planets more habitable.{{sfn|Vinson|Tamayo|Hansen|2019|p=5747}} Other processes that can prevent synchronous rotation are [[torque]]s induced by stable [[Ellipsoid|triaxial]] deformation of the planets,{{efn|Where a planet, rather than being a symmetric sphere, has a different radius for each of the three main axes.{{sfn|Elshaboury|Abouelmagd|Kalantonis|Perdios|2016|p=5}}}} which would allow them to enter 3:2 resonances.{{sfn|Zanazzi|Lai|2017|p=2879}}

The planets are likely to undergo substantial [[tidal heating]]{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=7}} due to deformations arising from their orbital eccentricities and gravitational interactions with one another.{{sfn|Barr|Dobos|Kiss|2018|pp=1–2}} Such heating would facilitate volcanism and [[degassing]]{{efn|Degassing is the release of gases, which can end up forming an atmosphere, from the mantle or from magma.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Degassing}}}} especially on the innermost planets, with degassing facilitating the establishment of atmospheres.{{sfn|Kislyakova|Noack|Johnstone|Zaitsev|2017|p=880}} According to Luger ''et al.'' (2017), tidal heating of the four innermost planets is expected to be greater than [[Earth's internal heat budget|Earth's inner heat flux]].{{sfn|Luger|Sestovic|Kruse|Grimm|2017|p=2}} For the outer planets Quick ''et al.'' (2020) noted that their tidal heating could be comparable to that in the Solar System bodies [[Europa (moon)|Europa]], [[Enceladus]] and [[Triton (moon)|Triton]],{{sfn|Quick|Roberge|Mlinar|Hedman|2020|p=19}} and may be sufficient to drive detectable [[cryovolcanic]] activity.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=13}}

Tidal heating could influence temperatures of the night sides and [[Cold trap (astronomy)|cold areas where volatiles may be trapped]], and gases are expected to accumulate; it would also influence the properties of any subsurface oceans{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=8}} where [[cryovolcanism]],{{efn|Cryovolcanism occurs when steam or liquid water, or aqueous fluids, erupt to a planet surface ordinarily too cold to host liquid water.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=2}}}}{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=14}} [[volcanism]] and [[hydrothermal vent]]ing{{efn|Hydrothermal vents are hot springs that occur underwater, and are hypothesised to be places where life could originate.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Hot Vent Microbiology}}}} could occur.{{sfn|Kendall|Byrne|2020|p=1}} It may further be sufficient to melt the [[mantle (geology)|mantle]]s of the four innermost planets, in whole or in part,{{sfn|Kislyakova|Noack|Johnstone|Zaitsev|2017|p=878}} potentially forming subsurface magma oceans.{{sfn|Barr|Dobos|Kiss|2018|p=12}} This heat source is likely dominant over [[radioactive decay]], both of which have substantial uncertainties and are considerably less than the stellar radiation received.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=14}} Intense tides could fracture the planets' [[crust (geology)|crust]]s even if they are not sufficiently strong to trigger the onset of [[plate tectonics]].{{sfn|Zanazzi|Triaud|2019|p=61}} Tides can also occur in the [[Atmospheric tide|planetary atmospheres]].{{sfn|Navarro|Merlis|Cowan|Gomez|2022|p=4}}

=== Skies and impact of stellar light ===
[[File:Comparison of TRAPPIST-1 to the Solar System.jpg|thumb|Relative sizes, densities{{efn|Not accounting for [[gravitational compression]].{{sfn|JPL|2021}}}} and illumination of the TRAPPIST-1 system compared to the [[inner planets]] of the Solar System|alt=TRAPPIST-1 planets are of similar or smaller size than Earth and have similar or smaller densities|upright=2]]

Because most of TRAPPIST-1's radiation is in the infrared region, there may be very little visible light on the planets' surfaces; Amaury Triaud, one of the system's co-discoverers, said the skies would never be brighter than Earth's sky at sunset{{sfn|Srinivas|2017|p=16}} and only a little brighter than a night with a [[full moon]]. Ignoring atmospheric effects, illumination would be orange-red.{{sfn|Radnóti|2021|p=4}} For TRAPPIST-1e, the central star would be four times as wide in the sky as the Sun in Earth's.{{sfn|Walsh|2024|p=203}} All of the planets would be visible from each other and would, in many cases, appear larger than Earth's Moon in the sky of Earth,{{sfn|Angosto|Zaragoza|Melón|2017|p=86}} and each would be recognizable as a planet rather than a star.{{sfn|Walsh|2024|p=203}} They would undergo noticeable [[Retrograde motion|retrograde]] motions in the sky.{{sfn|Wang|Lu|Liu|Chen|2025|p=7}} Observers on TRAPPIST-1e, f and g, however, could never experience a total [[eclipse|stellar eclipse]].{{efn|That is, the inner planets could never cover the entire disk of TRAPPIST-1 from the vantage point of these planets.{{sfn|Veras|Breedt|2017|p=2677}}}}{{sfn|Veras|Breedt|2017|p=2677}} Assuming the existence of atmospheres, the star's long-wavelength radiation would be absorbed to a greater degree by water and carbon dioxide than sunlight on Earth; it would also be scattered less by the atmosphere{{sfn|O'Malley-James|Kaltenegger|2017|p=27}} and less reflected by ice,{{sfn|Bourrier|de Wit|Bolmont|Stamenković|2017|p=7}} although the development of highly reflective [[hydrohalite]] ice may negate this effect.{{sfn|Shields|Carns|2018|p=1}} The same amount of radiation results in a warmer planet compared to Sun-like [[insolation|irradiation]];{{sfn|O'Malley-James|Kaltenegger|2017|p=27}} more radiation would be absorbed by the planets' upper atmosphere than by the lower layers, making the atmosphere [[atmospheric stability|more stable]] and less prone to [[convection]].{{sfn|Eager|Reichelt|Mayne|Lambert|2020|p=10}}

=== Habitable zone ===
{{further|Habitability of red dwarf systems}}
[[File:PIA21424 - The TRAPPIST-1 Habitable Zone.jpg|alt=1e, 1f and 1g is in the habitable zone|thumb|upright=2|[[Habitable zone]]s of TRAPPIST-1 and the [[Solar System]]. The displayed planetary surfaces are speculative.]]

For a dim star like TRAPPIST-1, the [[habitable zone]]{{efn|The [[habitable zone]] is the region around a star where temperatures are neither too hot nor too cold for the existence of liquid water; it is also called the "[[Goldilocks and the Three Bears|Goldilocks]] zone".{{sfn|Cisewski|2017|p=23}}{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} }} is located closer to the star than for the Sun.{{sfn|O'Malley-James|Kaltenegger|2017|p=26}} Three or four{{sfn|Wilson|Froning|Duvvuri|France|2021|p=1}} planets might be located in the habitable zone; these include {{em|e}}, {{em|f}} and {{em|g}};{{sfn|O'Malley-James|Kaltenegger|2017|p=26}} or {{em|d}}, {{em|e}} and {{em|f}}.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} {{As of|2017}}, this is the largest-known number of planets within the habitable zone of any known star or [[star system]].{{sfn|Awiphan|2018|p=13}} The presence of liquid water on any of the planets depends on several other factors, such as [[albedo]] (reflectivity),{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Albedo}} the presence of an atmosphere{{sfn|Alberti|Carbone|Lepreti|Vecchio|2017|p=6}} and any [[greenhouse effect]].{{sfn|Barstow|Irwin|2016|p=92}} Surface conditions are difficult to constrain without better knowledge of the planets' atmospheres.{{sfn|Alberti|Carbone|Lepreti|Vecchio|2017|p=6}} A synchronously rotating planet might not entirely freeze over if it receives too little radiation from its star because the day-side could be sufficiently heated to halt the progress of [[glaciation]].{{sfn|Checlair|Menou|Abbot|2017|p=9}} Other factors for the occurrence of liquid water include the presence of oceans and vegetation;{{sfn|Kral|Wyatt|Triaud|Marino|2018|p=2649}} the reflective properties of the land surface; the configuration of continents and oceans;{{sfn|Rushby|Shields|Wolf|Laguë|2020|p=13}} the presence of clouds;{{sfn|Carone|Keppens|Decin|Henning|2018|p=4677}} and [[sea ice]] dynamics.{{sfn|Yang|Ji|2018|p=1}} The effects of volcanic activity may extend the system's habitable zone to TRAPPIST-1h.{{sfn|O'Malley-James|Kaltenegger|2019|p=4542}} Even if the outer planets are too cold to be habitable, they may have ice-covered subsurface oceans{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=9}} that may harbour life.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=1}}

Intense [[extreme ultraviolet]] (XUV) and [[X-ray]] radiation{{sfn|Bourrier|de Wit|Bolmont|Stamenković|2017|p=2}} can split water into its component parts of hydrogen and oxygen, and heat the upper atmosphere until they escape from the planet. This was thought to have been particularly important early in the star's history, when radiation was more intense and could have heated every planet's water to its boiling point.{{sfn|Bourrier|de Wit|Bolmont|Stamenković|2017|p=7}} This process is believed to have removed water from [[Venus]].{{sfn|Bolmont|Selsis|Owen|Ribas|2017|p=3729}} In the case of TRAPPIST-1, different studies with different assumptions on the [[Chemical kinetics|kinetics]], [[Thermodynamics|energetics]] and XUV emissions have come to different conclusions on whether any TRAPPIST-1 planet may retain substantial amounts of water. Because the planets are most likely synchronised to their host star, any water present could become trapped on the planets' night sides and would be unavailable to support life unless heat transport by the atmosphere{{sfn|Bolmont|Selsis|Owen|Ribas|2017|p=3739}} or tidal heating are intense enough to melt ice.{{sfn|Bolmont|Selsis|Owen|Ribas|2017|p=3740}} 

=== Moons ===
No [[exomoons|moons]] with a size comparable to Earth's have been detected in the TRAPPIST-1 system,{{sfn|Kane|2017|p=4}} and they are unlikely in such a densely packed planetary system. This is because moons would likely be either destroyed by their planet's gravity after entering its [[Roche limit]]{{efn|The Roche limit is the distance at which a body is ripped apart by tides.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Roche Limit}}}} or stripped from the planet by leaving its [[Hill sphere|Hill radius]]{{efn|The Hill radius is the maximum distance at which a planet's gravity can hold a moon without the star's gravity ripping the moon off.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Hill Radius/Sphere}}}}{{sfn|Kane|2017|p=3}} Although the TRAPPIST-1 planets appear in an analysis of potential [[exomoon]] hosts, they do not appear in the list of habitable-zone exoplanets that could host a moon for at least one [[Hubble time]],{{sfn|Martínez-Rodríguez|Caballero|Cifuentes|Piro|2019|p=8}} a timeframe  slightly longer than the current age of the Universe.{{sfn|Martínez-Rodríguez|Caballero|Cifuentes|Piro|2019|p=6}} Despite these factors, it is possible the planets could host moons.{{sfn|Allen|Becker|Fuse|2018|p=1}}

=== Magnetic effects ===
The TRAPPIST-1 planets are expected to be within the [[Alfvén surface]] of their host star,{{sfn|Farrish|Alexander|Maruo|DeRosa|2019|p=7}} the area around the star within which any planet would directly magnetically interact with the [[Stellar corona|corona]] of the star, possibly destabilising any atmosphere the planet has.{{sfn|Farrish|Alexander|Maruo|DeRosa|2019|p=6}} Stellar energetic particles would not create a substantial [[Ionising radiation|radiation hazard]] for organisms on TRAPPIST-1 planets if atmospheres reached pressures of about {{val|1|ul=bar}}.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=164}} Estimates of radiation fluxes have considerable uncertainties due to the lack of knowledge about the structure of TRAPPIST-1's magnetic field.{{sfn|Fraschetti|Drake|Alvarado-Gómez|Moschou|2019|p=11}} [[Induction heating]] from the star's time-varying electrical and magnetic fields{{sfn|Kislyakova|Noack|Johnstone|Zaitsev|2017|p=878}}{{sfn|Grayver|Bower|Saur|Dorn|2022|p=9}} may occur on its planets{{sfn|Chao|deGraffenried|Lach|Nelson|2021|p=5}} but this would make no substantial contribution to their energy balance{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=14}} and is vastly exceeded by tidal heating.{{sfn|Quick|Roberge|Mlinar|Hedman|2020|p=19}}

=== Formation history ===
The TRAPPIST-1 planets most likely formed further from the star and [[planetary migration|migrated]] inwards,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=36}} although it is possible they formed in their current locations.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=9}} According to the most popular theory on the formation of the TRAPPIST-1 planets (Ormel ''et al.'' (2017)),{{sfn|Childs|Shakespeare|Rice|Yang|2023|p=3750}} the planets formed when a [[streaming instability]]{{efn|A streaming instability is a process where interactions between gas and solid particles cause the latter to clump together in filaments. These filaments can give rise to the precursor bodies of planets.{{sfn|Ormel|Liu|Schoonenberg|2017|p=3}}}} at the [[Frost line (astrophysics)|water-ice line]] gave rise to [[planetary embryo|precursor bodies]], which accumulated additional fragments and migrated inwards, eventually giving rise to planets.{{sfn|Liu|Ji|2020|p=24}} The migration may initially have been fast and later slowed,{{sfn|Ogihara|Kokubo|Nakano|Suzuki|2022|p=6}} and tidal effects may have further influenced the formation processes.{{sfn|Brasser|Pichierri|Dobos|Barr|2022|p=2374}} The distribution of the fragments would have controlled the final mass of the planets, which would consist of approximately 10% water consistent with observational inference.{{sfn|Liu|Ji|2020|p=24}} Resonant chains of planets like those of TRAPPIST-1 usually become unstable when the gas disk that gave rise to them dissipates, but in this case, the planets remained in resonance.{{sfn|Bean|Raymond|Owen|2021|p=9}} The resonance may have been either present from the system's formation and was preserved when the planets simultaneously moved inwards,{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=13}} or it might have formed later when inward-migrating planets accumulated at the outer edge of the gas disk and interacted with each other.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=9}} Inward-migrating planets would contain substantial amounts of water—too much for it to entirely escape—whereas planets that formed in their current location would most likely lose all water.{{sfn|Marino|Wyatt|Kennedy|Kama|2020|p=6067}}{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=9–10}} According to Flock ''et al.'' (2019), the orbital distance of the innermost planet TRAPPIST-1b is consistent with the expected radius of an inward-moving planet around a star that was one order of magnitude brighter in the past,{{sfn|Flock|Turner|Mulders|Hasegawa|2019|p=10}} and with the cavity in the [[Protoplanetary disk|protoplanetary disc]] created by TRAPPIST-1's magnetic field.{{sfn|Heising|Sasselov|Hernquist|Luisa Tió Humphrey|2021|p=5}} Alternatively, TRAPPIST-1h may have formed in or close to its current location.{{sfn|Gressier|Mori|Changeat|Edwards|2022|p=2}} 

The presence of other bodies and [[planetesimal]]s early in the system's history would have destabilised the TRAPPIST-1 planets' resonance if the bodies were massive enough.{{sfn|Raymond|Izidoro|Bolmont|Dorn|2021|p=1}} Raymond ''et al.'' (2021) concluded the TRAPPIST-1 planets assembled in one to two million years, after which time little additional mass was accreted.{{sfn|Raymond|Izidoro|Bolmont|Dorn|2021|p=2}} This would limit any late delivery of water to the planets{{sfn|Raymond|Izidoro|Bolmont|Dorn|2021|p=3}} and also implies the planets [[Clearing the neighbourhood|cleared the neighbourhood]]{{efn|According to the [[International Astronomical Union]] criteria, a body has to clear its neighbourhood to qualify as a planet in the Solar System.{{sfn|Raymond|Izidoro|Bolmont|Dorn|2021|p=4}}}} of any additional material.{{sfn|Raymond|Izidoro|Bolmont|Dorn|2021|p=4}} The lack of giant [[impact event]]s (the rapid formation of the planets would have quickly exhausted pre-planetary material) would help the planets preserve their volatile materials,{{sfn|Gabriel|Horn|2021|p=6}} only once the planet formation process was complete.{{sfn|Childs|Shakespeare|Rice|Yang|2023|p=3762}}

Due to a combination of high insolation, the greenhouse effect of water vapour atmospheres and remnant heat from the process of planet assembly, the TRAPPIST-1 planets would likely have initially had molten surfaces. Eventually the surfaces would cool until the magma oceans solidified, which in the case of TRAPPIST-1b may have taken between a few billions of years, or a few millions of years. The outer planets would then have become cold enough for water vapour to condense.{{sfn|Krissansen-Totton|Fortney|2022|p=8}}

== List of planets ==
{{wide image|TRAPPIST-1_system_to_scale.svg|2048px|The TRAPPIST-1 system with distances to scale, compared with the [[Lunar distance (astronomy)|Moon-Earth distance]]|alt=Distances between TRAPPIST-1 planets are roughly comparable with Earth-Moon distances}}

=== TRAPPIST-1b ===
{{Main|TRAPPIST-1b}}
TRAPPIST-1b has a [[semi-major axis]] of 0.0115 astronomical units ({{convert|0.0115|AU|e6km|abbr=unit|disp=output only}}){{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and an orbital period of 1.51 Earth days. It is tidally locked to its star. The planet is outside the habitable zone;{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=222}} its expected irradiation is more than four times that of Earth{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=222}} and the [[James Webb Space Telescope]] (JWST) has measured a [[brightness temperature]] of {{val|508|26|27|u=K}} on the day side.{{sfn|Lim|Benneke|Doyon|MacDonald|2023|p=2}} TRAPPIST-1b has a slightly larger measured radius and mass than Earth but estimates of its density imply it does not exclusively consist of rock.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=24}} Owing to its black-body temperature of {{cvt|124|C|K}}, TRAPPIST-1b may have had a runaway greenhouse effect similar to that of Venus;{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} JWST observations indicate that it has either no atmosphere at all or one nearly devoid of CO<sub>2</sub>.{{sfn|Ih|Kempton|Whittaker|Lessard|2023|p=5}} Based on several climate models, the planet would have been desiccated by TRAPPIST-1's stellar wind and radiation;{{sfn|Linsky|2019|pp=198–199}}{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=28}} it could be quickly losing hydrogen and therefore any hydrogen-dominated atmosphere.{{efn|On the basis of the [[Lyman-alpha]] radiation emissions, TRAPPIST-1b may be losing hydrogen at a rate of {{val|4.6e7||u=g/s}}.{{sfn|Grenfell|Leconte|Forget|Godolt|2020|p=11}}}} Water, if any exists, could persist only in specific settings on the planet,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=29}} whose surface temperature could be as high as {{cvt|1200|C|K}}, making TRAPPIST-1b a candidate [[Lava planet|magma ocean planet]].{{sfn|Grenfell|Leconte|Forget|Godolt|2020|p=18}} According to JWST observations, the planet has an albedo of about zero.{{sfn|Lim|Benneke|Doyon|MacDonald|2023|p=7}}

=== TRAPPIST-1c ===
[[File:TRAPPIST-1 c Light Curve.jpg|thumb|right|Infrared measurements by the [[NASA]] / [[ESA]] / [[Canadian Space Agency]] / [[James Webb Space Telescope]] of TRAPPIST-1 c indicate that it is likely not as Venus-like as once imagined.]] 
{{Main|TRAPPIST-1c}}
TRAPPIST-1c has a semi-major axis of {{convert|0.0158|AU|e6km|abbr=unit}}{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and orbits its star every 2.42 Earth days. It is close enough to TRAPPIST-1 to be tidally locked.{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=222}} JWST observations have ruled out the existence of Venus-like atmospheres,{{sfn|Lincowski|Meadows|Zieba|Kreidberg|2023|p=8}} or CO<sub>2</sub>-rich atmospheres{{sfn|Lim|Benneke|Doyon|MacDonald|2023|p=9}} without a [[temperature inversion]].{{sfn|Ducrot|Lagage|Min|Gillon|2024|p=3}} Airlessness is possible,{{sfn|Ducrot|Lagage|Min|Gillon|2024|p=2}} but only if the surface is subject to rapid volcanic overprinting which is expected given the amount of tidal heating.{{sfn|Ducrot|Lagage|Min|Gillon|2024|p=3}} However, water vapour- or oxygen-rich atmospheres or no-atmosphere scenarios are possible.{{sfn|Lincowski|Meadows|Zieba|Kreidberg|2023|p=8}} These data imply that relative to Earth or Venus, TRAPPIST-1 c has a lower [[carbon]] content.{{sfn|Teixeira|Morley|Foley|Unterborn|2023|p=12}} TRAPPIST-1c is outside the habitable zone{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=222}} as it receives about twice as much stellar irradiation as Earth{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=21}} and thus either is or has been a runaway greenhouse.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} Based on several climate models, the planet would have been desiccated by TRAPPIST-1's stellar wind and radiation.{{sfn|Linsky|2019|pp=198–199}} TRAPPIST-1c could harbour water only in specific settings on its surface.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=29}} Observations in 2017 showed no escaping hydrogen,{{sfn|Wilson|Froning|Duvvuri|France|2021|p=2}} but observations by the [[Hubble Space Telescope]] (HST) in 2020 indicated that hydrogen may be escaping at a rate of {{val|1.4e7|u=g/s}}.{{sfn|Grenfell|Leconte|Forget|Godolt|2020|p=11}}

=== TRAPPIST-1d ===
{{Main|TRAPPIST-1d}}
TRAPPIST-1d has a semi-major axis of {{convert|0.022|AU|e6km|abbr=unit}} and an orbital period of 4.05 Earth days. It is more massive but less dense than Mars.{{sfn|Stevenson|2019|p=329}} Based on [[Fluid dynamics|fluid dynamical]] arguments, TRAPPIST-1d is expected to have weak temperature gradients on its surface if it is tidally locked,{{sfn|Pierrehumbert|Hammond|2019|p=285}} and may have significantly different [[stratospheric]] dynamics than that of Earth.{{sfn|Carone|Keppens|Decin|Henning|2018|p=4683}} Several climate models suggest that the planet may{{sfn|Linsky|2019|pp=198–199}} or may not have been desiccated by TRAPPIST-1's stellar wind and radiation;{{sfn|Linsky|2019|pp=198–199}} density estimates, if confirmed, indicate it is not dense enough to consist solely of rock.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=24}} The current state of TRAPPIST-1d depends on its rotation and climatic factors like [[cloud feedback]];{{efn|Clouds on the day side reflecting starlight could cool TRAPPIST-1d down to temperatures that allow the presence of liquid water.{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=17}}}}{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=1}} it is close to the inner edge of the habitable zone, but the existence of either liquid water or alternatively a runaway greenhouse effect (that would render it uninhabitable) are dependent on detailed atmospheric conditions.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=5–6}} Water could persist in specific settings on the planet.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=29}}

=== TRAPPIST-1e ===
{{Main|TRAPPIST-1e}}
TRAPPIST-1e has a semi-major axis of {{convert|0.029|AU|e6km|abbr=unit}}{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and orbits its star every 6.10 Earth days.{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=10}} It has density similar that of Earth.{{sfn|Stevenson|2019|p=327}} Based on several climate models, the planet is the most likely of the system to have retained its water,{{sfn|Linsky|2019|pp=198–199}} and the most likely to have liquid water for many climate states. A dedicated climate model project called TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) has been launched to study its potential climate states.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=29–30}} Based on observations of its [[Lyman-alpha]] radiation emissions, TRAPPIST-1e may be losing hydrogen at a rate of {{val|0.6e7|u=g/s}}.{{sfn|Grenfell|Leconte|Forget|Godolt|2020|p=11}}

TRAPPIST-1e is in a comparable position within the habitable zone to that of [[Proxima Centauri b]],{{efn|The exoplanet [[Proxima Centauri b]] resides in the habitable zone of the [[Proxima Centauri|nearest star]] to the Solar System.{{sfn|Meadows|Arney|Schwieterman|Lustig-Yaeger|2018|p=133}}}}{{sfn|Janjic|2017|p=61}}{{sfn|Meadows|Arney|Schwieterman|Lustig-Yaeger|2018|p=141}} which also has an Earth-like density.{{sfn|Stevenson|2019|p=327}} TRAPPIST-1e could have retained masses of water equivalent to several of Earth's oceans.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} Moderate quantities of carbon dioxide could warm TRAPPIST-1e to temperatures suitable for the presence of liquid water.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=28}}

=== TRAPPIST-1f ===
{{Main|TRAPPIST-1f}}
TRAPPIST-1f has a semi-major axis of {{convert|0.038|AU|e6km|abbr=unit}}{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and orbits its star every 9.21 Earth days.{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=10}} It is likely too distant from its host star to sustain liquid water, being instead an entirely glaciated [[ice planet|snowball planet]]{{sfn|Linsky|2019|pp=198–199}} that might host a subsurface ocean.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=4}} Moderate quantities of CO<sub>2</sub> could warm TRAPPIST-1f to temperatures suitable for the presence of liquid water.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=29}} Lakes or ponds with liquid water might form in places where tidal heating is concentrated.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=11}} TRAPPIST-1f may have retained masses of water equivalent to several of Earth's oceans{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} and which could comprise up to half of the planet's mass;{{sfn|Kane|Arney|Byrne|Dalba|2021|p=16}} it could thus be an [[ocean planet]].{{efn|Ocean bodies can still be referred to as such when they are covered by ice.{{sfn|Kane|Arney|Byrne|Dalba|2021|p=14}}}}{{sfn|Kane|Arney|Byrne|Dalba|2021|p=17}}

=== TRAPPIST-1g ===
{{Main|TRAPPIST-1g}}
TRAPPIST-1g has a semi-major axis of {{convert|0.047|AU|e6km|abbr=unit}}{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and orbits its star every 12.4 Earth days.{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=10}} It is likely too distant from its host star to sustain liquid water, being instead a snowball planet{{sfn|Linsky|2019|pp=198–199}} that might host a subsurface ocean.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=4}} Moderate quantities of CO<sub>2</sub>{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=29}} or internal heat from radioactive decay and tidal heating may warm its surface to above the melting point of water.{{sfn|Quick|Roberge|Mendoza|Quintana|2023}}{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=171}} TRAPPIST-1g may have retained masses of water equivalent to several of Earth's oceans;{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} density estimates of the planet, if confirmed, indicate it is not dense enough to consist solely of rock.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=24}} Up to half of its mass may be water.{{sfn|Kane|Arney|Byrne|Dalba|2021|p=16}}

=== TRAPPIST-1h ===
{{Main|TRAPPIST-1h}}
TRAPPIST-1h has a semi-major axis of {{convert|0.062|AU|e6km|abbr=unit}}; it is the system's least-massive-known planet{{sfn|Grimm|Demory|Gillon|Dorn|2018|p=6}} and orbits its star every 18.9 Earth days.{{sfn|Agol|Dorn|Grimm|Turbet|2021|p=10}} It is likely too distant from its host star to sustain liquid water and may be a snowball planet,{{sfn|Quick|Roberge|Mendoza|Quintana|2023}}{{sfn|Linsky|2019|pp=198–199}} or have a methane/nitrogen atmosphere resembling that of [[Titan (moon)|Titan]].{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=2}} It might host a subsurface ocean.{{sfn|Quick|Roberge|Mendoza|Quintana|2023|p=4}} Large quantities of CO<sub>2</sub>, hydrogen or methane,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=30}} or  internal heat from radioactive decay and tidal heating,{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=171}} would be needed to warm TRAPPIST-1h to the point where liquid water could exist.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=30}} TRAPPIST-1h could have retained masses of water equivalent to several of Earth's oceans.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}}

=== Data table ===
{| class="wikitable sortable" style="margin-left: auto; margin-right: auto; border: none; font-size: 95%;text-align:center"
|+ TRAPPIST-1 planets data table{{sfn|Delrez|Gillon|Triaud|Demory|2018|pp=3577–3597}}{{sfn|Grimm|Demory|Gillon|Dorn|2018}}{{sfn|Agol|Dorn|Grimm|Turbet|2021}}
|-
! Planet
! [[Earth mass|Mass]] ({{Earth mass}})
! [[Semi-major axis|{{Nowrap|Semi-major}} axis]] ([[Astronomical unit|au]])
! [[Semi-major axis|{{Nowrap|Semi-major}} axis]] ([[kilometer|km]])
! {{Nowrap|[[Orbital period]]}} (days)
! [[Orbital eccentricity]]{{sfn|Grimm|Demory|Gillon|Dorn|2018}}
! [[Orbital inclination]]{{sfn|Agol|Dorn|Grimm|Turbet|2021|loc=Tables}}
! [[Radius]] ({{Earth radius}})
! [[Radiant flux]]{{sfn|Agol|Dorn|Grimm|Turbet|2021|loc=Tables}}
! Temperature {{sfn|Grimm|Demory|Gillon|Dorn|2018}}
! {{Nowrap|[[Surface gravity]]}} (g){{sfn|Agol|Dorn|Grimm|Turbet|2021|loc=Tables}}
! ORb<br/>{{Efn|Approximate orbital resonance with TRAPPIST-1b|name=Orbital resonance with TRAPPIST-1b}}
! ORi<br/>{{Efn|Approximate orbital resonance with inward planet|Approximate orbital resonance with inward planet}}
|-
| [[TRAPPIST-1b|b]]
| 1.374<br><small>{{±|0.069}}</small>
| 0.01154<br><small>{{±|0.0001}}</small>
| 1,726,000<br><small>{{±|15,000 km}}</small>
| 1.510826<small><br>{{±|0.000006}}</small>
| 0.00622<br><small>{{±|0.00304}}</small>
| 89.728<br><small>{{±|0.165°}}</small>
| 1.116<br><small>{{±|0.014|0.012}}</small>
| 4.153<br><small>{{±|0.160}}</small>
| 397.6{{±|3.8}}K<br><small>(124.5 ± 3.8 °C; 256.0 ± 6.8 °F){{efn|Measured surface temperature of {{cvt|503|K|C F}}.{{sfn|Greene|Bell|Ducrot|Dyrek|2023}}}}</small>
| 1.102<br><small>{{±|0.052}}</small>
| —
| —
|-
| [[TRAPPIST-1c|c]]
| 1.308<br><small>{{±|0.056}}</small>
| 0.01580<br><small>{{±|0.00013}}</small>
| 2,370,000<br><small>{{±|19,500}}</small>
| 2.421937<small><br>{{±|0.000018}}</small>
| 0.00654<br><small>{{±|0.00188}}</small>
| 89.778<br><small>{{±|0.118°}}</small>
| 1.097<br><small>{{±|0.014|0.012}}</small>
| 2.214<br><small>{{±|0.085}}</small>
| 339.7{{±|3.3}}K<br><small>(66.6 ± 3.3 °C; 151.8 ± 5.9 °F)</small>
| 1.086<br><small>{{±|0.043}}</small>
| 5:8
| 5:8
|-
| [[TRAPPIST-1d|d]]
| 0.388<br><small>{{±|0.012}}</small>
| 0.02227<br><small>{{±|0.00019}}</small>
| 3,340,500<br><small>{{±|28,500}}</small>
| 4.049219<small><br>{{±|0.000026}}</small>
| 0.00837<br><small>{{±|0.00093}}</small>
| 89.896<br><small>{{±|0.077°}}</small>
| 0.770<br><small>{{±|0.011|0.010}}</small>
| 1.115<br><small>{{±|0.04}}</small>
| 286.2{{±|2.8}}K<br><small>(13.1 ± 2.8 °C; 55.5 ± 5.0 °F)</small>
| 0.624<br><small>{{±|0.019}}</small>
| 3:8
| 3:5
|-
| [[TRAPPIST-1e|e]]
| 0.692<br><small>{{±|0.022}}</small>
| 0.02925<br><small>{{±|0.00025}}</small>
| 4,387,500<br><small>{{±|37,500}}</small>
| 6.101013<small><br>{{±|0.000035}}</small>
| 0.00510<br><small>{{±|0.00058}}</small>
| 89.793<br><small>{{±|0.048°}}</small>
| 0.920<br><small>{{±|0.013|0.012}}</small>
| 0.646<br><small>{{±|0.025}}</small>
| 249.7{{±|2.4}}K<br><small>(−23.5 ± 2.4 °C; −10.2 ± 4.3 °F)</small>
| 0.817<br><small>{{±|0.024}}</small>
| 1:4
| 2:3
|-
| [[TRAPPIST-1f|f]]
| 1.039<br><small>{{±|0.031}}</small>
| 0.03849<br><small>{{±|0.00033}}</small>
| 5,773,500<br><small>{{±|49,500}}</small>
| 9.207540<small><br>{{±|0.000032}}</small>
| 0.01007<br><small>{{±|0.00068}}</small>
| 89.740<br><small>{{±|0.019°}}</small>
| 1.045<br><small>{{±|0.013|0.012}}</small>
| 0.373<br><small>{{±|0.014}}</small>
| 217.7{{±|2.1}}K<br><small>(−55.5 ± 2.1 °C; −67.8 ± 3.8 °F)</small>
| 0.951<br><small>{{±|0.024}}</small>
| 1:6
| 2:3
|-
| [[TRAPPIST-1g|g]]
| 1.321<br><small>{{±|0.038}}</small>
| 0.04683<br><small>{{±|0.0004}}</small>
| 7,024,500<br><small>{{±|60,000}}</small>
| 12.352446<small><br>{{±|0.000054}}</small>
| 0.00208<br><small>{{±|0.00058}}</small>
| 89.742<br><small>{{±|0.012°}}</small>
| 1.129<br><small>{{±|0.015|0.013}}</small>
| 0.252<br><small>{{±|0.010}}</small>
| 197.3{{±|1.9}}K<br><small>(−75.8 ± 1.9 °C; −104.5 ± 3.4 °F)</small>
| 1.035<br><small>{{±|0.026}}</small>
| 1:8
| 3:4
|-
| [[TRAPPIST-1h|h]]
| 0.326<br><small>{{±|0.020}}</small>
| 0.06189<br><small>{{±|0.00053}}</small>
| 9,283,500<br><small>{{±|79,500}}</small>
| 18.772866<small><br>{{±|0.000214}}</small>
| 0.00567<br><small>{{±|0.00121}}</small>
| 89.805<br><small>{{±|0.013°}}</small>
| 0.775<br><small>{{±|0.014|0.014}}</small>
| 0.144<br><small>{{±|0.006}}</small>
| 171.7{{±|1.7}}K<br><small>(−101.5 ± 1.7 °C; −150.6 ± 3.1 °F)</small>
| 0.570<br><small>{{±|0.038}}</small>
| 1:12
| 2:3
|}

== Potential planetary atmospheres==
[[File:Curvas de luz de los siete planetas de TRAPPIST-1 durante su tránsito.png|alt=Lengthening brightness dips from 1b to 1h. Shallowest to deepest dips: 1h, 1d, 1e, 1f, 1g, 1c, 1b.|thumb|upright=1.5|Graph showing dips in brightness in TRAPPIST-1 star by the planet's [[Astronomical transit|transits]] or obstruction of starlight. Larger planets create deeper dips and further planets create longer dips.]]

{{As of|2023}}, the existence of an atmosphere around TRAPPIST-1b has been ruled out by James Webb Space Telescope observations, and there is no evidence for the other planets in the system,{{efn|Bourrier ''et al.'' (2017) interpreted UV absorption data from the [[Hubble Space Telescope]] as implying the outer TRAPPIST-1 planets still have an atmosphere.{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=3}}}}{{sfn|Ih|Kempton|Whittaker|Lessard|2023|p=1}} but atmospheres are not ruled out{{sfn|Lim|Benneke|Doyon|MacDonald|2023|p=9}}{{efn|Computer modelling indicates that the non-existence of an atmosphere around TRAPPIST-1 b and c does not imply the lack of same around the other planets.{{sfn|Teixeira|Morley|Foley|Unterborn|2023|pp=8,9}}}} and could be detected in the future.{{sfn|Fortney|2018|p=17}} The outer planets are more likely to have atmospheres than the inner planets.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=36}} Several studies have simulated how different atmospheric scenarios would look to observers, and the chemical processes underpinning these atmospheric compositions.{{sfn|Wunderlich|Scheucher|Godolt|Grenfell|2020|pp=26–27}} The visibility of an exoplanet and of its atmosphere scale with the inverse square of the radius of its host star.{{sfn|Fortney|2018|p=17}}
Detection of individual components of the atmospheres—in particular CO<sub>2</sub>, ozone and water{{sfn|Zhang|Zhou|Rackham|Apai|2018|p=1}}—would also be possible, although different components would require different conditions and different numbers of transits.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=33}} A contamination of the atmospheric signals through patterns in the stellar photosphere is a further impediment to detection.{{sfn|Ducrot|Gillon|Delrez|Agol|2020|p=2}}{{sfn|Howard|Kowalski|Flagg|MacGregor|2023|p=2}}

The existence of atmospheres around TRAPPIST-1's planets depends on the balance between the amount of atmosphere initially present, its rate of evaporation, and the rate at which it is built back up by meteorite impacts{{efn|Impact events can also remove atmospheres, but a high rate of such "impact erosion" implies a mass of meteorites that is not compatible with the properties of the TRAPPIST-1 system.{{sfn|Teixeira|Morley|Foley|Unterborn|2023|p=10}}}},{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} incoming material from a protoplanetary disk{{efn|A protoplanetary disk is a disk of matter surrounding a star. Planets are thought to form in such disks.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Protoplanetary Disk}}}},{{sfn|Kral|Davoult|Charnay|2020|p=770}} and outgassing and volcanic activity.{{sfn|Hori|Ogihara|2020|p=1}} Impact events may be particularly important in the outer planets because they can both add and remove volatiles; addition is likely dominant in the outermost planets where impact velocities are slower.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=10}}{{sfn|Kral|Wyatt|Triaud|Marino|2018|p=2670}} The formation conditions of the planets would give them large initial quantities of volatile materials,{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=36}} including oceans over 100 times larger than those of Earth.{{sfn|Lingam|Loeb|2019a|p=8}}

If the planets are tidally locked to TRAPPIST-1, surfaces that permanently face away from the star can cool sufficiently for any atmosphere to freeze out on the night side.{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=9}} This frozen-out atmosphere could be recycled through glacier-like flows to the day side with assistance from tidal or [[Geothermal energy|geothermal]] heating from below, or could be stirred by impact events. These processes could allow an atmosphere to persist.{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=10}} In a [[carbon dioxide]] (CO<sub>2</sub>) atmosphere, carbon-dioxide ice is denser than water ice, under which it tends to be buried. CO<sub>2</sub>–water compounds named [[clathrate]]s{{efn|A clathrate is a chemical compound where one compound (or chemical element) e.g. carbon dioxide (or xenon), is trapped within a cage-like assembly of molecules from another compound.{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=14}}}} can form. Further complications are a potential runaway [[feedback loop]] between melting ice and evaporation, and the greenhouse effect.{{sfn|Turbet|Bolmont|Leconte|Forget|2018|pp=14–15}}

[[Numerical model]]ling and observations constrain the properties of hypothetical atmospheres around TRAPPIST-1 planets:{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=36}}
* Theoretical calculations{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=23}} and observations have ruled out the possibility the TRAPPIST-1 planets have hydrogen-rich{{sfn|Kane|Arney|Byrne|Dalba|2021|p=17}}{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=14}} or [[helium]]-rich atmospheres.{{sfn|Gressier|Mori|Changeat|Edwards|2022|p=6}} Hydrogen-rich [[exosphere]]s{{efn|The exosphere is the region of an atmosphere where density is so low that atoms or molecules no longer collide. It is formed by [[atmospheric escape]] and the presence of a hydrogen-rich exosphere implies the presence of water.{{sfn|dos Santos|Bourrier|Ehrenreich|Kameda|2019|p=1}}}} may be detectable{{sfn|dos Santos|Bourrier|Ehrenreich|Kameda|2019|p=11}} but have not been reliably detected,{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=15}} except perhaps for TRAPPIST-1b and 1c by Bourrier ''et al.'' (2017).{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=3}}{{sfn|Gressier|Mori|Changeat|Edwards|2022|p=2}}
* Water-dominated atmospheres, though suggested by some density estimates, are improbable for the planets because they are expected to be unstable under the conditions around TRAPPIST-1, especially early in the star's life.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=24}} The spectral properties of the planets imply they do not have a cloud-free, water-rich atmosphere.{{sfn|Edwards|Changeat|Mori|Anisman|2020|p=11}}
* [[Oxygen]]-dominated atmospheres can form when radiation splits water into hydrogen and oxygen, and the hydrogen escapes due to its lighter mass. The existence of such an atmosphere and its mass depends on the initial water mass, on whether the oxygen is dragged out of the atmosphere by escaping hydrogen and of the state of the planet's surface; a partially molten surface could absorb sufficient quantities of oxygen to remove an atmosphere.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=24–26}}{{sfn|Teixeira|Morley|Foley|Unterborn|2023|p=2}}
* Atmospheres formed by [[ammonia]] and/or [[methane]] near TRAPPIST-1 would be destroyed by the star's radiation at a sufficient rate to quickly remove an atmosphere. The rate at which ammonia or methane are produced, possibly by organisms, would have to be considerably larger than that on Earth to sustain such an atmosphere. It is possible the development of organic [[haze]]s from ammonia or methane [[photodissociation|photolysis]] could shield the remaining molecules from degradation caused by radiation.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=26–27}} Ducrot ''et al.'' (2020) interpreted observational data as implying methane-dominated atmospheres are unlikely around TRAPPIST-1 planets.{{sfn|Ducrot|Gillon|Delrez|Agol|2020|p=19}}
* [[Nitrogen]]-dominated atmospheres are particularly unstable with respect to [[atmospheric escape]], especially on the innermost planets, although the presence of CO<sub>2</sub> may slow evaporation.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=27–28}} Unless the TRAPPIST-1 planets initially contained far more nitrogen than Earth, they are unlikely to have retained such atmospheres.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=37}}
* CO<sub>2</sub>-dominated atmospheres escape slowly because CO<sub>2</sub> effectively radiates away energy and thus does not readily reach escape velocity; on a synchronously rotating planet, however, CO<sub>2</sub> can freeze out on the night side, especially if there are no other gases in the atmosphere. The decomposition of CO<sub>2</sub> caused by radiation could yield substantial amounts of oxygen, [[carbon monoxide]] (CO),{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=28}} and [[ozone]].{{sfn|Wunderlich|Scheucher|Godolt|Grenfell|2020|p=2}}

Theoretical modelling by Krissansen-Totton and Fortney (2022) suggests the inner planets most likely have oxygen-and-CO<sub>2</sub>-rich atmospheres, if any.{{sfn|Krissansen-Totton|Fortney|2022|p=14}} If the planets have an atmosphere, the amount of precipitation, its form and location would be determined by the presence and position of mountains and oceans, and the rotation period.{{sfn|Stevenson|2019|pp=330–332}} Planets in the habitable zone are expected to have an atmospheric circulation regime resembling Earth's tropical regions with largely uniform temperatures.{{sfn|Zhang|2020|p=57}} Whether [[greenhouse gas]]es can accumulate on the outer TRAPPIST-1 planets in sufficient quantities to warm them to the melting point of water is controversial; on a synchronously rotating planet, CO<sub>2</sub> could freeze and precipitate on the night side, and ammonia and methane would be destroyed by XUV radiation from TRAPPIST-1.{{sfn|Airapetian|Barnes|Cohen|Collinson|2020|p=159}} Carbon dioxide freezing-out can occur only on the outermost planets unless special conditions are met, and other volatiles do not freeze out.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}}

=== Stability ===
[[File:Curva de luz de TRAPPIST-1 que muestra los eventos de disminución de la luz causados por el tránsito de los planetas.png|alt=see caption|thumb|upright=2|Observed brightness of the TRAPPIST-1 star, showing large variation in brightness. The graph displays dips, indicating the transit of exoplanets. The planet corresponding to the dips in brightness are plotted below with diamond markers.]]

The emission of extreme ultraviolet (XUV) radiation by a star has an important influence on the stability of its planets' atmospheres, their composition and the habitability of their surfaces.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}} It can cause the ongoing removal of atmospheres from planets.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} XUV radiation-induced atmospheric escape has been observed on gas giants.{{sfn|Wheatley|Louden|Bourrier|Ehrenreich|2017|p=74}} M dwarfs emit large amounts of XUV radiation;{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}} TRAPPIST-1 and the Sun emit about the same amount of XUV radiation{{efn|Different sources estimate that TRAPPIST-1 emits as much as the Sun at [[solar minimum]],{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=3}} the same amount{{sfn|Ducrot|Gillon|Delrez|Agol|2020|p=2}} or more than the Sun.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=7–8}}}}  and because TRAPPIST-1's planets are much closer to the star than the Sun's, they receive much more intense{{efn|The fraction of radiation in the XUV is estimated to range 6-9*10^-4 or 10^-3.51 of the total luminosity.{{snf|Davoudi|Rackham|Gillon|Wit|2024|p=1}}}} irradiation.{{sfn|Fabbian|Simoniello|Collet|Criscuoli|2017|p=770}} TRAPPIST-1 has been emitting radiation for much longer than the Sun.{{sfn|Acton|Slavney|Arvidson|Gaddis|2017|p=33}} The process of atmospheric escape has been modelled mainly in the context of hydrogen-rich atmospheres and little quantitative research has been done on those of other compositions such as water and CO<sub>2</sub>.{{sfn|Gillon|Meadows|Agol|Burgasser|2020|p=14}}

TRAPPIST-1 has moderate to high stellar activity{{efn|Stellar activity is the occurrence of luminosity changes, mostly in the X-ray bands, caused by a star's magnetic field.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Activity (Magnetic)}}}},{{sfn|Gillon|Jehin|Lederer|Delrez|2016|p=221}} and this may be another difficulty for the persistence of atmospheres and water on the planets:{{sfn|Marov|Shevchenko|2020|p=865}}
* Dwarfs of the spectral class M have intense flares;{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}} TRAPPIST-1 averages one flare every two days{{sfn|Vida|Kővári|Pál|Oláh|2017|p=2}} and about four to six [[superflare]]s{{efn|Flares with an energy of over {{convert|1e33|erg|J}}.{{sfn|Vida|Kővári|Leitzinger|Odert|2024|p=1}}}} per year.{{sfn|Glazier|Howard|Corbett|Law|2020|p=9}} Such flares would have only small impacts on atmospheric temperatures but would substantially affect the stability and chemistry of atmospheres.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}} According to Samara, Patsourakos and Georgoulis (2021), the TRAPPIST-1 planets are unlikely to be able to retain atmospheres against [[coronal mass ejection]]s.{{sfn|Samara|Patsourakos|Georgoulis|2021|p=1}}
* The stellar wind from TRAPPIST-1 may have a pressure 1,000 times larger than [[Solar wind|that of the Sun]] at Earth's orbit, which could destabilise atmospheres of the star's planets{{sfn|Linsky|2019|p=191}} up to planet f. The pressure would push the wind deep into the atmospheres,{{sfn|Linsky|2019|pp=198–199}} facilitating loss of water and evaporation of the atmospheres.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}}{{sfn|Turbet|Bolmont|Leconte|Forget|2018|p=2}} Stellar wind-driven escape in the Solar System is largely independent from planetary properties such as mass,{{sfn|Dong|Jin|Lingam|Airapetian|2018|p=262}} scaling instead with the stellar wind mass flux impacting the planet.{{sfn|Teixeira|Morley|Foley|Unterborn|2023|p=5}} Stellar wind from TRAPPIST-1 could remove the atmospheres of its planets on a timescale of 100 million to 10 billion years.{{sfn|Dong|Jin|Lingam|Airapetian|2018|p=264}}
* [[Ohmic heating]]{{efn|Ohmic heating takes place when electrical currents excited by the stellar wind flow through parts of the atmosphere, heating it.{{sfn|Cohen|Glocer|Garraffo|Drake|2018|p=1}}}} of the atmosphere of TRAPPIST-1e, f, and g amounts to five to fifteen times the heating from XUV radiation; if the heat is effectively absorbed, it could destabilise the atmospheres.{{sfn|Linsky|2019|p=189}}

The star's history also influences the atmospheres of its planets.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|pp=3,5}} Immediately after its formation, TRAPPIST-1 would have been in a [[Pre-main-sequence star|pre-main-sequence state]], which may have lasted between hundreds of millions{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}} and two billion years.{{sfn|Ducrot|Gillon|Delrez|Agol|2020|p=2}} While in this state, it would have been considerably brighter than it is today and the star's intense irradiation would have impacted the atmospheres of surrounding planets, vaporising all common volatiles such as ammonia, CO<sub>2</sub>, [[sulfur dioxide]] and water.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=5}} Thus, all of the system's planets would have been heated to a [[runaway greenhouse]]{{efn|In a runaway greenhouse, all water on a planet is in the form of vapour.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=5}}}} for at least part of their existence.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=6}} The XUV radiation would have been even higher during the pre-main-sequence stage.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=8}}

== Possible life ==
Life may be possible in the TRAPPIST-1 system, and some of the star's planets are considered promising targets for its detection.{{sfn|Marov|Shevchenko|2020|p=865}} On the basis of atmospheric stability, TRAPPIST-1e is theoretically the planet most likely to harbour life; the probability that it does is considerably less than that of Earth. There are an array of factors at play:{{sfn|Lingam|Loeb|2018a|p=122}}{{sfn|Pidhorodetska|Fauchez|Villanueva|Domagal-Goldman|2020|p=2}}
* Due to multiple interactions, TRAPPIST-1 planets are expected to have intense tides.{{sfn|Lingam|Loeb|2018b|p=973}} If oceans are present,{{efn|Non-ocean bearing planets can also be subject to [[tidal heating]] (or flexing), resulting in structural deformation.{{sfn|Barr|Dobos|Kiss|2018|p=6}}}} the tides could: lead to alternate flooding and drying of coastal landscapes triggering chemical reactions conducive to the development of life;{{sfn|Lingam|Loeb|2018b|pp=969–970}} favour the evolution of [[biological rhythm]]s such as the day-night cycle that otherwise would not develop in a synchronously rotating planet;{{sfn|Lingam|Loeb|2018b|p=971}} mix oceans, thus supplying and redistributing nutrients;{{sfn|Lingam|Loeb|2018b|p=972}} and stimulate periodic expansions of marine organisms similar to [[red tide]]s on Earth.{{sfn|Lingam|Loeb|2018b|p=975}}
* TRAPPIST-1 may not produce sufficient quantities of radiation for [[photosynthesis]] to support an Earth-like biosphere.{{sfn|Lingam|Loeb|2019a|p=11}}{{sfn|Covone|Ienco|Cacciapuoti|Inno|2021|p=3332}}{{sfn|Lingam|Loeb|2021|p=347}} Mullan and Bais (2018) speculated that radiation from flares may increase the photosynthetic potential of TRAPPIST-1,{{sfn|Mullan|Bais|2018|p=11}} but according to Lingam and Loeb (2019), the potential would still be small.{{sfn|Lingam|Loeb|2019b|p=5926}}
* Due to the proximity of the TRAPPIST-1 planets, it is possible rock-encased [[microorganism]]s ripped{{efn|For example, meteorite impacts could break off rocks from planets at a sufficient speed that they escape its gravity.{{sfn|Goldsmith|2018|p=124}}}} from one planet may arrive at another planet while still viable inside the rock, allowing life to [[panspermia|spread between the planets]] if it originates on one.{{sfn|Goldsmith|2018|p=124}}
* Too much UV radiation from a star can sterilise the surface of a planet{{sfn|Barth|Carone|Barnes|Noack|2021|p=1326}}{{sfn|O'Malley-James|Kaltenegger|2017|p=26}} but too little may not allow the formation of chemical compounds that give rise to life.{{sfn|Harbach|Moschou|Garraffo|Drake|2021|p=3}}{{sfn|Ranjan|Wordsworth|Sasselov|2017|pp=2,9}} Inadequate production of [[hydroxyl radical]]s by low stellar-UV emission may allow gases such as carbon monoxide that are toxic to higher life to accumulate in the planets' atmospheres.{{sfn|Schwieterman|Reinhard|Olson|Harman|2019|p=5}} The possibilities range from UV fluxes from TRAPPIST-1 being unlikely to be much larger than these of [[early Earth]]—even in the event that TRAPPIST-1's emissions of UV radiation are high{{sfn|O'Malley-James|Kaltenegger|2017|p=30}}—to being sufficient to sterilise the planets if they do not have protective atmospheres.{{sfn|Valio|Estrela|Cabral|Grangeiro|2018|p=179}} {{As of|2020}} it is unclear which effect would predominate around TRAPPIST-1,{{sfn|Ducrot|Gillon|Delrez|Agol|2020|p=2}} although observations with the Kepler Space Telescope and the [[Evryscope]] telescopes indicate the UV flux may be insufficient for the formation of life or its sterilisation.{{sfn|Glazier|Howard|Corbett|Law|2020|p=9}}
* Intense flaring activity of the host star—that could alter nearby planets' atmospheres irreversibly and significantly—raised doubts of the habitability of the system.{{sfn|Vida|Kővári|Pál|Oláh|2017|p=5}}
* Although initial water reservoirs could have been lost during the early life of the system due to the stellar activity, a potential subsequent water delivery event, like the late heavy bombardment in the Solar system, could replenish planetary water reservoirs.{{sfn|Dencs|Regály|2019}}
* The outer planets in the TRAPPIST-1 system could host subsurface oceans similar to those of Enceladus and Europa in the Solar System.{{sfn|Quick|Roberge|Mendoza|Quintana|2023}}{{sfn|Lingam|Loeb|2019c|p=112}} [[Chemolithotrophy]], the growth of organisms based on non-organic [[reducing agent|reduced compounds]],{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Chemolithotroph}} could sustain life in such oceans.{{sfn|Kendall|Byrne|2020|p=1}} Very deep oceans may be inimical to the development of life.{{sfn|Barth|Carone|Barnes|Noack|2021|p=1344}}
* Some planets of the TRAPPIST-1 system may have enough water to completely submerge their surfaces.{{sfn|Guimond|Rudge|Shorttle|2022|pp=16–17}} If so, this would have important effects on the [[abiogenesis|possibility of life developing]] on the planets, and on their climates,{{sfn|Guimond|Rudge|Shorttle|2022|p=1}} as [[weathering]] would decrease, starving the oceans of nutrients like [[phosphorus]] as well as potentially leading to the accumulation of carbon dioxide in their atmospheres.{{sfn|Glaser|Hartnett|Desch|Unterborn|2020|p=7}}

TRAPPIST-1 is well-suited to the search of [[technosignature]]s that would indicate the existence of past or present technology in the TRAPPIST-1 system.{{sfn|Tusay|Sheikh|Sneed|Farah|2024|p=15}} Searches in 2017 found only signals coming from Earth,{{sfn|Pinchuk|Margot|Greenberg|Ayalde|2019|p=1}} others in 2024 found nothing{{sfn|Tusay|Sheikh|Sneed|Farah|2024|p=1}} although their sensitivity is low.{{sfn|Tusay|Sheikh|Sneed|Farah|2024|p=16}} In less than two millennia, Earth will be transiting in front of the Sun from the viewpoint of TRAPPIST-1, making the detection of life on Earth from TRAPPIST-1 possible.{{sfn|Kaltenegger|Faherty|2021|p=505}}

== Reception and scientific importance ==
[[File:Trappist1-final-hour-long-cadence.gif|thumb|[[Kepler space telescope|Kepler]] image of TRAPPIST-1|alt=GIF image of a pixellated star]]

=== Public reaction and cultural impact ===
[[File:TRAPPIST-1e Const CMYK Print.png|thumb|alt=Planet hop from TRAPPIST-1e – Voted best 'hab zone' vacation within 12 parsecs of Earth|Fictional TRAPPIST-1e tourism poster made by NASA]]

The discovery of the TRAPPIST-1 planets drew widespread attention in major world newspapers, social media, [[streaming television]] and websites.{{sfn|Short|Stapelfeldt|2017|pp=1, 28}}{{sfn|Díaz|2017|pp=185–186}} {{As of|2017}}, the discovery of TRAPPIST-1 led to the largest single-day web traffic to the NASA website.{{sfn|Short|Stapelfeldt|2017|p=28}} NASA started a public campaign on [[Twitter]] to find names for the planets, which drew responses of varying seriousness, although the names of the planets will be decided by the [[International Astronomical Union]].{{sfn|Physics World|2017|p=1}} The dynamics of the TRAPPIST-1 planetary system have been represented as music, such as [[Tim Pyle]]'s ''Trappist Transits'',{{sfn|Riber|2018|p=1}} in Isolation's single ''Trappist-1 (A Space Anthem)''{{sfn|Howell|2020|loc=p.&nbsp;3–34}} and Leah Asher's piano work ''TRAPPIST-1''.{{sfn|McKay|2021|p=14}} The alleged discovery of an [[SOS signal]] from TRAPPIST-1 was an [[April Fools]] prank by researchers at the [[High Energy Stereoscopic System]] in Namibia.{{sfn|Janjic|2017|p=57}} In 2018, Aldo Spadon created a [[giclée]] ([[digital artwork]]) named "TRAPPIST-1 Planetary System as seen from Space".{{sfn|Kanas|2019|p=488}} A website was dedicated to the TRAPPIST-1 system.{{sfn|Gibb|2022|p=2}}

Exoplanets are often featured in science-fiction works; books, comics and video games have featured the TRAPPIST-1 system, the earliest being ''The Terminator'', a short story by Swiss author [[Laurence Suhner]] published in the academic journal that announced the system's discovery.{{sfn|Gillon|2020a|p=35}}{{sfn|Walsh|2024|p=204}} At least one conference was organised to recognise works of fiction featuring TRAPPIST-1.{{sfn|Gillon|2020b|p=50}} The planets have been used as the basis of science education competitions{{sfn|Sein|Duncan|Zhong|Koock|2021|p=3}} and school projects,{{sfn|Hughes|2022|p=148}}{{sfn|Lane|Gadbury|Ginger|Yi|2022|p=5}} their surfaces portrayed in artistic imagery.{{sfn|Tasker|2024|p=278}} Websites offering TRAPPIST-1-like planets as settings of [[virtual reality]] simulations exist,{{sfn|Paladini|2019|pp=239,254}} such as the "Exoplanet Travel Bureau"{{sfn|Exoplanet Travel Bureau|2021}} and the "Exoplanets Excursion"—both by NASA.{{sfn|AAS|2020|p=309}} Scientific accuracy has been a point of discussion for such cultural depictions of TRAPPIST-1 planets.{{sfn|Fidrick|Yeung|Niemack|Dixon|2020|pp=1–2}}

=== Scientific importance ===
TRAPPIST-1 has drawn intense scientific interest.{{sfn|Deming|Knutson|2020|p=459}} Its planets are the most easily studied exoplanets within their star's habitable zone owing to their relative closeness, the small size of their host star, and because from Earth's perspective they frequently pass in front of their host star.{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=3}} Future observations with space-based observatories and ground-based facilities may allow further insights into their properties such as density, atmospheres and biosignatures.{{efn|Biosignatures are properties of a planet that can be detected from far away and which suggest the existence of life, such as atmospheric gases that are produced by biological processes.{{sfn|Grenfell|2017|p=2}}}} TRAPPIST-1 planets{{sfn|Madhusudhan|2019|p=652}}{{sfn|Turbet|Bolmont|Bourrier|Demory|2020|p=31}} are considered an important observation target for the James Webb Space Telescope{{efn|{{As of|2017}} they were among the smallest planets known where JWST would be able to detect atmospheres.{{sfn|Morley|Kreidberg|Rustamkulov|Robinson|2017|p=1}} It is possible the JWST may not have time to reliably detect certain biosignatures such as methane and ozone.{{sfn|Chiao|2019|p=880}}}}{{sfn|Deming|Knutson|2020|p=459}} and other telescopes under construction;{{sfn|Kral|Wyatt|Triaud|Marino|2018|p=2649}} JWST began investigating the TRAPPIST-1 planets in 2023.{{sfn|Ih|Kempton|Whittaker|Lessard|2023|p=1}} Together with the discovery of Proxima Centauri b, the discovery of the TRAPPIST-1 planets and the fact that at least three of the planets are within the habitable zone has led to an increase in studies on planetary habitability.{{sfn|Lingam|Loeb|2018a|p=116}} The planets are considered prototypical for the research on [[Habitability of red dwarf systems|habitability of M dwarfs]].{{sfn|Madhusudhan|2020|loc=p.&nbsp;I-7}} The star has been the subject of detailed studies{{sfn|Linsky|2019|p=198}} of its various aspects{{sfn|Delrez|Murray|Pozuelos|Narita|2022|p=32}} including the possible effects of vegetation on its planets; the possibility of detecting oceans on its planets using starlight reflected off their surfaces;{{sfn|Kopparla|Natraj|Crisp|Bott|2018|p=1}} possible efforts to [[terraforming|terraform]] its planets;{{sfn|Sleator|Smith|2017|pp=1–2}} and difficulties any inhabitants of the planets would encounter with discovering certain [[laws of physics]] ([[general relativity]], [[Kepler's laws]]{{sfn|Wang|Lu|Liu|Chen|2025|p=18}} and the [[law of gravitation]]{{sfn|Wang|2022|p=10}}) and with [[interstellar travel]].{{sfn|Lingam|Loeb|2018c}}

The role EU funding played in the discovery of TRAPPIST-1 has been cited as an example of the importance of EU projects,{{sfn|Rinaldi|Núñez Ferrer|2017|pp=1–2}} and the involvement of a Moroccan observatory and a Saudi Arabian university as an indication of the [[Islamic world|Islamic]] and [[Arab world]]'s role in science. The original discoverers were affiliated with universities spanning Africa, Europe, and North America,{{sfn|Malik|Determann|2024|p=1}}{{sfn|Determann|2019|pp=168–169}} and the discovery of TRAPPIST-1 is considered to be an example of the importance of co-operation between observatories.{{sfn|Gutiérrez|Arnold|Copley|Copperwheat|2019|p=41}} It is also one of the major astronomical discoveries from Chilean observatories.{{sfn|Guridi|Pertuze|Pfotenhauer|2020|p=5}}

=== Exploration ===
TRAPPIST-1 is too distant from Earth to be reached by humans with current or expected technology.{{sfn|Euroschool|2018|p=10}} Spacecraft mission designs using present-day rockets and [[gravity assist]]s would need hundreds of millennia to reach TRAPPIST-1; even a theoretical interstellar probe travelling at near the [[speed of light]] would need decades to reach the star. The speculative [[Breakthrough Starshot]] proposal for sending small, laser-accelerated, uncrewed probes would require around two centuries to reach TRAPPIST-1.{{sfn|Srinivas|2017|p=19}}

== See also ==
{{div col|colwidth=30}}
* [[HD 10180]], a star with at least six known planets, and three more exoplanet candidates
* [[HD 110067]], star with six known planets all orbiting in a rhythmic resonance
* [[LHS 1140]], another star with a planetary system suitable for atmospheric studies
* [[List of potentially habitable exoplanets]]
* [[LP 890-9]], another cool star with a planetary system
* [[Tabby's Star]], another star with notable transit data
{{div col end}}
{{clear}}

== Notes ==
{{notelist}}

== References ==
{{Reflist|25em}}

=== Sources ===
{{refbegin|35em}}
* {{cite conference|book-title=Abstracts of the 235th AAS Meeting |title=Special Session 001 |url=https://assets.pubpub.org/rynkboj6/71582749259388.pdf |publisher=American Astronomical Society |date=January 2020 |ref={{harvid|AAS|2020}}|location=[[Honolulu, Hawaii]]}}
* {{cite journal|last1=Acton|first1=C.|last2=Slavney|first2=S.|last3=Arvidson|first3=R. E.|last4=Gaddis|first4=L. R.|last5=Gordon|first5=M.|last6=Lavoie|first6=S.|year=2017|title=The planetary data system|journal=Lunar Planet. Inf. Bull.|volume=150|pages=2–11|url=https://www.lpi.usra.edu/publications/newsletters/lpib/lpib150.pdf}}
* {{cite journal |last1=Agol |first1=Eric |last2=Dorn |first2=Caroline |last3=Grimm |first3=Simon L. |last4=Turbet |first4=Martin |last5=Ducrot |first5=Elsa |last6=Delrez |first6=Laetitia |last7=Gillon |first7=Michaël |last8=Demory |first8=Brice-Olivier |last9=Burdanov |first9=Artem |last10=Barkaoui |first10=Khalid |last11=Benkhaldoun |first11=Zouhair |last12=Bolmont |first12=Emeline |last13=Burgasser |first13=Adam |last14=Carey |first14=Sean |last15=de Wit |first15=Julien |last16=Fabrycky |first16=Daniel |last17=Foreman-Mackey |first17=Daniel |last18=Haldemann |first18=Jonas |last19=Hernandez |first19=David M. |last20=Ingalls |first20=James |last21=Jehin |first21=Emmanuel |last22=Langford |first22=Zachary |last23=Leconte |first23=Jérémy |last24=Lederer |first24=Susan M. |last25=Luger |first25=Rodrigo |last26=Malhotra |first26=Renu |last27=Meadows |first27=Victoria S. |last28=Morris |first28=Brett M. |last29=Pozuelos |first29=Francisco J. |last30=Queloz |first30=Didier |last31=Raymond |first31=Sean N. |last32=Selsis |first32=Franck |last33=Sestovic |first33=Marko |last34=Triaud |first34=Amaury H. M. J. |last35=Van Grootel |first35=Valérie |title=Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides |journal=The Planetary Science Journal |issn=2632-3338|date=1 February 2021 |volume=2 |issue=1 |pages=1 |doi=10.3847/psj/abd022 |arxiv=2010.01074 |bibcode=2021PSJ.....2....1A |s2cid=222125312 |language=en |doi-access=free }}
* {{cite journal |last1=Airapetian |first1=V. S. |last2=Barnes |first2=R. |last3=Cohen |first3=O. |last4=Collinson |first4=G. A. |last5=Danchi |first5=W. C. |last6=Dong |first6=C. F. |last7=Del Genio |first7=A. D. |last8=France |first8=K. |last9=Garcia-Sage |first9=K. |last10=Glocer |first10=A. |last11=Gopalswamy |first11=N. |last12=Grenfell |first12=J. L. |last13=Gronoff |first13=G. |last14=Güdel |first14=M. |last15=Herbst |first15=K. |last16=Henning |first16=W. G. |last17=Jackman |first17=C. H. |last18=Jin |first18=M. |last19=Johnstone |first19=C. P. |last20=Kaltenegger |first20=L. |last21=Kay |first21=C. D. |last22=Kobayashi |first22=K. |last23=Kuang |first23=W. |last24=Li |first24=G. |last25=Lynch |first25=B. J. |last26=Lüftinger |first26=T. |last27=Luhmann |first27=J. G. |last28=Maehara |first28=H. |last29=Mlynczak |first29=M. G. |last30=Notsu |first30=Y. |last31=Osten |first31=R. A. |last32=Ramirez |first32=R. M. |last33=Rugheimer |first33=S. |last34=Scheucher |first34=M. |last35=Schlieder |first35=J. E. |last36=Shibata |first36=K. |last37=Sousa-Silva |first37=C. |last38=Stamenković |first38=V. |last39=Strangeway |first39=R. J. |last40=Usmanov |first40=A. V. |last41=Vergados |first41=P. |last42=Verkhoglyadova |first42=O. P. |last43=Vidotto |first43=A. A. |last44=Voytek |first44=M. |last45=Way |first45=M. J. |last46=Zank |first46=G. P. |last47=Yamashiki |first47=Y. |title=Impact of space weather on climate and habitability of terrestrial-type exoplanets |journal=International Journal of Astrobiology |issn=1475-3006|date=April 2020 |volume=19 |issue=2 |pages=136–194 |doi=10.1017/S1473550419000132|arxiv=1905.05093 |bibcode=2020IJAsB..19..136A |s2cid=152282234 }}
* {{cite journal |last1=Alberti |first1=Tommaso |last2=Carbone |first2=Vincenzo |last3=Lepreti |first3=Fabio |last4=Vecchio |first4=Antonio |title=Comparative Climates of the Trappist-1 Planetary System: Results from a Simple Climate-vegetation Model |journal=The Astrophysical Journal |date=18 July 2017 |volume=844 |issue=1 |pages=19 |doi=10.3847/1538-4357/aa78a2 |arxiv=1706.06005 |bibcode=2017ApJ...844...19A |s2cid=118972556 |language=en |doi-access=free }}
* {{cite conference |last1=Allen |first1=John |last2=Becker |first2=Christopher |last3=Fuse |first3=Christopher |title=Stability of Moons in the Trappist-1 System |journal=American Astronomical Society Meeting Abstracts #231 |date=1 January 2018 |volume=231 |pages=148.21 |bibcode=2018AAS...23114821A |conference=American Astronomical Society, AAS Meeting #231|location=[[National Harbor, Maryland]]}}
* {{cite report|last1=Angosto|first1=María Cascales|first2=Federico Mayor|last2=Zaragoza|first3=José Miguel Ortiz|last3=Melón|title=Premios Nobel 2016|trans-title=Nobel Prizes 2016|publisher=Centro de Estudios Ramón Areces|year=2017|url=https://www.fundacionareces.es/recursos/doc/portal/2019/04/23/premios-nobel-2019.pdf|language=es}}
* {{cite journal |last1=Aschwanden |first1=Markus J. |last2=Scholkmann |first2=Felix |last3=Béthune |first3=William |last4=Schmutz |first4=Werner |last5=Abramenko |first5=Valentina |last6=Cheung |first6=Mark C. M. |last7=Müller |first7=Daniel |last8=Benz |first8=Arnold |last9=Chernov |first9=Guennadi |last10=Kritsuk |first10=Alexei G. |last11=Scargle |first11=Jeffrey D. |last12=Melatos |first12=Andrew |last13=Wagoner |first13=Robert V. |last14=Trimble |first14=Virginia |last15=Green |first15=William H. |title=Order out of Randomness: Self-Organization Processes in Astrophysics |journal=Space Science Reviews | issn=1572-9672 |date=March 2018 |volume=214 |issue=2 |pages=55 |doi=10.1007/s11214-018-0489-2|arxiv=1708.03394 |bibcode=2018SSRv..214...55A |s2cid=119064521 }}
* {{cite book |last1=Awiphan |first1=Supachai |title=Exomoons to Galactic Structure |series=Springer Theses |date=2018 |doi=10.1007/978-3-319-90957-8 |isbn=978-3-319-90956-1 |language=en-gb}}
* {{cite journal |last1=Barnes |first1=J. R. |last2=Jenkins |first2=J. S. |last3=Jones |first3=H. R. A. |last4=Jeffers |first4=S. V. |last5=Rojo |first5=P. |last6=Arriagada |first6=P. |last7=Jordán |first7=A. |last8=Minniti |first8=D. |last9=Tuomi |first9=M. |last10=Pinfield |first10=D. |last11=Anglada-Escudé |first11=G. |title=Precision radial velocities of 15 M5–M9 dwarfs |journal=Monthly Notices of the Royal Astronomical Society |date=11 April 2014 |volume=439 |issue=3 |pages=3094–3113 |doi=10.1093/mnras/stu172|doi-access=free |s2cid=16005221 |bibcode=2014MNRAS.439.3094B |arxiv=1401.5350}}
* {{cite journal |last1=Barr |first1=Amy C. |last2=Dobos |first2=Vera |last3=Kiss |first3=László L. |title=Interior structures and tidal heating in the TRAPPIST-1 planets |journal=Astronomy & Astrophysics |date=1 May 2018 |volume=613 |pages=A37 |doi=10.1051/0004-6361/201731992 |arxiv=1712.05641 |bibcode=2018A&A...613A..37B |s2cid=119516532 |language=en |issn=0004-6361}}
* {{cite journal |last1=Barstow |first1=J. K. |last2=Irwin |first2=P. G. J. |title=Habitable worlds with JWST: transit spectroscopy of the TRAPPIST-1 system? |journal=Monthly Notices of the Royal Astronomical Society: Letters | issn=1745-3933 |date=1 September 2016 |volume=461 |issue=1 |pages=L92–L96 |arxiv=1605.07352 |bibcode=2016MNRAS.461L..92B |doi=10.1093/mnrasl/slw109 |doi-access=free |s2cid=17058804 }}
* {{cite journal |last1=Barth |first1=Patrick |last2=Carone |first2=Ludmila |last3=Barnes |first3=Rory |last4=Noack |first4=Lena |last5=Mollière |first5=Paul |last6=Henning |first6=Thomas |title=Magma Ocean Evolution of the TRAPPIST-1 Planets |journal=Astrobiology |date=1 November 2021 |volume=21 |issue=11 |pages=1325–1349 |doi=10.1089/ast.2020.2277 |pmid=34314604 |arxiv=2008.09599 |bibcode=2021AsBio..21.1325B |s2cid=221246323 |issn=1531-1074}}
* {{cite journal |last1=Bean |first1=Jacob L. |last2=Raymond |first2=Sean N. |last3=Owen |first3=James E. |title=The Nature and Origins of Sub-Neptune Size Planets |journal=Journal of Geophysical Research: Planets |date=2021 |volume=126 |issue=1 |pages=e2020JE006639 |doi=10.1029/2020JE006639 |pmid=33680689 |pmc=7900964 |arxiv=2010.11867 |bibcode=2021JGRE..12606639B |language=en |issn=2169-9100}}
* {{cite journal |last1=Bolmont |first1=E. |last2=Selsis |first2=F. |last3=Owen |first3=J. E. |last4=Ribas |first4=I. |last5=Raymond |first5=S. N. |last6=Leconte |first6=J. |last7=Gillon |first7=M. |title=Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1 |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=21 January 2017 |volume=464 |issue=3 |pages=3728–3741 |arxiv=1605.00616 |bibcode=2017MNRAS.464.3728B |doi=10.1093/mnras/stw2578 |doi-access=free |s2cid=53687987 }}
* {{cite journal |last1=Bourrier |first1=V. |last2=de Wit |first2=J. |last3=Bolmont |first3=E. |last4=Stamenković |first4=V. |last5=Wheatley |first5=P. J. |last6=Burgasser |first6=A. J. |last7=Delrez |first7=L. |last8=Demory |first8=B.-O. |last9=Ehrenreich |first9=D. |last10=Gillon |first10=M. |last11=Jehin |first11=E. |last12=Leconte |first12=J. |last13=Lederer |first13=S. M. |last14=Lewis |first14=N. |last15=Triaud |first15=A. H. M. J. |last16=Van Grootel |first16=V.|title=Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets |journal=The Astronomical Journal |date=31 August 2017 |volume=154 |issue=3 |pages=121 |doi=10.3847/1538-3881/aa859c |arxiv=1708.09484 |bibcode=2017AJ....154..121B |hdl=1721.1/112267 |s2cid=44398519 |language=en |doi-access=free }}
* {{cite journal |last1=Brasser |first1=R. |last2=Pichierri |first2=G. |last3=Dobos |first3=V. |last4=Barr |first4=A. C. |title=Long-term tidal evolution of the TRAPPIST-1 system |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=29 July 2022 |volume=515 |issue=2 |pages=2373–2385 |doi=10.1093/mnras/stac1907 |doi-access=free |url=https://academic.oup.com/mnras/article-abstract/515/2/2373/6639872|arxiv=2207.05336 }}
* {{cite journal |last1=Burgasser |first1=Adam J. |last2=Mamajek |first2=Eric E. |title=On the Age of the TRAPPIST-1 System |journal=The Astrophysical Journal |date=17 August 2017 |volume=845 |issue=2 |pages=110 |doi=10.3847/1538-4357/aa7fea |arxiv=1706.02018 |bibcode=2017ApJ...845..110B |s2cid=119464994 |language=en |doi-access=free }}
* {{cite journal |last1=Carone |first1=L. |last2=Keppens |first2=R. |last3=Decin |first3=L. |last4=Henning |first4=Th. |title=Stratosphere circulation on tidally locked ExoEarths |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=1 February 2018 |volume=473 |issue=4 |pages=4672–4685 |arxiv=1711.11446 |bibcode=2018MNRAS.473.4672C |doi=10.1093/mnras/stx2732 |doi-access=free |s2cid=119049536 }}
* {{cite journal |last1=Chao |first1=Keng-Hsien |last2=deGraffenried |first2=Rebecca |last3=Lach |first3=Mackenzie |last4=Nelson |first4=William |last5=Truax |first5=Kelly |last6=Gaidos |first6=Eric |title=Lava worlds: From early earth to exoplanets |journal=Geochemistry |date=1 May 2021 |volume=81 |issue=2 |pages=125735 |doi=10.1016/j.chemer.2020.125735 |arxiv=2012.07337 |bibcode=2021ChEG...81l5735C |s2cid=229153893 |language=en |issn=0009-2819}}
* {{cite journal |last1=Checlair |first1=Jade |last2=Menou |first2=Kristen |last3=Abbot |first3=Dorian S. |title=No Snowball on Habitable Tidally Locked Planets |journal=The Astrophysical Journal |date=18 August 2017 |volume=845 |issue=2 |pages=132 |doi=10.3847/1538-4357/aa80e1 |arxiv=1705.08904 |bibcode=2017ApJ...845..132C |s2cid=13719958 |doi-access=free }}
* {{cite journal |last1=Chiao |first1=May |title=An infrared selfie |journal=Nature Astronomy |date=October 2019 |volume=3 |issue=10 |pages=880 |doi=10.1038/s41550-019-0919-4 |bibcode=2019NatAs...3..880C |s2cid=204718432 |language=en |issn=2397-3366|doi-access=free }}
* {{cite journal |last1=Childs |first1=Anna C. |last2=Martin |first2=Rebecca G. |last3=Livio |first3=Mario |title=Life on Exoplanets in the Habitable Zone of M Dwarfs? |journal=The Astrophysical Journal Letters |date=1 October 2022 |volume=937 |issue=2 |pages=L41 |doi=10.3847/2041-8213/ac9052 |arxiv=2209.02860 |bibcode=2022ApJ...937L..41C |s2cid=252110686 |doi-access=free }}
* {{cite journal |last1=Childs |first1=Anna C. |last2=Shakespeare |first2=Cody |last3=Rice |first3=David R. |last4=Yang |first4=Chao-Chin |last5=Steffen |first5=Jason H. |title=Composition constraints of the TRAPPIST-1 planets from their formation |journal=Monthly Notices of the Royal Astronomical Society |date=24 July 2023 |volume=524 |issue=3 |pages=3749–3768 |doi=10.1093/mnras/stad2110 |doi-access=free |url=https://academic.oup.com/mnras/article/524/3/3749/7225533 |language=en|arxiv=2307.04989 }}
* {{cite journal |last1=Cisewski |first1=Jessi |title=In search of Earth analogues |journal=Significance |date=2017 |volume=14 |issue=2 |pages=22–25 |doi=10.1111/j.1740-9713.2017.01017.x |s2cid=157345539 |language=en |issn=1740-9713|doi-access=free }}
* {{Cite journal|last1=Cloutier|first1=Ryan|last2=Triaud|first2=Amaury H. M. J.|date=11 November 2016|title=Prospects for detecting the Rossiter–McLaughlin effect of Earth-like planets: the test case of TRAPPIST-1b and c|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=462|issue=4|pages=4018–4027|arxiv=1608.01334 |bibcode=2016MNRAS.462.4018C |doi=10.1093/mnras/stw1953 |doi-access=free |s2cid=16147394 |issn=0035-8711}}
* {{cite journal |last1=Cohen |first1=Ofer |last2=Glocer |first2=Alex |last3=Garraffo |first3=Cecilia |last4=Drake |first4=Jeremy J. |last5=Bell |first5=Jared M. |title=Energy Dissipation in the Upper Atmospheres of TRAPPIST-1 Planets |journal=The Astrophysical Journal |date=23 March 2018 |volume=856 |issue=1 |pages=L11 |doi=10.3847/2041-8213/aab5b5 |pmid=32944211 |pmc=7493050 |arxiv=1803.05089 |bibcode=2018ApJ...856L..11C |language=en |doi-access=free }}
* {{Cite journal |title=The Solar Neighborhood. XVI. Parallaxes from CTIOPI: Final Results from the 1.5 m Telescope Program |last1=Costa |first1=E. |last2=Méndez |first2=R. A. |last3=Jao |first3=W.-C. |last4=Henry |first4=T. J. |last5=Subasavage |first5=J. P. |last6=Ianna |first6=P. A. |journal=[[The Astronomical Journal]] |volume=132 |pages=1234 |number=3 |date=4 August 2006 |doi=10.1086/505706 |bibcode=2006AJ....132.1234C |s2cid=18952940 |citeseerx=10.1.1.622.2310}}
* {{cite journal |last1=Covone |first1=Giovanni |last2=Ienco |first2=Riccardo M. |last3=Cacciapuoti |first3=Luca |last4=Inno |first4=Laura |title=Efficiency of the oxygenic photosynthesis on Earth-like planets in the habitable zone |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=11 August 2021 |volume=505 |issue=3 |pages=3329–3335 |arxiv=2104.01425 |doi=10.1093/mnras/stab1357 |doi-access=free |bibcode=2021MNRAS.505.3329C |s2cid=233025250 }}
* {{cite journal |title=VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) |journal=CDS/ADC Collection of Electronic Catalogues |page=II/246 |last1=Cutri |first1=R. M. |last2=Skrutskie |first2=M. F. |last3=Van Dyk |first3=S. |last4=Beichman |first4=C. A. |last5=Carpenter |first5=J. M. |last6=Chester |first6=T. |last7=Cambresy |first7=L. |last8=Evans |first8=T. |last9=Fowler |first9=J. |last10=Gizis |first10=J. |last11=Howard |first11=E. |last12=Huchra |first12=J. |last13=Jarrett |first13=T. |last14=Kopan |first14=E. L. |last15=Kirkpatrick |first15=J. D. |last16=Light |first16=R. M. |last17=Marsh |first17=K. A. |last18=McCallon |first18=H. |last19=Schneider |first19=S. |last20=Stiening |first20=R. |last21=Sykes |first21=M. |last22=Weinberg |first22=M. |last23=Wheaton |first23=W. A. |last24=Wheelock |first24=S. |last25=Zacarias |first25=N. |number=2246 |date=June 2003 |bibcode=2003yCat.2246....0C}}
* {{cite journal |last1=Davoudi |first1=Fatemeh |last2=Rackham |first2=Benjamin V. |last3=Gillon |first3=Michaël |last4=Wit |first4=Julien de |last5=Burgasser |first5=Adam J. |last6=Delrez |first6=Laetitia |last7=Iyer |first7=Aishwarya |last8=Ducrot |first8=Elsa |title=Updated Spectral Characteristics for the Ultracool Dwarf TRAPPIST-1 |journal=The Astrophysical Journal Letters |date=July 2024 |volume=970 |issue=1 |pages=L4 |doi=10.3847/2041-8213/ad5c6c |doi-access=free |language=en |issn=2041-8205}}
* {{cite journal |last1=Delrez |first1=L. |last2=Gillon |first2=M. |last3=Triaud |first3=A. H. M. J. |last4=Demory |first4=B-O. |last5=de Wit |first5=J. |last6=Ingalls |first6=J. G. |last7=Agol |first7=E. |last8=Bolmont |first8=E. |last9=Burdanov |first9=A. |last10=Burgasser |first10=A. J. |last11=Carey |first11=S. J. |last12=Jehin |first12=E. |last13=Leconte |first13=J. |last14=Lederer |first14=S. |last15=Queloz |first15=D. |last16=Selsis |first16=F. |last17=Van Grootel |first17=V. |title=Early 2017 observations of TRAPPIST-1 with Spitzer |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=11 April 2018 |volume=475 |issue=3 |pages=3577–3597 |arxiv=1801.02554 |bibcode=2018MNRAS.475.3577D |doi=10.1093/mnras/sty051 |doi-access=free |s2cid=54649681 }}
* {{cite journal |last1=Delrez |first1=L. |last2=Murray |first2=C. A. |last3=Pozuelos |first3=F. J. |last4=Narita |first4=N. |last5=Ducrot |first5=E. |last6=Timmermans |first6=M. |last7=Watanabe |first7=N. |last8=Burgasser |first8=A. J. |last9=Hirano |first9=T. |last10=Rackham |first10=B. V. |last11=Stassun |first11=K. G. |last12=Van Grootel |first12=V. |last13=Aganze |first13=C. |last14=Cointepas |first14=M. |last15=Howell |first15=S. |last16=Kaltenegger |first16=L. |last17=Niraula |first17=P. |last18=Sebastian |first18=D. |last19=Almenara |first19=J. M. |last20=Barkaoui |first20=K. |last21=Baycroft |first21=T. A. |last22=Bonfils |first22=X. |last23=Bouchy |first23=F. |last24=Burdanov |first24=A. |last25=Caldwell |first25=D. A. |last26=Charbonneau |first26=D. |last27=Ciardi |first27=D. R. |last28=Collins |first28=K. A. |last29=Daylan |first29=T. |last30=Demory |first30=B.-O. |last31=de Wit |first31=J. |last32=Dransfield |first32=G. |last33=Fajardo-Acosta |first33=S. B. |last34=Fausnaugh |first34=M. |last35=Fukui |first35=A. |last36=Furlan |first36=E. |last37=Garcia |first37=L. J. |last38=Gnilka |first38=C. L. |last39=Gómez Maqueo Chew |first39=Y. |last40=Gómez-Muñoz |first40=M. A. |last41=Günther |first41=M. N. |last42=Harakawa |first42=H. |last43=Heng |first43=K. |last44=Hooton |first44=M. J. |last45=Hori |first45=Y. |last46=Ikoma |first46=M. |last47=Jehin |first47=E. |last48=Jenkins |first48=J. M. |last49=Kagetani |first49=T. |last50=Kawauchi |first50=K. |last51=Kimura |first51=T. |last52=Kodama |first52=T. |last53=Kotani |first53=T. |last54=Krishnamurthy |first54=V. |last55=Kudo |first55=T. |last56=Kunovac |first56=V. |last57=Kusakabe |first57=N. |last58=Latham |first58=D. W. |last59=Littlefield |first59=C. |last60=McCormac |first60=J. |last61=Melis |first61=C. |last62=Mori |first62=M. |last63=Murgas |first63=F. |last64=Palle |first64=E. |last65=Pedersen |first65=P. P. |last66=Queloz |first66=D. |last67=Ricker |first67=G. |last68=Sabin |first68=L. |last69=Schanche |first69=N. |last70=Schroffenegger |first70=U. |last71=Seager |first71=S. |last72=Shiao |first72=B. |last73=Sohy |first73=S. |last74=Standing |first74=M. R. |last75=Tamura |first75=M. |last76=Theissen |first76=C. A. |last77=Thompson |first77=S. J. |last78=Triaud |first78=A. H. M. J. |last79=Vanderspek |first79=R. |last80=Vievard |first80=S. |last81=Wells |first81=R. D. |last82=Winn |first82=J. N. |last83=Zou |first83=Y. |last84=Zúñiga-Fernández |first84=S. |last85=Gillon |first85=M. |title=Two temperate super-Earths transiting a nearby late-type M dwarf |journal=Astronomy & Astrophysics |date=8 September 2022 |volume=667 |pages=A59 |doi=10.1051/0004-6361/202244041 |arxiv=2209.02831 |bibcode=2022A&A...667A..59D |s2cid=252110654 |url=https://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/202244041 |language=en |issn=0004-6361|via=[[arXiv]]}}
* {{cite journal |last1=Deming |first1=Drake |last2=Knutson |first2=Heather A. |title=Highlights of exoplanetary science from Spitzer |journal=Nature Astronomy |date=May 2020 |volume=4 |issue=5 |pages=453–466 |doi=10.1038/s41550-020-1100-9 |arxiv=2005.11331 |bibcode=2020NatAs...4..453D |s2cid=218870017 |language=en |issn=2397-3366}}
* {{cite journal |last1=Demory |first1=B.-O. |last2=Pozuelos |first2=F. J. |last3=Chew |first3=Y. Gómez Maqueo |last4=Sabin |first4=L. |last5=Petrucci |first5=R. |last6=Schroffenegger |first6=U. |last7=Grimm |first7=S. L. |last8=Sestovic |first8=M. |last9=Gillon |first9=M. |last10=McCormac |first10=J. |last11=Barkaoui |first11=K. |last12=Benz |first12=W. |last13=Bieryla |first13=A. |last14=Bouchy |first14=F. |last15=Burdanov |first15=A. |last16=Collins |first16=K. A. |last17=Wit |first17=J. de |last18=Dressing |first18=C. D. |last19=Garcia |first19=L. J. |last20=Giacalone |first20=S. |last21=Guerra |first21=P. |last22=Haldemann |first22=J. |last23=Heng |first23=K. |last24=Jehin |first24=E. |last25=Jofré |first25=E. |last26=Kane |first26=S. R. |last27=Lillo-Box |first27=J. |last28=Maigné |first28=V. |last29=Mordasini |first29=C. |last30=Morris |first30=B. M. |last31=Niraula |first31=P. |last32=Queloz |first32=D. |last33=Rackham |first33=B. V. |last34=Savel |first34=A. B. |last35=Soubkiou |first35=A. |last36=Srdoc |first36=G. |last37=Stassun |first37=K. G. |last38=Triaud |first38=A. H. M. J. |last39=Zambelli |first39=R. |last40=Ricker |first40=G. |last41=Latham |first41=D. W. |last42=Seager |first42=S. |last43=Winn |first43=J. N. |last44=Jenkins |first44=J. M. |last45=Calvario-Velásquez |first45=T. |last46=Herrera |first46=J. A. Franco |last47=Colorado |first47=E. |last48=Zepeda |first48=E. O. Cadena |last49=Figueroa |first49=L. |last50=Watson |first50=A. M. |last51=Lugo-Ibarra |first51=E. E. |last52=Carigi |first52=L. |author52-link=Leticia Carigi|last53=Guisa |first53=G. |last54=Herrera |first54=J. |last55=Díaz |first55=G. Sierra |last56=Suárez |first56=J. C. |last57=Barrado |first57=D. |last58=Batalha |first58=N. M. |last59=Benkhaldoun |first59=Z. |last60=Chontos |first60=A. |last61=Dai |first61=F. |last62=Essack |first62=Z. |last63=Ghachoui |first63=M. |last64=Huang |first64=C. X. |last65=Huber |first65=D. |last66=Isaacson |first66=H. |last67=Lissauer |first67=J. J. |last68=Morales-Calderón |first68=M. |last69=Robertson |first69=P. |last70=Roy |first70=A. |last71=Twicken |first71=J. D. |last72=Vanderburg |first72=A. |last73=Weiss |first73=L. M. |title=A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266 |journal=Astronomy & Astrophysics |date=1 October 2020 |volume=642 |pages=A49 |doi=10.1051/0004-6361/202038616 |arxiv=2009.04317 |bibcode=2020A&A...642A..49D |s2cid=221554586 |language=en |issn=0004-6361}}
* {{Cite journal |last1=Dencs |first1=Zoltán |last2=Regály |first2=Zsolt |title=Water delivery to the TRAPPIST-1 planets |journal=Monthly Notices of the Royal Astronomical Society |date=August 2019 |volume=487 |issue=2 |pages=2191 |arxiv= 1905.11298 |doi=10.1093/mnras/stz1412 |bibcode=2019MNRAS.487.2191D |language=en |doi-access=free }}
* {{cite book |last1=Determann |first1=Jörg Matthias |title=Space science and the Arab world: astronauts, observatories and nationalism in the Middle East |date=2019 |isbn=978-1-83860-015-0 |oclc=1122719747 |url=https://www.worldcat.org/oclc/1122719747|publisher=Bloomsbury Publishing}}
* {{cite journal|last=Díaz|first=R. F.|title=Exploring new worlds. A review on extrasolar planet observations|journal=Boletin de la Asociacion Argentina de Astronomia la Plata Argentina|volume=59|year=2017|pages=183–189|bibcode=2017BAAA...59..183D }}
* {{cite journal |last1=Dong |first1=Chuanfei |last2=Jin |first2=Meng |last3=Lingam |first3=Manasvi |last4=Airapetian |first4=Vladimir S. |last5=Ma |first5=Yingjuan |last6=van der Holst |first6=Bart |title=Atmospheric escape from the TRAPPIST-1 planets and implications for habitability |journal=Proceedings of the National Academy of Sciences |date=9 January 2018 |volume=115 |issue=2 |pages=260–265 |doi=10.1073/pnas.1708010115 |pmid=29284746 |pmc=5777028 |arxiv=1705.05535 |bibcode=2018PNAS..115..260D |s2cid=31195274 |language=en |issn=0027-8424|doi-access=free }}
* {{cite journal |last1=dos Santos |first1=Leonardo A.|last2=Bourrier |first2=Vincent |last3=Ehrenreich |first3=David |last4=Kameda |first4=Shingo |title=Observability of hydrogen-rich exospheres in Earth-like exoplanets |journal=Astronomy & Astrophysics |date=1 February 2019 |volume=622 |pages=A46 |doi=10.1051/0004-6361/201833392 |arxiv=1812.02145|bibcode=2019A&A...622A..46D|s2cid=119013251 |language=en |issn=0004-6361}}
* {{cite journal |last1=Ducrot |first1=E. |last2=Gillon |first2=M. |last3=Delrez |first3=L. |last4=Agol |first4=E. |last5=Rimmer |first5=P. |last6=Turbet |first6=M. |last7=Günther |first7=M. N. |last8=Demory |first8=B.-O. |last9=Triaud |first9=A. H. M. J. |last10=Bolmont |first10=E. |last11=Burgasser |first11=A. |last12=Carey |first12=S. J. |last13=Ingalls |first13=J. G. |last14=Jehin |first14=E. |last15=Leconte |first15=J. |last16=Lederer |first16=S. M. |last17=Queloz |first17=D. |last18=Raymond |first18=S. N. |last19=Selsis |first19=F. |last20=Van Grootel |first20=V. |last21=Wit |first21=J. de |title=TRAPPIST-1: Global results of the Spitzer Exploration Science Program Red Worlds |journal=Astronomy & Astrophysics |date=1 August 2020 |volume=640 |pages=A112 |doi=10.1051/0004-6361/201937392 |arxiv=2006.13826 |bibcode=2020A&A...640A.112D |s2cid=220041987 |language=en |issn=0004-6361}}
* {{cite journal |last=Ducrot |first=Elsa |date=2 April 2021 |title=A brief history of the TRAPPIST-1 system Article sur invitation – Invited paper |url=https://popups.uliege.be/0037-9565/index.php?id=10277 |journal=Bulletin de la Société Royale des Sciences de Liège |volume=90 |doi=10.25518/0037-9565.10277 |s2cid=246354436 |language=en |issn=0037-9565|doi-access=free }}
* {{cite journal |last1=Ducrot |first1=Elsa |last2=Lagage |first2=Pierre-Olivier |last3=Min |first3=Michiel |last4=Gillon |first4=Michaël |last5=Bell |first5=Taylor J. |last6=Tremblin |first6=Pascal |last7=Greene |first7=Thomas |last8=Dyrek |first8=Achrène |last9=Bouwman |first9=Jeroen |last10=Waters |first10=Rens |last11=Güdel |first11=Manuel |last12=Henning |first12=Thomas |last13=Vandenbussche |first13=Bart |last14=Absil |first14=Olivier |last15=Barrado |first15=David |last16=Boccaletti |first16=Anthony |last17=Coulais |first17=Alain |last18=Decin |first18=Leen |last19=Edwards |first19=Billy |last20=Gastaud |first20=René |last21=Glasse |first21=Alistair |last22=Kendrew |first22=Sarah |last23=Olofsson |first23=Goran |last24=Patapis |first24=Polychronis |last25=Pye |first25=John |last26=Rouan |first26=Daniel |last27=Whiteford |first27=Niall |last28=Argyriou |first28=Ioannis |last29=Cossou |first29=Christophe |last30=Glauser |first30=Adrian M. |last31=Krause |first31=Oliver |last32=Lahuis |first32=Fred |last33=Royer |first33=Pierre |last34=Scheithauer |first34=Silvia |last35=Colina |first35=Luis |last36=van Dishoeck |first36=Ewine F. |last37=Ostlin |first37=Göran |last38=Ray |first38=Tom P. |last39=Wright |first39=Gillian |title=Combined analysis of the 12.8 and 15 μm JWST/MIRI eclipse observations of TRAPPIST-1 b |journal=Nature Astronomy |date=16 December 2024 |doi=10.1038/s41550-024-02428-z|arxiv=2412.11627 }}
* {{cite journal |last1=Eager |first1=Jake K. |last2=Reichelt |first2=David J. |last3=Mayne |first3=Nathan J. |last4=Lambert |first4=F. Hugo |last5=Sergeev |first5=Denis E. |last6=Ridgway |first6=Robert J. |last7=Manners |first7=James |last8=Boutle |first8=Ian A. |last9=Lenton |first9=Timothy M. |last10=Kohary |first10=Krisztian |title=Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets |journal=Astronomy & Astrophysics |date=1 July 2020 |volume=639 |pages=A99 |doi=10.1051/0004-6361/202038089 |arxiv=2005.13002 |bibcode=2020A&A...639A..99E |s2cid=218900900 |language=en |issn=0004-6361}}
* {{cite journal |last1=Edwards |first1=Billy |last2=Changeat |first2=Quentin |last3=Mori |first3=Mayuko |last4=Anisman |first4=Lara O. |last5=Morvan |first5=Mario |last6=Yip |first6=Kai Hou |last7=Tsiaras |first7=Angelos |last8=Al-Refaie |first8=Ahmed |last9=Waldmann |first9=Ingo |last10=Tinetti |first10=Giovanna |title=Hubble WFC3 Spectroscopy of the Habitable-zone Super-Earth LHS 1140 b |journal=The Astronomical Journal |date=24 December 2020 |volume=161 |issue=1 |pages=44 |arxiv=2011.08815 |doi=10.3847/1538-3881/abc6a5 |s2cid=226975730 |language=en |doi-access=free |bibcode=2021AJ....161...44E }}
* {{cite journal |last1=Elshaboury |first1=S. M. |last2=Abouelmagd |first2=Elbaz I. |last3=Kalantonis |first3=V. S. |last4=Perdios |first4=E. A. |title=The planar restricted three-body problem when both primaries are triaxial rigid bodies: Equilibrium points and periodic orbits |journal=Astrophysics and Space Science |date=25 August 2016 |volume=361 |issue=9 |pages=315 |doi=10.1007/s10509-016-2894-x |bibcode=2016Ap&SS.361..315E |s2cid=254252200 |url=https://link.springer.com/article/10.1007/s10509-016-2894-x |language=en |issn=1572-946X}}
* {{cite web|url=https://exoplanets.nasa.gov/alien-worlds/exoplanet-travel-bureau/explore-trappist-1d/?travel_bureau=true/|access-date=16 November 2021|title=Explore the Surface – TRAPPIST 1d|website=Exoplanet Travel Bureau|publisher=[[NASA]]|ref={{harvid|Exoplanet Travel Bureau|2021}}}}
* {{cite journal |last1=Fabbian |first1=D. |last2=Simoniello |first2=R. |last3=Collet |first3=R. |last4=Criscuoli |first4=S. |last5=Korhonen |first5=H. |last6=Krivova |first6=N. A. |last7=Oláh |first7=K. |last8=Jouve |first8=L. |last9=Solanki |first9=S. K. |last10=Alvarado-Gómez |first10=J. D. |last11=Booth |first11=R. |last12=García |first12=R. A. |last13=Lehtinen |first13=J. |last14=See |first14=V. |title=The variability of magnetic activity in solar-type stars |journal=Astronomische Nachrichten |date=2017 |volume=338 |issue=7 |pages=753–772 |bibcode=2017AN....338..753F |doi=10.1002/asna.201713403 |s2cid=53572712 |language=en |issn=1521-3994|doi-access=free }}
* {{cite journal |last1=Farrish |first1=Alison O. |last2=Alexander |first2=David |last3=Maruo |first3=Mei |last4=DeRosa |first4=Marc |last5=Toffoletto |first5=Frank |last6=Sciola |first6=Anthony M. |title=Characterizing the Magnetic Environment of Exoplanet Stellar Systems |journal=The Astrophysical Journal |date=30 October 2019 |volume=885 |issue=1 |pages=51 |doi=10.3847/1538-4357/ab4652 |bibcode=2019ApJ...885...51F |s2cid=209907654 |language=en|doi-access=free }}
* {{cite conference |last1=Fidrick |first1=Dawn |last2=Yeung |first2=Gee |last3=Niemack |first3=Bob |last4=Dixon |first4=Don |title=The Art and Science of Imaging Worlds: Griffith Observatory's planetarium show Signs of Life |conference=ACM SIGGRAPH 2020 Talks |date=17 August 2020 |pages=1–2 |doi=10.1145/3388767.3411060 |url=https://dl.acm.org/doi/abs/10.1145/3388767.3411060 |isbn=9781450379717 |s2cid=221178064 }}
* {{cite journal |last1=Fischer |first1=Christian |last2=Saur |first2=Joachim |title=Time-variable Electromagnetic Star–Planet Interaction: The TRAPPIST-1 System as an Exemplary Case |journal=The Astrophysical Journal |date=14 February 2019 |volume=872 |issue=1 |pages=113 |doi=10.3847/1538-4357/aafaf2 |arxiv=1901.02747 |bibcode=2019ApJ...872..113F |s2cid=119326120 |language=en |doi-access=free }}
* {{cite journal |last1=Flock |first1=Mario |last2=Turner |first2=Neal J. |last3=Mulders |first3=Gijs D. |last4=Hasegawa |first4=Yasuhiro |last5=Nelson |first5=Richard P. |last6=Bitsch |first6=Bertram |title=Planet formation and migration near the silicate sublimation front in protoplanetary disks |journal=Astronomy & Astrophysics |date=1 October 2019 |volume=630 |pages=A147 |doi=10.1051/0004-6361/201935806 |arxiv=1910.03901 |bibcode=2019A&A...630A.147F |s2cid=203027318 |language=en |issn=0004-6361}}
* {{Cite book |last=Fortney|first=Jonathan J.|chapter=Modeling Exoplanetary Atmospheres: An Overview|date=2018|title=Astrophysics of Exoplanetary Atmospheres|series=Astrophysics and Space Science Library|volume=450|pages=51–88|editor-last=Bozza|editor-first=Valerio|place=Cham|publisher=Springer International Publishing|doi=10.1007/978-3-319-89701-1_2|arxiv=1804.08149|isbn=978-3-319-89700-4|s2cid=59406383|editor-last2=Mancini|editor-first2=Luigi|editor-last3=Sozzetti|editor-first3=Alessandro}}
* {{cite journal |last1=Fraire |first1=Juan Andres |last2=Feldmann |first2=Marius |last3=Walter |first3=Felix |last4=Fantino |first4=Elena |last5=Burleigh |first5=Scott C. |title=Networking in Interstellar Dimensions: Communicating With TRAPPIST-1 |journal=IEEE Transactions on Aerospace and Electronic Systems |date=August 2019 |volume=55 |issue=4 |pages=1656–1665 |doi=10.1109/TAES.2018.2874149 |bibcode=2019ITAES..55.1656F |s2cid=117702090 |url=https://ieeexplore.ieee.org/document/8481450 |issn=1557-9603|hdl=11336/105240 |hdl-access=free }}
* {{cite journal |last1=Fraschetti |first1=F. |last2=Drake |first2=J. J. |last3=Alvarado-Gómez |first3=J. D. |last4=Moschou |first4=S. P. |last5=Garraffo |first5=C. |last6=Cohen |first6=O. |title=Stellar Energetic Particles in the Magnetically Turbulent Habitable Zones of TRAPPIST-1-like Planetary Systems |journal=The Astrophysical Journal |date=18 March 2019 |volume=874 |issue=1 |pages=21 |doi=10.3847/1538-4357/ab05e4 |arxiv=1902.03732 |bibcode=2019ApJ...874...21F |hdl=10150/633277 |s2cid=119081355 |language=en |doi-access=free }}
* {{cite journal |last1=Gabriel |first1=Travis S. J. |last2=Horn |first2=Harrison W.|title=Dependencies of Mantle Shock Heating in Pairwise Accretion |journal=The Astrophysical Journal Letters |date=1 July 2021 |volume=915 |issue=2 |pages=L32 |doi=10.3847/2041-8213/abffd1 |bibcode=2021ApJ...915L..32G |s2cid=235817461 |language=en|doi-access=free }}
* {{cite web|publisher=[[European Space Agency]]|year=2021|url=http://vizier.u-strasbg.fr/viz-bin/VizieR-S?Gaia%20EDR3%202635476908753563008|title=Gaia Early Data Release 3 (EDR3)|website=ESA Gaia Archive|access-date=1 September 2023|ref={{harvid|Gaia EDR3|2021}}}}
* {{cite book |url=http://link.springer.com/10.1007/978-3-642-11274-4 |title=Encyclopedia of Astrobiology |date=2011 |publisher=Springer Berlin Heidelberg |isbn=978-3-642-11271-3 |editor-last1=Gargaud |editor-first1=Muriel |editor-last2=Amils |editor-first2=Ricardo |editor-last3=Quintanilla |editor-first3=José Cernicharo |editor-last4=Cleaves |editor-first4=Henderson James |editor-last5=Irvine |editor-first5=William M. |editor-last6=Pinti |editor-first6=Daniele L. |editor-last7=Viso |editor-first7=Michel |location=Berlin, Heidelberg |language=en |doi=10.1007/978-3-642-11274-4 |bibcode=2011eab..book.....G |s2cid=90186988}}
* {{cite journal |last1=Gibb |first1=Bruce C. |title=Beyond Hubble |journal=Nature Chemistry |date=27 October 2022 |volume=14 |issue=11 |pages=1207–1209 |doi=10.1038/s41557-022-01080-2 |pmid=36302866 |bibcode=2022NatCh..14.1207G |s2cid=253184326 |url=https://www.nature.com/articles/s41557-022-01080-2 |language=en |issn=1755-4349}}
* {{cite journal |last1=Gillon |first1=Michaël |title=Life under another Sun: From Science Fiction to Science |journal=European Review |date=February 2020 |volume=28 |issue=1 |pages=18–39 |doi=10.1017/S1062798719000267 |hdl=2268/254712 |s2cid=210575064 |language=en |issn=1062-7987 |ref={{harvid|Gillon|2020a}}|hdl-access=free}}
* {{cite report |last=Gillon |first=Michaël |year=2020 |pages=49–52 |title=TRAPPIST-1: Toward the Comparative Study of Temperate Terrestrial Worlds |url=https://www.torrossa.com/en/resources/an/4847782 |url-access=subscription |ref={{harvid|Gillon|2020b}}}}
* {{cite conference |url=https://orbi.uliege.be/handle/2268/159868 |conference=Protostars and Planets VI |last1=Gillon |first1=M. |last2=Jehin |first2=E. |last3=Delrez |first3=L. |last4=Magain |first4=P. |last5=Opitom |first5=C. |last6=Sohy |first6=S. |location=Heidelberg |date=July 2013 |title=SPECULOOS: search for habitable planets eclipsing ULtra-cOOl stars|hdl=2268/159868 |format=PDF}}
* {{cite journal |last1=Gillon |first1=Michaël |last2=Jehin |first2=Emmanuël |last3=Lederer |first3=Susan M. |last4=Delrez |first4=Laetitia |last5=de Wit |first5=Julien |last6=Burdanov |first6=Artem |last7=Van Grootel |first7=Valérie |last8=Burgasser |first8=Adam J. |last9=Triaud |first9=Amaury H. M. J. |last10=Opitom |first10=Cyrielle |last11=Demory |first11=Brice-Olivier |last12=Sahu |first12=Devendra K. |last13=Bardalez Gagliuffi |first13=Daniella |last14=Magain |first14=Pierre |last15=Queloz |first15=Didier |title=Temperate Earth-sized planets transiting a nearby ultracool dwarf star |journal=Nature |date=May 2016 |volume=533 |issue=7602 |pages=221–224 |doi=10.1038/nature17448 |pmid=27135924 |pmc=5321506 |arxiv=1605.07211 |bibcode=2016Natur.533..221G |language=en |issn=1476-4687}}
* {{cite journal |last1=Gillon |first1=Michaël |last2=Triaud |first2=Amaury H. M. J. |last3=Demory |first3=Brice-Olivier |last4=Jehin |first4=Emmanuël |last5=Agol |first5=Eric |last6=Deck |first6=Katherine M. |last7=Lederer |first7=Susan M. |last8=de Wit |first8=Julien |last9=Burdanov |first9=Artem |last10=Ingalls |first10=James G. |last11=Bolmont |first11=Emeline |last12=Leconte |first12=Jeremy |last13=Raymond |first13=Sean N. |last14=Selsis |first14=Franck |last15=Turbet |first15=Martin |last16=Barkaoui |first16=Khalid |last17=Burgasser |first17=Adam |last18=Burleigh |first18=Matthew R. |last19=Carey |first19=Sean J. |last20=Chaushev |first20=Aleksander |last21=Copperwheat |first21=Chris M. |last22=Delrez |first22=Laetitia |last23=Fernandes |first23=Catarina S. |last24=Holdsworth |first24=Daniel L. |last25=Kotze |first25=Enrico J. |last26=Van Grootel |first26=Valérie |last27=Almleaky |first27=Yaseen |last28=Benkhaldoun |first28=Zouhair |last29=Magain |first29=Pierre |last30=Queloz |first30=Didier |title=Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1 |journal=Nature |date=February 2017 |volume=542 |issue=7642 |pages=456–460 |doi=10.1038/nature21360 |pmid=28230125 |pmc=5330437 |arxiv=1703.01424 |bibcode=2017Natur.542..456G |s2cid=4391722 |language=en |issn=1476-4687}}
* {{cite journal |last1=Gillon |first1=Michaël |last2=Meadows |first2=Victoria |last3=Agol |first3=Eric |last4=Burgasser |first4=Adam J. |last5=Deming |first5=Drake |last6=Doyon |first6=René |last7=Fortney |first7=Jonathan |last8=Kreidberg |first8=Laura |last9=Owen |first9=James |last10=Selsis |first10=Franck |last11=de Wit |first11=Julien |first12=Jacob |last12=Lustig-Yaeger |first13=Benjamin V. |last13=Rackham |date=2 December 2020 |title=The TRAPPIST-1 JWST Community Initiative |url=https://baas.aas.org/pub/2020i0208/release/1 |language=en |volume=52 |issue=2 |doi=10.3847/25c2cfeb.afbf0205 |journal=Bulletin of the AAS |page=0208 |arxiv=2002.04798 |bibcode=2020BAAS...52.0208G |s2cid=211082517 |doi-access=free}}
* {{cite journal |last1=Gizis |first1=John E. |last2=Monet |first2=David G. |last3=Reid |first3=I. Neill |last4=Kirkpatrick |first4=J. Davy |last5=Liebert |first5=James |last6=Williams |first6=Rik J. |title=New Neighbors from 2MASS: Activity and Kinematics at the Bottom of the Main Sequence |journal=The Astronomical Journal |date=August 2000 |volume=120 |issue=2 |pages=1085–1099 |doi=10.1086/301456|arxiv=astro-ph/0004361 |bibcode=2000AJ....120.1085G |s2cid=18819321 }}
* {{cite journal |last1=Glaser |first1=Donald M. |last2=Hartnett |first2=Hilairy Ellen |last3=Desch |first3=Steven J. |last4=Unterborn |first4=Cayman T. |last5=Anbar |first5=Ariel |last6=Buessecker |first6=Steffen |last7=Fisher |first7=Theresa |last8=Glaser |first8=Steven |last9=Kane |first9=Stephen R. |last10=Lisse |first10=Carey M. |last11=Millsaps |first11=Camerian |last12=Neuer |first12=Susanne |last13=O’Rourke |first13=Joseph G. |last14=Santos |first14=Nuno |last15=Walker |first15=Sara Imari |last16=Zolotov |first16=Mikhail |title=Detectability of Life Using Oxygen on Pelagic Planets and Water Worlds |journal=The Astrophysical Journal |date=April 2020 |volume=893 |issue=2 |pages=163 |doi=10.3847/1538-4357/ab822d |arxiv=2004.03631 |bibcode=2020ApJ...893..163G |language=en |issn=0004-637X |doi-access=free }}
* {{cite journal |last1=Glazier |first1=Amy L. |last2=Howard |first2=Ward S. |last3=Corbett |first3=Hank |last4=Law |first4=Nicholas M. |last5=Ratzloff |first5=Jeffrey K. |last6=Fors |first6=Octavi |last7=del Ser |first7=Daniel |title=Evryscope and K2 Constraints on TRAPPIST-1 Superflare Occurrence and Planetary Habitability |journal=The Astrophysical Journal |date=27 August 2020 |volume=900 |issue=1 |pages=27 |doi=10.3847/1538-4357/aba4a6 |arxiv=2006.14712 |bibcode=2020ApJ...900...27G |s2cid=220128346 |language=en |doi-access=free }}
* {{cite book |last1=Goldsmith |first1=Donald |title=Exoplanets: Hidden Worlds and the Quest for Extraterrestrial Life |date=10 September 2018 |publisher=Harvard University Press |isbn=978-0-674-98889-7 |doi=10.4159/9780674988897|bibcode=2018ehwq.book.....G |s2cid=240182683 }}
* {{cite journal |last1=Gonzales |first1=Eileen C. |last2=Faherty |first2=Jacqueline K.|author-link2=Jackie Faherty |last3=Gagné |first3=Jonathan |last4=Teske |first4=Johanna |last5=McWilliam |first5=Andrew |last6=Cruz |first6=Kelle |title=A Reanalysis of the Fundamental Parameters and Age of TRAPPIST-1 |journal=The Astrophysical Journal |date=29 November 2019 |volume=886 |issue=2 |pages=131 |doi=10.3847/1538-4357/ab48fc |arxiv=1909.13859 |bibcode=2019ApJ...886..131G |s2cid=203594024 |language=en |doi-access=free }}
* {{cite journal |last1=Grayver |first1=Alexander |last2=Bower |first2=Dan J. |last3=Saur |first3=Joachim |last4=Dorn |first4=Caroline |last5=Morris |first5=Brett M. |title=Interior Heating of Rocky Exoplanets from Stellar Flares with Application to TRAPPIST-1 |journal=The Astrophysical Journal Letters |date=7 December 2022 |volume=941 |issue=1 |pages=L7 |doi=10.3847/2041-8213/aca287 |arxiv=2211.06140 |bibcode=2022ApJ...941L...7G |s2cid=253499175 |language=en |doi-access=free }}
* {{cite journal |last1=Grenfell |first1=John Lee |title=A review of exoplanetary biosignatures |journal=Physics Reports |date=13 November 2017 |volume=713 |pages=1–17 |doi=10.1016/j.physrep.2017.08.003 |arxiv=1710.03976 |bibcode=2017PhR...713....1G |s2cid=119400674 |language=en |issn=0370-1573}}
* {{cite journal |last1=Grenfell |first1=John Lee |last2=Leconte |first2=Jeremy |last3=Forget |first3=François |last4=Godolt |first4=Mareike |last5=Carrión-González |first5=Óscar |last6=Noack |first6=Lena |last7=Tian |first7=Feng |last8=Rauer |first8=Heike |last9=Gaillard |first9=Fabrice |last10=Bolmont |first10=Émeline |last11=Charnay |first11=Benjamin |last12=Turbet |first12=Martin |title=Possible Atmospheric Diversity of Low Mass Exoplanets – Some Central Aspects |journal=Space Science Reviews | issn=1572-9672 |date=August 2020 |volume=216 |issue=5 |pages=98 |doi=10.1007/s11214-020-00716-4|arxiv=2101.01277 |bibcode=2020SSRv..216...98G |s2cid=225473867 }}
* {{cite journal |last1=Gressier |first1=A. |last2=Mori |first2=M. |last3=Changeat |first3=Q. |last4=Edwards |first4=B. |last5=Beaulieu |first5=J.-P. |last6=Marcq |first6=E. |last7=Charnay |first7=B. |title=Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations |journal=Astronomy & Astrophysics |year=2022 |volume=658 |pages=A133 |doi=10.1051/0004-6361/202142140 |arxiv=2112.05510 |bibcode=2022A&A...658A.133G |s2cid=245091619 |language=en |issn=0004-6361|via=[[arXiv]]}}
* {{cite journal |last1=Grimm |first1=Simon L. |last2=Demory |first2=Brice-Olivier |last3=Gillon |first3=Michaël |last4=Dorn |first4=Caroline |last5=Agol |first5=Eric |last6=Burdanov |first6=Artem |last7=Delrez |first7=Laetitia |last8=Sestovic |first8=Marko |last9=Triaud |first9=Amaury H. M. J. |last10=Turbet |first10=Martin |last11=Bolmont |first11=Émeline |last12=Caldas |first12=Anthony |last13=Wit |first13=Julien de |last14=Jehin |first14=Emmanuël |last15=Leconte |first15=Jérémy |last16=Raymond |first16=Sean N. |last17=Van Grootel |first17=Valérie |last18=Burgasser |first18=Adam J. |last19=Carey |first19=Sean |last20=Fabrycky |first20=Daniel |last21=Heng |first21=Kevin |last22=Hernandez |first22=David M. |last23=Ingalls |first23=James G. |last24=Lederer |first24=Susan |last25=Selsis |first25=Franck |last26=Queloz |first26=Didier |title=The nature of the TRAPPIST-1 exoplanets |journal=Astronomy & Astrophysics |date=1 May 2018 |volume=613 |pages=A68 |doi=10.1051/0004-6361/201732233 |arxiv=1802.01377 |bibcode=2018A&A...613A..68G |s2cid=3441829 |language=en |issn=0004-6361}}
* {{cite journal |last1=Guimond |first1=Claire Marie |last2=Rudge |first2=John F. |last3=Shorttle |first3=Oliver |title=Blue Marble, Stagnant Lid: Could Dynamic Topography Avert a Waterworld? |journal=The Planetary Science Journal |issn=2632-3338|date=1 March 2022 |volume=3 |issue=3 |pages=66 |doi=10.3847/psj/ac562e |arxiv=2201.05636 |bibcode=2022PSJ.....3...66G |s2cid=246015582 |doi-access=free }}
* {{cite journal |last1=Guridi |first1=Jose A. |last2=Pertuze |first2=Julio A. |last3=Pfotenhauer |first3=Sebastian M. |title=Natural laboratories as policy instruments for technological learning and institutional capacity building: The case of Chile's astronomy cluster |journal=Research Policy |date=1 March 2020 |volume=49 |issue=2 |pages=103899 |doi=10.1016/j.respol.2019.103899 |s2cid=197453914 |language=en |issn=0048-7333}}
* {{cite journal |last1=Günther |first1=Maximilian N. |last2=Berardo |first2=David A. |last3=Ducrot |first3=Elsa |last4=Murray |first4=Catriona A. |last5=Stassun |first5=Keivan G. |last6=Olah |first6=Katalin |last7=Bouma |first7=L. G. |last8=Rappaport |first8=Saul |last9=Winn |first9=Joshua N. |last10=Feinstein |first10=Adina D. |last11=Matthews |first11=Elisabeth C. |last12=Sebastian |first12=Daniel |last13=Rackham |first13=Benjamin V. |last14=Seli |first14=Bálint |last15=J. Triaud |first15=Amaury H. M. |last16=Gillen |first16=Edward |last17=Levine |first17=Alan M. |last18=Demory |first18=Brice-Olivier |last19=Gillon |first19=Michaël |last20=Queloz |first20=Didier |last21=Ricker |first21=George R. |last22=Vanderspek |first22=Roland K. |last23=Seager |first23=Sara |last24=Latham |first24=David W. |last25=Jenkins |first25=Jon M. |last26=Brasseur |first26=C. E. |last27=Colón |first27=Knicole D. |last28=Daylan |first28=Tansu |last29=Delrez |first29=Laetitia |last30=Fausnaugh |first30=Michael |last31=Garcia |first31=Lionel J. |last32=Jayaraman |first32=Rahul |last33=Jehin |first33=Emmanuel |last34=Kristiansen |first34=Martti H. |last35=Kruijssen |first35=J. M. Diederik |last36=Pedersen |first36=Peter Pihlmann |last37=Pozuelos |first37=Francisco J. |last38=Rodriguez |first38=Joseph E. |last39=Wohler |first39=Bill |last40=Zhan |first40=Zhuchang |title=Complex Modulation of Rapidly Rotating Young M Dwarfs: Adding Pieces to the Puzzle |journal=The Astronomical Journal |date=1 April 2022 |volume=163 |issue=4 |pages=144 |doi=10.3847/1538-3881/ac503c |arxiv=2008.11681 |bibcode=2022AJ....163..144G |s2cid=221319588 |language=en |doi-access=free }}
* {{cite journal |last1=Gutiérrez |first1=C. M. |last2=Arnold |first2=D. |last3=Copley |first3=D. |last4=Copperwheat |first4=C. M. |last5=Harvey |first5=E. |last6=Jermak |first6=H. |last7=Knapen |first7=J. |last8=McGrath |first8=A. |last9=Oria |first9=A. |last10=Rebolo |first10=R. |last11=Steele |first11=I. A. |last12=Torres |first12=M. |title=The new 4-m robotic telescope |journal=Astronomische Nachrichten |date=2019 |volume=340 |issue=1–3 |pages=40–45 |doi=10.1002/asna.201913556 |bibcode=2019AN....340...40G |s2cid=133136386 |language=en |issn=1521-3994|doi-access=free }}
* {{cite journal |last1=Hakim |first1=Kaustubh |last2=Rivoldini |first2=Attilio |last3=Van Hoolst |first3=Tim |last4=Cottenier |first4=Stefaan |last5=Jaeken |first5=Jan |last6=Chust |first6=Thomas |last7=Steinle-Neumann |first7=Gerd |title=A new ab initio equation of state of hcp-Fe and its implication on the interior structure and mass-radius relations of rocky super-Earths |journal=Icarus |date=1 October 2018 |volume=313 |pages=61–78 |doi=10.1016/j.icarus.2018.05.005 |arxiv=1805.10530 |bibcode=2018Icar..313...61H |s2cid=119442637 |language=en |issn=0019-1035}}
* {{cite book |title=Handbook of Scientific Tables |date=May 2022 |doi=10.1142/9789813278523_0001|author=National Astronomical Observatory of Japan|isbn=978-981-3278-53-0 |ref={{harvid|Handbook of Scientific Tables|2022}}}}
* {{cite journal |last1=Harbach |first1=Laura M. |last2=Moschou |first2=Sofia P. |last3=Garraffo |first3=Cecilia |last4=Drake |first4=Jeremy J. |last5=Alvarado-Gómez |first5=Julián D. |last6=Cohen |first6=Ofer |last7=Fraschetti |first7=Federico |title=Stellar Winds Drive Strong Variations in Exoplanet Evaporative Outflow Patterns and Transit Absorption Signatures |journal=The Astrophysical Journal |date=1 June 2021 |volume=913 |issue=2 |pages=130 |doi=10.3847/1538-4357/abf63a |arxiv=2012.05922 |bibcode=2021ApJ...913..130H |s2cid=228375956 |language=en |doi-access=free }}
* {{cite journal |last1=Heising |first1=Matthew Z. |last2=Sasselov |first2=Dimitar D. |last3=Hernquist |first3=Lars |last4=Luisa Tió Humphrey |first4=Ana |title=How Flat Can a Planetary System Get? I. The Case of TRAPPIST-1 |journal=The Astrophysical Journal |date=1 June 2021 |volume=913 |issue=2 |pages=126 |bibcode=2021ApJ...913..126H |doi=10.3847/1538-4357/abf8a8 |s2cid=219262616 |language=en|doi-access=free }}
* {{cite journal |last1=Hori |first1=Yasunori |last2=Ogihara |first2=Masahiro |title=Do the TRAPPIST-1 Planets Have Hydrogen-rich Atmospheres? |journal=The Astrophysical Journal |date=28 January 2020 |volume=889 |issue=2 |pages=77 |doi=10.3847/1538-4357/ab6168 |arxiv=1912.05749 |bibcode=2020ApJ...889...77H |s2cid=209324289 |language=en |doi-access=free }}
* {{cite journal |last1=Howard |first1=Ward S. |last2=Kowalski |first2=Adam F. |last3=Flagg |first3=Laura |last4=MacGregor |first4=Meredith A. |last5=Lim |first5=Olivia |last6=Radica |first6=Michael |last7=Piaulet |first7=Caroline |last8=Roy |first8=Pierre-Alexis |last9=Lafrenière |first9=David |last10=Benneke |first10=Björn |last11=Brown |first11=Alexander |last12=Espinoza |first12=Néstor |last13=Doyon |first13=René |last14=Coulombe |first14=Louis-Philippe |last15=Johnstone |first15=Doug |last16=Cowan |first16=Nicolas B. |last17=Jayawardhana |first17=Ray |last18=Turner |first18=Jake D. |last19=Dang |first19=Lisa |title=Characterizing the Near-infrared Spectra of Flares from TRAPPIST-1 during JWST Transit Spectroscopy Observations |journal=The Astrophysical Journal |date=1 December 2023 |volume=959 |issue=1 |pages=64 |doi=10.3847/1538-4357/acfe75 |doi-access=free |arxiv=2310.03792 |bibcode=2023ApJ...959...64H }}
* {{cite journal |last1=Howell |first1=Steve B. |last2=Everett |first2=Mark E. |last3=Horch |first3=Elliott P. |last4=Winters |first4=Jennifer G. |last5=Hirsch |first5=Lea |last6=Nusdeo |first6=Dan |last7=Scott |first7=Nicholas J. |title=Speckle Imaging Excludes Low-Mass Companions Orbiting the Exoplanet Host Star Trappist-1 |journal=The Astrophysical Journal |date=13 September 2016 |volume=829 |issue=1 |pages=L2 |doi=10.3847/2041-8205/829/1/l2 |arxiv=1610.05269 |bibcode=2016ApJ...829L...2H |s2cid=119183657 |language=en |doi-access=free }}
* {{cite book |url=https://iopscience.iop.org/book/978-0-7503-2296-6 |title=The NASA Kepler Mission |date=September 2020 |publisher=IOP Publishing |isbn=978-0-7503-2296-6 |editor-last=Howell |editor-first=Steve B. |doi=10.1088/2514-3433/ab9823ch3 |s2cid=224941774}}
* {{cite book |last1=Hughes |first1=Janette |editor-first1=Janette |editor-last1=Hughes |title=Making, makers, makerspaces : the shift to making in 20 schools |date=2022 |location=Cham |doi=10.1007/978-3-031-09819-2 |isbn=978-3-031-09819-2 |s2cid=251731356 |url=https://link.springer.com/book/10.1007/978-3-031-09819-2 |publisher=Springer |language=en}}
* {{cite journal |last1=Ih |first1=Jegug |last2=Kempton |first2=Eliza M.-R. |last3=Whittaker |first3=Emily A. |last4=Lessard |first4=Madeline |title=Constraining the Thickness of TRAPPIST-1 b's Atmosphere from Its JWST Secondary Eclipse Observation at 15 μm |journal=The Astrophysical Journal Letters |date=July 2023 |volume=952 |issue=1 |pages=L4 |doi=10.3847/2041-8213/ace03b |arxiv=2305.10414 |bibcode=2023ApJ...952L...4I |language=en |issn=2041-8205 |doi-access=free }}
* {{cite book |last1=Janjic |first1=Aleksandar |title=Lebensraum Universum |date=2017 |doi=10.1007/978-3-662-54787-8 |bibcode=2017leun.book.....J |isbn=978-3-662-54786-1 |language=en-gb}}
* {{cite web|url=https://photojournal.jpl.nasa.gov/catalog/PIA24371|access-date=31 August 2023|publisher=Jet Propulsion Laboratory|title=Comparison of TRAPPIST-1 to the Solar System|date=22 January 2021|ref={{harvid|JPL|2021}}}}
* {{cite journal |last1=Kaltenegger |first1=L. |last2=Faherty |first2=J. K. |title=Past, present and future stars that can see Earth as a transiting exoplanet |journal=Nature |date=June 2021 |volume=594 |issue=7864 |pages=505–507 |doi=10.1038/s41586-021-03596-y |pmid=34163055 |arxiv=2107.07936 |bibcode=2021Natur.594..505K |s2cid=235626242 |language=en |issn=1476-4687}}
* {{Cite book|last=Kanas|first=Nick|title=Star Maps: History, Artistry, and Cartography|date=2019|publisher=Springer International Publishing|isbn=978-3-030-13612-3|language=en|doi=10.1007/978-3-030-13613-0|s2cid=239353025}}
* {{cite journal |last1=Kane |first1=Stephen R. |last2=Arney |first2=Giada N. |last3=Byrne |first3=Paul K. |last4=Dalba |first4=Paul A. |last5=Desch |first5=Steven J. |last6=Horner |first6=Jonti |last7=Izenberg |first7=Noam R. |last8=Mandt |first8=Kathleen E. |last9=Meadows |first9=Victoria S. |last10=Quick |first10=Lynnae C. |title=The Fundamental Connections between the Solar System and Exoplanetary Science |journal=Journal of Geophysical Research: Planets | issn=2169-9100 |date=February 2021 |volume=126 |issue=2 |doi=10.1029/2020JE006643|arxiv=2012.11628 |bibcode=2021JGRE..12606643K |s2cid=233442891 }}
* {{cite journal |last1=Kane |first1=Stephen R. |title=Worlds without Moons: Exomoon Constraints for Compact Planetary Systems |journal=The Astrophysical Journal |date=13 April 2017 |volume=839 |issue=2 |pages=L19 |doi=10.3847/2041-8213/aa6bf2 |arxiv=1704.01688 |bibcode=2017ApJ...839L..19K |s2cid=119380874 |language=en |doi-access=free }}
* {{cite journal |last1=Kane |first1=Stephen R. |last2=Jansen |first2=Tiffany |last3=Fauchez |first3=Thomas |last4=Selsis |first4=Franck |last5=Ceja |first5=Alma Y. |title=Phase Modeling of the TRAPPIST-1 Planetary Atmospheres |journal=The Astronomical Journal |date=6 January 2021 |volume=161 |issue=2 |pages=53 |doi=10.3847/1538-3881/abcfbe |arxiv=2012.00080 |bibcode=2021AJ....161...53K |s2cid=227238721 |language=en |doi-access=free }}
* {{Cite conference|last1=Kendall|first1=M.|last2=Byrne|first2=P. K.|date=1 March 2020|title=Assessing Geological Conditions at the Ocean Floors of the TRAPPIST-1 Rocky Planets|url=https://www.hou.usra.edu/meetings/lpsc2020/pdf/3030.pdf|bibcode=2020LPI....51.3030K|pages=3030|conference=51st Lunar and Planetary Science Conference|location=[[The Woodlands, Texas]]}}
* {{cite journal |last1=Kislyakova |first1=K. G. |last2=Noack |first2=L. |last3=Johnstone |first3=C. P. |last4=Zaitsev |first4=V. V. |last5=Fossati |first5=L. |last6=Lammer |first6=H. |last7=Khodachenko |first7=M. L. |last8=Odert |first8=P. |last9=Güdel |first9=M. |title=Magma oceans and enhanced volcanism on TRAPPIST-1 planets due to induction heating |journal=Nature Astronomy |date=December 2017 |volume=1 |issue=12 |pages=878–885 |doi=10.1038/s41550-017-0284-0 |arxiv=1710.08761 |bibcode=2017NatAs...1..878K |s2cid=119429870 |language=en |issn=2397-3366}}
* {{cite journal |last1=Kochukhov |first1=Oleg |title=Magnetic fields of M dwarfs |journal=The Astronomy and Astrophysics Review |date=December 2021 |volume=29 |issue=1 |pages=1 |doi=10.1007/s00159-020-00130-3|arxiv=2011.01781 |bibcode=2021A&ARv..29....1K |s2cid=226237078 | issn=1432-0754 }}
* {{cite journal |last1=Kopparla |first1=Pushkar |last2=Natraj |first2=Vijay |last3=Crisp |first3=David |last4=Bott |first4=Kimberly |last5=Swain |first5=Mark R. |last6=Yung |first6=Yuk L. |title=Observing Oceans in Tightly Packed Planetary Systems: Perspectives from Polarization Modeling of the TRAPPIST-1 System |journal=The Astronomical Journal |date=10 September 2018 |volume=156 |issue=4 |pages=143 |doi=10.3847/1538-3881/aad9a1 |bibcode=2018AJ....156..143K |s2cid=125467757 |url=https://resolver.caltech.edu/CaltechAUTHORS:20190102-155140312 |language=en|doi-access=free }}
* {{cite journal |last1=Kral |first1=Quentin |last2=Wyatt |first2=Mark C. |last3=Triaud |first3=Amaury H. M. J. |last4=Marino |first4=Sebastian |last5=Thébault |first5=Philippe |last6=Shorttle |first6=Oliver |title=Cometary impactors on the TRAPPIST-1 planets can destroy all planetary atmospheres and rebuild secondary atmospheres on planets f, g, and h |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=11 September 2018 |volume=479 |issue=2 |pages=2649–2672 |arxiv=1802.05034 |bibcode=2018MNRAS.479.2649K |doi=10.1093/mnras/sty1677 |doi-access=free |s2cid=118880067 }}
* {{cite journal |last1=Kral |first1=Quentin |last2=Davoult |first2=Jeanne |last3=Charnay |first3=Benjamin |title=Formation of secondary atmospheres on terrestrial planets by late disk accretion |journal=Nature Astronomy |date=August 2020 |volume=4 |issue=8 |pages=769–775 |doi=10.1038/s41550-020-1050-2 |arxiv=2004.02496 |bibcode=2020NatAs...4..769K |s2cid=214802025 |language=en |issn=2397-3366}}
* {{cite journal |last1=Krissansen-Totton |first1=J. |last2=Fortney |first2=J. J. |title=Predictions for Observable Atmospheres of Trappist-1 Planets from a Fully Coupled Atmosphere–Interior Evolution Model |journal=The Astrophysical Journal |date=1 July 2022 |volume=933 |issue=1 |pages=115 |doi=10.3847/1538-4357/ac69cb |arxiv=2207.04164 |bibcode=2022ApJ...933..115K |s2cid=250374670 |language=en |doi-access=free }}
* {{cite journal |last1=Lane |first1=H. Chad |last2=Gadbury |first2=Matthew |last3=Ginger |first3=Jeff |last4=Yi |first4=Sherry |last5=Comins |first5=Neil |last6=Henhapl |first6=Jack |last7=Rivera-Rogers |first7=Aidan |title=Triggering STEM Interest With Minecraft in a Hybrid Summer Camp |journal=Innovations in Remote Instruction |date=28 November 2022 |volume=3 |issue=4 |doi=10.1037/tmb0000077 |s2cid=254344269 |url=https://tmb.apaopen.org/pub/5pkfd4sc/release/1?readingCollection=2cd16b3a |language=en|doi-access=free }}
* {{cite journal |last1=Lienhard |first1=F. |last2=Queloz|first2=D. |last3=Gillon |first3=M. |last4=Burdanov |first4=A. |last5=Delrez |first5=L. |last6=Ducrot |first6=E. |last7=Handley |first7=W. |last8=Jehin |first8=E. |last9=Murray |first9=C. A. |last10=Triaud |first10=A. H. M. J. |last11=Gillen |first11=E. |last12=Mortier|first12=A. |last13=Rackham |first13=B. V. |year=2020 |title=Global Analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey |journal=Monthly Notices of the Royal Astronomical Society |volume=497 |issue=3 |pages=3790–3808 |arxiv=2007.07278 |bibcode=2020MNRAS.497.3790L |doi=10.1093/mnras/staa2054 |doi-access=free |s2cid=220525769 |issn=1365-2966}}
* {{cite journal |last1=Lim |first1=Olivia |last2=Benneke |first2=Björn |last3=Doyon |first3=René |last4=MacDonald |first4=Ryan J. |last5=Piaulet |first5=Caroline |last6=Artigau |first6=Étienne |last7=Coulombe |first7=Louis-Philippe |last8=Radica |first8=Michael |last9=L’Heureux |first9=Alexandrine |last10=Albert |first10=Loïc |last11=Rackham |first11=Benjamin V. |last12=Wit |first12=Julien de |last13=Salhi |first13=Salma |last14=Roy |first14=Pierre-Alexis |last15=Flagg |first15=Laura |last16=Fournier-Tondreau |first16=Marylou |last17=Taylor |first17=Jake |last18=Cook |first18=Neil J. |last19=Lafrenière |first19=David |last20=Cowan |first20=Nicolas B. |last21=Kaltenegger |first21=Lisa |last22=Rowe |first22=Jason F. |last23=Espinoza |first23=Néstor |last24=Dang |first24=Lisa |last25=Darveau-Bernier |first25=Antoine |title=Atmospheric Reconnaissance of TRAPPIST-1 b with JWST/NIRISS: Evidence for Strong Stellar Contamination in the Transmission Spectra |journal=The Astrophysical Journal Letters |date=September 2023 |volume=955 |issue=1 |pages=L22 |doi=10.3847/2041-8213/acf7c4 |arxiv=2309.07047 |bibcode=2023ApJ...955L..22L |language=en |issn=2041-8205 |doi-access=free }}
* {{cite journal |last1=Lincowski |first1=Andrew P. |last2=Meadows |first2=Victoria S. |last3=Zieba |first3=Sebastian |last4=Kreidberg |first4=Laura |last5=Morley |first5=Caroline |last6=Gillon |first6=Michaël |last7=Selsis |first7=Franck |last8=Agol |first8=Eric |last9=Bolmont |first9=Emeline |last10=Ducrot |first10=Elsa |last11=Hu |first11=Renyu |last12=Koll |first12=Daniel D. B. |last13=Lyu |first13=Xintong |last14=Mandell |first14=Avi |last15=Suissa |first15=Gabrielle |last16=Tamburo |first16=Patrick |title=Potential Atmospheric Compositions of TRAPPIST-1 c Constrained by JWST/MIRI Observations at 15 μm |journal=The Astrophysical Journal Letters |date=1 September 2023 |volume=955 |issue=1 |pages=L7 |doi=10.3847/2041-8213/acee02 |arxiv=2308.05899 |bibcode=2023ApJ...955L...7L |doi-access=free }}
* {{cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |title=Physical constraints on the likelihood of life on exoplanets |journal=International Journal of Astrobiology |issn=1475-3006|date=April 2018 |volume=17 |issue=2 |pages=116–126 |doi=10.1017/S1473550417000179 |arxiv=1707.02996 |bibcode=2018IJAsB..17..116L |s2cid=35978131 |language=en |ref={{harvid|Lingam|Loeb|2018a}}}}
* {{cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |title=Implications of Tides for Life on Exoplanets |journal=Astrobiology |date=July 2018 |volume=18 |issue=7 |pages=967–982 |doi=10.1089/ast.2017.1718 |pmid=30010383 |arxiv=1707.04594 |bibcode=2018AsBio..18..967L |s2cid=51628150 |issn=1531-1074 |ref={{harvid|Lingam|Loeb|2018b}}}}
* {{Cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |date=August 2018 |title=Limitations of Chemical Propulsion for Interstellar Escape from Habitable Zones Around Low-mass Stars |journal=Research Notes of the AAS |volume=2 |issue=3 |pages=154 |doi=10.3847/2515-5172/aadcf4 |arxiv=1808.08141 |bibcode=2018RNAAS...2..154L |s2cid=119470444 |issn=2515-5172|ref={{harvid|Lingam|Loeb|2018c}} |doi-access=free }}
* {{cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |title=Colloquium: Physical constraints for the evolution of life on exoplanets |journal=Reviews of Modern Physics |date=11 June 2019 |volume=91 |issue=2 |pages=021002 |doi=10.1103/RevModPhys.91.021002 |arxiv=1810.02007 |bibcode=2019RvMP...91b1002L |s2cid=85501199 |ref={{harvid|Lingam|Loeb|2019a}}}}
* {{cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |title=Photosynthesis on habitable planets around low-mass stars |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=1 June 2019 |volume=485 |issue=4 |pages=5924–5928 |arxiv=1901.01270 |bibcode=2019MNRAS.485.5924L |doi=10.1093/mnras/stz847 |doi-access=free |s2cid=84843940 |ref={{harvid|Lingam|Loeb|2019b}}}}
* {{cite journal |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Abraham |title=Subsurface exolife |journal=International Journal of Astrobiology |issn=1475-3006|date=April 2019 |volume=18 |issue=2 |pages=112–141 |doi=10.1017/S1473550418000083 |arxiv=1711.09908 |bibcode=2019IJAsB..18..112L |s2cid=102480854 |ref={{harvid|Lingam|Loeb|2019c}}}}
* {{cite book |last1=Lingam |first1=Manasvi |last2=Loeb |first2=Avi |title=Life in the Cosmos |date=21 June 2021 |publisher=Harvard University Press |doi=10.4159/9780674259959 |isbn=978-0-674-25995-9 |s2cid=242834912 |language=en}}
* {{Cite book|last=Linsky|first=Jeffrey|title=Host Stars and their Effects on Exoplanet Atmospheres: An Introductory Overview|date=2019|publisher=Springer International Publishing|isbn=978-3-030-11451-0|series=Lecture Notes in Physics|volume=955|language=en|doi=10.1007/978-3-030-11452-7|s2cid=181923774}}
* {{cite journal |last1=Liu |first1=Beibei |last2=Ji |first2=Jianghui |title=A tale of planet formation: from dust to planets |journal=Research in Astronomy and Astrophysics |date=October 2020 |volume=20 |issue=10 |pages=164 |doi=10.1088/1674-4527/20/10/164 |arxiv=2009.02321 |bibcode=2020RAA....20..164L |s2cid=221507902 |language=en}}
* {{cite journal |last1=Luger |first1=Rodrigo |last2=Sestovic |first2=Marko |last3=Kruse |first3=Ethan |last4=Grimm |first4=Simon L. |last5=Demory |first5=Brice-Olivier |last6=Agol |first6=Eric |last7=Bolmont |first7=Emeline |last8=Fabrycky |first8=Daniel |last9=Fernandes |first9=Catarina S. |last10=Van Grootel |first10=Valérie |last11=Burgasser |first11=Adam |last12=Gillon |first12=Michaël |last13=Ingalls |first13=James G. |last14=Jehin |first14=Emmanuël |last15=Raymond |first15=Sean N. |last16=Selsis |first16=Franck |last17=Triaud |first17=Amaury H. M. J. |last18=Barclay |first18=Thomas |last19=Barentsen |first19=Geert |last20=Howell |first20=Steve B. |last21=Delrez |first21=Laetitia |last22=de Wit |first22=Julien |last23=Foreman-Mackey |first23=Daniel |last24=Holdsworth |first24=Daniel L. |last25=Leconte |first25=Jérémy |last26=Lederer |first26=Susan |last27=Turbet |first27=Martin |last28=Almleaky |first28=Yaseen |last29=Benkhaldoun |first29=Zouhair |last30=Magain |first30=Pierre |last31=Morris |first31=Brett M. |last32=Heng |first32=Kevin |last33=Queloz |first33=Didier |title=A seven-planet resonant chain in TRAPPIST-1 |journal=Nature Astronomy |date=22 May 2017 |volume=1 |issue=6 |page=0129 |doi=10.1038/s41550-017-0129 |arxiv=1703.04166 |bibcode=2017NatAs...1E.129L |s2cid=54770728 |language=en |issn=2397-3366}}
* {{cite journal |last1=Madhusudhan |first1=Nikku |title=Exoplanetary Atmospheres: Key Insights, Challenges, and Prospects |journal=Annual Review of Astronomy and Astrophysics |date=18 August 2019 |volume=57 |issue=1 |pages=617–663 |doi=10.1146/annurev-astro-081817-051846 |arxiv=1904.03190 |bibcode=2019ARA&A..57..617M |s2cid=102350577 |language=en |issn=0066-4146}}
* {{Cite book|last=Madhusudhan|first=Nikku|title=Exofrontiers: big questions in exoplanetary science|date=2020|isbn=978-0-7503-1472-5|oclc=1285004266|publisher=IOP Publishing}}
* {{cite book|last1=Malik|first1=Shoaib Ahmed|first2=Jörg Matthias|last2=Determann|title=Islamic Theology and Extraterrestrial Life: New Frontiers in Science and Religion|year=2024|pages=1-256}}
* {{cite journal |last1=Maltagliati |first1=Luca |title=Exoplanets: Why should we care about TRAPPIST-1? |journal=Nature Astronomy |date=27 March 2017 |volume=1 |issue=4 |page=0104 |doi=10.1038/s41550-017-0104 |bibcode=2017NatAs...1E.104M |s2cid=125667140 |language=en |issn=2397-3366}}
* {{cite journal |last1=Marino |first1=S. |last2=Wyatt |first2=M. C. |last3=Kennedy |first3=G. M. |last4=Kama |first4=M. |last5=Matrà |first5=L. |last6=Triaud |first6=A. H. M. J. |last7=Henning |first7=Th. |title=Searching for a dusty cometary belt around TRAPPIST-1 with ALMA |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=11 March 2020 |volume=492 |issue=4 |pages=6067–6073 |arxiv=1909.09158 |bibcode=2020MNRAS.492.6067M |doi=10.1093/mnras/staa266 |doi-access=free |s2cid=202712440 }}
* {{cite journal |last1=Marov |first1=M. Ya. |last2=Shevchenko |first2=I. I. |title=Exoplanets: nature and models |journal=Physics-Uspekhi |date=September 2020 |volume=63 |issue=9 |pages=837–871 |doi=10.3367/ufne.2019.10.038673 |bibcode=2020PhyU...63..837M |s2cid=209965726 |language=en |issn=1063-7869}}
* {{cite journal |last1=Martin |first1=Rebecca G. |last2=Livio |first2=Mario |title=Asteroids and Life: How Special Is the Solar System? |journal=The Astrophysical Journal Letters |date=1 February 2022 |volume=926 |issue=2 |pages=L20 |doi=10.3847/2041-8213/ac511c |arxiv=2202.01352 |bibcode=2022ApJ...926L..20M |s2cid=246485608 |language=en |doi-access=free }}
* {{cite journal |last1=Martínez-Rodríguez |first1=Héctor |last2=Caballero |first2=José Antonio |last3=Cifuentes |first3=Carlos |last4=Piro |first4=Anthony L. |last5=Barnes |first5=Rory |title=Exomoons in the Habitable Zones of M Dwarfs |journal=The Astrophysical Journal |date=26 December 2019 |volume=887 |issue=2 |pages=261 |doi=10.3847/1538-4357/ab5640 |arxiv=1910.12054 |bibcode=2019ApJ...887..261M |s2cid=204904780 |language=en |doi-access=free }}
* {{cite journal |last1=McDonough |first1=William F. |last2=Yoshizaki |first2=Takashi |title=Terrestrial planet compositions controlled by accretion disk magnetic field |journal=Progress in Earth and Planetary Science |date=2 July 2021 |volume=8 |issue=1 |pages=39 |doi=10.1186/s40645-021-00429-4 |bibcode=2021PEPS....8...39M |s2cid=235701559 |issn=2197-4284|doi-access=free }}
* {{Cite book|last=McKay|first=Tristan|url=https://www.cambridge.org/core/elements/semiotic-approach-to-open-notations/567788704882E093CF8032B846CC49AF|title=A Semiotic Approach to Open Notations: Ambiguity as Opportunity|date=2021|publisher=Cambridge University Press|isbn=978-1-108-81332-7|series=Elements in Music since 1945}}
* {{cite book |last1=Meadows |first1=Victoria S. |last2=Schmidt |first2=Britney E. |title=Planetary astrobiology |date=2020 |isbn=978-0-8165-4006-8 |oclc=1096534611 |url=https://www.worldcat.org/oclc/1096534611 |language=English|publisher=University of Arizona Press}}
* {{cite journal |last1=Meadows |first1=Victoria S. |last2=Arney |first2=Giada N. |last3=Schwieterman |first3=Edward W. |last4=Lustig-Yaeger |first4=Jacob |last5=Lincowski |first5=Andrew P. |last6=Robinson |first6=Tyler |last7=Domagal-Goldman |first7=Shawn D. |last8=Deitrick |first8=Russell |last9=Barnes |first9=Rory K. |last10=Fleming |first10=David P. |last11=Luger |first11=Rodrigo |last12=Driscoll |first12=Peter E. |last13=Quinn |first13=Thomas R. |last14=Crisp |first14=David |title=The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants |journal=Astrobiology |date=1 February 2018 |volume=18 |issue=2 |pages=133–189 |doi=10.1089/ast.2016.1589 |pmid=29431479 |pmc=5820795 |arxiv=1608.08620 |bibcode=2018AsBio..18..133M |issn=1531-1074}}
* {{cite journal |last1=Miles-Páez |first1=P. A. |last2=Zapatero Osorio|first2=M. R. |last3=Pallé |first3=E. |last4=Metchev |first4=S. A. |title=Time-resolved image polarimetry of TRAPPIST-1 during planetary transits |journal=Monthly Notices of the Royal Astronomical Society: Letters |date=21 March 2019 |volume=484 |issue=1 |pages=L38–L42 |arxiv=1901.02041 |bibcode=2019MNRAS.484L..38M |doi=10.1093/mnrasl/slz001 |doi-access=free |s2cid=119095657 |issn=1745-3925}}
* {{cite journal |last1=Morley |first1=Caroline V. |last2=Kreidberg |first2=Laura |last3=Rustamkulov |first3=Zafar |last4=Robinson |first4=Tyler |last5=Fortney |first5=Jonathan J. |title=Observing the Atmospheres of Known Temperate Earth-sized Planets with JWST |journal=The Astrophysical Journal |date=22 November 2017 |volume=850 |issue=2 |pages=121 |doi=10.3847/1538-4357/aa927b |arxiv=1708.04239 |bibcode=2017ApJ...850..121M |doi-access=free }}
* {{cite journal |last1=Morris |first1=Brett M. |last2=Agol |first2=Eric |last3=Davenport |first3=James R. A. |last4=Hawley |first4=Suzanne L. |title=Possible Bright Starspots on TRAPPIST-1 |journal=The Astrophysical Journal |date=11 April 2018 |volume=857 |issue=1 |pages=39 |doi=10.3847/1538-4357/aab6a5|arxiv=1803.04543 |bibcode=2018ApJ...857...39M |s2cid=55891098 |doi-access=free }}
* {{cite journal |last1=Morris |first1=Brett M. |last2=Agol |first2=Eric |last3=Hebb |first3=Leslie |last4=Hawley |first4=Suzanne L. |last5=Gillon |first5=Michaël |last6=Ducrot |first6=Elsa |last7=Delrez |first7=Laetitia |last8=Ingalls |first8=James |last9=Demory |first9=Brice-Olivier |title=Non-detection of Contamination by Stellar Activity in the Spitzer Transit Light Curves of TRAPPIST-1 |journal=The Astrophysical Journal Letters |date=17 August 2018 |volume=863 |issue=2 |pages=L32 |doi=10.3847/2041-8213/aad8aa |arxiv=1808.02808 |bibcode=2018ApJ...863L..32M |s2cid=53332500 |language=en |doi-access=free }}
* {{Cite journal|last1=Mullan|first1=D. J.|last2=Bais|first2=H. P.|date=27 September 2018|title=Photosynthesis on a Planet Orbiting an M Dwarf: Enhanced Effectiveness during Flares|journal=The Astrophysical Journal|language=en|volume=865|issue=2|pages=101|doi=10.3847/1538-4357/aadfd1|arxiv=1807.05267|bibcode=2018ApJ...865..101M|s2cid=119073856 |doi-access=free }}
* {{cite journal |last1=Mullan |first1=D. J. |last2=Paudel |first2=R. R. |title=Origin of Radio-quiet Coronal Mass Ejections in Flare Stars |journal=The Astrophysical Journal |date=27 February 2019 |volume=873 |issue=1 |pages=1 |doi=10.3847/1538-4357/ab041b |arxiv=1902.00810 |bibcode=2019ApJ...873....1M |s2cid=119420075 |language=en |doi-access=free }}
* {{cite web|url=https://nationalmaglab.org/about-the-maglab/around-the-lab/maglab-dictionary/tesla/|access-date=16 May 2023|date=18 November 2022|title=Tesla Definition|publisher=[[National High Magnetic Field Laboratory]]|ref={{harvid|MagLab|2022}}}}
* {{cite journal |last1=Navarro |first1=Thomas |last2=Merlis |first2=Timothy M. |last3=Cowan |first3=Nicolas B. |last4=Gomez |first4=Natalya |title=Atmospheric Gravitational Tides of Earth-like Planets Orbiting Low-mass Stars |journal=The Planetary Science Journal |issn=2632-3338|date=15 July 2022 |volume=3 |issue=7 |pages=162 |doi=10.3847/PSJ/ac76cd |arxiv=2207.06974 |bibcode=2022PSJ.....3..162N |s2cid=250526799 |language=en |doi-access=free }}
* {{cite journal |last1=Ogihara |first1=Masahiro |last2=Kokubo |first2=Eiichiro |last3=Nakano |first3=Ryuunosuke |last4=Suzuki |first4=Takeru K. |title=Rapid-then-slow migration reproduces mass distribution of TRAPPIST-1 system |journal=Astronomy & Astrophysics |date=1 February 2022 |volume=658 |pages=A184 |doi=10.1051/0004-6361/202142354 |arxiv=2201.08840 |bibcode=2022A&A...658A.184O |s2cid=246210342 |url=https://www.aanda.org/articles/aa/abs/2022/02/aa42354-21/aa42354-21.html |language=en |issn=0004-6361}}
* {{cite journal |last1=O'Malley-James |first1=Jack T. |last2=Kaltenegger |first2=L. |title=UV surface habitability of the TRAPPIST-1 system |journal=Monthly Notices of the Royal Astronomical Society: Letters | issn=1745-3933 |date=July 2017 |volume=469 |issue=1 |pages=L26–L30 |doi=10.1093/mnrasl/slx047|doi-access=free |arxiv=1702.06936 }}
* {{cite journal |last1=O'Malley-James |first1=Jack T. |last2=Kaltenegger |first2=Lisa |title=Biofluorescent Worlds – II. Biological fluorescence induced by stellar UV flares, a new temporal biosignature |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=1 October 2019 |volume=488 |issue=4 |pages=4530–4545 |doi=10.1093/mnras/stz1842 |doi-access=free |arxiv=1608.06930 }}
* {{cite journal |last1=Ormel |first1=Chris W. |last2=Liu |first2=Beibei |last3=Schoonenberg |first3=Djoeke |title=Formation of TRAPPIST-1 and other compact systems |journal=Astronomy & Astrophysics |date=1 August 2017 |volume=604 |pages=A1 |doi=10.1051/0004-6361/201730826 |arxiv=1703.06924 |bibcode=2017A&A...604A...1O |s2cid=4606360 |language=en |issn=0004-6361}}
* {{cite book |last1=Paladini |first1=Stefania |title=The New Frontiers of Space: Economic Implications, Security Issues and Evolving Scenarios |date=2019 |publisher=Springer |isbn=978-3-030-19941-8}}
* {{cite journal |title=Churchill's big idea |journal=Physics World | issn=2058-7058 |date=April 2017 |volume=30 |issue=4 |pages=3 |doi=10.1088/2058-7058/30/4/1 |ref={{harvid|Physics World|2017}} |language=en}}
* {{cite journal |last1=Pidhorodetska |first1=Daria |last2=Fauchez |first2=Thomas J. |last3=Villanueva |first3=Geronimo L. |last4=Domagal-Goldman |first4=Shawn D. |last5=Kopparapu |first5=Ravi K. |title=Detectability of Molecular Signatures on TRAPPIST-1e through Transmission Spectroscopy Simulated for Future Space-based Observatories |journal=The Astrophysical Journal Letters |date=July 2020 |volume=898 |issue=2 |pages=L33 |doi=10.3847/2041-8213/aba4a1 |arxiv=2001.01338 |bibcode=2020ApJ...898L..33P |hdl=11603/20595 |s2cid=209862793 |language=en |doi-access=free }}
* {{cite journal |last1=Pierrehumbert |first1=Raymond T. |last2=Hammond |first2=Mark |title=Atmospheric Circulation of Tide-Locked Exoplanets |journal=Annual Review of Fluid Mechanics |date=5 January 2019 |volume=51 |issue=1 |pages=275–303 |doi=10.1146/annurev-fluid-010518-040516 |bibcode=2019AnRFM..51..275P |s2cid=125645319 |language=en |issn=0066-4189|doi-access=free }}
* {{cite journal |last1=Pinchuk |first1=Pavlo |last2=Margot |first2=Jean-Luc |last3=Greenberg |first3=Adam H. |last4=Ayalde |first4=Thomas |last5=Bloxham |first5=Chad |last6=Boddu |first6=Arjun |last7=Chinchilla-Garcia |first7=Luis Gerardo |last8=Cliffe |first8=Micah |last9=Gallagher |first9=Sara |last10=Hart |first10=Kira |last11=Hesford |first11=Brayden |last12=Mizrahi |first12=Inbal |last13=Pike |first13=Ruth |last14=Rodger |first14=Dominic |last15=Sayki |first15=Bade |last16=Schneck |first16=Una |last17=Tan |first17=Aysen |last18=Xiao |first18=Yinxue "Yolanda" |last19=Lynch |first19=Ryan S. |title=A Search for Technosignatures from TRAPPIST-1, LHS 1140, and 10 Planetary Systems in the Kepler Field with the Green Bank Telescope at 1.15–1.73 GHz |journal=The Astronomical Journal |date=19 February 2019 |volume=157 |issue=3 |pages=122 |doi=10.3847/1538-3881/ab0105 |arxiv=1901.04057 |bibcode=2019AJ....157..122P |s2cid=113397518 |language=en |doi-access=free }}
* {{cite journal |last1=Pineda |first1=J. Sebastian |last2=Hallinan |first2=Gregg |title=A Deep Radio Limit for the TRAPPIST-1 System |journal=The Astrophysical Journal |date=24 October 2018 |volume=866 |issue=2 |pages=155 |doi=10.3847/1538-4357/aae078 |arxiv=1806.00480 |bibcode=2018ApJ...866..155P |s2cid=119209821 |language=en |doi-access=free }}
* {{Cite journal |last1=Quick |first1=Lynnae C. |last2=Roberge |first2=Aki |last3=Mlinar |first3=Amy Barr |last4=Hedman |first4=Matthew M. |date=August 2020|title=Forecasting Rates of Volcanic Activity on Terrestrial Exoplanets and Implications for Cryovolcanic Activity on Extrasolar Ocean Worlds |journal=Publications of the Astronomical Society of the Pacific |volume=132 |issue=1014 |pages=084402 |doi=10.1088/1538-3873/ab9504 |bibcode=2020PASP..132h4402Q |s2cid=219964895 |issn=0004-6280|doi-access=free }}
* {{cite journal |last1=Quick |first1=Lynnae C. |last2=Roberge |first2=Aki |last3=Mendoza |first3=Guadalupe Tovar |last4=Quintana |first4=Elisa V. |last5=Youngblood |first5=Allison A. |title=Prospects for Cryovolcanic Activity on Cold Ocean Planets |journal=The Astrophysical Journal |date=1 October 2023 |volume=956 |issue=1 |pages=29 |doi=10.3847/1538-4357/ace9b6 |bibcode=2023ApJ...956...29Q |doi-access=free }}
* {{cite journal |last1=Radnóti |first1=Katalin |title=Exoplanets in physics classes |journal=Journal of Physics: Conference Series | issn=1742-6596 |date=1 May 2021 |volume=1929 |issue=1 |pages=012015 |doi=10.1088/1742-6596/1929/1/012015 |bibcode=2021JPhCS1929a2015R |s2cid=235591431 |language=en|doi-access=free |hdl=10831/111866 |hdl-access=free }}
* {{cite journal |last1=Ranjan |first1=Sukrit |last2=Wordsworth |first2=Robin |last3=Sasselov |first3=Dimitar D. |title=The Surface UV Environment on Planets Orbiting M Dwarfs: Implications for Prebiotic Chemistry and the Need for Experimental Follow-up |journal=The Astrophysical Journal |date=11 July 2017 |volume=843 |issue=2 |pages=110 |doi=10.3847/1538-4357/aa773e |arxiv=1705.02350 |bibcode=2017ApJ...843..110R |s2cid=119502156 |language=en |doi-access=free }}
* {{cite journal |last1=Raymond |first1=Sean N. |last2=Izidoro |first2=Andre |last3=Bolmont |first3=Emeline |last4=Dorn |first4=Caroline |last5=Selsis |first5=Franck |last6=Turbet |first6=Martin |last7=Agol |first7=Eric |last8=Barth |first8=Patrick |last9=Carone |first9=Ludmila |last10=Dasgupta |first10=Rajdeep |last11=Gillon |first11=Michael |last12=Grimm |first12=Simon L. |title=An upper limit on late accretion and water delivery in the TRAPPIST-1 exoplanet system |journal=Nature Astronomy |date=25 November 2021 |volume=6 |pages=80–88 |doi=10.1038/s41550-021-01518-6 |arxiv=2111.13351 |s2cid=244668317 |language=en |issn=2397-3366}}
* {{cite web |title=Red Dwarf |url=https://astronomy.swin.edu.au/cosmos/r/red+dwarf |website=COSMOS - The SAO Encyclopedia of Astronomy |access-date=31 July 2022|ref={{harvid|The SAO Encyclopedia of Astronomy|2022|loc=Red Dwarf}}|publisher=[[Swinburne University of Technology]]}}
* {{cite conference|conference=The 24th International Conference on Auditory Display (ICAD 2018)|date=June 2018|location=[[Michigan Technological University]]|title=PLANETHESIZER: SONIFICATION CONCERT|first=Adrián García|last=Riber|url=http://icad2018.icad.org/wp-content/uploads/2018/06/ICAD2018_paper_43.pdf}}
* {{cite web |last1=Rinaldi |first1=David |last2=Núñez Ferrer |first2=Jorge |title=Cheers to a new solar system – and EU investment strategy. CEPS Commentary, 7 March 2017 |website=CEPS |date=March 2017 |url=http://aei.pitt.edu/85024/}}
* {{Cite journal |last1=Roettenbacher |first1=Rachael M. |last2=Kane |first2=Stephen R. |date=14 December 2017 |title=The Stellar Activity of TRAPPIST-1 and Consequences for the Planetary Atmospheres |journal=The Astrophysical Journal |volume=851 |issue=2 |pages=77 |doi=10.3847/1538-4357/aa991e |arxiv=1711.02676 |bibcode=2017ApJ...851...77R |s2cid=73535657 |doi-access=free }}
* {{cite journal |last1=Rushby |first1=Andrew J. |last2=Shields |first2=Aomawa L. |last3=Wolf |first3=Eric T. |last4=Laguë |first4=Marysa |last5=Burgasser |first5=Adam |title=The Effect of Land Albedo on the Climate of Land-dominated Planets in the TRAPPIST-1 System |journal=The Astrophysical Journal |date=26 November 2020 |volume=904 |issue=2 |pages=124 |doi=10.3847/1538-4357/abbe04 |arxiv=2011.03621 |bibcode=2020ApJ...904..124R |s2cid=226281770 |language=en |doi-access=free }}
* {{cite journal |last1=Sakaue |first1=Takahito |last2=Shibata |first2=Kazunari |title=An M Dwarf's Chromosphere, Corona, and Wind Connection via Nonlinear Alfvén Waves |journal=The Astrophysical Journal |date=1 September 2021 |volume=919 |issue=1 |pages=29 |doi=10.3847/1538-4357/ac0e34 |arxiv=2106.12752 |bibcode=2021ApJ...919...29S |s2cid=235624132 |language=en |doi-access=free }}
* {{cite journal |last1=Samara |first1=Evangelia |last2=Patsourakos |first2=Spiros |last3=Georgoulis |first3=Manolis K. |title=A Readily Implemented Atmosphere Sustainability Constraint for Terrestrial Exoplanets Orbiting Magnetically Active Stars |journal=The Astrophysical Journal Letters |date=1 March 2021 |volume=909 |issue=1 |pages=L12 |doi=10.3847/2041-8213/abe416 |arxiv=2102.07837 |bibcode=2021ApJ...909L..12S |s2cid=231933691 |language=en |doi-access=free }}
* {{cite journal |last1=Schlichting |first1=Hilke E. |last2=Young |first2=Edward D. |title=Chemical Equilibrium between Cores, Mantles, and Atmospheres of Super-Earths and Sub-Neptunes and Implications for Their Compositions, Interiors, and Evolution |journal=The Planetary Science Journal |issn=2632-3338|date=1 May 2022 |volume=3 |issue=5 |pages=127 |doi=10.3847/psj/ac68e6 |arxiv=2107.10405 |bibcode=2022PSJ.....3..127S |s2cid=236171388 |language=en |doi-access=free }}
* {{cite journal |last1=Schneider |first1=J. |last2=Dedieu |first2=C. |last3=Sidaner |first3=P. Le |last4=Savalle |first4=R. |last5=Zolotukhin |first5=I. |title=Defining and cataloging exoplanets: the exoplanet.eu database |journal=Astronomy & Astrophysics |date=1 August 2011 |volume=532 |pages=A79 |doi=10.1051/0004-6361/201116713 |arxiv=1106.0586 |bibcode=2011A&A...532A..79S |s2cid=55994657 |url=https://www.aanda.org/articles/aa/abs/2011/08/aa16713-11/aa16713-11.html |language=en |issn=0004-6361}}
* {{cite journal |last1=Schwieterman |first1=Edward W. |last2=Reinhard |first2=Christopher T. |last3=Olson |first3=Stephanie L. |last4=Harman |first4=Chester E. |last5=Lyons |first5=Timothy W. |title=A Limited Habitable Zone for Complex Life |journal=The Astrophysical Journal |date=10 June 2019 |volume=878 |issue=1 |pages=19 |doi=10.3847/1538-4357/ab1d52 |arxiv=1902.04720 |bibcode=2019ApJ...878...19S |s2cid=118948604 |language=en |doi-access=free }}
* {{cite book |title=The Euroschool on Exotic Beams - Vol. 5 |series=Lecture Notes in Physics |date=2018 |volume=948 |doi=10.1007/978-3-319-74878-8 |isbn=978-3-319-74878-8 |s2cid=220615062 |ref={{harvid|Euroschool|2018}} |language=en-gb|editor-last1=Scheidenberger|editor-first1=Christoph |editor-last2=Pfützner|editor-first2=Marek }}
* {{cite conference |last1=Sein |first1=Alexandr |last2=Duncan |first2=Colton |last3=Zhong |first3=Patrick |last4=Koock |first4=Elise |last5=Lee |first5=Waylon |last6=Jakubik |first6=Connor |last7=McHenry |first7=Neil |last8=Bruno |first8=Ashley |last9=Chamitoff |first9=Gregory |title=AIAA Scitech 2021 Forum |chapter=STEM Education Through Virtual Space System Design Competitions |year=2021 |doi=10.2514/6.2021-0481 |publisher=American Institute of Aeronautics and Astronautics |isbn=978-1-62410-609-5|conference=AIAA Scitech 2021 Forum |s2cid=234272238 }}
* {{cite journal |last1=Shields |first1=Aomawa L. |last2=Ballard |first2=Sarah |last3=Johnson |first3=John Asher |title=The habitability of planets orbiting M-dwarf stars |journal=Physics Reports |date=5 December 2016 |volume=663 |pages=1–38 |doi=10.1016/j.physrep.2016.10.003 |arxiv=1610.05765 |bibcode=2016PhR...663....1S |s2cid=119248081 |language=en |issn=0370-1573}}
* {{cite journal |last1=Shields |first1=Aomawa L. |last2=Carns |first2=Regina C. |title=Hydrohalite Salt-albedo Feedback Could Cool M-dwarf Planets |journal=The Astrophysical Journal |date=25 October 2018 |volume=867 |issue=1 |pages=11 |doi=10.3847/1538-4357/aadcaa |arxiv=1808.09977 |bibcode=2018ApJ...867...11S |s2cid=76652437 |language=en |doi-access=free }}
* {{cite report|last1=Short|first1=Kendra|first2=Karl|last2=Stapelfeldt|title=Exoplanet exploration program update|year=2017|url=https://trs.jpl.nasa.gov/bitstream/handle/2014/48124/CL%2317-2776.pdf?sequence=1|archive-url=https://web.archive.org/web/20211209151630/https://trs.jpl.nasa.gov/bitstream/handle/2014/48124/CL%2317-2776.pdf|archive-date=9 December 2021|url-status=dead|publisher=[[NASA Exoplanet Exploration Program]]}}
* {{cite journal |last1=Sleator |first1=Roy D. |last2=Smith |first2=Niall |title=TRAPPIST-1: The dawning of the age of Aquarius |journal=Bioengineered |date=4 May 2017 |volume=8 |issue=3 |pages=194–195 |doi=10.1080/21655979.2017.1306998 |pmid=28324663 |pmc=5470511 |issn=2165-5979}}
* {{cite journal |last1=Snellen |first1=Ignas A. G. |title=Earth's seven sisters |journal=Nature |date=February 2017 |volume=542 |issue=7642 |pages=421–422 |doi=10.1038/542421a |pmid=28230129 |hdl=1887/75076 |s2cid=205092857 |language=en |issn=1476-4687|hdl-access=free }}
* {{Cite journal|last=Srinivas|first=Susheela|date=August 2017|title=Are There Habitable Worlds Out There? – The Quest for Exoplanets|url=http://nopr.niscpr.res.in/bitstream/123456789/42535/1/SR%2054%288%29%2014-20.pdf|journal=Science Reporter |volume=54 |issue=8 |pages=14–20 |language=en-US|issn=0036-8512}}
* {{Cite book|last=Stevenson|first=David S.|title=Red Dwarfs: Their Geological, Chemical, and Biological Potential for Life|date=2019|publisher=Springer International Publishing|isbn=978-3-030-25549-7|language=en|doi=10.1007/978-3-030-25550-3|s2cid=203546646}}
* {{cite journal |last1=Tasker |first1=Elizabeth |title=Imagining other worlds Alien Earths: The New Science of Planet Hunting in the Cosmos Lisa Kaltenegger St. Martin's Press, 2024. 288 pp. |journal=Science |date=19 April 2024 |volume=384 |issue=6693 |pages=278 |doi=10.1126/science.ado1465 |url=https://www.science.org/doi/full/10.1126/science.ado1465 |language=en}}
* {{cite journal |last1=Teixeira |first1=Katie E. |last2=Morley |first2=Caroline V. |last3=Foley |first3=Bradford J. |last4=Unterborn |first4=Cayman T. |title=The Carbon-deficient Evolution of TRAPPIST-1c |journal=The Astrophysical Journal |date=December 2023 |volume=960 |issue=1 |pages=44 |doi=10.3847/1538-4357/ad0cec |doi-access=free |language=en |issn=0004-637X|arxiv=2311.17699 }}
* {{cite journal |last1=Turbet |first1=Martin |last2=Bolmont |first2=Emeline |last3=Leconte |first3=Jeremy |last4=Forget |first4=François |last5=Selsis |first5=Franck |last6=Tobie |first6=Gabriel |last7=Caldas |first7=Anthony |last8=Naar |first8=Joseph |last9=Gillon |first9=Michaël |title=Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets |journal=Astronomy & Astrophysics |date=1 April 2018 |volume=612 |pages=A86 |doi=10.1051/0004-6361/201731620 |arxiv=1707.06927 |bibcode=2018A&A...612A..86T |s2cid=53990543 |language=en |issn=0004-6361}}
* {{cite journal |last1=Turbet |first1=Martin |last2=Bolmont |first2=Emeline |last3=Bourrier |first3=Vincent |last4=Demory |first4=Brice-Olivier |last5=Leconte |first5=Jérémy |last6=Owen |first6=James |last7=Wolf |first7=Eric T. |title=A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System |journal=Space Science Reviews | issn=1572-9672 |date=August 2020 |volume=216 |issue=5 |pages=100 |doi=10.1007/s11214-020-00719-1 |pmid=32764836 |pmc=7378127 |arxiv=2007.03334 |bibcode=2020SSRv..216..100T }}
* {{cite journal |last1=Tusay |first1=Nick |last2=Sheikh |first2=Sofia Z. |last3=Sneed |first3=Evan L. |last4=Farah |first4=Wael |last5=Pollak |first5=Alexander W. |last6=Cruz |first6=Luigi F. |last7=Siemion |first7=Andrew |last8=DeBoer |first8=David R. |last9=Wright |first9=Jason T. |title=A Radio Technosignature Search of TRAPPIST-1 with the Allen Telescope Array |journal=The Astronomical Journal |date=1 December 2024 |volume=168 |issue=6 |pages=283 |doi=10.3847/1538-3881/ad823c |doi-access=free |arxiv=2409.08313 }}
* {{Cite book |last=Walsh |first=Kevin J. E. |url=https://link.springer.com/10.1007/978-3-031-68218-6 |title=Planets of the Known Galaxy: Fact and Fiction About the Nearest Stars and Their Worlds |date=2024 |publisher=Springer Nature Switzerland |isbn=978-3-031-68217-9 |series=Science and Fiction |location=Cham |language=en |doi=10.1007/978-3-031-68218-6}}
* {{cite journal |last1=Wang |first1=Jessie |title=Law of Gravity Blurred by Perturbed Planetary Orbits for Alien Observers |journal=Journal of Physics: Conference Series | issn=1742-6596|date=1 June 2022 |volume=2287 |issue=1 |pages=012039 |doi=10.1088/1742-6596/2287/1/012039 |bibcode=2022JPhCS2287a2039W |s2cid=250290787 |language=en|doi-access=free }}
* {{cite journal |last1=Wang |first1=Nan |last2=Lu |first2=Lu-Yao |last3=Liu |first3=Hui-Gen |last4=Chen |first4=An-Dong |last5=Lu |first5=Tiger |last6=Cui |first6=Ao-Ran |last7=Wang |first7=Jun-Kai |title=Development of Gravity Theories in the View of TRAPPIST-1e |journal=Research in Astronomy and Astrophysics |date=1 January 2025 |volume=25 |issue=1 |pages=015003 |doi=10.1088/1674-4527/ad9254 |url=https://iopscience.iop.org/article/10.1088/1674-4527/ad9254 |issn=1674-4527}}
* {{cite journal |last1=Wheatley |first1=Peter J. |last2=Louden |first2=Tom |last3=Bourrier |first3=Vincent |last4=Ehrenreich |first4=David |last5=Gillon |first5=Michaël |title=Strong XUV irradiation of the Earth-sized exoplanets orbiting the ultracool dwarf TRAPPIST-1 |journal=Monthly Notices of the Royal Astronomical Society: Letters | issn=1745-3933 |date=11 February 2017 |volume=465 |issue=1 |pages=L74–L78 |arxiv=1605.01564 |bibcode=2017MNRAS.465L..74W |doi=10.1093/mnrasl/slw192 |doi-access=free |s2cid=30087787 }}
* {{cite journal |last1=Wilson |first1=David J. |last2=Froning |first2=Cynthia S. |last3=Duvvuri |first3=Girish M. |last4=France |first4=Kevin |last5=Youngblood |first5=Allison |last6=Schneider |first6=P. Christian |last7=Berta-Thompson |first7=Zachory |last8=Brown |first8=Alexander |last9=Buccino |first9=Andrea P. |last10=Hawley |first10=Suzanne |last11=Irwin |first11=Jonathan |last12=Kaltenegger |first12=Lisa |last13=Kowalski |first13=Adam |last14=Linsky |first14=Jeffrey |last15=Parke Loyd |first15=R. O. |last16=Miguel |first16=Yamila |last17=Pineda |first17=J. Sebastian |last18=Redfield |first18=Seth |last19=Roberge |first19=Aki |last20=Rugheimer |first20=Sarah |last21=Tian |first21=Feng |last22=Vieytes |first22=Mariela |title=The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1 |journal=The Astrophysical Journal |date=1 April 2021 |volume=911 |issue=1 |pages=18 |doi=10.3847/1538-4357/abe771 |arxiv=2102.11415 |bibcode=2021ApJ...911...18W |s2cid=232014177 |language=en |doi-access=free }}
* {{cite journal |last1=Wolf |first1=Eric T. |title=Assessing the Habitability of the TRAPPIST-1 System Using a 3D Climate Model |journal=The Astrophysical Journal Letters |date=6 April 2017 |volume=839 |issue=1 |pages=L1 |doi=10.3847/2041-8213/aa693a |arxiv=1703.05815 |bibcode=2017ApJ...839L...1W |s2cid=119082049 |language=en |doi-access=free }}
* {{cite journal |last1=Wunderlich |first1=Fabian |last2=Scheucher |first2=Markus |last3=Godolt |first3=M. |last4=Grenfell |first4=J. L. |last5=Schreier |first5=F. |last6=Schneider |first6=P. C. |last7=Wilson |first7=D. J. |last8=Sánchez-López |first8=A. |last9=López-Puertas |first9=M. |last10=Rauer |first10=H. |title=Distinguishing between Wet and Dry Atmospheres of TRAPPIST-1 e and f |journal=The Astrophysical Journal |date=29 September 2020 |volume=901 |issue=2 |pages=126 |doi=10.3847/1538-4357/aba59c |arxiv=2006.11349 |bibcode=2020ApJ...901..126W |s2cid=219966834 |language=en |doi-access=free }}
* {{cite journal |last1=Valio |first1=Adriana |last2=Estrela |first2=Raissa |last3=Cabral |first3=Luisa |last4=Grangeiro |first4=Abel |title=The biological impact of superflares on planets in the Habitable Zone |journal=Proceedings of the International Astronomical Union |date=August 2018 |volume=14 |issue=S345 |pages=176–180 |doi=10.1017/S1743921319002035 |s2cid=216905441 |language=en |issn=1743-9213}}
* {{cite journal |last1=Van Hoolst |first1=Tim |last2=Noack |first2=Lena |last3=Rivoldini |first3=Attilio |title=Exoplanet interiors and habitability |journal=Advances in Physics: X |date=1 January 2019 |volume=4 |issue=1 |pages=1630316 |doi=10.1080/23746149.2019.1630316 |bibcode=2019AdPhX...430316V |s2cid=198417434 |doi-access=free }}
* {{cite journal |last1=Veras |first1=Dimitri |last2=Breedt |first2=Elmé |title=Eclipse, transit and occultation geometry of planetary systems at exo-syzygy |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=1 July 2017 |volume=468 |issue=3 |pages=2672–2683 |doi=10.1093/mnras/stx614 |doi-access=free |arxiv=1703.03414 }}
* {{Cite journal |last1=Vida |first1=Krisztián |last2=Kővári |first2=Zsolt |last3=Pál |first3=András |last4=Oláh |first4=Katalin |last5=Kriskovics |first5=Levente |title=Frequent flaring in the TRAPPIST-1 system – unsuited for life? |journal=The Astrophysical Journal |date=2 June 2017 |volume=841 |issue=2 |pages=124 |arxiv=1703.10130 |doi=10.3847/1538-4357/aa6f05 |bibcode=2017ApJ...841..124V |s2cid=118827117 |language=en |doi-access=free }}
* {{Cite journal |last1=Vida |first1=Krisztián |last2=Kővári |first2=Zsolt |last3=Leitzinger |first3=Martin |last4=Odert |first4=Petra |last5=Oláh |first5=Katalin |last6=Seli |first6=Bálint |last7=Kriskovics |first7=Levente |last8=Greimel |first8=Robert |last9=Görgei |first9=Anna |title=Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era |journal=Universe |bibcode=2024Univ...10..313V |date=31 July 2024 |volume=10 |issue=8 |pages=313 |arxiv=2407.16446 |doi=10.3390/universe10080313 |language=en |doi-access=free }}
* {{Cite journal |last1=Vinson |first1=Alec M. |last2=Tamayo |first2=Daniel |last3=Hansen |first3=Brad M. S. |title=The Chaotic Nature of TRAPPIST-1 Planetary Spin States |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=1 August 2019 |volume=488 |issue=4 |pages=5739–5747 |arxiv=1905.11419 |bibcode=2019MNRAS.488.5739V |doi=10.1093/mnras/stz2113 |doi-access=free |s2cid=167217467 |language=en}}
* {{cite conference |last1=Yang |first1=J. |last2=Ji |first2=W. |title=Proxima b, TRAPPIST 1e, and LHS 1140b: Increased Ice Coverages by Sea Ice Dynamics |journal=AGU Fall Meeting Abstracts |date=1 December 2018 |volume=2018 |pages=P43G–3826 |bibcode=2018AGUFM.P43G3826Y |conference=American Geophysical Union, Fall Meeting 2018|location=[[Washington DC]]}}
* {{cite journal |last1=Zanazzi |first1=J. J. |last2=Lai |first2=Dong |title=Triaxial deformation and asynchronous rotation of rocky planets in the habitable zone of low-mass stars |journal=Monthly Notices of the Royal Astronomical Society | issn=1365-2966 |date=11 August 2017 |volume=469 |issue=3 |pages=2879–2885 |arxiv=1702.07327 |bibcode=2017MNRAS.469.2879Z |doi=10.1093/mnras/stx1076 |doi-access=free |s2cid=119430179 }}
* {{cite journal |last1=Zanazzi |first1=J. J. |last2=Triaud |first2=Amaury H. M. J. |title=The ability of significant tidal stress to initiate plate tectonics |journal=Icarus |date=1 June 2019 |volume=325 |pages=55–66 |arxiv=1711.09898 |doi=10.1016/j.icarus.2019.01.029 |bibcode=2019Icar..325...55Z |s2cid=96450290 |language=en |issn=0019-1035}}
* {{Cite journal|last=Zhang|first=Xi|date=July 2020|title=Atmospheric regimes and trends on exoplanets and brown dwarfs|journal=Research in Astronomy and Astrophysics|language=en|volume=20|issue=7|pages=099|doi=10.1088/1674-4527/20/7/99|arxiv=2006.13384|bibcode=2020RAA....20...99Z|s2cid=220042096|issn=1674-4527}}
* {{cite journal |last1=Zhang |first1=Zhanbo |last2=Zhou |first2=Yifan |last3=Rackham |first3=Benjamin V. |last4=Apai |first4=Dániel |title=The Near-infrared Transmission Spectra of TRAPPIST-1 Planets b, c, d, e, f, and g and Stellar Contamination in Multi-epoch Transit Spectra |journal=The Astronomical Journal |date=4 October 2018 |volume=156 |issue=4 |pages=178 |doi=10.3847/1538-3881/aade4f |arxiv=1802.02086 |bibcode=2018AJ....156..178Z |hdl=10150/631598 |s2cid=118938032 |language=en |doi-access=free }}
* {{cite journal |last1=Greene |first1=Thomas P. |last2=Bell |first2=Taylor J. |last3=Ducrot |first3=Elsa |last4=Dyrek |first4=Achrène |last5=Lagage |first5=Pierre-Olivier |last6=Fortney |first6=Jonathan J. |date=March 2023 |title=Thermal Emission from the Earth-sized Exoplanet TRAPPIST-1 b using JWST |journal=[[Nature (journal)|Nature]] |volume=618 |issue=7963 |pages=39–42 |doi=10.1038/s41586-023-05951-7 |pmid=36972683 |arxiv=2303.14849 |bibcode=2023Natur.618...39G|s2cid=257767242 }}
{{refend}}

== Further reading==
* {{cite journal |last1=Arcand |first1=Kimberly K. |last2=Price |first2=Sara R. |last3=Watzke |first3=Megan |title=Holding the Cosmos in Your Hand: Developing 3D Modeling and Printing Pipelines for Communications and Research |journal=Frontiers in Earth Science |date=2020 |volume=8 |pages=541 |doi=10.3389/feart.2020.590295 |arxiv=2012.02789 |bibcode=2020FrEaS...8..541A |issn=2296-6463|ref=none|doi-access=free }}
* {{cite report |last1=Dzombeta |first1=Krstinja |last2=Percy |first2=John |title=Flare Stars: A Short Review |date=31 October 2019 |url=https://tspace.library.utoronto.ca/handle/1807/97060 |language=en-ca|ref=none}}
* {{cite journal |last1=Fauchez |first1=Thomas J. |last2=Turbet |first2=Martin |last3=Wolf |first3=Eric T. |last4=Boutle |first4=Ian |last5=Way |first5=Michael J. |last6=Del Genio |first6=Anthony D. |last7=Mayne |first7=Nathan J. |last8=Tsigaridis |first8=Konstantinos |last9=Kopparapu |first9=Ravi K. |last10=Yang |first10=Jun |last11=Forget |first11=Francois |last12=Mandell |first12=Avi |last13=Domagal Goldman |first13=Shawn D. |title=TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0 |journal=Geoscientific Model Development |date=21 February 2020 |volume=13 |issue=2 |pages=707–716 |doi=10.5194/gmd-13-707-2020 |arxiv=2002.10950 |bibcode=2020GMD....13..707F |s2cid=211296491 |url=https://gmd.copernicus.org/articles/13/707/2020/gmd-13-707-2020.html |language=English |issn=1991-959X|ref=none |doi-access=free }}

== External links ==
{{Commons category}}
* {{cite web |url=http://www.trappist.one/ |website=TRAPPIST.one |title=The discovery team's official website}}
* {{cite web |title=Ultracool dwarf with planets |series=ESOcast 83 |publisher=European Southern Observatory |url=http://www.eso.org/public/videos/eso1615a/}}

{{TRAPPIST-1}}
{{Stars of Aquarius|collapsed=yes}}
{{2016 in space}}
{{2017 in space}}
{{Portal bar|Astronomy|Biology|Outer space|Star}}
[[Category:TRAPPIST-1| ]]
[[Category:2017 in outer space]]
[[Category:2MASS objects|J23062928-0502285]]
[[Category:Aquarius (constellation)]]
[[Category:M-type main-sequence stars]]
[[Category:Planetary systems with seven confirmed planets]]
[[Category:Planetary transit variables]]
[[Category:Astronomical objects discovered in 1999]]