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{{Short description|Red dwarf star with Earth-like planet}} ...nown as '''SPECULOOS-2''' or '''TOI-4306''', is a high proper motion [[red dwarf]] star located {{convert|105|ly|pc|lk=on}} away from the [[Solar System]] i ...

{{Short description|A measure for the size of planets and other Solar System objects}} ...les/aa/pdf/2011/04/aa15811-10.pdf|title=Distorted, nonspherical transiting planets: impact on the transit depth and on the radius determination|first1=J.|last ...

....jpg|thumb|510x510px|Though differing in size and temperature, terrestrial planets of the Solar System were reported to have high Earth Similarity Index value ...rankings. The webpage also ranks what it describes as the habitability of planets and moons according to three criteria: the location in the habitable zone, ...

| type = [[White dwarf]] + [[red dwarf]] | component1 = White dwarf ...

{{short description|Lowest possible mass of the celestial object}} ...ne-of-sight]], so the real [[orbital inclination]]s and true masses of the planets are generally unknown.<ref name="Astrobiology"/> This is a result of '''si ...

...tural satellite|moon]] of the [[trans-Neptunian object|trans-Neptunian]] [[dwarf planet]] [[Makemake]].<ref name="Parker2016"/><ref name="PlanetarySociety"/ ...[[Herschel Space Observatory|Herschel]]'' space telescopes showed that the dwarf planet emits more thermal radiation than expected for its size and brightne ...

| discovery_method = [[Methods of detecting extrasolar planets#Radial velocity|Radial velocity]] ([[European Southern Observatory]]) ...f> is an [[exoplanet]] orbiting within the [[habitable zone]] of the [[red dwarf]] star [[Gliese 667 C]], which is a member of the [[Gliese 667]] triple sta ...

...ng within the [[Circumstellar habitable zone|habitable zone]] of the [[red dwarf]] [[Kepler-1229]], located about 870 [[light year]]s (267 [[parsec]]s) from {{See also|Habitability of red dwarf systems}} ...

...6,500|ly|pc|abbr=off|sp=us}} away from [[Earth]]. It orbits with a [[brown dwarf]] or [[Super-Jupiter]] companion with a period of 9.2 hours with an eclipse == Planets == ...

...er, about 35% of the mass consists of stars that have evolved into [[white dwarf]]s or other [[stellar remnant]]s. The remainder of lost mass consists of st ...title=Planets around evolved intermediate-mass stars. II. Are there really planets around IC 4651 No. 9122, NGC 2423 No. 3, and NGC 4349 No. 127? |journal=[[A ...

[[File:2022 229 Display.jpg|thumb|Exoplanet and Brown Dwarf Models displayed at Clifton Park Museum.]] ...170416044528/http://www.sify.com/news/astronomy-dabbler-discovers-four-new-planets-news-international-lben4jeiiacsi.html|archive-date=2017-04-16}}</ref><ref n ...

...ost distant observed natural object in the [[Solar System]], after [[Eris (dwarf planet)|Eris]] and {{mpl|2014 UZ|224}}.{{efn|name=UZ}} ...wing it up and refining its orbit. It is expected to come to [[Opposition (planets)|opposition]] in the [[constellation]] of [[Aries (constellation)|Aries]] a ...

{{Short description|Sub-brown dwarf in the constellation Hydra}} | type = [[Sub-brown dwarf]] ...

...by an amateur is the [[Gravitational microlensing#Detection of extrasolar planets|microlensing exoplanet]] [[Kojima-1Lb]].<ref name="Fukui2019"/> ...ve formed in a closer orbit around the star via [[Nebular hypothesis#Giant planets|core accretion or disk instability]] and was later dynamically disturbed in ...

...bited by a massive, 'dark' secondary that is actually itself a close [[red dwarf]] binary, making a hierarchal triple system. ...main sequence star. This was interpreted as the companion being a [[white dwarf]]. ...

| type = red dwarf ...taken with GMOS at [[Gemini South]], which showed a spectral type of [[red dwarf|M5.5/M6]] and strong [[Hydrogen-alpha]] emission. The [[astrometry]] showed ...

...ebble accretion in the inner Solar System resulting in smaller terrestrial planets, a small mass of [[Mars]] and a low mass asteroid belt. ...rechts|first1=M.|last2=Johansen|first2=A.|title=Forming the cores of giant planets from the radial pebble flux in protoplanetary discs|journal=Astronomy & Ast ...

...iated energy about [[red giant]] stars and [[White dwarf|white]] and [[red dwarf]] stars could support a time-integrated ''BIOTA'' up to 10⁴⁶ kg- ...e results allow assessing the soil fertilities of the parent asteroids and planets, and the amounts of biomass that they can sustain.<ref name="Mautner-2002" ...

...large [[trans-Neptunian object|trans-Neptunian]] [[dwarf planet]] [[Orcus (dwarf planet)|Orcus]]. It was discovered by [[Michael E. Brown|Michael Brown]] an ...pr09"/>}} On 23 March 2009, Brown asked readers of his [[blog]] to suggest possible names for the satellite, with the best one to be submitted to the [[Interna ...

| type2 = [[Brown dwarf]]<ref name=Meshkat2015/><ref name=Franson2022/> ...g star, estimated 30 to 200 million years old, and is orbited by a [[brown dwarf]] companion. [[Parallax]] measurements by the [[Gaia (spacecraft)|Gaia]] sp ...