View source for List of directly imaged exoplanets

{{Short description|Exoplanets confirmed or discovered from direct imaging}}
{{use dmy dates|date=August 2024}}
{{cs1 config |display-authors=6|name-list-style=vanc }}
[[File:HR 8799 Orbiting Exoplanets.gif|thumb|right|Motion interpolation of seven images of the [[HR 8799]] system taken from the [[W. M. Keck Observatory]] over seven years, featuring four [[exoplanet]]s]]
This is a '''list of extrasolar planets that have been directly observed''', sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star.  Currently, this list includes both [[Methods of detecting extrasolar planets#Direct imaging|directly imaged]] planets and imaged planetary-mass companions (objects that orbit a star but formed through a binary-star-formation process, not a planet-formation process). This list does not include free-floating planetary-mass objects in star-forming regions or young associations, which are also referred to as [[rogue planet]]s.

The data given for each planet is taken from the latest published paper on the planet to have that data. In many cases it is not possible to have an exact value, and an estimated range is instead provided. The coldest and oldest planet directly imaged is [[Epsilon Indi Ab]], which has six times Jupiter's mass, an effective temperature of 275 K, and an age of about 3.5{{nbs}}Ga.
This list includes the four members of the multi-planet system that orbit [[HR 8799]].

It is unlikely or at least unclear if objects on a wide orbit (≥100 AU) formed in [[Circumstellar disc|circumstellar disks]] and these objects are therefore more often referred as planetary-mass companions.<ref>{{Cite journal |last=Bowler |first=Brendan P. |date=2016-10-01 |title=Imaging Extrasolar Giant Planets |url=https://ui.adsabs.harvard.edu/abs/2016PASP..128j2001B |journal=Publications of the Astronomical Society of the Pacific |volume=128 |issue=968 |pages=102001 |arxiv=1605.02731 |bibcode=2016PASP..128j2001B |doi=10.1088/1538-3873/128/968/102001 |issn=0004-6280 |archive-date=2 October 2023 |access-date=26 April 2024 |archive-url=https://web.archive.org/web/20231002123826/https://ui.adsabs.harvard.edu/abs/2016PASP..128j2001B |url-status=live }}</ref><ref name=":2" /><ref name=":3" /> Only in rare cases, such as for [[HD 106906 b]], the formation of the object in the disk is seen plausible.

== Key ==
Exoplanets have been discovered using several different methods for collecting or combining direct images to isolate planets from the background light of their star. [[Aperture masking interferometry|Non-Redundant Aperture Masking Interferometry]] is a method of combining the views of multiple telescopes into a single image, while the other methods are algorithms for combining multiple direct images taken from the same telescope.

* '''ADI''' = Angular Differential Imaging
*'''KLIP''' = Karhunen–Loève Image Processing
* '''LOCI''' = Locally Optimized Combination of Images
* '''NRM''' = Non-Redundant [[Aperture masking interferometry|Aperture Masking Interferometry]]
* '''RSDI''' = Reference Star Differential Imaging
*'''SDI''' = Spectral Differential Imaging
* '''TLOCI''' = Template Locally Optimized Combination of Images

== Exoplanets ==
Although listed in the table below, the identities of [[Candidate 1]], [[FW Tau b]], 2MASS J044144 b, and HD 100546 b are disputed. They may not actually be true exoplanets.
<span style="margin:0px; padding-bottom:1px; font-size:90%; display:block;"><span style="border:#aaa solid 1px;>&nbsp;&nbsp;†&nbsp;&nbsp;</span>&nbsp;There is no consensus whether these companions of stars should be considered [[sub-brown dwarf]]s or planets</span>
Check https://exoplanetarchive.ipac.caltech.edu/docs/imaging.html to see more directly imaged planets. It contains an updated table of all of them.
{{sticky header}}
{| class="sortable wikitable sticky-header"
|-
! scope="col" | [[Star]]
! scope="col" | [[Exoplanet]]
! scope="col" class="unsortable" | Image
! scope="col" | [[Planetary mass|Mass]] ([[Jupiter mass|M<sub>J</sub>]])
! scope="col" | [[Radius]] ([[Jupiter radius|R<sub>J</sub>]])
! scope="col" | [[Orbital period|Period]] ([[Year|yr]])
! scope="col" | Observed separation ([[Astronomical Unit|AU]])
! scope="col" | [[Orbital eccentricity|Eccentricity]]
! scope="col" | Distance to Earth (ly)
! scope="col" | Year of discovery
! scope="col" | Imaging technique
! scope="col" class="unsortable" | Ref(s).
|-
![[WISE 0146+4234]]
|WISE 0146+4234 B† 
| style="background-color: black;" | [[File:WISE 0146+4234 AB.jpg|50px]]
|{{Ntsh|10}}10 ±4
|
|10
|{{Val|0.93|0.12|0.16}}
|
|63
|2015
|AO
|
|-
![[WISE J0336−0143|WISE J0336-0143]]
|WISE J0336-0143 B† 
| style="background-color: black;" |
|{{Ntsh|4}}4-12.5
|
|5-9
|{{Val|0.97|0.05|0.09}}
|
|33
|2023
|source subtraction
|<ref>{{Cite journal |last1=Calissendorff |first1=Per |last2=De Furio |first2=Matthew |last3=Meyer |first3=Michael |last4=Albert |first4=Loïc |last5=Aganze |first5=Christian |last6=Ali-Dib |first6=Mohamad |last7=Bardalez Gagliuffi |first7=Daniella C. |last8=Baron |first8=Frederique |last9=Beichman |first9=Charles A. |last10=Burgasser |first10=Adam J. |last11=Cushing |first11=Michael C. |last12=Faherty |first12=Jacqueline Kelly |last13=Fontanive |first13=Clémence |last14=Gelino |first14=Christopher R. |last15=Gizis |first15=John E. |date=2023-04-01 |title=JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05-014350.4 |journal=The Astrophysical Journal |volume=947 |issue=2 |pages=L30 |arxiv=2303.16923 |bibcode=2023ApJ...947L..30C |doi=10.3847/2041-8213/acc86d |issn=0004-637X |doi-access=free}}</ref>
|-
! scope="row" | [[Alpha Centauri A]]
| [[Alpha Centauri Ab]] (?)
| style="background-color: black;" | [[File:Candidate1 Discovery.png|50px]]
| {{Ntsh|0.11}}0.11±0.05
| {{Ntsh|0.459}}0.459±0.17
| ~1
| 1.1
|
| 4.37
| 2021
|
|
|-
![[CFBDSIR J145829+101343]]
|CFBDSIR J145829+101343 b
| style="background-color: black;" | [[File:Brown Dwarf Binary CFBDSIR 1458+10.tif|50px]]
|{{Ntsh|10.5}}10.5{{±|4.5}}
|
|27.5{{±|7.5}}
|2.6{{±|0.3}}
|
|104
|2011
|Direct imaging
|
|-
! rowspan="2" |[[HD 206893]]
|HD 206893 c
| rowspan="2" style="background-color: black;" |
|{{Ntsh|12.7}}{{Val|12.7|1.2|1.0}}
|{{Ntsh|1.46}}{{Val|1.46|0.18|0.06}}
|5.7
|{{Val|3.53|0.08|0.06}}
|{{Val|0.41|0.03}}
| rowspan="2" |133
|2023
|interferometry
|<ref name=":0">{{Cite journal |last1=Hinkley |first1=S. |last2=Lacour |first2=S. |last3=Marleau |first3=G. -D. |last4=Lagrange |first4=A.-M. |last5=Wang |first5=J. J. |last6=Kammerer |first6=J. |last7=Cumming |first7=A. |last8=Nowak |first8=M. |last9=Rodet |first9=L. |last10=Stolker |first10=T. |last11=Balmer |first11=W. -O. |last12=Ray |first12=S. |last13=Bonnefoy |first13=M. |last14=Mollière |first14=P. |last15=Lazzoni |first15=C. |date=2023-03-01 |title=Direct discovery of the inner exoplanet in the HD 206893 system. Evidence for deuterium burning in a planetary-mass companion |url=https://ui.adsabs.harvard.edu/abs/2023A&A...671L...5H |journal=Astronomy and Astrophysics |volume=671 |pages=L5 |arxiv=2208.04867 |bibcode=2023A&A...671L...5H |doi=10.1051/0004-6361/202244727 |issn=0004-6361}}</ref>
|-
|HD 206893 B†
|{{Ntsh|28}}{{Val|28.0|2.2|2.1}}
|{{Ntsh|1.25}}{{Val|1.25|0.02}}
|26
|{{Val|9.6|0.4|0.3}}
|{{Val|0.14|0.05}}
|2017
|ADI, PCA
|<ref>{{Cite journal |last1=Milli |first1=J. |last2=Hibon |first2=P. |last3=Christiaens |first3=V. |last4=Choquet |first4=É. |last5=Bonnefoy |first5=M. |last6=Kennedy |first6=G. M. |last7=Wyatt |first7=M. C. |last8=Absil |first8=O. |last9=Gómez González |first9=C. A. |last10=del Burgo |first10=C. |last11=Matrà |first11=L. |last12=Augereau |first12=J. -C. |last13=Boccaletti |first13=A. |last14=Delacroix |first14=C. |last15=Ertel |first15=S. |date=2017-01-01 |title=Discovery of a low-mass companion inside the debris ring surrounding the F5V star HD 206893 |url=https://ui.adsabs.harvard.edu/abs/2017A%26A...597L...2M |journal=Astronomy and Astrophysics |volume=597 |pages=L2 |arxiv=1612.00333 |bibcode=2017A&A...597L...2M |doi=10.1051/0004-6361/201629908 |issn=0004-6361 |archive-date=1 December 2023 |access-date=4 February 2024 |archive-url=https://web.archive.org/web/20231201043913/https://ui.adsabs.harvard.edu/abs/2017A%26A...597L...2M |url-status=live }}</ref><ref name=":0" />
|-
![[WISE 1217+1626]]
|WISE 1217+1626 A b
| style="background-color: black;"| [[File:WISE 1217+1626 AB Hubble WFC3IR.jpg|50px]]
|{{Ntsh|22}}22{{±|2}}
|{{Ntsh|0.934}}0.934{{±|0.029}}
|130-210
|8.0{{±|1.3}}
|
|30.4
|2012
|Direct imaging
|<ref name=":1" />
|-
![[AF Leporis]]
|AF Lep b
| style="background-color: black;" | [[File:Potw2308a(1).jpg|50px]]
|{{Ntsh|2}}2-5.5
|
|20.6
|8
|0.47
|87
|2023
|Direct imaging
|<ref name="Franson Bowler Zhou Pearce 2023 p. L19">{{Cite journal |last1=Franson |first1=Kyle |last2=Bowler |first2=Brendan P. |last3=Zhou |first3=Yifan |last4=Pearce |first4=Tim D. |last5=Bardalez Gagliuffi |first5=Daniella C. |last6=Biddle |first6=Lauren I. |last7=Brandt |first7=Timothy D. |last8=Crepp |first8=Justin R. |last9=Dupuy |first9=Trent J. |last10=Faherty |first10=Jacqueline |last11=Jensen-Clem |first11=Rebecca |last12=Morgan |first12=Marvin |last13=Sanghi |first13=Aniket |last14=Theissen |first14=Christopher A. |last15=Tran |first15=Quang H. |date=2023 |title=Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged inside the Debris Disk of the Young Star AF Lep |journal=The Astrophysical Journal Letters |publisher=American Astronomical Society |volume=950 |issue=2 |page=L19 |arxiv=2302.05420 |bibcode=2023ApJ...950L..19F |doi=10.3847/2041-8213/acd6f6 |s2cid=256808203 |doi-access=free |last16=Wolf |first16=Trevor N.}}</ref><ref>{{Cite journal |last1=Mesa |first1=D. |last2=Gratton |first2=R. |last3=Kervella |first3=P. |last4=Bonavita |first4=M. |last5=Desidera |first5=S. |last6=D'Orazi |first6=V. |last7=Marino |first7=S. |last8=Zurlo |first8=A. |last9=Rigliaco |first9=E. |date=2023-02-13 |title=AF Lep b: The lowest-mass planet detected by coupling astrometric and direct imaging data |journal=Astronomy & Astrophysics |volume=672 |pages=A93 |arxiv=2302.06213 |bibcode=2023A&A...672A..93M |doi=10.1051/0004-6361/202345865}}</ref><ref>{{Cite journal |last1=De Rosa |first1=Robert J. |last2=Nielsen |first2=Eric L. |last3=Wahhaj |first3=Zahed |last4=Ruffio |first4=Jean-Baptise |last5=Kalas |first5=Paul G. |last6=Peck |first6=Anne E. |last7=Hirsch |first7=Lea A. |last8=Roberson |first8=William |date=2023-02-13 |title=Direct imaging discovery of a super-Jovian around the young Sun-like star AF Leporis |journal=Astronomy & Astrophysics |volume=672 |pages=A94 |arxiv=2302.06332 |bibcode=2023A&A...672A..94D |doi=10.1051/0004-6361/202345877}}</ref>
|-
! scope="row" | [[Beta Pictoris]]
| [[Beta Pictoris b]]
| style="background-color: black;" | [[File:Beta Pictoris b orbit animated (2013-2018).gif|50px]]
| {{Ntsh|12.7}}12.7{{±|0.3}}
| {{Ntsh|1.46}}1.46{{±|0.01}}<ref name="Chilcote2017">{{Cite journal |last1=Chilcote |first1=Jeffrey |last2=Pueyo |first2=Laurent |last3=Rosa |first3=Robert J. De |last4=Vargas |first4=Jeffrey |last5=MacIntosh |first5=Bruce |last6=Bailey |first6=Vanessa P. |last7=Barman |first7=Travis |last8=Bauman |first8=Brian |last9=Bruzzone |first9=Sebastian |last10=Bulger |first10=Joanna |last11=Burrows |first11=Adam S. |last12=Cardwell |first12=Andrew |last13=Chen |first13=Christine H. |last14=Cotten |first14=Tara |last15=Dillon |first15=Daren |year=2017 |title=1–2.4μm Near-IR Spectrum of the Giant Planet β Pictoris b Obtained with the Gemini Planet Imager |journal=The Astronomical Journal |volume=153 |issue=4 |at=182 |arxiv=1703.00011 |bibcode=2017AJ....153..182C |doi=10.3847/1538-3881/aa63e9 |s2cid=23669676 |doi-access=free |last16=Doyon |first16=Rene |last17=Draper |first17=Zachary H. |last18=Duchêne |first18=Gaspard |last19=Dunn |first19=Jennifer |last20=Erikson |first20=Darren |last21=Fitzgerald |first21=Michael P. |last22=Follette |first22=Katherine B. |last23=Gavel |first23=Donald |last24=Goodsell |first24=Stephen J. |last25=Graham |first25=James R. |last26=Greenbaum |first26=Alexandra Z. |last27=Hartung |first27=Markus |last28=Hibon |first28=Pascale |last29=Hung |first29=Li-Wei |last30=Ingraham |first30=Patrick}}</ref>
| 22.47{{±|3.77|2.26}}
| 9
| 0.08{{±|0.09|0.05}}
| {{sort|0063|63.4{{±|0.1}}}}
| 2008
| RSDI
| <ref>{{Cite journal |last1=Wang |first1=Jason J. |last2=Graham |first2=James R. |last3=Pueyo |first3=Laurent |last4=Kalas |first4=Paul |last5=Millar-Blanchaer |first5=Maxwell A. |last6=Ruffio |first6=Jean-Baptiste |last7=De Rosa |first7=Robert J. |last8=Ammons |first8=S. Mark |last9=Arriaga |first9=Pauline |last10=Bailey |first10=Vanessa P. |last11=Barman |first11=Travis S. |last12=Bulger |first12=Joanna |last13=Burrows |first13=Adam S. |last14=Cardwell |first14=Andrew |last15=Chen |first15=Christine H. |date=2016-10-01 |title=The Orbit and Transit Prospects for β Pictoris b Constrained With One Milliarcsecond Astrometry |journal=The Astronomical Journal |volume=152 |issue=4 |pages=97 |arxiv=1607.05272 |bibcode=2016AJ....152...97W |doi=10.3847/0004-6256/152/4/97 |issn=0004-6256 |s2cid=119181273 |doi-access=free}}</ref><ref>{{Cite journal |last1=Bonnefoy |first1=M. |last2=Marleau |first2=G.-D. |last3=Galicher |first3=R. |last4=Beust |first4=H. |last5=Lagrange |first5=A.-M. |last6=Baudino |first6=J.-L. |last7=Chauvin |first7=G. |last8=Borgniet |first8=S. |last9=Meunier |first9=N. |last10=Rameau |first10=J. |last11=Boccaletti |first11=A. |last12=Cumming |first12=A. |last13=Helling |first13=C. |last14=Homeier |first14=D. |last15=Allard |first15=F. |date=July 2014 |title=Physical and orbital properties of β Pictoris b |url=http://www.aanda.org/10.1051/0004-6361/201424041 |journal=Astronomy & Astrophysics |volume=567 |pages=L9 |arxiv=1407.4001 |bibcode=2014A&A...567L...9B |doi=10.1051/0004-6361/201424041 |issn=0004-6361 |s2cid=55863534}}</ref><ref name="CurrieBurrows2013">{{Cite journal |last1=Currie |first1=Thayne |last2=Burrows |first2=Adam |last3=Madhusudhan |first3=Nikku |last4=Fukagawa |first4=Misato |last5=Girard |first5=Julien H. |last6=Dawson |first6=Rebekah |last7=Murray-Clay |first7=Ruth |last8=Kenyon |first8=Scott |last9=Kuchner |first9=Marc |last10=Matsumura |first10=Soko |last11=Jayawardhana |first11=Ray |last12=Chambers |first12=John |last13=Bromley |first13=Ben |year=2013 |title=A Combined Very Large Telescope and Gemini Study of the Atmosphere of the Directly Imaged Planet, β Pictoris b |journal=The Astrophysical Journal |volume=776 |issue=1 |pages=15 |arxiv=1306.0610 |bibcode=2013ApJ...776...15C |doi=10.1088/0004-637X/776/1/15 |issn=0004-637X |s2cid=118825345}}</ref><ref>{{Cite journal |last1=Morzinski |first1=Katie M. |last2=Males |first2=Jared R. |last3=Skemer |first3=Andy J. |last4=Close |first4=Laird M. |last5=Hinz |first5=Phil M. |last6=Rodigas |first6=T. J. |last7=Puglisi |first7=Alfio |last8=Esposito |first8=Simone |last9=Riccardi |first9=Armando |last10=Pinna |first10=Enrico |last11=Xompero |first11=Marco |last12=Briguglio |first12=Runa |last13=Bailey |first13=Vanessa P. |last14=Follette |first14=Katherine B. |last15=Kopon |first15=Derek |date=2015-12-15 |title=Magellan Adaptive Optics First-Light Observations of the Exoplanet β PIC b. II. 3–5 μ m Direct Imaging With MagAO+Clio, and the Empirical Bolometric Luminosity of a Self-Luminous Giant Planet |url=https://iopscience.iop.org/article/10.1088/0004-637X/815/2/108 |journal=The Astrophysical Journal |volume=815 |issue=2 |pages=108 |arxiv=1511.02894 |bibcode=2015ApJ...815..108M |doi=10.1088/0004-637X/815/2/108 |issn=1538-4357 |s2cid=118559024}}</ref>
|-
![[LP 852-7]]
|WD 1202–232 b
| style="background-color: black;" | [[File:WD 1202-232 MIRI.jpg|50px]]
|{{Ntsh|1}}1-7
|
|50
|11.47
|
|34
|2024 (unconfirmed)
|PSF-subtraction
|<ref name="Mullally2024">{{Cite journal |last1=Mullally |first1=Susan E. |last2=Debes |first2=John |last3=Cracraft |first3=Misty |last4=Mullally |first4=Fergal |last5=Poulsen |first5=Sabrina |last6=Albert |first6=Loic |last7=Thibault |first7=Katherine |last8=Reach |first8=William T. |last9=Hermes |first9=J. J. |last10=Barclay |first10=Thomas |last11=Kilic |first11=Mukremin |last12=Quintana |first12=Elisa V. |date=24 Jan 2024 |title=JWST Directly Images Giant Planet Candidates Around Two Metal-Polluted White Dwarf Stars |journal=The Astrophysical Journal Letters |volume=962 |issue=2 |pages=L32 |arxiv=2401.13153 |bibcode=2024ApJ...962L..32M |doi=10.3847/2041-8213/ad2348 |doi-access=free}}</ref>
|-
! scope="row" | [[51 Eridani]]
| [[51 Eridani b]]
| style="background-color: black;" | [[File:51 Eridani b orbit animated (2014-2018).gif|50px]]
| {{Ntsh|2.6}}2.6
| {{Ntsh|1}}1.0
| ?
| 13
| ?
| {{sort|0096|96}}
| 2014
| ADI, KLIP
| <ref>{{Cite journal |last1=Macintosh |first1=B. |last2=Graham |first2=J. R. |last3=Barman |first3=T. |last4=De Rosa |first4=R. J. |last5=Konopacky |first5=Q. |last6=Marley |first6=M. S. |last7=Marois |first7=C. |last8=Nielsen |first8=E. L. |last9=Pueyo |first9=L. |last10=Rajan |first10=A. |last11=Rameau |first11=J. |last12=Saumon |first12=D. |last13=Wang |first13=J. J. |last14=Patience |first14=J. |last15=Ammons |first15=M. |display-authors=etal |date=2015-10-02 |title=Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager |url=https://www.science.org/doi/10.1126/science.aac5891 |journal=Science |language=en |volume=350 |issue=6256 |pages=64–67 |arxiv=1508.03084 |bibcode=2015Sci...350...64M |doi=10.1126/science.aac5891 |issn=0036-8075 |pmid=26272904 |s2cid=8177945 |archive-date=6 October 2024 |access-date=28 August 2024 |archive-url=https://web.archive.org/web/20241006062606/https://www.science.org/doi/10.1126/science.aac5891 |url-status=live }}</ref>
|-
![[WISE 1711+3500]]
|WISE 1711+3500 B
| style="background-color: black;" | [[File:W1711 JWST MIRI.jpg|50px]]
|{{Ntsh|8.7}}8.7-22
|
|280-430
|15{{±|2}}
|
|62
|2012
|laser AO
|<ref name=":1">{{Cite journal |last1=Liu |first1=Michael C. |last2=Dupuy |first2=Trent J. |last3=Bowler |first3=Brendan P. |last4=Leggett |first4=S. K. |last5=Best |first5=William M. J. |date=2012-10-01 |title=Two Extraordinary Substellar Binaries at the T/Y Transition and the Y-band Fluxes of the Coolest Brown Dwarfs |url=https://iopscience.iop.org/article/10.1088/0004-637X/758/1/57 |journal=The Astrophysical Journal |volume=758 |issue=1 |pages=57 |arxiv=1206.4044 |bibcode=2012ApJ...758...57L |doi=10.1088/0004-637X/758/1/57 |issn=0004-637X}}</ref>
|-
! rowspan="4" scope="row" | [[HR 8799]]
| [[HR 8799 e]]
| rowspan="4" style="background-color: black;" | [[File:HR 8799 Orbiting Exoplanets.gif|50px]]
| {{Ntsh|7}}7.0
| {{Ntsh|1.3}}1.3
| 49
| 14.5
| 0.14
| {{sort|0128|128}}
| 2010
| ADI, LOCI
|
|-
| [[HR 8799 d]]
| {{Ntsh|7}}7.0
| {{Ntsh|1.3}}1.3
| 100
| 24.5
| 0.09
| {{sort|0128|128}}
| 2008
| ADI, LOCI
|
|-
| [[HR 8799 c]]
| {{Ntsh|7}}7.0
| {{Ntsh|1.3}}1.3
| 189
| 37.4
| 0.24
| {{sort|0128|128}}
| 2008
| ADI, LOCI
|
|-
| [[HR 8799 b]]
| {{Ntsh|5}}5.0
| {{Ntsh|1.2}}1.2
| 474
| 69.2
| 0.17
| {{sort|0128|128}}
| 2008
| ADI, LOCI
|
|-
! scope="row" | [[2MASS J04414489+2301513|2M J044144]]
| 2M J044144 b†
| style="background-color: black;" | [[File:Brown dwarf 2M J044144 and planet.jpg|50px]]
| {{Ntsh|5}}5–10
|
|
| 15
|
| {{sort|0456|456}}
| 2010
| Direct imaging
|
|-
! scope="row" | [[29 Cygni]]
| [[HIP 99770 b]]
| style="background-color: black;" | [[File:HIP 99770 b.png|50px]]
| {{Ntsh|13.9}}13.9-16.1
| {{Ntsh|1.05}}1.05
| 51.0
| 16.9
| 0.25
| 130.9
| 2022
| ALOCI
| <ref name="Currie2022b">{{Citation |last1=Currie |first1=Thayne |title=Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star |journal=Science |volume=380 |issue=6641 |pages=198–203 |year=2023 |arxiv=2212.00034 |bibcode=2023Sci...380..198C |doi=10.1126/science.abo6192 |pmid=37053312 |last2=Brandt |first2=G. Mirek |last3=Brandt |first3=Timothy D. |last4=Lacy |first4=Brianna |last5=Burrows |first5=Adam |last6=Guyon |first6=Olivier |last7=Tamura |first7=Motohide |last8=Liu |first8=Ranger Y. |last9=Sagynbayeva |first9=Sabina |last10=Tobin |first10=Taylor |last11=Chilcote |first11=Jeffrey |last12=Groff |first12=Tyler |last13=Marois |first13=Christian |last14=Thompson |first14=William |last15=Murphy |first15=Simon J. |last16=Kuzuhara |first16=Masayuki |last17=Lawson |first17=Kellen |last18=Lozi |first18=Julien |last19=Deo |first19=Vincent |last20=Vievard |first20=Sebastien |last21=Skaf |first21=Nour |last22=Uyama |first22=Taichi |last23=Jovanovic |first23=Nemanja |last24=Martinache |first24=Frantz |last25=Kasdin |first25=N. Jeremy |last26=Kudo |first26=Tomoyuki |last27=McElwain |first27=Michael |last28=Janson |first28=Markus |last29=Wisniewski |first29=John |last30=Hodapp |first30=Klaus}}</ref>
|-
![[HD 28736|HIP 21152]]
|HIP 21152 b
| style="background-color: black;"|
|{{Ntsh|26}}{{Val|24|6|4}}
|
|60.3
|{{Val|17|5|4}}
|{{Val|0.36|0.37|0.25}}
|141
|2022
|Direct imaging
|<ref>{{Cite journal |last1=Kuzuhara |first1=Masayuki |last2=Currie |first2=Thayne |last3=Takarada |first3=Takuya |last4=Brandt |first4=Timothy D. |last5=Sato |first5=Bun'ei |last6=Uyama |first6=Taichi |last7=Janson |first7=Markus |last8=Chilcote |first8=Jeffrey |last9=Tobin |first9=Taylor |last10=Lawson |first10=Kellen |last11=Hori |first11=Yasunori |last12=Guyon |first12=Olivier |last13=Groff |first13=Tyler D. |last14=Lozi |first14=Julien |last15=Vievard |first15=Sebastien |date=2022-08-01 |title=Direct-imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS |journal=The Astrophysical Journal |volume=934 |issue=2 |pages=L18 |bibcode=2022ApJ...934L..18K |doi=10.3847/2041-8213/ac772f |issn=0004-637X |doi-access=free|arxiv=2205.02729 }}</ref>
|-
!HR 2562
|[[HR 2562 b]]
| style="background-color: black;"|
|{{Ntsh|8}}8-18.5
|{{Ntsh|1.11}}1.11{{±|0.11}}
|
|20.3{{±|0.3}}
|
|111
|2016
|Direct imaging
|<ref>{{Citation |last1=Godoy |first1=Nicolás |title=A new atmospheric characterization of the sub-stellar companion HR\,2562\,B with JWST/MIRI observations |date=2024-09-06 |arxiv=2409.04524 |last2=Choquet |first2=Elodie |last3=Serabyn |first3=Eugene |last4=Danielski |first4=Camilla |last5=Stolker |first5=Tomas |last6=Charnay |first6=Benjamin |last7=Hinkley |first7=Sasha |last8=Lagage |first8=Pierre-Olivier |last9=Ressler |first9=Michale E.}}</ref>
|-
! scope="row" rowspan="2" | [[PDS 70]]
| [[PDS 70 b]]
| style="background-color: black;" | [[File:PDS 70.jpg|50px]]
| {{Ntsh|3.2}}{{Val|3.2|3.3|1.6}}
| {{Ntsh|2.72}}{{Val|2.72|0.39|0.34}}
|
| 21
|
| 370
| 2018
| ADI, TLOCI
|
|-
| [[PDS 70 c]]
| style="background-color: black;" | [[File:PDS 70 - eso2111b (cropped).jpg|50px]]
| {{Ntsh|7.5}}{{Val|7.5|4.7|4.2}}
| {{Ntsh|2.04}}{{Val|2.04|1.22|0.89}}
|
| 35
|
| 370
| 2019
| SDI
|
|-
![[HIP 81208|HIP 81208 C]]
|HIP 81208 Cb†
| style="background-color: black;" |[[File:New planetary-mass object found in quadruple system (potw2338a).jpg|50x50px]]
|{{Ntsh|14.8}}14.8{{±|0.4}}
|
|~285
|23
|
|485
|2023
|
|<ref>{{Cite journal |last1=Chomez |first1=A. |last2=Squicciarini |first2=V. |last3=Lagrange |first3=A. -M. |last4=Delorme |first4=P. |last5=Viswanath |first5=G. |last6=Janson |first6=M. |last7=Flasseur |first7=O. |last8=Chauvin |first8=G. |last9=Langlois |first9=M. |last10=Rubini |first10=P. |last11=Bergeon |first11=S. |last12=Albert |first12=D. |last13=Bonnefoy |first13=M. |last14=Desidera |first14=S. |last15=Engler |first15=N. |date=2023-08-01 |title=An imaged 15 MJup companion within a hierarchical quadruple system |url=https://ui.adsabs.harvard.edu/abs/2023A%26A...676L..10C |journal=Astronomy and Astrophysics |volume=676 |pages=L10 |arxiv=2307.01195 |bibcode=2023A&A...676L..10C |doi=10.1051/0004-6361/202347044 |issn=0004-6361 |archive-date=6 October 2023 |access-date=10 February 2024 |archive-url=https://web.archive.org/web/20231006045924/https://ui.adsabs.harvard.edu/abs/2023A%26A...676L..10C |url-status=live }}</ref>
|-
![[PZ Telescopii]]
|PZ Telescopii b
| style="background-color: black;" |[[File:NICI image of PZ Tel A and B (geminiann10013a).jpg|50px]]
|{{Ntsh|27}}{{Val|27|25|9}}
|
|120.5
|{{Val|27|14|4}}
|{{Val|0.52|0.36|0.32}}
|154
|2010
|Direct imaging, radial velocity
|
|-
![[Epsilon Indi A#Characteristics|Epsilon Indi A]] 
|[[Epsilon Indi Ab]]
| style="background-color: black;" |[[File:Epsilon Indi Ab (MIRI Image).png|50x50px]]
|{{Ntsh|5.75}}5.75-6.91
|{{Ntsh|1.08}}1.08{{Efn|Calculated, using the [[Stefan-Boltzmann law]] and the planet's [[effective temperature]] and luminosity, with respect to the [[Sun|solar]] nominal effective temperature of 5,772&nbsp;[[Kelvin|K]]:<math display="block">\sqrt{\biggl(\frac{5,772}{275}\biggr)^4 \cdot 10^{-7.2}} = 0.1106\ R_\odot.</math>}}
|{{Val|180|32|31}}
|{{Val|28.4|10|7.2}}
|0.40
|12
|2018 (RV), 2024 (images)
|coronagraphic images
|<ref>{{Cite web |last=information@eso.org |title=Webb images cold exoplanet 12 light-years away {{!}} ESA/Webb |url=https://esawebb.org/news/weic2421/ |access-date=2024-07-24 |website=esawebb.org |language=en |archive-date=24 July 2024 |archive-url=https://web.archive.org/web/20240724164512/https://esawebb.org/news/weic2421/ |url-status=live }}</ref><ref name="Feng2024">{{Citation |last=Feng |first=Fabo |title=Lessons learned from the detection of wide companions by radial velocity and astrometry |date=2024-12-19 |arxiv=2412.14542 |last2=Xiao |first2=Guang-Yao |last3=Jones |first3=Hugh R. A. |last4=Jenkins |first4=James S. |last5=Pena |first5=Pablo |last6=Sun |first6=Qinghui}}</ref>
|-
![[LAWD 83]]
|WD 2105–82 b
| style="background-color: black;" |[[File:WD 2105‑82.jpg|50x50px]]
|{{Ntsh|1}}1-2
|
|243
|34.62
|
|52.7
|2024 (unconfirmed)
|PSF-subtraction
|<ref name="Mullally2024" />
|-
![[HD 169142]]
|HD 169142 b
| style="background-color: black;" | [[File:Protoplanet HD 169142b.gif|50px]]
|{{Ntsh|1}}1-4
|
|
|37.2
|
|115
|2019/2023
|pseudo-ADI, PDI, ASDI, ADI
|<ref>{{Cite journal |last1=Gratton |first1=R. |last2=Ligi |first2=R. |last3=Sissa |first3=E. |last4=Desidera |first4=S. |last5=Mesa |first5=D. |last6=Bonnefoy |first6=M. |last7=Chauvin |first7=G. |last8=Cheetham |first8=A. |last9=Feldt |first9=M. |last10=Lagrange |first10=A. M. |last11=Langlois |first11=M. |last12=Meyer |first12=M. |last13=Vigan |first13=A. |last14=Boccaletti |first14=A. |last15=Janson |first15=M. |date=2019-03-01 |title=Blobs, spiral arms, and a possible planet around HD 169142 |url=https://ui.adsabs.harvard.edu/abs/2019A&A...623A.140G |journal=Astronomy and Astrophysics |volume=623 |pages=A140 |arxiv=1901.06555 |bibcode=2019A&A...623A.140G |doi=10.1051/0004-6361/201834760 |issn=0004-6361}}</ref><ref>{{Cite journal |last1=Hammond |first1=Iain |last2=Christiaens |first2=Valentin |last3=Price |first3=Daniel J. |last4=Toci |first4=Claudia |last5=Pinte |first5=Christophe |last6=Juillard |first6=Sandrine |last7=Garg |first7=Himanshi |date=2023-03-01 |title=Confirmation and keplerian motion of the gap-carving protoplanet HD 169142 b |journal=Monthly Notices of the Royal Astronomical Society |volume=522 |issue=1 |pages=L51–L55 |arxiv=2302.11302 |bibcode=2023MNRAS.522L..51H |doi=10.1093/mnrasl/slad027 |issn=0035-8711 |doi-access=free}}</ref>
|-
! scope="row" | [[2M1207]]
| [[2M1207b]] †
| style="background-color: black;" | [[File:2M1207b - First image of an exoplanet.jpg|50px]]
| {{Ntsh|4.2}}4.2
| {{Ntsh|1.11}}1.11
| 1620
| 40.6
| 0.37
| {{sort|0170|170}}
| 2004
| Direct imaging
|
|-
! scope="row" | [[59 Virginis]]
| [[Gliese 504 b]]†
| style="background-color: black;" | [[File:Composite combines Subaru images of GJ 504 (no labels).jpg|50px]]
| {{Ntsh|4}}4{{±|4.5|1}}
| {{Ntsh|0.96}}0.96
| 
| 43.5
| 
| {{sort|0057|57.27}}
| 2013
| ADI, LOCI
|
|-
![[2MASS J01225093−2439505|2MASS J01225093-2439505]]
|2MASS J01225093-2439505 b
| style="background-color: black;" |
|{{Ntsh|24.5}}24.5{{±|2.5}}
|{{Ntsh|1}}1.0
|
|52
|
|110
|2013
|Direct imaging
|
|-
![[KR Muscae]]
|HD 100546 b
| style="background-color: black;" |[[File:VLT image of the protoplanet around the young star HD 100546.jpg|50px]]
|{{Ntsh|8.5}}8.50±4.00
|
|
|53±2
|
|353
|2014
|Direct imaging
|
|-
! scope="row" | [[Kappa Andromedae]]
| [[Kappa Andromedae b]]
| style="background-color: black;" | [[File:HR 8976 exoplanet.jpg|50px]]
| {{Ntsh|13}}13{{±|12|2}}
|
| {{val|242|-|900}}
| 55
| {{val|0.69|-|0.85}}
| {{sort|0168|168.0}}
| 2013
| ADI, LOCI
|
|-
! scope="row" | [[HD 95086]]
| [[HD 95086 b]]
| style="background-color: black;" | [[File:VLT image of exoplanet HD 95086 b.jpg|50px]]
| {{Ntsh|5}}5.0
|
| ?
| 56
| ?
| {{sort|0295|295}}
| 2013
| ADI, LOCI
|
|-
![[Delorme 1]] (AB)
|Delorme 1 (AB) b†
| style="background-color: black;" | [[File:Delorme 1 (AB)b HST WFC3.jpg|50px]]
|{{Ntsh|12}}12-14
|
|
|84
|
|154
|2013
|AO
|<ref>{{Cite journal |last1=Delorme |first1=P. |last2=Gagné |first2=J. |last3=Girard |first3=J. H. |last4=Lagrange |first4=A. M. |last5=Chauvin |first5=G. |last6=Naud |first6=M. -E. |last7=Lafrenière |first7=D. |last8=Doyon |first8=R. |last9=Riedel |first9=A. |last10=Bonnefoy |first10=M. |last11=Malo |first11=L. |date=2013-05-01 |title=Direct-imaging discovery of a 12-14 Jupiter-mass object orbiting a young binary system of very low-mass stars |journal=Astronomy and Astrophysics |volume=553 |pages=L5 |arxiv=1303.4525 |bibcode=2013A&A...553L...5D |doi=10.1051/0004-6361/201321169 |issn=0004-6361 |doi-access=free}}</ref><ref name="Eriksson2020">{{Cite journal |last1=Eriksson |first1=Simon C. |last2=Asensio Torres |first2=Rubén |last3=Janson |first3=Markus |last4=Aoyama |first4=Yuhiko |last5=Marleau |first5=Gabriel-Dominique |last6=Bonnefoy |first6=Mickael |last7=Petrus |first7=Simon |date=2020-06-01 |title=Strong Halpha emission and signs of accretion in a circumbinary planetary mass companion from MUSE |url=http://adsabs.harvard.edu/abs/2020A%26A...638L...6E |journal=Astronomy and Astrophysics |volume=638 |pages=L6 |arxiv=2005.11725 |bibcode=2020A&A...638L...6E |doi=10.1051/0004-6361/202038131 |issn=0004-6361 |s2cid=218870278 |archive-date=3 December 2022 |access-date=27 August 2024 |archive-url=https://web.archive.org/web/20221203100926/https://adsabs.harvard.edu/abs/2020A%26A...638L...6E |url-status=live }}</ref>
|-
! scope="row" | [[HIP 65426]]
| [[HIP 65426 b]]
| style="background-color: black;" | [[File:The unusual exoplanet HIP 65426b — SPHERE's first.jpg|50px]]
| {{Ntsh|6}}6-12
| {{Ntsh|1.5}}1.5
| 600
| 92
|
| {{sort|0363|363}}
| 2017
| ADI, TLOCI
| <ref>{{Cite web |title=ESO's SPHERE Unveils its First Exoplanet |url=https://www.eso.org/public/announcements/ann17041/ |access-date=29 November 2017 |website=www.eso.org |archive-date=8 July 2017 |archive-url=https://web.archive.org/web/20170708225259/http://www.eso.org/public/announcements/ann17041/ |url-status=live }}</ref><ref>{{Cite journal |last1=Chauvin |first1=G. |last2=Desidera |first2=S. |last3=Lagrange |first3=A.-M. |last4=Vigan |first4=A. |last5=Gratton |first5=R. |last6=Langlois |first6=M. |last7=Bonnefoy |first7=M. |last8=Beuzit |first8=J.-L. |last9=Feldt |first9=M. |last10=Mouillet |first10=D. |last11=Meyer |first11=M. |last12=Cheetham |first12=A. |last13=Biller |first13=B. |last14=Boccaletti |first14=A. |last15=D’Orazi |first15=V. |date=September 2017 |title=Discovery of a warm, dusty giant planet around HIP 65426 |url=http://www.aanda.org/10.1051/0004-6361/201731152 |journal=Astronomy & Astrophysics |volume=605 |pages=L9 |arxiv=1707.01413 |bibcode=2017A&A...605L...9C |doi=10.1051/0004-6361/201731152 |issn=0004-6361 |s2cid=102344893}}</ref>
|-
! scope="row" | [[AB Aurigae]]
| [[AB Aurigae b]]
| style="background-color: black;" | [[File:Subaru AB Aur b.png|50px]]
| {{Ntsh|9}}9-12
| {{Ntsh|2.75}}2.75
| ?
| 93
| 0.19-0.60
| 508
| 2022
| ADI/RSDI, ALOCI
| <ref name="Currie2022">{{Cite journal |last1=Currie |first1=Thayne |last2=Lawson |first2=Kellen |last3=Schneider |first3=Glenn |last4=Lyra |first4=Wladimir |last5=Wisniewski |first5=John |last6=Grady |first6=Carol |last7=Guyon |first7=Olivier |last8=Tamura |first8=Motohide |last9=Kotani |first9=Takayuki |last10=Kawahara |first10=Hajime |last11=Brandt |first11=Timothy |last12=Uyama |first12=Taichi |last13=Muto |first13=Takayuki |last14=Dong |first14=Ruobing |last15=Kudo |first15=Tomoyuki |display-authors=3 |date=4 April 2022 |title=Images of embedded Jovian planet formation at a wide separation around AB Aurigae |journal=Nature Astronomy |publisher=Springer Science and Business Media LLC |volume=6 |issue=6 |pages=751–759 |arxiv=2204.00633 |bibcode=2022NatAs...6..751C |doi=10.1038/s41550-022-01634-x |issn=2397-3366 |s2cid=247940163 |last16=Hashimoto |first16=Jun |last17=Fukagawa |first17=Misato |last18=Wagner |first18=Kevin |last19=Lozi |first19=Julien |last20=Chilcote |first20=Jeffrey |last21=Tobin |first21=Taylor |last22=Groff |first22=Tyler |last23=Ward-Duong |first23=Kimberly |last24=Januszewski |first24=William |last25=Norris |first25=Barnaby |last26=Tuthill |first26=Peter |last27=van der Marel |first27=Nienke |last28=Sitko |first28=Michael |last29=Deo |first29=Vincent |last30=Vievard |first30=Sebastien |last31=Jovanovic |first31=Nemanja |last32=Martinache |first32=Frantz |last33=Skaf |first33=Nour}}</ref>
|-
![[HD 36112|MWC 758]]
|MWC 758 c
| style="background-color: black;" |
|
|
|
|100
|
|508
|2023
|Direct imaging
|
|-
![[GQ Lupi]]
|[[GQ Lupi b]]
| style="background-color: black;" |[[File:The Sub-Stellar Companion to GQ Lupi.jpg|50px]]
|{{Ntsh|1}}1–36
|{{Ntsh|3}}3
|
|100
|
|495
|2004
|Direct imaging
|
|-
! scope="row" | [[VHS 1256-1257]]
| VHS 1256 b †
| style="background-color: black;" | [[File:VHS J1256-1257.jpg|50px]]
| {{Ntsh|11.2}}11.2
|
| 3900
| 102
|
| {{sort|0040|40}}
| 2015
| Direct imaging
|
|-
!YSES 2
|[[YSES 2 b]]
| style="background-color: black;" |[[File:YSES2b-exoplanet-SPHERE-VLT-ESO-YSES-2020.jpg|50x50px]]
|{{Ntsh|6.3}}{{Val|6.3|1.6|0.9}}
|
|
|115
|
|359
|2021
|reference star image subtraction
|<ref>{{Cite journal |last1=Bohn |first1=Alexander J. |last2=Ginski |first2=Christian |last3=Kenworthy |first3=Matthew A. |last4=Mamajek |first4=Eric E. |last5=Pecaut |first5=Mark J. |last6=Mugrauer |first6=Markus |last7=Vogt |first7=Nikolaus |last8=Adam |first8=Christian |last9=Meshkat |first9=Tiffany |last10=Reggiani |first10=Maddalena |last11=Snik |first11=Frans |date=2021-04-01 |title=Discovery of a directly imaged planet to the young solar analog YSES 2 |url=https://ui.adsabs.harvard.edu/abs/2021A%26A...648A..73B |journal=Astronomy and Astrophysics |volume=648 |pages=A73 |arxiv=2104.08285 |bibcode=2021A&A...648A..73B |doi=10.1051/0004-6361/202140508 |issn=0004-6361 |archive-date=25 September 2023 |access-date=4 February 2024 |archive-url=https://web.archive.org/web/20230925010151/https://ui.adsabs.harvard.edu/abs/2021A%26A...648A..73B |url-status=live }}</ref>
|-
!2MASS J04372171+2651014
|[[2M0437 b]]
| style="background-color: black;" |
|{{Ntsh|3}}3-5
|
|
|118
|
|418
|2021
|AO
|<ref>{{Cite journal |last1=Gaidos |first1=E. |last2=Hirano |first2=T. |last3=Kraus |first3=A. L. |last4=Kuzuhara |first4=M. |last5=Zhang |first5=Z. |last6=Lee |first6=R. A. |last7=Salama |first7=M. |last8=Berger |first8=T. A. |last9=Grunblatt |first9=S. K. |last10=Ansdell |first10=M. |last11=Liu |first11=M. C. |last12=Harakawa |first12=H. |last13=Hodapp |first13=K. W. |last14=Jacobson |first14=S. |last15=Konishi |first15=M. |date=2022-05-01 |title=Zodiacal exoplanets in time (ZEIT) XII: a directly imaged planetary-mass companion to a young Taurus M dwarf star |journal=Monthly Notices of the Royal Astronomical Society |volume=512 |issue=1 |pages=583–601 |arxiv=2110.08655 |bibcode=2022MNRAS.512..583G |doi=10.1093/mnras/stab3069 |issn=0035-8711 |doi-access=free}}</ref>
|-
! scope="row" | ROXs 42B
| [[ROXs 42Bb]]
| style="background-color: black;" |[[File:ROXs 42B MUSE IR.jpg|50px]]
| {{Ntsh|9}}9{{±|3}}
| {{Ntsh|2.83}}{{val|2.83|0.01}}
| 1968.3
| {{sort|0157|157}}
| {{unknown}}
| {{sort|0440|440{{±|16}}}}
| 2013
| Direct imaging
| <ref name="Currie2013">{{Cite journal |last1=Currie |first1=Thayne |last2=Daemgen |first2=Sebastian |last3=Debes |first3=John |last4=Lafreniere |first4=David |last5=Itoh |first5=Yoichi |last6=Jayawardhana |first6=Ray |last7=Ratzka |first7=Thorsten |last8=Correia |first8=Serge |year=2014 |title=Direct Imaging and Spectroscopy of a Candidate Companion Below/Near the Deuterium-Burning Limit In The Young Binary Star System, ROXs 42B |journal=The Astrophysical Journal Letters |volume=780 |issue=2 |pages=30 |arxiv=1310.4825 |bibcode=2014ApJ...780L..30C |doi=10.1088/2041-8205/780/2/L30 |s2cid=118464822}}</ref>
|-
![[2MASS J02192210-3925225]]
|2MASS J02192210-3925225 b
| style="background-color: black;" |[[File:2MASS J02192210-3925225 b legacy dr10.jpg|50x50px]]
|{{Ntsh|13.9}}13.9{{±|1.1}}
|{{Ntsh|1.44}}1.44{{±|0.03}}
|
|160
|
|131
|2015
|Direct imaging
|<ref>{{Cite journal |last1=Artigau |first1=Étienne |last2=Gagné |first2=Jonathan |last3=Faherty |first3=Jacqueline |last4=Malo |first4=Lison |last5=Naud |first5=Marie-Eve |last6=Doyon |first6=René |last7=Lafrenière |first7=David |last8=Beletsky |first8=Yuri |date=2015-06-01 |title=BANYAN. VI. Discovery of a Companion at the Brown Dwarf/Planet-Mass Limit to a Tucana-Horologium M Dwarf |url=https://ui.adsabs.harvard.edu/abs/2015ApJ...806..254A/abstract |journal=The Astrophysical Journal |volume=806 |issue=2 |pages=254 |arxiv=1505.01747 |bibcode=2015ApJ...806..254A |doi=10.1088/0004-637X/806/2/254 |issn=0004-637X |archive-date=26 August 2024 |access-date=26 August 2024 |archive-url=https://web.archive.org/web/20240826132027/https://ui.adsabs.harvard.edu/abs/2015ApJ...806..254A/abstract |url-status=live }}</ref>
|-
! rowspan="2" |[[TYC 8998-760-1]]
|TYC 8998-760-1 b †
| rowspan="2" style="background-color: black;" |[[File:First ever image of a multi-planet system around a Sun-like star.tif|50x50px]]
|{{Ntsh|14}}14{{±|3}}
|
|
|160
|
| rowspan="2" |309
|2020
| rowspan="2" |imaging + coronagraph
|<ref>{{Cite journal |last1=Bohn |first1=A. J. |last2=Kenworthy |first2=M. A. |last3=Ginski |first3=C. |last4=Manara |first4=C. F. |last5=Pecaut |first5=M. J. |last6=de Boer |first6=J. |last7=Keller |first7=C. U. |last8=Mamajek |first8=E. E. |last9=Meshkat |first9=T. |last10=Reggiani |first10=M. |last11=Todorov |first11=K. O. |last12=Snik |first12=F. |date=2020-02-01 |title=The Young Suns Exoplanet Survey: Detection of a wide-orbit planetary-mass companion to a solar-type Sco-Cen member |journal=Monthly Notices of the Royal Astronomical Society |volume=492 |issue=1 |pages=431–443 |arxiv=1912.04284 |bibcode=2020MNRAS.492..431B |doi=10.1093/mnras/stz3462 |issn=0035-8711 |doi-access=free}}</ref>
|-
|TYC 8998-760-1 c
|{{Ntsh|6}}6{{±|1}}
|
|
|320
|
|2020
|<ref>{{Cite journal |last1=Bohn |first1=Alexander J. |last2=Kenworthy |first2=Matthew A. |last3=Ginski |first3=Christian |last4=Rieder |first4=Steven |last5=Mamajek |first5=Eric E. |last6=Meshkat |first6=Tiffany |last7=Pecaut |first7=Mark J. |last8=Reggiani |first8=Maddalena |last9=de Boer |first9=Jozua |last10=Keller |first10=Christoph U. |last11=Snik |first11=Frans |last12=Southworth |first12=John |date=2020-07-01 |title=Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1 |journal=The Astrophysical Journal |volume=898 |issue=1 |pages=L16 |arxiv=2007.10991 |bibcode=2020ApJ...898L..16B |doi=10.3847/2041-8213/aba27e |issn=0004-637X |doi-access=free}}</ref>
|-
![[NIRISS-NGC1333-10]]
|NIRISS-NGC1333-10 B
| style="background-color: black;" |[[File:NIRISS-NGC1333-10.png|50px]]
|{{Ntsh|15}}~15
|
|
|164
|
|978
|2024
|direct imaging +slitless spectroscopy
|<ref>{{Cite journal |last1=Langeveld |first1=Adam B. |last2=Scholz |first2=Aleks |last3=Mužić |first3=Koraljka |last4=Jayawardhana |first4=Ray |last5=Capela |first5=Daniel |last6=Albert |first6=Loïc |last7=Doyon |first7=René |last8=Flagg |first8=Laura |last9=de Furio |first9=Matthew |last10=Johnstone |first10=Doug |last11=Lafrèniere |first11=David |last12=Meyer |first12=Michael |date=2024-08-22 |title=The JWST/NIRISS Deep Spectroscopic Survey for Young Brown Dwarfs and Free-Floating Planets |journal=AJ |volume=168 |issue=4 |page=179 |arxiv=2408.12639 |doi=10.3847/1538-3881/ad6f0c |doi-access=free}}</ref>
|-
!CFHTWIR-Oph 98
|[[CFHTWIR-Oph 98 b]]
| style="background-color: black;" | [[File:CFHTWIR-Oph 98 AB WFC3.jpg|50px]]
|{{Ntsh|7.8}}{{Val|7.8|0.7|0.8}}
|{{Ntsh|1.86}}1.86±0.05
|~22000
|200±6
|
|447
|2021
|Direct imaging
|
|-
![[CHXR 73]]
|CHXR 73 b
| style="background-color: black;" |[[File:Hubbledwarf.jpg|50px]]
|{{Ntsh|12.569}}{{Val|12.569|8.379|5.237}}
|
|
|210
|
|620
|2006
|Direct imaging
|
|-
![[ROXs 12]]
|ROXs 12 b
| style="background-color: black;" | [[File:ROXs 12 MUSE.png|50px]]
|{{Ntsh|16}}16{{±|4}}
|
|
|214
|0.83
|452
|2013
|Direct imaging
|
|-
![[2MASS J22362452+4751425]]
|2M2236+4751 b†
| style="background-color: black;" | [[File:2M2236+4751 b.jpg|50px]]
|{{Ntsh|11}}11-14
|
|
|230
|
|205
|2017
|AO
|<ref>{{Cite journal |last1=Bowler |first1=Brendan P. |last2=Liu |first2=Michael C. |last3=Mawet |first3=Dimitri |last4=Ngo |first4=Henry |last5=Malo |first5=Lison |last6=Mace |first6=Gregory N. |last7=McLane |first7=Jacob N. |last8=Lu |first8=Jessica R. |last9=Tristan |first9=Isaiah I. |last10=Hinkley |first10=Sasha |last11=Hillenbrand |first11=Lynne A. |last12=Shkolnik |first12=Evgenya L. |last13=Benneke |first13=Björn |last14=Best |first14=William M. J. |date=2017-01-01 |title=Planets around Low-mass Stars (PALMS). VI. Discovery of a Remarkably Red Planetary-mass Companion to the AB Dor Moving Group Candidate 2MASS J22362452+4751425* |journal=The Astronomical Journal |volume=153 |issue=1 |pages=18 |arxiv=1611.00364 |bibcode=2017AJ....153...18B |doi=10.3847/1538-3881/153/1/18 |issn=0004-6256 |doi-access=free}}</ref>
|-
![[Mu2 Scorpii]]
|Mu2 Scorpii b†l
| style="background-color: black;" |
|{{Ntsh|14.4}}14.4±0.8
|
|
|242.4
|0.56
|474
|2022
|Direct imaging
|
|-
![[Oph 11|Ophiuchi 11]]
|Ophiuchi 11 b
| style="background-color: black;" |[[File:Oph 1622 eso0629b.jpg|50px]]
|{{Ntsh|21}}21±3
|
|20,000
|243±55
|
|400
|2006
|Direct imaging
|
|-
![[AB Pictoris]]
|[[AB Pictoris b]]†
| style="background-color: black;" | [[File:The Star AB Pictoris and its Companion - Phot-14d-05-normal.jpg|50px]]
|{{Ntsh|10}}{{val|10|1}}<ref>{{Cite journal |last1=Palma-Bifani |first1=P. |last2=Chauvin |first2=G. |last3=Bonnefoy |first3=M. |last4=Rojo |first4=P. M. |last5=Petrus |first5=S. |last6=Rodet |first6=L. |last7=Langlois |first7=M. |last8=Allard |first8=F. |last9=Charnay |first9=B. |last10=Desgrange |first10=C. |last11=Homeier |first11=D. |last12=Lagrange |first12=A.-M. |last13=Beuzit |first13=J.-L. |last14=Baudoz |first14=P. |last15=Boccaletti |first15=A. |date=2023 |title=Peering into the young planetary system AB Pic |journal=Astronomy & Astrophysics |volume=670 |pages=A90 |arxiv=2211.01474 |doi=10.1051/0004-6361/202244294 |last16=Chomez |first16=A. |last17=Delorme |first17=P. |last18=Desidera |first18=S. |last19=Feldt |first19=M. |last20=Ginski |first20=C. |last21=Gratton |first21=R. |last22=Maire |first22=A.-L. |last23=Meyer |first23=M. |last24=Samland |first24=M. |last25=Snellen |first25=I. |last26=Vigan |first26=A. |last27=Zhang |first27=Y.}}</ref>
|{{Ntsh|1.75}}1.75
|
|260
|
|164
|2005
|imaging+ coronagraph
|<ref>{{Cite journal |last1=Chauvin |first1=G. |last2=Lagrange |first2=A. -M. |last3=Zuckerman |first3=B. |last4=Dumas |first4=C. |last5=Mouillet |first5=D. |last6=Song |first6=I. |last7=Beuzit |first7=J. -L. |last8=Lowrance |first8=P. |last9=Bessell |first9=M. S. |date=2005-08-01 |title=A companion to AB Pic at the planet/brown dwarf boundary |journal=Astronomy and Astrophysics |volume=438 |issue=3 |pages=L29–L32 |arxiv=astro-ph/0504658 |bibcode=2005A&A...438L..29C |doi=10.1051/0004-6361:200500111 |issn=0004-6361 |doi-access=free}}</ref><ref>{{Cite journal |last1=Bonnefoy |first1=M. |last2=Chauvin |first2=G. |last3=Lagrange |first3=A. -M. |last4=Rojo |first4=P. |last5=Allard |first5=F. |last6=Pinte |first6=C. |last7=Dumas |first7=C. |last8=Homeier |first8=D. |date=2014-02-01 |title=A library of near-infrared integral field spectra of young M-L dwarfs |journal=Astronomy and Astrophysics |volume=562 |pages=A127 |arxiv=1306.3709 |bibcode=2014A&A...562A.127B |doi=10.1051/0004-6361/201118270 |issn=0004-6361 |doi-access=free}}</ref>
|-
![[GSC 6214-00210]]
|GSC 6214-00210 b†
| style="background-color: black;" |[[File:GSC 6214-00210 B MIRI.jpg|50x50px]]
|{{Ntsh|14}}14 ± 2
|
|
|320
|
|355
|2008/2011
|
|<ref>{{Cite journal |last1=Bowler |first1=Brendan P. |last2=Liu |first2=Michael C. |last3=Kraus |first3=Adam L. |last4=Mann |first4=Andrew W. |last5=Ireland |first5=Michael J. |date=2011-12-01 |title=A Disk around the Planetary-mass Companion GSC 06214-00210 b: Clues about the Formation of Gas Giants on Wide Orbits |url=https://ui.adsabs.harvard.edu/abs/2011ApJ...743..148B |journal=The Astrophysical Journal |volume=743 |issue=2 |pages=148 |arxiv=1109.5693 |bibcode=2011ApJ...743..148B |doi=10.1088/0004-637X/743/2/148 |issn=0004-637X |archive-date=6 September 2024 |access-date=9 March 2024 |archive-url=https://web.archive.org/web/20240906023413/https://ui.adsabs.harvard.edu/abs/2011ApJ...743..148B |url-status=live }}</ref>
|-
! scope="row" | [[FW Tauri]]
| FW Tauri b†
| style="background-color: black;" | [[File:FW Tau Hubble.jpg|50px]]
| {{Ntsh|10}}10±4
or star<ref>{{Cite journal |last1=Mora |first1=Ariel |last2=Wu |first2=Ya-Lin |last3=Bowler |first3=Brendan P. |last4=Sheehan |first4=Patrick |date=2020-01-01 |title=Measuring the Mass of the Faint Companion to FW Tau with ALMA |journal=Research Notes of the American Astronomical Society |volume=4 |issue=1 |pages=9 |bibcode=2020RNAAS...4....9M |doi=10.3847/2515-5172/ab6852 |issn=2515-5172 |doi-access=free}}</ref>
|
| ~12,000<ref>{{Cite encyclopedia |title=Planet FW Tau b. |encyclopedia=[[Extrasolar Planets Encyclopaedia]] |url=https://exoplanet.eu/catalog/fw_tau_b--1480/ |access-date=21 Feb 2018}}</ref>
| 330
| ?
| {{sort|0472|472.93}}<ref>{{Cite web |title=FW Tauri |url=https://www.universeguide.com/star/fwtau |access-date=21 Feb 2018 |website=Universe Guide |archive-date=21 February 2018 |archive-url=https://web.archive.org/web/20180221161709/https://www.universeguide.com/star/fwtau |url-status=live }}</ref>
| 2013
| Direct imaging
|<ref>{{Cite journal |last1=Wu |first1=Ya-Lin |last2=Sheehan |first2=Patrick D. |date=2017-09-08 |title=An ALMA Dynamical Mass Estimate of the Proposed Planetary-mass Companion FW Tau C |journal=The Astrophysical Journal |volume=846 |issue=2 |pages=L26 |arxiv=1708.08122 |bibcode=2017ApJ...846L..26W |doi=10.3847/2041-8213/aa8771 |issn=2041-8213 |doi-access=free |hdl-access=free |hdl=10150/625808}}</ref><ref>{{Cite journal |last1=Mora |first1=Ariel |last2=Wu |first2=Ya-Lin |last3=Bowler |first3=Brendan P. |last4=Sheehan |first4=Patrick |date=2020-01-08 |title=Measuring the Mass of the Faint Companion to FW Tau with ALMA |journal=Research Notes of the AAS |volume=4 |issue=1 |pages=9 |bibcode=2020RNAAS...4....9M |doi=10.3847/2515-5172/ab6852 |issn=2515-5172 |doi-access=free}}</ref>
|-
![[DH Tauri]]
|DH Tauri b†
| style="background-color: black;" | [[File:DH Tauri.jpg|50px]]
|{{Ntsh|11}}11±3
|{{Ntsh|2.7}}2.7±0.8
|
|330
|
|441
|2005/2014
|Coronagraph, AO
|<ref>{{Cite journal |last1=Itoh |first1=Yoichi |last2=Hayashi |first2=Masahiko |last3=Tamura |first3=Motohide |last4=Tsuji |first4=Takashi |last5=Oasa |first5=Yumiko |last6=Fukagawa |first6=Misato |last7=Hayashi |first7=Saeko S. |last8=Naoi |first8=Takahiro |last9=Ishii |first9=Miki |last10=Mayama |first10=Satoshi |last11=Morino |first11=Jun-ichi |last12=Yamashita |first12=Takuya |last13=Pyo |first13=Tae-Soo |last14=Nishikawa |first14=Takayuki |last15=Usuda |first15=Tomonori |date=2005-02-01 |title=A Young Brown Dwarf Companion to DH Tauri |url=https://ui.adsabs.harvard.edu/abs/2005ApJ...620..984I |journal=The Astrophysical Journal |volume=620 |issue=2 |pages=984–993 |arxiv=astro-ph/0411177 |bibcode=2005ApJ...620..984I |doi=10.1086/427086 |issn=0004-637X |s2cid=53632705 |archive-date=17 January 2024 |access-date=23 October 2023 |archive-url=https://web.archive.org/web/20240117002245/https://ui.adsabs.harvard.edu/abs/2005ApJ...620..984I |url-status=live }}</ref><ref>{{Cite journal |last1=Zhou |first1=Yifan |last2=Herczeg |first2=Gregory J. |last3=Kraus |first3=Adam L. |last4=Metchev |first4=Stanimir |last5=Cruz |first5=Kelle L. |date=2014-03-01 |title=Accretion onto Planetary Mass Companions of Low-mass Young Stars |journal=The Astrophysical Journal |volume=783 |issue=1 |pages=L17 |arxiv=1401.6545 |bibcode=2014ApJ...783L..17Z |doi=10.1088/2041-8205/783/1/L17 |issn=0004-637X |doi-access=free |hdl-access=free |hdl=2152/43090}}</ref>
|-
! scope="row" | [[1RXS J160929.1−210524|1RXS J1609]]
| [[1RXS 1609 b]]†
| style="background-color: black;" | [[File:1RXS1609B MIRI.jpg|50x50px]]
| {{Ntsh|8}}8–14
| {{Ntsh|1.7}}1.7
| 6518
| 331.1
| 0.08
| {{sort|0470|470}}
| 2008/2010
| Direct imaging
|
|-
![[HIP 79098|HIP 79098 AB]]
|HIP 79098 AB b
| style="background-color: black;" |
|{{Ntsh|20.5}}20.5±4.5
|
|
|345±6
|
|500
|2019
|Direct imaging
|
|-
![[CT Chamaeleontis]]
|CT Chamaeleontis b†
| style="background-color: black;" |[[File:CT Cha B MIRI.jpg|50px]]
|{{Ntsh|17}}17±6
|{{Ntsh|2.2}}2.20{{±|0.81|0.60}}
|
|440
|
|625
|2007
|Direct imaging
|
|-
! scope="row" | [[HD 203030]]
| [[HD 203030#Planetary system|HD 203030 B]]
| style="background-color: black;" | [[File:Spitzer IRAC HD 203030B.jpg|50px]]
| {{Ntsh|11}}11{{±|4|3}}
|
|
| 487
|
| 128
| 2006
| SDI
| <ref name="Miles-Paez2017">{{Cite journal |last1=Miles-Páez |first1=Paulo A. |last2=Metchev |first2=Stanimir |last3=Luhman |first3=Kevin L. |last4=Marengo |first4=Massimo |last5=Hulsebus |first5=Alan |year=2017 |title=The Prototypical Young L/T-Transition Dwarf HD 203030B Likely Has Planetary Mass |journal=The Astronomical Journal |volume=154 |issue=6 |page=262 |arxiv=1710.11274 |bibcode=2017AJ....154..262M |doi=10.3847/1538-3881/aa9711 |s2cid=67821107 |doi-access=free}}</ref>
|-
![[HD 129116|b Centauri]]
|[[b Centauri b]]
| style="background-color: black;" |[[File:Eso2118b.jpg|50x50px]]
|{{Ntsh|10.9}}10.9{{±|1.6}}
|
|
|556
|
|330
|2021
|coronagraph+ classical angular differential imaging
|<ref>{{Cite journal |last1=Janson |first1=Markus |last2=Gratton |first2=Raffaele |last3=Rodet |first3=Laetitia |last4=Vigan |first4=Arthur |last5=Bonnefoy |first5=Mickaël |last6=Delorme |first6=Philippe |last7=Mamajek |first7=Eric E. |last8=Reffert |first8=Sabine |last9=Stock |first9=Lukas |last10=Marleau |first10=Gabriel-Dominique |last11=Langlois |first11=Maud |last12=Chauvin |first12=Gaël |last13=Desidera |first13=Silvano |last14=Ringqvist |first14=Simon |last15=Mayer |first15=Lucio |date=2021-12-01 |title=A wide-orbit giant planet in the high-mass b Centauri binary system |url=https://ui.adsabs.harvard.edu/abs/2021Natur.600..231J |journal=Nature |volume=600 |issue=7888 |pages=231–234 |arxiv=2112.04833 |bibcode=2021Natur.600..231J |doi=10.1038/s41586-021-04124-8 |issn=0028-0836 |pmid=34880428 |s2cid=245005994 |archive-date=30 May 2024 |access-date=4 February 2024 |archive-url=https://web.archive.org/web/20240530050454/https://ui.adsabs.harvard.edu/abs/2021Natur.600..231J |url-status=live }}</ref>
|-
! scope="row" | [[HD 106906]]
| [[HD 106906 b]]†
| style="background-color: black;" | [[File:HD 106906 b imaged by SPHERE.jpg|50px]]
| {{Ntsh|11}}11±2
|
|
| 650
|
| {{sort|0300|300}}
| 2013
| ADI
|
|-
![[UScoCTIO 108|USco CTIO 108]]
|USco CTIO 108 b
| style="background-color: black;" |[[File:UScoCTIO 108 legacy dr10.jpg|50px]]
|{{Ntsh|14}}14{{±|2|8}}
|
|
|670
|
|473
|2008
|Direct imaging
|
|-
![[2MASS J23225240-6151114]]
|2MASS J23225299-6151275
| style="background-color: black;" |[[File:2MASS J23225240-6151114 and companion.jpg|50px]]
|{{Ntsh|12.6}}12.6-13.3<ref name="Baig2024b" />
|
|
|705
|
|138.4
|2014
|Direct imaging
|<ref>{{Cite journal |last1=Gagné |first1=Jonathan |last2=Lafrenière |first2=David |last3=Doyon |first3=René |last4=Malo |first4=Lison |last5=Artigau |first5=Étienne |date=2014-03-01 |title=BANYAN. II. Very Low Mass and Substellar Candidate Members to Nearby, Young Kinematic Groups with Previously Known Signs of Youth |url=https://ui.adsabs.harvard.edu/abs/2014ApJ...783..121G/abstract |journal=The Astrophysical Journal |volume=783 |issue=2 |pages=121 |arxiv=1312.5864 |bibcode=2014ApJ...783..121G |doi=10.1088/0004-637X/783/2/121 |issn=0004-637X |archive-date=16 August 2024 |access-date=16 August 2024 |archive-url=https://web.archive.org/web/20240816125233/https://ui.adsabs.harvard.edu/abs/2014ApJ...783..121G/abstract |url-status=live }}</ref><ref>{{Cite journal |last1=Calissendorff |first1=Per |last2=Janson |first2=Markus |last3=Asensio-Torres |first3=Rubén |last4=Köhler |first4=Rainer |date=2019-07-01 |title=Spectral characterization of newly detected young substellar binaries with SINFONI |url=https://ui.adsabs.harvard.edu/abs/2019A%26A...627A.167C |journal=Astronomy and Astrophysics |volume=627 |pages=A167 |arxiv=1906.05871 |bibcode=2019A&A...627A.167C |doi=10.1051/0004-6361/201935319 |issn=0004-6361 |archive-date=17 December 2024 |access-date=6 January 2025 |archive-url=https://web.archive.org/web/20241217040255/https://ui.adsabs.harvard.edu/abs/2019A%26A...627A.167C |url-status=live }}</ref>
|-
![[HIP 78530]]
|HIP 78530 b
| style="background-color: black;" |
|{{Ntsh|23}}23±1
|
|
|740±60
|
|446
|2010
|Direct imaging
|
|-
![[HN Pegasi]]
|HN Pegasi b
| style="background-color: black;" |[[File:HN Pegasi B.jpg|50px]]
|{{Ntsh|22}}22±9.4
|{{Ntsh|1.05}}{{Val|1.05|0.14|0.06}}
|
|773±13
|
|59
|2006
|Direct imaging
|
|-
![[FU Tauri]]
|FU Tauri b
| style="background-color: black;" |[[File:FU Tau B.jpg|50px]]
|{{Ntsh|16}}16
|
|
|800
|
|429
|2008
|Direct imaging
|
|-
![[SR 12 (star)|SR 12]]
|SR 12(AB) c†
| style="background-color: black;" |[[File:SR 12 C.jpg|50x50px]]
|{{Ntsh|11}}11
|
|
|980
|
|337
|2011
|
|<ref name=":2">{{Cite journal |last1=Wu |first1=Ya-Lin |last2=Bowler |first2=Brendan P. |last3=Sheehan |first3=Patrick D. |last4=Close |first4=Laird M. |last5=Eisner |first5=Joshua A. |last6=Best |first6=William M. J. |last7=Ward-Duong |first7=Kimberly |last8=Zhu |first8=Zhaohuan |last9=Kraus |first9=Adam L. |date=2022-05-01 |title=ALMA Discovery of a Disk around the Planetary-mass Companion SR 12 c |journal=The Astrophysical Journal |volume=930 |issue=1 |pages=L3 |arxiv=2204.06013 |bibcode=2022ApJ...930L...3W |doi=10.3847/2041-8213/ac6420 |issn=0004-637X |doi-access=free}}</ref>
|-
![[2MASS J05581644–4501559]]
|0558 B
| style="background-color: black;" | [[File:0558AB legacy dr10.jpg|50px]]
|{{Ntsh|6}}6-12
|
|
|1,043
|
|88
|2024
|Direct imaging
|<ref>{{Cite journal |last1=Marocco |first1=Federico |last2=Kirkpatrick |first2=J. Davy |last3=Schneider |first3=Adam C. |last4=Meisner |first4=Aaron M. |last5=Popinchalk |first5=Mark |last6=Gelino |first6=Christopher R. |last7=Faherty |first7=Jacqueline K. |last8=Burgasser |first8=Adam J. |last9=Caselden |first9=Dan |last10=Gagné |first10=Jonathan |last11=Aganze |first11=Christian |last12=Bardalez-Gagliuffi |first12=Daniella C. |last13=Casewell |first13=Sarah L. |last14=Hsu |first14=Chih-Chun |last15=Kiman |first15=Rocio |date=2024-04-22 |title=Thirteen New M Dwarf + T Dwarf Pairs Identified with WISE/NEOWISE |journal=The Astrophysical Journal |volume=967 |issue=2 |page=147 |arxiv=2404.14324 |bibcode=2024ApJ...967..147M |doi=10.3847/1538-4357/ad3f1d |doi-access=free |first16=Peter R. M. |last16=Eisenhardt |first17=Marc J. |last17=Kuchner |first18=Daniel |last18=Stern |first19=Léopold |last19=Gramaize |first20=Arttu |last20=Sainio |first21=Thomas P. |last21=Bickle |first22=Austin |last22=Rothermich |first23=William |last23=Pendrill |first24=Melina |last24=Thévenot |first25=Martin |last25=Kabatnik |first26=Giovanni |last26=Colombo |first27=Hiro |last27=Higashimura |first28=Frank |last28=Kiwy |first29=Elijah J. |last29=Marchese |first30=Nikolaj Stevnbak |last30=Andersen |first31=Christopher |last31=Tanner |first32=Jim |last32=Walla |first33=Zbigniew |last33=Wedracki |last34=The Backyard Worlds Collaboration}}</ref>
|-
! scope="row" | [[Ross 458]]
| [[Ross 458(AB) c]]†
| style="background-color: black;" | [[File:DT Virginis.jpg|50px]]
| {{Ntsh|8.5}}8.5
| {{Ntsh|1.8}}1.8
| 33,081
| 1,167.7
| 0.17
| {{sort|0038|38}}<ref name="Ross 458(AB) c">{{Cite encyclopedia |title=Ross 458(AB) c |encyclopedia=[[Extrasolar Planets Encyclopaedia]] |url=https://exoplanet.eu/catalog/ross_458_ab_c--845/ |access-date=2012-10-24}}</ref>
| 2011
| Direct imaging
|
|-
! scope="row" | BD+60 1417
| [[BD+60 1417b]]†
| style="background-color: black;" | [[File:Exoplanet BD+60 1417b.jpg|50px]]
| {{Ntsh|13.47}}13.47±5.67
| {{Ntsh|1.31}}1.31±0.06
|
| 1,662
|
| 144±13
| 2021
| Direct imaging
| <ref>{{Cite journal |last1=Faherty |first1=Jacqueline K. |last2=Gagné |first2=Jonathan |last3=Popinchalk |first3=Mark |last4=Vos |first4=Johanna M. |last5=Burgasser |first5=Adam J. |last6=Schümann |first6=Jörg |last7=Schneider |first7=Adam C. |last8=Kirkpatrick |first8=J. Davy |last9=Meisner |first9=Aaron M. |last10=Kuchner |first10=Marc J. |last11=Bardalez Gagliuffi |first11=Daniella C. |date=2021-12-01 |title=A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9 |journal=The Astrophysical Journal |volume=923 |issue=1 |pages=48 |arxiv=2112.04678 |bibcode=2021ApJ...923...48F |doi=10.3847/1538-4357/ac2499 |issn=0004-637X |s2cid=245005964 |doi-access=free}}</ref>
|-
![[SE 70]]
|S Ori 68
| style="background-color: black;" | [[File:SE 70+S Ori 68 ESO VHS.jpg|50px]]
|{{Ntsh|5}}5
|
|
|1,700
|
|1,290
|2006
|Direct imaging
|<ref>{{Cite journal |last1=Caballero |first1=J. A. |last2=Martín |first2=E. L. |last3=Dobbie |first3=P. D. |last4=Barrado Y Navascués |first4=D. |date=2006-12-01 |title=Are isolated planetary-mass objects really isolated?. A brown dwarf-exoplanet system candidate in the σ Orionis cluster |url=https://ui.adsabs.harvard.edu/abs/2006A&A...460..635C |journal=Astronomy and Astrophysics |volume=460 |issue=2 |pages=635–640 |arxiv=astro-ph/0608659 |bibcode=2006A&A...460..635C |doi=10.1051/0004-6361:20066162 |issn=0004-6361}}</ref>
|-
![[UPM J1040-3551]]
|CWISE J104053.42–355029.7
| style="background-color: black;" | [[File:UPM J1040–3551 legacy dr10.jpg|50px]]
|{{Ntsh|3}}3 or 31
|
|
|1,700
|
| 82.5
| 2024
|Direct imaging
|<ref name=":5" /><ref name="Leggett&Tremblin2024">{{cite arxiv |eprint=2411.03549 |class=astro-ph |first=S. K. |last=Leggett |first2=Pascal |last2=Tremblin |author-link= |title=Redshifting the Study of Cold Brown Dwarfs and Exoplanets: the Mid-Infrared Wavelength Region as an Indicator of Surface Gravity and Mass |date=5 Nov 2024}}</ref>
|-
![[2MASS J0249-0557]]AB
|2MASS J0249-0557c†
| style="background-color: black;" |[[File:2MASS J0249-0557 c.jpg|50px]]
|{{Ntsh|11.6}}{{Val|11.6|1.3|1.0}}
|
|
|1,950
|
|159
|2018
|Direct imaging
|<ref name=":3">{{Cite journal |last1=Dupuy |first1=Trent J. |last2=Liu |first2=Michael C. |last3=Allers |first3=Katelyn N. |last4=Biller |first4=Beth A. |last5=Kratter |first5=Kaitlin M. |last6=Mann |first6=Andrew W. |last7=Shkolnik |first7=Evgenya L. |last8=Kraus |first8=Adam L. |last9=Best |first9=William M. J. |date=2018-08-01 |title=The Hawaii Infrared Parallax Program. III. 2MASS J0249-0557 c: A Wide Planetary-mass Companion to a Low-mass Binary in the β Pic Moving Group |journal=The Astronomical Journal |volume=156 |issue=2 |pages=57 |arxiv=1807.05235 |bibcode=2018AJ....156...57D |doi=10.3847/1538-3881/aacbc2 |issn=0004-6256 |doi-access=free}}</ref>
|-
! scope="row" | [[GU Piscium]]
| [[GU Piscium b]]†
| style="background-color: black;" | [[File:GUPscb GMOSiz WIRCamJ noinset.jpg|50px]]
| {{Ntsh|11}}11±2
|
| 163,000
| 2,000
|
| {{sort|0155|155}}
| 2014
| Direct imaging
|
|-
![[LOri 167]]
|LOri 167B
| style="background-color: black;" | [[File:LOri 167 AB Spitzer IRAC.jpg|50px]]
|{{Ntsh|8}}{{Val|8|5|1}}
|
|
|2,000
|
|1,300
|2007
|Direct imaging
|<ref>{{Cite journal |last1=Barrado Y Navascués |first1=D. |last2=Bayo |first2=A. |last3=Morales-Calderón |first3=M. |last4=Huélamo |first4=N. |last5=Stauffer |first5=J. R. |last6=Bouy |first6=H. |date=2007-06-01 |title=The young, wide and very low mass visual binary Lambda Orionis 167 |url=https://ui.adsabs.harvard.edu/abs/2007A%26A...468L...5B |journal=Astronomy and Astrophysics |volume=468 |issue=1 |pages=L5–L8 |arxiv=0704.2469 |bibcode=2007A&A...468L...5B |doi=10.1051/0004-6361:20077258 |issn=0004-6361 |archive-date=24 September 2024 |access-date=6 January 2025 |archive-url=https://web.archive.org/web/20240924222509/https://ui.adsabs.harvard.edu/abs/2007A%26A...468L...5B |url-status=live }}</ref>
|-
![[GSC 00568-01752]]
|SDSS J2249+0044AB
| style="background-color: black;" | [[File:GSC 00568-01752 and companion.jpg|50px]]
|{{Ntsh|12.5}}{{Val|12.5|0.2}} (for single object)
|
|
|2264
|
|146.7
|2010/2024
|Direct imaging
|<ref>{{Cite journal |last1=Allers |first1=K. N. |last2=Liu |first2=Michael C. |last3=Dupuy |first3=Trent J. |last4=Cushing |first4=Michael C. |date=2010-05-01 |title=Discovery of A Young L Dwarf Binary, SDSS J224953.47+004404.6AB |url=https://ui.adsabs.harvard.edu/abs/2010ApJ...715..561A |journal=The Astrophysical Journal |volume=715 |issue=1 |pages=561–571 |arxiv=0912.4687 |bibcode=2010ApJ...715..561A |doi=10.1088/0004-637X/715/1/561 |issn=0004-637X |archive-date=15 August 2024 |access-date=14 August 2024 |archive-url=https://web.archive.org/web/20240815123946/https://ui.adsabs.harvard.edu/abs/2010ApJ...715..561A |url-status=live }}</ref><ref name="Baig2024">{{Cite journal |last1=Baig |first1=Sayan |last2=Smart |first2=R. L. |last3=Jones |first3=Hugh R. A. |last4=Gagné |first4=Jonathan |last5=Pinfield |first5=D. J. |last6=Cheng |first6=Gemma |last7=Moranta |first7=Leslie |date=2024-08-13 |title=The Gaia Ultracool Dwarf Sample -- V: The Ultracool Dwarf Companion catalogue |journal=Monthly Notices of the Royal Astronomical Society |volume=533 |issue=4 |pages=3784–3810 |arxiv=2408.07024 |bibcode=2024MNRAS.533.3784B |doi=10.1093/mnras/stae2005 |doi-access=free}}</ref><ref name="Baig2024b">{{Cite journal |last=Baig |first=Sayan |date=2024-08-13 |title=The Ultracool Dwarf Companion catalouge |url=https://zenodo.org/records/13312178 |journal=Zenodo |doi=10.5281/zenodo.13312178 |archive-date=14 August 2024 |access-date=14 August 2024 |archive-url=https://web.archive.org/web/20240814083210/https://zenodo.org/records/13312178 |url-status=live }}</ref>
|-
! scope="row" | [[WD 0806-661]]
| [[WD 0806-661 b|WD 0806-661 B]]†
| style="background-color: black;" | [[File:WD 0806-661 AB.jpg|50px]]
| {{Ntsh|7}}7–9
|
|
| 2,500
|
| {{sort|0062|62}}
| 2011
| Direct imaging
|
|-
![[USco1621 A]]
|USco1621 b
| style="background-color: black;" | [[File:USco 1621 ESO VHS.jpg|50px]]
|{{Ntsh|16}}16±2
|
|
|2,880±20
|
|452
|2019
|Direct imaging
|<ref name=":4">{{Cite journal |last1=Chinchilla |first1=Patricia |last2=Béjar |first2=Víctor J. S. |last3=Lodieu |first3=Nicolas |last4=Gauza |first4=Bartosz |last5=Zapatero Osorio |first5=Maria Rosa |last6=Rebolo |first6=Rafael |last7=Garrido |first7=Antonio Pérez |last8=Alvarez |first8=Carlos |last9=Manjavacas |first9=Elena |date=2020-01-01 |title=USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius |url=https://ui.adsabs.harvard.edu/abs/2020A%26A...633A.152C/abstract |journal=Astronomy and Astrophysics |volume=633 |pages=A152 |arxiv=1912.04150 |bibcode=2020A&A...633A.152C |doi=10.1051/0004-6361/201936130 |issn=0004-6361 |archive-date=10 February 2023 |access-date=6 January 2025 |archive-url=https://web.archive.org/web/20230210085852/https://ui.adsabs.harvard.edu/abs/2020A%26A...633A.152C/abstract |url-status=live }}</ref>
|-
![[USco1556 A]]
|USco1556 b
| style="background-color: black;" | [[File:USco 1556 legacy dr10.jpg|50px]]
|{{Ntsh|15}}15±2
|
|
|3,500±40
|
|461
|2019
|Direct imaging
|<ref name=":4" />
|-
! scope="row" | [[L 34-26]]
| [[COCONUTS-2b]]†
| style="background-color: black;" | [[File:COCONUTS-2b.jpg|50px]]
| {{Ntsh|6.3}}{{Val|6.3|1.5|1.9}}
| {{Ntsh|1.1}}{{Val|1.1|0.03}}
| ~1,100,000
| 6,471
|
| 35.51±0.01
| 2021/2011
| Direct imaging
| <ref>{{Cite journal |last1=Zhang |first1=Zhoujian |last2=Liu |first2=Michael C. |last3=Claytor |first3=Zachary R. |last4=Best |first4=William M. J. |last5=Dupuy |first5=Trent J. |last6=Siverd |first6=Robert J. |date=2021-08-01 |title=The Second Discovery from the COol Companions ON Ultrawide orbiTS (COCONUTS) Program: A Cold Wide-Orbit Exoplanet around a Young Field M Dwarf at 10.9 pc |journal=The Astrophysical Journal Letters |volume=916 |issue=2 |pages=L11 |arxiv=2107.02805 |bibcode=2021ApJ...916L..11Z |doi=10.3847/2041-8213/ac1123 |issn=2041-8205 |s2cid=236464073 |doi-access=free |hdl=20.500.11820/4f26e8e5-5d42-4259-bc20-fcb093d664b6}}</ref>
|-
! scope="row" | [[TYC 9486-927-1]]
| [[2MASS J2126–8140]]
| style="background-color: black;" | [[File:Image of TYC 9486-927-1 and 2MASS J2126.jpg|50px]]
| {{Ntsh|13.3}}13.3±1.7
|
| ~900,000
| 6,684
| ?
| 80.72±13.86
| 2016/2006
| Direct imaging
| <ref>{{Cite journal |last1=Deacon |first1=N. R. |last2=Schlieder |first2=J. E. |last3=Murphy |first3=S. J. |date=2016-02-23 |title=A nearby young M dwarf with a wide, possibly planetary-mass companion |journal=Monthly Notices of the Royal Astronomical Society |volume=457 |issue=3 |pages=3191–3199 |arxiv=1601.06162 |bibcode=2016MNRAS.457.3191D |doi=10.1093/mnras/stw172 |issn=0035-8711 |s2cid=18220333 |doi-access=free |hdl-access=free |hdl=2299/17156}}</ref>
|-
![[GJ 900]]
|CW2335+0142
| style="background-color: black;" | [[File:GJ900 AB unWISE.jpg|50px]]
|{{Ntsh|10.5}}10.5
|
|
|12,000
|
|68
|2024
|Direct imaging
|<ref name=":5">{{Cite journal |last1=Rothermich |first1=Austin |last2=Faherty |first2=Jacqueline K. |author-link2=Jackie Faherty |last3=Bardalez-Gagliuffi |first3=Daniella |last4=Schneider |first4=Adam C. |last5=Kirkpatrick |first5=J. Davy |author-link5=J. Davy Kirkpatrick |last6=Meisner |first6=Aaron M. |last7=Burgasser |first7=Adam J. |last8=Kuchner |first8=Marc |author-link8=Marc Kuchner |last9=Allers |first9=Katelyn |last10=Gagné |first10=Jonathan |last11=Caselden |first11=Dan |last12=Calamari |first12=Emily |last13=Popinchalk |first13=Mark |last14=Gerasimov |first14=Roman |last15=Aganze |first15=Christian |date=7 Mar 2024 |title=89 New Ultracool Dwarf Co-Moving Companions Identified With The Backyard Worlds: Planet 9 Citizen Science Project |journal=AJ |volume=167 |issue=6 |page=253 |arxiv=2403.04592 |bibcode=2024AJ....167..253R |doi=10.3847/1538-3881/ad324e |doi-access=free |last16=Softich |first16=Emma |last17=Hsu |first17=Chin-Chun |last18=Karpoor |first18=Preethi |last19=Theissen |first19=Christopher A. |last20=Rees |first20=Jon |last21=Cecilio-Flores-Elie |first21=Rosario |last22=Cushing |first22=Michael C. |last23=Marocco |first23=Federico |last24=Casewell |first24=Sarah |last25=Hamlet |first25=Les |last26=Allen |first26=Michaela B. |last27=Beaulieu |first27=Paul |first28=Guillaume |last28=Colin |first29=Jean Marc |last29=Gantier |first30=Leopold |last30=Gramaize |first31=Peter |last31=Jałowiczor |first32=Martin |last32=Kabatnik |first33=Frank |last33=Kiwi |first34=David W. |last34=Martin |first35=Billy |last35=Pendrill |first36=Ben |last36=Pumphrey |first37=Arttu |last37=Sainio |first38=Jörg |last38=Schümann |first39=Nikolaj |last39=Stevnbak |first40=Guoyou |last40=Sun |first41=Christopher |last41=Tanner |first42=Vinod |last42=Thakur |first43=Melina |last43=Thévenot |first44=Zbigniew |last44=Wedracki}}</ref>
|-
![[BD+29 5007]]
|2MASS J2351+3010
| style="background-color: black;" | [[File:BD+29 5007 and companion.jpg|50px]]
|{{Ntsh|11.9}}{{Val|11.9|0.40|0.20}}
|
|
|22,106
|
|77.12
|2015 (age+mass)/ 2016 (co-movement)/ 2024 (both)
|Direct imaging
|<ref>{{Cite journal |last1=Gagné |first1=Jonathan |last2=Faherty |first2=Jacqueline K. |last3=Cruz |first3=Kelle L. |last4=Lafreniére |first4=David |last5=Doyon |first5=René |last6=Malo |first6=Lison |last7=Burgasser |first7=Adam J. |last8=Naud |first8=Marie-Eve |last9=Artigau |first9=Étienne |last10=Bouchard |first10=Sandie |last11=Gizis |first11=John E. |last12=Albert |first12=Loïc |date=2015-08-01 |title=BANYAN. VII. A New Population of Young Substellar Candidate Members of Nearby Moving Groups from the BASS Survey |url=https://ui.adsabs.harvard.edu/abs/2015ApJS..219...33G |journal=The Astrophysical Journal Supplement Series |volume=219 |issue=2 |pages=33 |arxiv=1506.07712 |bibcode=2015ApJS..219...33G |doi=10.1088/0067-0049/219/2/33 |issn=0067-0049 |archive-date=2 May 2023 |access-date=14 August 2024 |archive-url=https://web.archive.org/web/20230502180831/https://ui.adsabs.harvard.edu/abs/2015ApJS..219...33G |url-status=live }}</ref><ref>{{Cite journal |last1=Kirkpatrick |first1=J. Davy |last2=Kellogg |first2=Kendra |last3=Schneider |first3=Adam C. |last4=Fajardo-Acosta |first4=Sergio |last5=Cushing |first5=Michael C. |last6=Greco |first6=Jennifer |last7=Mace |first7=Gregory N. |last8=Gelino |first8=Christopher R. |last9=Wright |first9=Edward L. |last10=Eisenhardt |first10=Peter R. M. |last11=Stern |first11=Daniel |last12=Faherty |first12=Jacqueline K. |last13=Sheppard |first13=Scott S. |last14=Lansbury |first14=George B. |last15=Logsdon |first15=Sarah E. |date=2016-06-01 |title=The AllWISE Motion Survey, Part 2 |journal=The Astrophysical Journal Supplement Series |volume=224 |issue=2 |pages=36 |arxiv=1603.08040 |bibcode=2016ApJS..224...36K |doi=10.3847/0067-0049/224/2/36 |issn=0067-0049 |doi-access=free}}</ref><ref name="Baig2024" /><ref name="Baig2024b" />
|}

== See also ==
* [[Lists of exoplanets]]
* [[List of largest exoplanets]]
* [[List of nearest exoplanets]]
* [[List of nearest terrestrial exoplanet candidates]]
* [[List of potentially habitable exoplanets]]
* [[List of stars with resolved images]]

== Notes ==
{{notelist}}

== References ==
{{reflist}}

== External links ==
{{Commons category|Direct images of exoplanets}}
* {{Cite encyclopedia |title=Candidates detected by imaging |encyclopedia=[[Extrasolar Planets Encyclopaedia]] |url=https://exoplanet.eu/catalog/ |access-date=2011-03-02 |date=1995}}
* {{Cite web |title=Exoplanets Data Explorer |url=http://exoplanets.org/table/ |access-date=2011-03-02}}
* https://www.eso.org/public/images/potw1624a/ - Retrieved 2016-06-16

{{exoplanet}}
{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}
[[Category:Exoplanets detected by direct imaging| ]]
[[Category:Lists of exoplanets|Directly imaged exoplanets]]
[[Category:Astronomy image articles]]