Short description: Exoplanets confirmed or discovered from direct imaging
Motion interpolation of seven images of the HR 8799 system taken from the W. M. Keck Observatory over seven years, featuring four exoplanets
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 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 planets.
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 lightest, coldest, and oldest planet directly imaged is Proxima Centauri c, which has seven times Earth's mass, an effective temperature of 39 K, and an age of about 4.8Ga.
This list includes the four members of the multi-planet system that orbit HR 8799.
Exoplanets have been discovered using several different methods for collecting or combining direct images to isolate planets from the background light of their star. 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.
TLOCI = Template Locally Optimized Combination of Images
Exoplanets
Although listed in the table below, the identities of Fomalhaut b and Candidate 1 are disputed. They may not actually be true exoplanets.
† There is no consensus whether these companions of stars should be considered sub-brown dwarfs or planets
Check https://exoplanetarchive.ipac.caltech.edu/docs/imaging.html to see more directly imaged planets. It contains an updated table of all of them.
↑Franson, Kyle; Bowler, Brendan P.; Zhou, Yifan; Pearce, Tim D.; Bardalez Gagliuffi, Daniella C.; Biddle, Lauren I.; Brandt, Timothy D.; Crepp, Justin R. et al. (2023). "Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged inside the Debris Disk of the Young Star AF Lep". The Astrophysical Journal Letters (American Astronomical Society) 950 (2): L19. doi:10.3847/2041-8213/acd6f6. Bibcode: 2023ApJ...950L..19F.
↑Mesa, D.; Gratton, R.; Kervella, P.; Bonavita, M.; Desidera, S.; D'Orazi, V.; Marino, S.; Zurlo, A. et al. (2023-02-13). "AF Lep b: The lowest-mass planet detected by coupling astrometric and direct imaging data". Astronomy & Astrophysics672: A93. doi:10.1051/0004-6361/202345865. Bibcode: 2023A&A...672A..93M.
↑De Rosa, Robert J.; Nielsen, Eric L.; Wahhaj, Zahed; Ruffio, Jean-Baptise; Kalas, Paul G.; Peck, Anne E.; Hirsch, Lea A.; Roberson, William (2023-02-13). "Direct imaging discovery of a super-Jovian around the young Sun-like star AF Leporis". Astronomy & Astrophysics672: A94. doi:10.1051/0004-6361/202345877. Bibcode: 2023A&A...672A..94D.
↑Morzinski (2015). "Magellan Adaptive Optics First-light Observations of the Exoplanet β Pic b. II. 3-5 μm Direct Imaging with MagAO+Clio, and the Empirical Bolometric Luminosity of a Self-luminous Giant Planet". The Astrophysical Journal815 (2): 108. doi:10.1088/0004-637X/815/2/108. Bibcode: 2015ApJ...815..108M.
↑Hammond, Iain; Christiaens, Valentin; Price, Daniel J.; Toci, Claudia; Pinte, Christophe; Juillard, Sandrine; Garg, Himanshi (2023-03-01). "Confirmation and keplerian motion of the gap-carving protoplanet HD 169142 b". Monthly Notices of the Royal Astronomical Society522 (1): L51–L55. doi:10.1093/mnrasl/slad027. ISSN0035-8711. Bibcode: 2023MNRAS.522L..51H.
↑Delorme, P.; Gagné, J.; Girard, J. H.; Lagrange, A. M.; Chauvin, G.; Naud, M. -E.; Lafrenière, D.; Doyon, R. et al. (2013-05-01). "Direct-imaging discovery of a 12-14 Jupiter-mass object orbiting a young binary system of very low-mass stars". Astronomy and Astrophysics553: L5. doi:10.1051/0004-6361/201321169. ISSN0004-6361. Bibcode: 2013A&A...553L...5D.
↑Currie, Thayne; Lawson, Kellen; Schneider, Glenn et al. (4 April 2022). "Images of embedded Jovian planet formation at a wide separation around AB Aurigae". Nature Astronomy (Springer Science and Business Media LLC) 6 (6): 751–759. doi:10.1038/s41550-022-01634-x. ISSN2397-3366. Bibcode: 2022NatAs...6..751C.
↑Currie, Thayne; Daemgen, Sebastian; Debes, John; Lafreniere, David; Itoh, Yoichi; Jayawardhana, Ray; Ratzka, Thorsten; Correia, Serge (2014). "Direct Imaging and Spectroscopy of a Candidate Companion Below/Near the Deuterium-Burning Limit In The Young Binary Star System, ROXs 42B". The Astrophysical Journal Letters780 (2): 30. doi:10.1088/2041-8205/780/2/L30. Bibcode: 2014ApJ...780L..30C.
↑Bowler, Brendan P.; Liu, Michael C.; Mawet, Dimitri; Ngo, Henry; Malo, Lison; Mace, Gregory N.; McLane, Jacob N.; Lu, Jessica R. et al. (2017-01-01). "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*". The Astronomical Journal153 (1): 18. doi:10.3847/1538-3881/153/1/18. ISSN0004-6256. Bibcode: 2017AJ....153...18B.
↑Chauvin, G.; Lagrange, A. -M.; Zuckerman, B.; Dumas, C.; Mouillet, D.; Song, I.; Beuzit, J. -L.; Lowrance, P. et al. (2005-08-01). "A companion to AB Pic at the planet/brown dwarf boundary". Astronomy and Astrophysics438 (3): L29–L32. doi:10.1051/0004-6361:200500111. ISSN0004-6361. Bibcode: 2005A&A...438L..29C.
↑Bonnefoy, M.; Chauvin, G.; Lagrange, A. -M.; Rojo, P.; Allard, F.; Pinte, C.; Dumas, C.; Homeier, D. (2014-02-01). "A library of near-infrared integral field spectra of young M-L dwarfs". Astronomy and Astrophysics562: A127. doi:10.1051/0004-6361/201118270. ISSN0004-6361. Bibcode: 2014A&A...562A.127B.
↑Zhou, Yifan; Herczeg, Gregory J.; Kraus, Adam L.; Metchev, Stanimir; Cruz, Kelle L. (2014-03-01). "Accretion onto Planetary Mass Companions of Low-mass Young Stars". The Astrophysical Journal783 (1): L17. doi:10.1088/2041-8205/783/1/L17. ISSN0004-637X. Bibcode: 2014ApJ...783L..17Z.
↑Miles-Páez, Paulo A.; Metchev, Stanimir; Luhman, Kevin L.; Marengo, Massimo; Hulsebus, Alan (2017). "The Prototypical Young L/T-Transition Dwarf HD 203030B Likely Has Planetary Mass". The Astronomical Journal154 (6): 262. doi:10.3847/1538-3881/aa9711. Bibcode: 2017AJ....154..262M.
↑Faherty, Jacqueline K.; Gagné, Jonathan; Popinchalk, Mark; Vos, Johanna M.; Burgasser, Adam J.; Schümann, Jörg; Schneider, Adam C.; Kirkpatrick, J. Davy et al. (2021-12-01). "A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9". The Astrophysical Journal923 (1): 48. doi:10.3847/1538-4357/ac2499. ISSN0004-637X. Bibcode: 2021ApJ...923...48F.
↑Dupuy, Trent J.; Liu, Michael C.; Allers, Katelyn N.; Biller, Beth A.; Kratter, Kaitlin M.; Mann, Andrew W.; Shkolnik, Evgenya L.; Kraus, Adam L. et al. (2018-08-01). "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". The Astronomical Journal156 (2): 57. doi:10.3847/1538-3881/aacbc2. ISSN0004-6256. Bibcode: 2018AJ....156...57D.
↑Zhang, Zhoujian; Liu, Michael C.; Claytor, Zachary R.; Best, William M. J.; Dupuy, Trent J.; Siverd, Robert J. (2021-08-01). "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". The Astrophysical Journal Letters916 (2): L11. doi:10.3847/2041-8213/ac1123. ISSN2041-8205. Bibcode: 2021ApJ...916L..11Z.
↑Deacon, N. R.; Schlieder, J. E.; Murphy, S. J. (2016-02-23). "A nearby young M dwarf with a wide, possibly planetary-mass companion". Monthly Notices of the Royal Astronomical Society457 (3): 3191–3199. doi:10.1093/mnras/stw172. ISSN0035-8711. Bibcode: 2016MNRAS.457.3191D.