List of directly imaged 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 least massive planet is Fomalhaut b, which has a mass of 2 MJ or less. The coldest and oldest is 59 Virginis b with a mean temperature of 240 °C and age of 100–500 million years.[1] This list includes the four members of the multi-planet system that orbit HR 8799.
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. 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
- LOCI = Locally Optimized Combination of Images
- NRM = Non-Redundant Aperture Masking Interferometry
- RSDI = Reference Star Differential Imaging
- TLOCI = Template Locally Optimized Combination of Images
Exoplanets
† There is no consensus whether these companions of stars should be considered sub-brown dwarfs or planets
Star | Exoplanet | Mass (MJ) | Radius (RJ) | Period (yr) | Observed separation (AU) | Eccentricity | Distance to Earth (ly) | Year of discovery | Imaging technique | Ref(s). |
---|---|---|---|---|---|---|---|---|---|---|
Beta Pictoris | Beta Pictoris b | 20 | 1.5±0.2 | 22.47+3.77 −2.26 | 9 | 0.08+0.09 −-0.05 | 63.4±0.1 | 2008 | RSDI | [2][3][4] |
51 Eridani | 51 Eridani b | 2.0 | 1.0 | ? | 13 | ? | 96 | 2014 | ADI, TLOCI | |
HR 8799 | HR 8799 e | 7.0 | 1.3 | 49 | 14.5 | 0.14 | 128 | 2010 | ADI, LOCI | |
HR 8799 d | 7.0 | 1.3 | 100 | 24.5 | 0.09 | 128 | 2008 | ADI, LOCI | ||
HR 8799 c | 7.0 | 1.3 | 189 | 37.4 | 0.24 | 128 | 2008 | ADI, LOCI | ||
HR 8799 b | 5.0 | 1.2 | 474 | 69.2 | 0.17 | 128 | 2008 | ADI, LOCI | ||
ROXs 42B | ROXs 42Bb† | 9±3 | 2.5 | Unknown | 157 | Unknown | 440±16 | 2013 | Direct imaging | [5] |
2M1207 | 2M1207b† | 4.2 | 1.5 | 1620 | 40.6 | 0.37 | 170 | 2004 | Direct imaging | |
1RXS J1609 | 1RXS 1609 b | 8–14 | 1.7 | 6518 | 331.1 | 0.08 | 470 | 2008 | Direct imaging | |
2M J044144 | 2M J044144 b† | 5–10 | 15 | 456 | 2010 | Direct imaging | ||||
Fomalhaut | Fomalhaut b | < 2.0 | 872–2000 | 116.0 | 25 | 2008/2012 | RSDI | |||
LkCa 15 | LkCa 15 b | 6.2 | 1.8 | 42315 | 23.5 | 0.32 | 477 | 2011 | NRM | |
WD 0806-661 | WD 0806-661 B† | 7–13 | ? | ? | 2500 | ? | 62 | 2011 | Direct imaging | |
DT Virginis | Ross 458(AB) c† | 8.5 | 1.8 | 33081 | 1167.7 | 0.17 | 38[6] | 2011 | Direct Imaging | |
HD 95086 | HD 95086 b | 5.0 | ? | ? | 56 | ? | 295 | 2013 | ADI, LOCI | |
59 Virginis | Gliese 504 b | 4+4.5 −1 | ? | ? | 43.5 | ? | 57.27 | 2013 | ADI, LOCI | |
FW Tauri | FW Tauri b† | 10±4 | ? | ? | 330 | ? | ? | 2013 | Direct imaging | |
HD 106906 | HD 106906 b | 11±2 | ? | ? | 650 | ? | 300 | 2013 | ADI | |
GU Piscium | GU Piscium b | 11±2 | 163000 | 2000 | 155 | 2014 | Direct imaging | |||
VHS 1256-1257 | VHS 1256 b | 11.2 | 3900 | 102 | 40 | 2015 | Direct imaging | |||
CVSO 30 | CVSO 30 c | 27000 | 660 | 1200 | 2016 | Direct imaging | ||||
HD 131399 A | HD 131399 Ab | 4±1 | ? | 550 | 82 | 0.35 | 320[7] | 2016 | ADI |
References
- ↑ Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504
- ↑ Wang et. al. (2016). "The Orbit and Transit Prospects for β Pictoris b Constrained with One Milliarcsecond Astrometry". The Astronomical Journal. 152 (4). Bibcode:2016AJ....152...97W. arXiv:1607.05272 . doi:10.3847/0004-6256/152/4/97.
- ↑ Bonnefoy et. al. (2014). "Physical and orbital properties of β Pictoris b". Astronomy & Astrophysics. 567. Bibcode:2014A&A...567L...9B. arXiv:1407.4001 . doi:10.1051/0004-6361/201424041.
- ↑ Currie, Thayne; Burrows, Adam; Madhusudhan, Nikku; Fukagawa, Misato; Girard, Julien H.; Dawson, Rebekah; Murray-Clay, Ruth; Kenyon, Scott; Kuchner, Marc; Matsumura, Soko; Jayawardhana, Ray; Chambers, John; Bromley, Ben (2013). "A Combined Very Large Telescope and Gemini Study of the Atmosphere of the Directly Imaged Planet, β Pictoris b". The Astrophysical Journal. 776 (1): 15. Bibcode:2013ApJ...776...15C. ISSN 0004-637X. arXiv:1306.0610 . doi:10.1088/0004-637X/776/1/15.
- ↑ Currie, Thayne; Burrows, Adam; Daemgen, Sebastian (2014). "A First-Look Atmospheric Modeling Study of the Young Directly-Imaged Planet-Mass Companion, ROXs 42Bb". arXiv:1404.0131 [astro-ph.SR].
- ↑ "Ross 458(AB) c". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Retrieved 2012-10-24.
- ↑ "Direct imaging discovery of a Jovian exoplanet within a triple-star system". Science magazine. AAAS. Retrieved 2016-07-08.
External links
Wikimedia Commons has media related to Direct images of exoplanets. |
- "Candidates detected by imaging". The Extrasolar Planets Encyclopaedia. Retrieved 2011-03-02.
- "Exoplanets Data Explorer". Retrieved 2011-03-02.
- https://www.eso.org/public/images/potw1624a/ - Retrieved 2016-06-16