List of exoplanet firsts
This is a list of exoplanet discoveries that were the first by several criteria, including:
- the detection method used,
- the planet type,
- the planetary system type,
- the star type,
and others.
The first
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First extrasolar planet discovered | HD 114762 b | HD 114762 | 1989 (Detected), 1991[1](Confirmed) | First exoplanet discovered.
|
By discovery method
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First planet discovered via pulsar timing | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | First super-earths.[2] |
First planet discovered via radial velocity | 51 Pegasi b | 51 Pegasi | 1995 | First planet found around a sun like star.[3] |
First planet discovered via transit | OGLE-TR-56 b | OGLE-TR-56 | 2002 | [4] This was also the second planet detected through transiting,[4] and the then farthest planet known at time of discovery.[4] The first extrasolar planet discovered to be transiting was HD 209458 b, which had already been discovered by the radial velocity method.[4][5] |
First planet discovered via gravitational lensing | OGLE-2003-BLG-235L b | OGLE-2003-BLG-235L / MOA-2003-BLG-53L | 2004 | This was discovered independently by the OGLE and MOA teams.[6] |
First exoplanet discovered by directly imaging the extrasolar planet | 2M1207 b | 2M1207 | 2004/
2005 |
May be a brown dwarf instead of a planet, depending on formation mechanism and definitions chosen. [7] |
First planet discovered through variable star timing | V391 Pegasi b | V391 Pegasi | 2007 | The planet was discovered by examining deviations from pulsation frequency from a subdwarf star.[8] |
First extrasolar planet discovered by indirect imaging (visible light) | Fomalhaut b | Fomalhaut | 2008 | Discovered by a light reflecting off of a dust cloud surrounding the planet.[9] First planet orbiting an ABO star. |
First extrasolar planet discovered by astrometric observations | HD 176051 b | HD 176051 A or HD 176051 B | 2010 | Orbits around one of the stars in a binary star system although it is not known which component it is orbiting around. |
First exoplanet discovered by orbital perturbations of another planet | Kepler-19c | Kepler-19 (KOI-84, TYC 3134-1549-1) | 2011 | Detected through transit-timing variation method. Its existence was inferred by the gravitational influence it had on the orbital periodicity of Kepler-19b.[10][11] |
First exoplanets discovered by orbital phase reflected light variations | Kepler-70b, Kepler-70c [12] | Kepler-70 | 2011 | |
First exoplanet discovered by transit-duration variation method | Kepler-88c | Kepler-88 (KOI-142) | 2013 | Both transit timing variation and transit-duration variation was measured to measure deviations from regular orbit of Kepler-88b. Deviations of the planet's transit duration and timing helped to discover Kepler-88c.[13] |
By detection method
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First planet detected via pulsar timing | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | [2] |
First planet detected via radial velocity | 51 Pegasi b | 51 Pegasi | 1995 | [3] |
First planet detected by transit method | HD 209458 b | HD 209458 | 1999 | This first exoplanet found to be transiting had already been discovered by the radial velocity method. This is also the first planet that has been detected through more than one method.[4][5] |
First directly imaged extrasolar planet (infrared) | 2M1207 b | 2M1207 | 2004 | May be a sub-brown dwarf instead of a planet, depending on formation mechanism and definitions chosen. If it is a planet, it is the first known planet around a brown dwarf. |
First planet with observed secondary eclipse (infrared) | HD 209458 b | HD 209458 | 2005 | Planet was discovered in the year 1999. This is the first direct detection of light from object with a clear planetary origin. |
First directly imaged extrasolar planet orbiting a 'normal' star. (infrared) | DH Tau b | DH Tau | 2005 | [14] Revised masses place it below the deuterium-burning limit. May be a brown dwarf companion. |
First extrasolar planet detected through polarimetry | HD 189733 b | HD 189733 | 2008 | HD 189733 b was discovered in 2005. |
First directly imaged extrasolar planet orbiting a sun-like star. (infrared) | 1RXS J160929.1−210524 b | 1RXS J160929.1−210524 | 2008 | [15] Revised mass places it at or above the deuterium-burning limit. May be a sub-brown dwarf instead of a planet, depending on formation mechanism and definitions chosen. |
First planets directly characterized through astrometric observations. | Gliese 876 b and Gliese 876 c | Gliese 876 | 2009 | |
First planet detected by orbital phase reflected light variations in visible light | CoRoT-1b[16] | CoRoT-1 | 2009 | The planet in question had already been discovered with transit method. |
First planets detected through ellipsoidal light variations of the host star | HAT-P-7b | HAT-P-7b | 2010 | [17] |
First planets detected through transit timing variation method | Kepler-9b, Kepler-9c | Kepler-9 | 2010 | Transit-timing variation was used to confirm both planets detected through transit method.[18] |
First planet detected through transit duration variation method | Kepler-16b | Kepler-16 | 2011 | Orbital motion of the stars causes transits of both components of Kepler-16 to deviate significantly. |
First planet detected with eclipsing binary timing with well-characterized orbit | Kepler-16b | Kepler-16 | 2011 | Kepler-16b itself was detected through transit method. There are stars with earlier detections through eclipsing binary timing. However, those signals have matched with unstable orbits or simply the exact orbits are not known.[19] |
First planet detected by light variations due to relativistic beaming | TrES-2b | TrES-2 | 2012 | [20] |
By system type
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First extrasolar planet discovered in a solitary star system | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | First extrasolar planets discovered[21]
|
First "free-floating" planet discovered[NB 1] | S Ori J053810.1-023626 (S Ori 70) |
N/A | 2004 | [22] Has a mass of 3 MJupiter, needs confirmation. |
First planet discovered in a multiple main-sequence star system | 55 Cancri b | 55 Cancri | 1996 | 55 Cnc has distant red dwarf companion.
|
First planet discovered in a circumbinary orbit | PSR B1620-26 b | PSR B1620-26 | 1993 | Orbits a pulsar and a white dwarf. Discovery confirmed in 2003. |
First multiple planet extrasolar system discovered | PSR B1257+12 A PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | First pulsar planetary system |
First multiple planet system in a multi-star system where multiple planets orbit multiple stars | Kepler-47b Kepler-47c |
Kepler-47 | 2012 | [23][24] NN Serpentis cataclysmic variable is suspected to have at least 2 planets at least in the year 2009.[25] |
First planet discovered in globular cluster | PSR B1620-26 b | PSR B1620-26 | 1993 | Located in Messier 4 |
First binary star system where both components have separate planetary systems | HD 20781 b HD 20781 c HD 20782 b |
HD 20781 HD 20782 |
2011 | |
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
No star system | ||||
First non-stellar planet | S Ori J053810.1-023626 (S Ori 70) |
N/A | 2004 | [22] |
Single star system | ||||
First planet in a solitary star system. | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | [21] |
Binary star system | ||||
First planet in a binary star system | 55 Cancri Ab | 55 Cancri | 1996 | |
First planet in a single-star orbit in a binary star system | 55 Cancri Ab | 55 Cancri | 1996 | |
First planet in a circumbinary orbit in a binary star system | PSR B1620-26 b | PSR B1620-26 | 1993 | The existence of the planet was confirmed in 2003. |
First planet in a circumbinary orbit in a binary star system around main-sequence stars | Kepler-16b | Kepler-16 | 2011 | The stars have spectral classes K and M. |
Trinary star system | ||||
First planet in a trinary star system | 16 Cygni Bb[26][27] | 16 Cygni | 1996 | The stars in this system are 16 Cygni A, 16 Cygni B and 16 Cygni C. |
First planet in a single star orbit in a trinary star system | 16 Cygni Bb[26][27] | 16 Cygni | 1996 | 16 Cygni A and Cygni C form a main pair with the semi-major axis being 73 AU. 16 Cygni B orbits 877 to 15,180 AU from the barycenter of the A and C pair. |
First planet in a multi-star orbit in a trinary star system | ||||
First planet in a circumbinary orbit in a trinary star system | ||||
First planet in a triple-star orbit in a trinary star system | ||||
Quadruple star system | ||||
First planet in a quadruple star system | PH1 or Kepler-64b | Kepler-64 | 2012 | [28] |
First planet in a multi-star orbit in a quadruple star system | PH1 or Kepler-64b | Kepler-64 | 2012 | [29] |
First planet in a single-star orbit in a quadruple star system | 30 Arietis BA b | 30 Arietis BA | 2009 | Quadruple nature of the system was revealed in 2015.[30] |
First circumbinary planet discovered in a quadruple star system | PH1 or Kepler-64b | Kepler-64 | 2012 | [29] |
By star type
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First pulsar planet discovered | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | [21][2] |
First known extrasolar planet orbiting a main sequence star (Sun-like) | 51 Pegasi b | 51 Pegasi | 1995 | First hot Jupiter.[21] |
First known planet orbiting an ABO star (blue-white star) | Fomalhaut b | Fomalhaut | 2008 | First extrasolar planet discovered by visible light image. |
First known planet orbiting a red dwarf | Gliese 876 b | Gliese 876 | 1998 | |
First known planet orbiting a giant star | Iota Draconis b | Iota Draconis | 2002 |
|
First known planet orbiting a white dwarf. | PSR B1620-26 b | PSR B1620-26 | 1993 |
|
First known planet orbiting a brown dwarf. | 2M1207 b | 2M1207 | 2004 | May in fact be a sub-brown dwarf instead of a planet, depending on formation mechanism and definitions chosen. First directly imaged planet. |
First "free-floating" planet discovered[NB 1] | S Ori J053810.1-023626 (S Ori 70) |
N/A | 2004 | [22] Has mass of 3 MJupiter, needs confirmation. |
By planet type
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First hot Jupiter | 51 Pegasi b | 51 Pegasi | 1995 | First planet discovered orbiting a main sequence star |
First extrasolar terrestrial planet orbiting a main sequence star | Mu Arae c | Mu Arae | 2004 | Terrestrial nature of this planet is not confirmed, as no radius measurements are available so the density is unknown. The minimum mass is comparable to that of Uranus, which is not a terrestrial planet. The first extrasolar planet known to have a density compatible with being a rocky planet is CoRoT-7b. |
First super-earth discovered[NB 2] | PSR B1257+12 B PSR B1257+12 C |
PSR B1257+12 | 1992 | [21] First planets discovered[21] |
First super-earth orbiting a main sequence star[NB 2] | Gliese 876 d | Gliese 876 | 2005 | Orbits a red dwarf star |
First icy extrasolar planet orbiting a main sequence star | OGLE-2005-BLG-390Lb | OGLE-2005-BLG-390L | 2006 | Orbits a red dwarf star. The icy nature of this planet is not confirmed, as no radius measurements are available so the density is unknown. The first extrasolar planet known to have a density compatible with being an icy planet is GJ 1214 b, though even for this case there are other possibilities for the composition. |
First evaporating planet discovered | HD 209458 b | HD 209458 | 1999 | First transiting planet[21] |
First Jupiter analogue | HIP 11915 b | HIP 11915 | 2015 | First gas giant located in outer planetary system of another star; previous gas giants had been discovered, but all closer to their star. The discovery raises the possibility that HIP 11915 will be the first Solar System analogue discovered. |
First ocean planet candidate; also first planet within the circumstellar habitable zone | Gliese 581 d | Gliese 581 | 2007 | Orbits a red dwarf star. This planet orbits a little too far from the star, but the greenhouse effect would be enough to make this planet habitable. The other ocean planet candidate GJ 1214 b was detected by transit in which the density was calculated and determined that this planet is an ocean planet. |
First "free-floating" planet discovered[NB 1] | S Ori J053810.1-023626 (S Ori 70) |
N/A | 2004 | [22] Has mass of 3 MJupiter, needs confirmation |
Other
Title | Planet | Star | Year | Notes |
---|---|---|---|---|
First extrasolar transiting planet | HD 209458 b | HD 209458 | 1999 | [5] OGLE-TR-56 b is the first planet found by transit method.[4] |
First map of an extrasolar planet released | HD 189733 b | HD 189733 | 2007 | The map in question is a thermal emission map.[31] |
First multi-planet extrasolar system directly imaged | HR 8799 b HR 8799 c HR 8799 d HR 8799 e |
HR 8799 | 2008 | |
First planet discovered with a retrograde orbit | WASP-17b | WASP-17 | 2009 | The planet HAT-P-7b was discovered before WASP-17b, but its retrograde nature was announced after that of WASP-17b. |
First extrasolar planet with serious potential to support life | Gliese 581 g | Gliese 581 | 2010 | This planet may be tidally locked to its parent star, but there could be a habitable band along the terminator. The other one is Kepler-22b. |
First planet discovered orbiting a Sun-like star in a star cluster | Pr0201b Pr0211b |
Pr0201 Pr0211 |
2012 | Beehive Cluster star cluster [32] |
First recorded planet-planet transit | Kepler-89d Kepler-89e |
Kepler-89 | 2012 | Kepler-89e was partially transiting Kepler-89d.[33] |
First transiting planet discovered in a star cluster | Kepler-66b Kepler-67b |
Kepler-66 Kepler-67 |
2013 | NGC 6811 star cluster; These two planets, were at the time of discovery, only two of six total planets known in star clusters.[34] |
First map of cloud coverage of an extrasolar planet | Kepler-7b | Kepler-7 | 2013 | Observations indicate cloud coverage in the west and clear skies in the east.[35] |
First not tidally locked extrasolar planet to have its day length measured | Beta Pictoris b | Beta Pictoris | 2014 | Rotation speed was calculated to be 8.1 hours.[36] |
See also
Notes
References
- ↑ Cochran, William D.; Hatzes, Artie P.; Hancock, Terry J. (10 October 1991). "Constraints on the Companion Object to HD 114762". The Astrophysical Journal 380: L35–L38. Bibcode:1991ApJ...380L..35C. doi:10.1086/186167.
- 1 2 3 Space.com, "Earth-Sized Planets Confirmed, But They're Dead Worlds", Robert Roy Britt, 29 May 2003 (accessed 20-10-2010)
- 1 2 Queloz, Didier (2006). "Extrasolar planets: Light through a gravitational lens". Nature 439 (7075): 400–401. Bibcode:2006Natur.439..400Q. doi:10.1038/439400a.
- 1 2 3 4 5 6 SpaceDaily.com, "Farthest Known Planet Opens the Door For Finding New Earths", 10 January 2003 (accessed 2010-10-24)
- 1 2 3 PhysOrg.com, "New Era in Planetary Science", 23 March 2005 (accessed 2010-10-24)
- ↑ Sky and Telescope, "First Planet Found by Microlensing", Alan M. MacRobert, 16 April 2004 (accessed 2010-10-24)
- ↑ ESO press releases
- ↑ http://www.nature.com/nature/journal/v449/n7159/abs/nature06143.html
- ↑ Kalas, Paul; et al. (2008-11-13). "Optical Images of an Exosolar Planet 25 Light-Years from Earth". Science 322 (5906): 1345–8. arXiv:0811.1994. Bibcode:2008Sci...322.1345K. doi:10.1126/science.1166609. PMID 19008414.
- ↑ TG Daily, "'Invisible' planet detected", Kate Taylor, 9 September 2011
- ↑ Time, "Found: A (So Far) Invisible World", Michael D. Lemonick, 9 September 2011
- ↑ Charpinet, S. and Fontaine, G. and Brassard, P. and Green, EM and Van Grootel, V. and Randall, SK and Silvotti, R. and Baran, AS and Østensen, RH and Kawaler, SD; et al. (2011). "A compact system of small planets around a former red-giant star". Nature 480 (7378) (Nature Publishing Group). pp. 496–499. doi:10.1038/nature10631.
- ↑ http://arxiv.org/pdf/1304.4283v1.pdf
- ↑ Mass was revised to about 11.5 Jupiter masses in 2006. The object was discovered in 2005.
- ↑ Exoplanet 'circles normal star', BBC News Online, September 15, 2008
- ↑ Ignas A. G. Snellen; Ernst J. W. de Mooij; Simon Albrecht (2009-05-28). "The changing phases of extrasolar planet CoRoT-1b". Nature 459 (7246): 543–545. arXiv:0904.1208. Bibcode:2009Natur.459..543S. doi:10.1038/nature08045. PMID 19478779.
- ↑ Discovery of Ellipsoidal Variations in the Kepler Light Curve of HAT-P-7: William F. Welsh, Jerome A. Orosz, Sara Seager, Jonathan J. Fortney, Jon Jenkins, Jason F. Rowe, David Koch, William J. Borucki
- ↑ http://www.nasa.gov/centers/ames/news/releases/2010/10-73AR.html
- ↑ Overbye, Dennis (2011-09-15). "NASA Detects Planet Dancing With a Pair of Stars". The New York Times. Retrieved 16 September 2011.
- ↑ Photometrically derived masses and radii of the planet and star in the TrES-2 system: Thomas Barclay, Daniel Huber, Jason F. Rowe, Jonathan J. Fortney, Caroline V. Morley, Elisa V. Quintana, Daniel C. Fabrycky, Geert Barentsen, Steven Bloemen, Jessie L. Christiansen, Brice-Olivier Demory, Benjamin J. Fulton, Jon M. Jenkins, Fergal Mullally, Darin Ragozzine, Shaun E. Seader, Avi Shporer, Peter Tenenbaum, Susan E. Thompson
- 1 2 3 4 5 6 7 Space.com, "Out There: A Strange Zoo of Other Worlds", Charles Q. Choi, 14 February 2010 (accessed 2010-10-20)
- 1 2 3 4 Space.com, "Mysterious Object Might be First Extrasolar Planet Photographed", Robert Roy Britt, 22 May 2002 (accessed 2010-10-24)
- ↑ Space.com, "Newfound 'Tatooine' Alien Planet Bodes Well for E.T. Search", Charles Q. Choi, 4 September 2012 (accessed 5 September 2012)
- ↑ SpaceDaily, "Astronomers Find First Multi-Planet System Around a Binary Star", 3 September 2012 (accessed 5 September 2012)
- ↑ http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/abs/2010/13/aa15472-10/aa15472-10.html
- 1 2 BUTLER P. & MARCY G., The Lick Observatory Planet Search in: Astronomical and Biochemical Origins and the Search for Life in the Universe, IAU Colloquium No. 161, Capri 1–5 July 1996, eds. C.B. Cosmovici, S. Bowyer, and D. Werthimer
- 1 2 E. Plávalová, N. A. Solovaya (2012). "Analysis of the motion of an extrasolar planet in a binary system". Astronomy & Astrophysics. arXiv:1212.3843. Bibcode:2013AJ....146..108P. doi:10.1088/0004-6256/146/5/108.
- ↑ NASA JPL, "Citizens Discover Four-Star Planet with NASA's Kepler", Whitney Clavin, 15 October 2012 (accessed 20 October 2012)
- 1 2 PlanetHunters.org, "PH1 : A planet in a four-star system", 15 October 2012 (accessed 20 October 2012)
- ↑ Guenther, E. W.; et al. (2009). "A substellar component orbiting the F-star 30 Arietis B". Astronomy and Astrophysics 507 (3): 1659–1665. arXiv:0912.4619. Bibcode:2009A&A...507.1659G. doi:10.1051/0004-6361/200912112.
- ↑ Knutson, Heather A.; David Charbonneau; Lori E. Allen; Jonathan J. Fortney; Eric Agol; Nicolas B. Cowan; Adam P. Showman; Curtis S. Cooper; S. Thomas Megeath (10 May 2007). "A map of the day–night contrast of the extrasolar planet HD 189733b". Nature 447 (7141): 183–186. arXiv:0705.0993. Bibcode:2007Natur.447..183K. doi:10.1038/nature05782. PMID 17495920.
- ↑ ScienceDaily, "First Planets Found Around Sun-Like Stars in a Cluster", 14 September 2012
- ↑ http://arxiv.org/abs/1310.5771
- ↑ SpaceDaily, First Transiting Planets in a Star Cluster Discovered, 27 June 2013
- ↑ http://www.nasa.gov/mission_pages/spitzer/news/spitzer20130930.html#.Uko8mrOXuPI
- ↑ Cowen, R. (2014-04-30). "First exoplanet seen spinning". Nature. doi:10.1038/nature.2014.15132.
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