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List of exoplanet search projects

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This article containsdynamic lists that may never be able to satisfy particular standards for completeness. You can help byediting the page to add missing items, with references toreliable sources.

The following is a list ofexoplanet search projects.

Ground-based search projects

[edit]
Project nameStatusNumber of exoplanets foundNotes
Anglo-Australian Planet Search (AAPS)Active28 (as of February 2014)
Automated Planet Finder (APF)Active0based at theLick Observatory (also known as the Rocky Planet Finder)[1]
Carl Sagan InstituteActive0
CARMENES[2]Active60+based atCalar Alto Observatory
CORALIE spectrographActive5based atLeonhard Euler Telescope
East-Asian Planet Search Network (EAPSNET)Active1
ELODIEDecommissioned4
EPICSFuture (2030?)N/Abased at theE-ELT[3][4]
ESPRESSOActiveN/Abased at theVLT[5][6]
EXPRESActiveN/Abased at theLowell Discovery Telescope[7]
FINDS Exo-EarthsActive0based at the 3m telescope atLick Observatory[8]
Gemini Planet Imager (GPI)Active1[9]
Geneva Extrasolar Planet SearchActive1+
High Accuracy Radial Velocity Planet Searcher (HARPS)Active130+[10]
HARPS-NActive18+[11]
HATNet and HATSouth Projects (HAT)Active109[12][13]
Hunt for Exomoons with Kepler (HEK)Active0 (A few candidates, includingKepler-1625 b I)
HiCIAOActive0
High Resolution Echelle Spectrometer (HIRES)Active7+[14]based at theW. M. Keck Observatory
KELTDecommissioned[15]26[15]
Lick–Carnegie Exoplanet Survey (LCES)Active1+
Magellan Planet Search ProgramActive10+
MARVELSActive1+[16]
MASCARAActive5[17]
MEarth ProjectActive3[18]
Microlensing Follow-Up Network (MicroFUN)Merged withPLANET10
Microlensing Observations in Astrophysics (MOA)Active8Mt. John University Observatory
MINiature Exoplanet Radial Velocity Array (MINERVA)Active0
N2K ConsortiumActive7
New Mexico Exoplanet Spectroscopic Survey Instrument (NESSI)Active0
Next-Generation Transit Survey (NGTS)Active20[19][20][21][22][23][24][25][26][27]atParanal, since 2015
Okayama Planet Search Program (OPSP)Active6
Optical Gravitational Lensing Experiment (OGLE)Active17+
PlanetPolDecommissioned0
PRL Advanced Radial-velocity All-sky Search (PARAS)Active3[28][29][30]Spectrograph integrated with the 1.2m Gurushikhar Observatory in Mount Abu, India.
Project 1640Active0+
Qatar Exoplanet Survey (QES)Active9[31]
Search for extraterrestrial intelligence (SETI)Active0
SOPHIE échelle spectrographActive0+[32]
Spectro-Polarimetric High-Contrast Exoplanet Research (SPHERE)Active1+[33]
SPECULOOSCommissioning-Searching 1,200 nearby "Ultra Cool Dwarfs" (M7 and later). Successor toTRAPPIST.[34]
Strategic Explorations of Exoplanets and Disks with Subaru (SEEDS)Active1+[35]
SuperWASP (WASP)Active191[36][37]
SystemicActive0an amateur search project
The Habitable Exoplanet Hunting ProjectActive1 (candidate)[38][39]International network of more than 30 observatories including universities and amateur astronomers.
Trans-Atlantic Exoplanet Survey (TrES)Decommissioned5
Transiting Planets and Planetesimals Small Telescope (TRAPPIST)Active7Searching 50 nearby "Ultra Cool Dwarfs" (M7 and later). Prototype forSPECULOOS.
XO Telescope (XO)Active7
ZIMPOL/CHEOPSActive0subsystem of theVLT-SPHERE instrument, based at theVLT[40]
COCONUTSActive3[41][42][43]Large-scale survey for wide-orbit planetary and substellar companions[44]

Space missions

[edit]

Past and current

[edit]
NameLaunch dateEnd dateNumber of exoplanets foundCurrent candidatesTelescope use
MOSTJune 20, 2003March 20191+0First spacecraft dedicated to the study ofasteroseismology
EPOXIJuly 21, 2005August 8, 201300Characterized planets and fly-by of comet
SWEEPS20062006160Based from theHST, a short 7 day mission looking for exoplanets
CoRoTDecember 27, 2006November 2, 201234600Mission to look for exoplanets using the transit method
KeplerMarch 7, 2009August 15, 20133,2464,711Mission to look for large numbers of exoplanets using the transit method
K2November 18, 2013October 30, 2018427891 (+627microlensing events)After thereaction wheels failed onKepler, this mission was created
GaiaDecember 19, 2013March 27, 202500Map 1 billion astronomical objects in the Milky Way (First data Release November 2, 2016)
ASTERIANovember 2017December 5, 201900CubeSat, technology demonstrator
TESSApril 18, 2018Ongoing233+3,876To search for new exoplanets; rotating so by the end of its two-year mission it will have observed stars from all over the sky. It is expected to find at least 3,000 new exoplanets.
CHEOPS2019[45]Ongoing2+0To learn more about how exoplanets form, probe atmospheres, and characterize super-Earths. 20% of time will be open to community use.[46] Duration: 3.5 (+ 3 goal) years
JWSTCommissioned on 25, December 2021Ongoing10To study atmospheres of known exoplanets and find some Jupiter-sized exoplanets Duration: 5 (+ 5 goal) years
2,757 (3,941 Total)[47]3,914

Planned

[edit]
NameLaunch dateMission objectivesDurationNotes
ARIEL2029 (Ariane 62)Observe exoplanets using the transit method, study and characterise the planets' chemical composition and thermal structures4 years
RSTOctober 2026To search for and study exoplanets while studyingdark matter. It is expected to find about 2,500 planets.6 years
PLATODecember 2026 (Ariane 62)To search for and characterize rocky planets around stars like our own.4 (+4 goal) years
TOLIMANend of 2026Detect exoplanets inAlpha Centauri usingastrometry.3 years

Proposed

[edit]

Canceled

[edit]

References

[edit]
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  2. ^"carmenes".carmenes. Retrieved2024-10-22.
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  5. ^ESO."ESO - Espresso".www.eso.org. Retrieved2016-07-08.
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  26. ^Jackman, James A. G.; Wheatley, Peter J.; Bayliss, Dan; Gill, Samuel; Hodgkin, Simon T.; Burleigh, Matthew R.; Braker, Ian P.; Günther, Maximilian N.; Louden, Tom; Turner, Oliver; Anderson, David R. (2019-11-11)."NGTS-7Ab: An ultra-short period brown dwarf transiting a tidally-locked and active M dwarf".Monthly Notices of the Royal Astronomical Society.489 (4):5146–5164.arXiv:1906.08219.doi:10.1093/mnras/stz2496.ISSN 0035-8711.
  27. ^McCormac, James; Gillen, Edward; Jackman, James A. G.; Brown, David J. A.; Bayliss, Daniel; Wheatley, Peter J.; West, Richard G.; Anderson, David R.; Armstrong, David J.; Bouchy, Francois; Briegal, Joshua T. (2020-03-21)."NGTS-10b: The shortest period hot Jupiter yet discovered".Monthly Notices of the Royal Astronomical Society.493 (1):126–140.arXiv:1909.12424.doi:10.1093/mnras/staa115.ISSN 0035-8711.
  28. ^"Discovery of a Sub-Saturn Exoplanet around a Sun-like star - ISRO".www.isro.gov.in. Retrieved2019-11-25.
  29. ^"Discovery".www.isro.gov.in.
  30. ^Khandelwal, Akanksha; Sharma, Rishikesh; Chakraborty, Abhijit; Chaturvedi, Priyanka; Ulmer-Moll, Solène; Ciardi, David R.; Boyle, Andrew W.; Baliwal, Sanjay; Bieryla, Allyson; Latham, David W.; Prasad, Neelam J. S. S. V.; Nayak, Ashirbad; Lendl, Monika; Mordasini, Christoph (April 1, 2023)."Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603".Astronomy & Astrophysics.672: L7.arXiv:2303.11841.Bibcode:2023A&A...672L...7K.doi:10.1051/0004-6361/202245608.S2CID 257637141 – via www.aanda.org.
  31. ^"Home - (QES)".qatarexoplanet.org. Archived from the original on 7 February 2022. Retrieved2019-05-04.
  32. ^"SOPHIE |".exoplanets.ch. Retrieved2016-07-08.
  33. ^"ESO's SPHERE Unveils its First Exoplanet".eso.org. 2017-07-06.
  34. ^Delrez, Laetitia; et al. (2018). "SPECULOOS: A network of robotic telescopes to hunt for terrestrial planets around the nearest ultracool dwarfs". In Spyromilio, Jason; Marshall, Heather K; Gilmozzi, Roberto (eds.).Ground-based and Airborne Telescopes VII. Vol. 10700. pp. 107001I.arXiv:1806.11205.Bibcode:2018SPIE10700E..1ID.doi:10.1117/12.2312475.ISBN 9781510619531.S2CID 119012966.
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  41. ^Zhang, Zhoujian; Liu, Michael C.; Hermes, J. J.; Magnier, Eugene A.; Marley, Mark S.; Tremblay, Pier-Emmanuel; Tucker, Michael A.; Do, Aaron; Payne, Anna V.; Shappee, Benjamin J. (2020-03-17)."COol Companions ON Ultrawide orbiTS (COCONUTS). I. A High-Gravity T4 Benchmark around an Old White Dwarf and A Re-Examination of the Surface-Gravity Dependence of the L/T Transition".The Astrophysical Journal.891 (2): 171.arXiv:2002.05723.Bibcode:2020ApJ...891..171Z.doi:10.3847/1538-4357/ab765c.ISSN 1538-4357.S2CID 211126544.
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