Star in the constellation Pegasus
WASP-10 is a star 461 light-years away in the constellation Pegasus . It hosts a transiting planet discovered by the SuperWASP project.[ 3]
The star is likely older than the Sun, has a fraction of heavy elements close to the solar abundance, and is rotating rapidly, being spun up by the tides raised by the giant planet on a close orbit.[ 7]
Planetary system
WASP-10 hosts one confirmed exoplanet , WASP-10b. It is a hot Jupiter discovered in 2008.[ 3]
A candidate second planet with a 5-day period, WASP-10c, was inferred from transit-timing variations of WASP-10b in 2010,[ 8] but this was refuted in 2013.[ 9] Instead, there may be a super-Jupiter planet or brown dwarf on a wide (at least 5 AU ) orbit, based on radial velocity observations.[ 10]
References
^ Roman, Nancy G. (1987). "Identification of a constellation from a position" . Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode :1987PASP...99..695R . doi :10.1086/132034 .
Constellation record for this object at VizieR .
^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ a b c Christian; Gibson, N. P.; Simpson, E. K.; Street, R. A.; Skillen, I.; Pollacco, D.; Collier Cameron, A.; Joshi, Y. C.; et al. (December 29, 2008). "WASP-10b: a 3MJ, gas-giant planet transiting a late-type K star" . Monthly Notices of the Royal Astronomical Society . 392 (4): 1585– 1590. arXiv :0806.1482 . Bibcode :2009MNRAS.392.1585C . doi :10.1111/j.1365-2966.2008.14164.x . S2CID 862722 .
^ Faedi, F.; Staley, T.; et al. (August 2013). "Lucky imaging of transiting planet host stars with LuckyCam" . Monthly Notices of the Royal Astronomical Society . 433 (3): 2097– 2106. arXiv :1305.3795 . Bibcode :2013MNRAS.433.2097F . doi :10.1093/mnras/stt885 .
^ a b c d e f "SIMBAD query result: GSC 02752-00114 -- Star" . Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-06 .
^ a b Bonomo, A. S.; Desidera, S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy & Astrophysics . 602 : A107. arXiv :1704.00373 . Bibcode :2017A&A...602A.107B . doi :10.1051/0004-6361/201629882 . S2CID 118923163 .
^ Maxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015), "A comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars", Astronomy & Astrophysics , 577 : A90, arXiv :1503.09111 , Bibcode :2015A&A...577A..90M , doi :10.1051/0004-6361/201525774 , S2CID 53324330
^ MacIejewski, G.; Dimitrov, D.; Neuhäuser, R.; Tetzlaff, N.; Niedzielski, A.; Raetz, St.; Chen, W. P.; Walter, F.; Marka, C.; Baar, S.; Krejcová, T.; Budaj, J.; Krushevska, V.; Tachihara, K.; Takahashi, H.; Mugrauer, M. (2011). "Transit timing variation and activity in the WASP-10 planetary system★" . Monthly Notices of the Royal Astronomical Society . 411 (2): 1204– 1212. arXiv :1009.4567 . Bibcode :2011MNRAS.411.1204M . doi :10.1111/j.1365-2966.2010.17753.x .
^ Barros, S. C. C.; Boué, G.; et al. (April 2013). "Transit timing variations in WASP-10b induced by stellar activity" . Monthly Notices of the Royal Astronomical Society . 430 (4): 3032– 3047. arXiv :1301.3760 . Bibcode :2013MNRAS.430.3032B . doi :10.1093/mnras/stt111 .
^ a b Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha; Bakos, Gaspar Á.; Batygin, Konstantin; Johnson, John Asher; Morton, Timothy D.; Muirhead, Philip S. (2014). "Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets". The Astrophysical Journal . 785 (2): 126. arXiv :1312.2954 . Bibcode :2014ApJ...785..126K . doi :10.1088/0004-637X/785/2/126 . S2CID 42687848 .
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