WASP-10

WASP-10 is a star in the constellation Pegasus. The SuperWASP project has observed and classified this star as a variable star, perhaps due to the eclipsing planet.[2]

WASP-10
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension  23h 15m 58.3005s[1]
Declination +31° 27 46.295[1]
Apparent magnitude (V) 12.7
Characteristics
Spectral type K5
Apparent magnitude (B) ~12.4[2]
Apparent magnitude (R) ~12.03[2]
Apparent magnitude (J) 10.603 ±0.026[2]
Apparent magnitude (H) 10.117 ±0.029[2]
Apparent magnitude (K) 9.983 ±0.018[2]
Variable type V*(1SWASP)[2]
Astrometry
Proper motion (μ) RA: 25.110±0.052[1] mas/yr
Dec.: −25.269±0.048[1] mas/yr
Parallax (π)7.0636 ± 0.0372[1] mas
Distance462 ± 2 ly
(141.6 ± 0.7 pc)
Details[3]
Mass0.71+0.086
0.071
 M
Radius0.783 −0.043+0.035 R
Temperature4675 ±100 K
Metallicity0.03±0.2
Rotation11.91±0.05 d
Age6.00±4.12 Gyr
Other designations
GSC 02752-00114, 2MASS J23155829+3127462, UCAC2 42862442, GSC2 N0013312406, 1SWASP J231558.30+312746.4, USNO-B1.0 1214-00586164, Gaia DR2 1909762228985058944[2]
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia
data

The star is likely older than Sun, has fraction of heavy elements close to solar abundance, and is rotating rapidly, being spun up by the tides raised by the giant planet on the close orbit.[3]

Planetary system

The WASP-10 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 3.06+0.23
0.21
 MJ
0.0371+0.0014
0.0013
3.0927616+0.0000112
0.0000182
0.057+0.011
0.005
1.08±0.02 RJ
c (unconfirmed) 0.1 MJ 5.23 days

WASP-10b is an extrasolar planet discovered in 2008.[4]

WASP-10c is an unconfirmed as in 2020[5] extrasolar planet inferred from transit time variations of WASP-10b's transits. It was discovered in 2010.[6]

High likelihood of another Super-Jupiter planet at wide (at least 5 astronomical units) orbit was reported in 2013.[7]

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See also

References

  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. "SIMBAD query result: GSC 02752-00114 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-06.
  3. A comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars, 2015, arXiv:1503.09111
  4. 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.
  5. Extrasolar Planets Encyclopaedia Planet WASP-10 c
  6. 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.
  7. 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.

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