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WASP-11/HAT-P-10
Observation data Epoch J2000.0 Equinox J2000.0
Constellation	Aries
Right ascension	03^h 09^m 28.5427^s^[1]
Declination	+30° 40′ 24.8688″^[1]
Apparent magnitude(V)	11.57 ± 0.15^[2]
Characteristics
Spectral type	K3V^[3]
Apparent magnitude(B)	12.58 ± 0.30^[2]
Apparent magnitude(V)	11.57 ± 0.15^[2]
Apparent magnitude(J)	10.015 ± 0.020^[4]
Apparent magnitude(H)	9.560 ± 0.019^[4]
Apparent magnitude(K)	9.421 ± 0.017^[4]
Astrometry
Proper motion(μ)	RA:3.856±0.267^[1]mas/yr Dec.:−44.826±0.213^[1]mas/yr
Parallax(π)	7.9921 ± 0.1325^[1]mas
Distance	408 ± 7 ly (125 ± 2 pc)
Details^[5]>
WASP-11 A
Mass	0.77 ± 0.02^[6]`M`_☉
Radius	0.74 ± 0.01^[6]`R`_☉
Luminosity	0.28 ± 0.002^[6]`L`_☉
Surface gravity(log g)	4.58 ± 0.02^[6]cgs
Temperature	4884±16^[6]K
Metallicity [Fe/H]	0.25 ± 0.07^[7]dex
Rotational velocity(v sin i)	1.9 ± 0.9^[7] km/s
Age	8.7 ± 3.5^[6]Gyr
WASP-11 B
Mass	0.34 `M`_☉
Temperature	3494±37^[8]K
Other designations
TYC 2340-1714-1, WASP-11, GSC 02340-01714, 2MASS J03092855+3040249, UCAC2 42532154, HAT-P-10, Gaia DR2 123376685084303360
Database references
SIMBAD	data
Extrasolar Planets Encyclopaedia	data

WASP-11/HAT-P-10 is a binary star. It is a primary main-sequenceorange dwarf star. Secondary is M-dwarf with a projected separation of 42 AU.^[8] The system is located about 408 light years away^[1] in the constellation Aries.^[2]^[9]

Planetary system[edit]

A semi-Jovian planet, WASP-11b/HAT-P-10b (WASP-11 A b/HAT-P-10 A b), was detected around the primary star independently by the Hungarian Automated Telescope Network and the Wide Angle Search for Planets teams both of which used the transit method.^[3]^[10]

The WASP-11/HAT-P-10 planetary system^[11]
Companion (in order from star)	Mass	Semimajor axis (AU)	Orbital period (days)	Eccentricity	Inclination	Radius
b	0.532+0.020 −0.021M_J	0.04376+0.00071 −0.00067	3.7224793±0.0000007	<0.03	89.03±0.34°	0.990±0.022R_J

References[edit]

^ ^a^b^c^d^e^fBrown, 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.
^ ^a^b^c^d'SIMBAD query result: NAME HAT P-10 -- Star'. Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-05.
^ ^a^bWest, R. G.; et al. (2009). 'The sub-Jupiter mass transiting exoplanet WASP-11b'. Astronomy and Astrophysics. 502 (1): 395–400. arXiv:0809.4597. Bibcode:2009A&A...502..395W. doi:10.1051/0004-6361/200810973. S2CID18189916.
^ ^a^b^cSkrutskie, M. F.; et al. (2006). 'The Two Micron All Sky Survey (2MASS)'. The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.Vizier catalog entry
^Quarles, Billy; Li, Gongjie; Kostov, Veselin; Haghighipour, Nader (2020), 'Orbital Stability of Circumstellar Planets in Binary Systems', The Astronomical Journal, 159 (3): 80, arXiv:1912.11019, doi:10.3847/1538-3881/ab64fa, S2CID209444271
^ ^a^b^c^d^e^fBonfanti, A.; et al. (2015). 'Revising the ages of planet-hosting stars'. Astronomy and Astrophysics. 575 (18). A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951. S2CID54555839.
^ ^a^bTorres, Guillermo; et al. (2012). 'Improved Spectroscopic Parameters for Transiting Planet Hosts'. The Astrophysical Journal. 757 (2). 161. arXiv:1208.1268. Bibcode:2012ApJ...757..161T. doi:10.1088/0004-637X/757/2/161. S2CID16580774.
^ ^a^bPiskorz, Danielle; Knutson, Heather A.; Ngo, Henry; Muirhead, Philip S.; Batygin, Konstantin; Crepp, Justin R.; Hinkley, Sasha; Morton, Timothy D. (2015), 'Friends of Hot Jupiters. III. An Infrared Spectroscopic Search for Low-Mass Stellar Companions', The Astrophysical Journal, 814 (2): 148, arXiv:1510.08062, doi:10.1088/0004-637X/814/2/148, S2CID11525988
^Mayor, M; Marmier, M; Lovis, C; Udry, S; Ségransan, D; Pepe, F; Benz, W; Bertaux, J. -L; Bouchy, F; Dumusque, X; Lo Curto, G; Mordasini, C; Queloz, D; Santos, N. C (2011). 'The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets'. arXiv:1109.2497 [astro-ph.EP].
^Bakos, G. Á.; et al. (2009). 'HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf'.

Planetary system[edit]

See also[edit]

References[edit]