WASP-11/HAT-P-10

WASP-11/HAT-P-10
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Aries
Right ascension 03h 09m 28.5432s[1]
Declination +30° 40′ 24.853″[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[2]
Apparent magnitude (H) 9.560 ± 0.019[2]
Apparent magnitude (K) 9.421 ± 0.017[2]
Astrometry
Proper motion (μ) RA: 3.522±1.680[1] mas/yr
Dec.: −43.789±0.866[1] mas/yr
Parallax (π)7.49 ± 0.58[1] mas
Distance440 ± 30 ly
(130 ± 10 pc)
Details
Mass0.77 ± 0.02[4] M☉
Radius0.74 ± 0.01[4] R☉
Luminosity0.28 ± 0.002[4] L☉
Surface gravity (log g)4.58 ± 0.02[4] cgs
Temperature4884 ± 16[4] K
Metallicity [Fe/H]0.25 ± 0.07[5] dex
Rotational velocity (v sin i)1.9 ± 0.9[5] km/s
Age8.7 ± 3.5[4] Gyr
Other designations
TYC 2340-1714-1, WASP-11, GSC 02340-01714, 2MASS J03092855+3040249, UCAC2 42532154, HAT-P-10
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia		data

WASP-11/HAT-P-10 is a binary star consisting a magnitude-12 main-sequence orange dwarf star and M-dwarf with separation of 42 AU. The system is located about 440 light years away in the constellation Aries.[2] [6]

Planetary system

A semi-Jovian planet, WASP-11b/HAT-P-10b (WASP-11 A b/HAT-P-10 A b), has been detected in 2008 around the primary star by two projects independently using the transit method in a circular orbit around this star.[3][7]

The WASP-11/HAT-P-10 planetary system
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
WASP-11b/HAT-P-10b 0.53 ± 0.07 MJ 0.0439+0.0006
−0.0009[7]		 3.722465+0.000006
−0.000008		 0 — 0.91+0.06
−0.03 RJ

See also

References

  1. 1 2 3 4 5 Brown, A. G. A; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. Gaia Data Release 1 catalog entry
  2. 1 2 3 4 5 6 7 "SIMBAD query result: NAME HAT P-10 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-05.
  3. 1 2 West, 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.
  4. 1 2 3 4 5 6 Bonfanti, 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.
  5. 1 2 Torres, 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.
  6. ↑ 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].
  7. 1 2 Bakos, G. Á.; et al. (2009). "HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf". The Astrophysical Journal. 696 (2): 1950–1955. arXiv:0809.4295. Bibcode:2009ApJ...696.1950B. doi:10.1088/0004-637X/696/2/1950.
  • "WASP-11%2FHAT-P-10". Exoplanets.

Coordinates: 03h 09m 28.55s, +30° 40′ 24.9″


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