WASP-11/HAT-P-10
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Aries |
Right ascension | 03h 09m 28.541s[1] |
Declination | +30° 40′ 24.84″[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: –3.1 ± 0.9[2] mas/yr Dec.: –40.2 ± 0.7[2] mas/yr |
Distance | 408+20 −16[4] ly (125+6 −5[4] pc) |
Details | |
Mass | 0.77 ± 0.02[5] M☉ |
Radius | 0.74 ± 0.01[5] R☉ |
Luminosity | 0.28 ± 0.002[5] L☉ |
Surface gravity (log g) | 4.58 ± 0.02[5] cgs |
Temperature | 4884 ± 16[5] K |
Metallicity [Fe/H] | 0.25 ± 0.07[6] dex |
Rotational velocity (v sin i) | 1.9 ± 0.9[6] km/s |
Age | 8.7 ± 3.5[5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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 400 light years away in the constellation Aries.[2] [7]
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][4]
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[4] |
3.722465+0.000006 −0.000008 |
0 | — | 0.91+0.06 −0.03 RJ |
See also
- HATNet Project or HAT
- SuperWASP or SWASP
References
- 1 2 Zacharias, N.; et al. (2013). "The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". The Astronomical Journal. 145 (2). 44. arXiv:1212.6182. Bibcode:2013AJ....145...44Z. doi:10.1088/0004-6256/145/2/44.Vizier catalog entry
- 1 2 3 4 5 6 7 8 9 "SIMBAD query result: NAME HAT P-10 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-05.
- 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.
- 1 2 3 4 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.
- 1 2 3 4 5 6 Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951.
- 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.
- ↑ http://arxiv.org/abs/1109.2497
External links
- "WASP-11%2FHAT-P-10". Exoplanets.
Coordinates: 03h 09m 28.55s, +30° 40′ 24.9″
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