Back WASP-10 German دبلیوایاسپی-۱۰ Persian WASP-10 Japanese WASP-10 Korean WASP-10 Polish WASP-10 Russian WASP-10 Swedish WASP-10 Ukrainian
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pegasus |
| Right ascension | 23h 15m 58.3006s[1] |
| Declination | +31° 27′ 46.296″[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: 25.050(12) mas/yr[1] Dec.: −25.366(11) mas/yr[1] |
| Parallax (π) | 7.0717 ± 0.0135 mas[1] |
| Distance | 461.2 ± 0.9 ly (141.4 ± 0.3 pc) |
| Details[3] | |
| Mass | 0.71+0.086 −0.071 M☉ |
| Radius | 0.783 −0.043+0.035 R☉ |
| Temperature | 4675 ±100 K |
| Metallicity | 0.03±0.2 |
| Rotation | 11.91±0.05 d |
| Age | 6.00±4.12 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
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]
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]
- ^ a b c d Cite error: The named reference
Gaia DR3was invoked but never defined (see the help page). - ^ a b c d e f g h "SIMBAD query result: GSC 02752-00114 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-06.
- ^ a b 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