HAT-P-3
Observation data Epoch 2000 Equinox 2000 | |
---|---|
Constellation | Ursa Major[1] |
Right ascension | 13h 44m 22.5949s[2] |
Declination | +48° 01′ 43.210″[2] |
Apparent magnitude (V) | 11.577 ± 0.067[3] |
Characteristics | |
Spectral type | K[4] |
Apparent magnitude (B) | 12.53 ± 0.20[5] |
Apparent magnitude (V) | 11.577 ± 0.067[3] |
Apparent magnitude (I) | 10.504 ± 0.079[3] |
Apparent magnitude (J) | ±0.022 9.936[6] |
Apparent magnitude (H) | ±0.028 9.542[6] |
Apparent magnitude (K) | ±0.025 9.448[6] |
Astrometry | |
Radial velocity (Rv) | ±0.1 −23.8[4] km/s |
Proper motion (μ) | RA: ±0.647 −20.426[2] mas/yr Dec.: ±0.893 −24.294[2] mas/yr |
Parallax (π) | 7.26 ± 0.48[2] mas |
Distance | 450 ± 30 ly (138 ± 9 pc) |
Absolute magnitude (MV) | 5.87 ± 0.15[7] |
Details | |
Mass | 0.917 ± 0.030[7] M☉ |
Radius | 0.799 ± 0.039[7] R☉ |
Luminosity | 0.435 ± 0.053[7] L☉ |
Surface gravity (log g) | 4.58 ± 0.03[8] cgs |
Temperature | 5224 ± 69[8] K |
Metallicity [Fe/H] | 0.41 ± 0.08[8] dex |
Rotational velocity (v sin i) | 1.5 ± 1.0[8] km/s |
Age | 1.6 +2.9 −1.3[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HAT-P-3, is a metal-rich K star located about 450 light-years away in the constellation Ursa Major. At a magnitude of about 11.5 it is not visible to the naked eye but is visible in a small to medium-sized amateur telescope. It is believed to be a relatively young star and has a slightly enhanced level of chromospheric activity.[4][9]
Planetary system
This star is home to the extrasolar planet HAT-P-3b discovered by the HATNet Project using the transit method.[4]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | +0.021 −0.022 0.609 MJ |
99+0.00062 −0.00065 0.038 |
7360±0.0000020 2.899 | <0.0100 | 87.07 ± 0.55° | 0.827 ± 0.055 RJ |
See also
References
- ↑ Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Vizier query form
- 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
- 1 2 3 Droege, Thomas F.; et al. (2006). "TASS Mark IV Photometric Survey of the Northern Sky". The Publications of the Astronomical Society of the Pacific. 118 (850): 1666–1678. arXiv:astro-ph/0610529. Bibcode:2006PASP..118.1666D. doi:10.1086/510197. JSTOR 10.1086/510197. Vizier catalog entry
- 1 2 3 4 Torres, G.; et al. (2007). "HAT-P-3b: A Heavy-Element-rich Planet Transiting a K Dwarf Star". The Astrophysical Journal Letters. 666 (2): L121–L124. arXiv:0707.4268. Bibcode:2007ApJ...666L.121T. doi:10.1086/521792.
- 1 2 "TYC 3466-819-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-10-29.
- 1 2 3 Skrutskie, 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
- 1 2 3 4 5 6 Chan, Tucker; et al. (2011). "The Transit Light-curve Project. XIV. Confirmation of Anomalous Radii for the Exoplanets TrES-4b, HAT-P-3b, and WASP-12b". The Astronomical Journal. 141 (6). 179. arXiv:1103.3078. Bibcode:2011AJ....141..179C. doi:10.1088/0004-6256/141/6/179.
- 1 2 3 4 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.
- ↑ Todorov, Kamen O.; et al. (2013). "Warm Spitzer Photometry of Three Hot Jupiters: HAT-P-3b, HAT-P-4b and HAT-P-12b". The Astrophysical Journal. 770 (2). 102. arXiv:1305.0833. Bibcode:2013ApJ...770..102T. doi:10.1088/0004-637X/770/2/102.
- ↑ Bonomo, A. S.; et al. (2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics. 602. A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882.
External links
- "HAT-P-3". Exoplanets. Retrieved 2009-05-18.
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