HAT-P-9
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 07h 20m 40.4565s[1] |
Declination | +37° 08′ 26.343″[1] |
Apparent magnitude (V) | 12.34 ± 0.27[2] |
Characteristics | |
Spectral type | F[3] |
Apparent magnitude (B) | 12.35 ± 0.23[2] |
Apparent magnitude (V) | 12.34 ± 0.27[2] |
Apparent magnitude (J) | 11.274 ± 0.022[2] |
Apparent magnitude (H) | 11.04 ± 0.03[2] |
Apparent magnitude (K) | 11.015 ± 0.021[2] |
Variable type | planetary transit[3] |
Astrometry | |
Radial velocity (Rv) | 20.69±2.27[1] km/s |
Proper motion (μ) | RA: −9.796 mas/yr[1] Dec.: −13.029 mas/yr[1] |
Parallax (π) | 2.1626±0.0140 mas[1] |
Distance | 1,508 ± 10 ly (462 ± 3 pc) |
Details | |
Mass | 1.281+0.057 −0.056[4] M☉ |
Radius | 1.338+0.065 −0.060[4] R☉ |
Luminosity | 2.62+0.26 −0.23[4] L☉ |
Surface gravity (log g) | 4.293+0.033 −0.035[4] cgs |
Temperature | 6253 ± 84[5] K |
Metallicity [Fe/H] | 0.16 ± 0.09[5] dex |
Rotational velocity (v sin i) | 13.4 ± 1.4[5] km/s |
Age | 1.6+1.8 −1.4[6] Gyr |
Other designations | |
Tevel, TOI-1731, TIC 371234684, TYC 2463-281-1, GSC 02463-00281, 2MASS J07204044+3708263, HAT-P-9[2] | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HAT-P-9 is a magnitude 12 F-type star approximately 1500 light-years away in the constellation Auriga.[2] A search for a binary companion star using adaptive optics at the MMT Observatory was negative.[7]
Naming
[edit]The star HAT-P-9 is named Tevel. The name was selected in the NameExoWorlds campaign by Israel, during the 100th anniversary of the IAU. The Hebrew word תֵבֵל tevel means "World" or "Universe".[8][9]
Planetary system
[edit]An exoplanet orbiting the star, HAT-P-9b, was discovered by the transit method on June 26, 2008. This is a low-density hot Jupiter, orbiting its star in just 3.9 days.[3]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b / Alef | 0.749+0.064 −0.063 MJ |
0.05287±0.00078 | 3.92281072(102) | 0.084+0.052 −0.047 |
86.44+0.37 −0.36° |
1.393+0.067 −0.065 RJ |
See also
[edit]References
[edit]- ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b c d e f g h "SIMBAD query result: TYC 2463-281-1 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-18.
- ^ a b c Shporer, Avi; et al. (2009). "HAT-P-9b: A Low-Density Planet Transiting a Moderately Faint F Star". The Astrophysical Journal. 690 (2): 1393–1400. arXiv:0806.4008. Bibcode:2009ApJ...690.1393S. doi:10.1088/0004-637X/690/2/1393. S2CID 930937.
- ^ a b c d e Wang, Yong-Hao; Wang, Songhu; et al. (February 2019). "Transiting Exoplanet Monitoring Project (TEMP). V. Transit Follow Up for HAT-P-9b, HAT-P-32b, and HAT-P-36b". The Astronomical Journal. 157 (2): 82. Bibcode:2019AJ....157...82W. doi:10.3847/1538-3881/aaf6b6.
- ^ a b c 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. S2CID 16580774.
- ^ Bonomo, A. S.; Desidera, S.; et al. (June 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 & Astrophysics. 602: A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. S2CID 118923163.
- ^ Adams, E. R.; et al. (2013). "Adaptive Optics Images. II. 12 Kepler Objects of Interest and 15 Confirmed Transiting Planets". The Astronomical Journal. 146 (1). 9. arXiv:1305.6548. Bibcode:2013AJ....146....9A. doi:10.1088/0004-6256/146/1/9. S2CID 119117620.
- ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
- ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
External links
[edit]- Image HAT-P-9
- "HAT-P-9". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-05-18.