HAT-P-33
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Gemini[1] |
Right ascension | 07h 32m 44.2186s[2] |
Declination | +33° 50′ 06.115″[2] |
Apparent magnitude (V) | 11.188[3] |
Characteristics | |
Spectral type | late-F[3] |
Astrometry | |
Proper motion (μ) | RA: ±1.667 −1.140[2] mas/yr Dec.: ±1.660 −2.467[2] mas/yr |
Parallax (π) | 2.40 ± 0.63[2] mas |
Distance | approx. 1,400 ly (approx. 400 pc) |
Details | |
Mass | ±0.040 1.375[3] M☉ |
Radius | ±0.034 1.637[3] R☉ |
Luminosity | ±0.33 4.15[3] L☉ |
Surface gravity (log g) | ±0.01 4.15[3] cgs |
Temperature | ±88 6446[3] K |
Metallicity [Fe/H] | ±0.08 0.07[3] dex |
Rotational velocity (v sin i) | ±0.5 13.7[3] km/s |
Age | ±0.3 2.3[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HAT-P-33 (2MASS J07324421+335006, GSC 2461-00988) is a late-F dwarf star. It is orbited by a planet HAT-P-33b.[3] A search for a binary companion star using adaptive optics at the MMT Observatory was negative.[4]
Planetary system
The transiting hot Jupiter exoplanet orbiting HAT-P-33 was discovered by the HATNet Project in 2011. An effort to detect transit timing variations due to other planets found none.[5]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | +0.13 −0.12 0.72 MJ |
±0.0018 0.0505 | 47472±0.00000088 3.474 | +0.11 −0.096 0.180 |
+1.2 −1.3 88.2° |
+0.26 −0.20 1.87 RJ |
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 4 5 6 7 8 9 10 11 Hartman, J. D.; et al. (2011). "HAT-P-32b and HAT-P-33b: Two Highly Inflated Hot Jupiters Transiting High-jitter Stars". The Astrophysical Journal. 742 (1). 59. arXiv:1106.1212. Bibcode:2011ApJ...742...59H. doi:10.1088/0004-637X/742/1/59.
- ↑ 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.
- 1 2 Wang, Yong-Hao; et al. (2017). "Transiting Exoplanet Monitoring Project (TEMP). II. Refined System Parameters and Transit Timing Analysis of HAT-P-33b". The Astronomical Journal. 154 (2). 49. arXiv:1705.08605. Bibcode:2017AJ....154...49W. doi:10.3847/1538-3881/aa7519.
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