HAT-P-6b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HAT-P-6 | |
Constellation | Andromeda[1] | |
Right ascension | (α) | 23h 39m 05.8108s[2] |
Declination | (δ) | +42° 27′ 57.502″[2] |
Distance | ±90 910[2] ly (±30 280[2] pc) | |
Spectral type | F | |
Orbital elements | ||
Semi-major axis | (a) | 39+0.00080 −0.00082 0.052[3] AU |
Eccentricity | (e) | <0.044[3] |
Orbital period | (P) | 985±0.000005 3.852[4] d |
Time of transit | (Tt) | 454035.67575±0.00028 2[4] JD |
Physical characteristics | ||
Mass | (m) | +0.039 −0.040 1.106[3] MJ |
Radius | (r) | 1.33 ± 0.061 RJ |
Density | (ρ) | 450 kg m−3 |
Discovery information | ||
Discovery date | October 15, 2007 | |
Discoverer(s) | Noyes et al. | |
Discovery method | transit | |
Discovery status | Published[4] | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HAT-P-6b is a transiting extrasolar planet[4] located approximately 650 light-years away in the constellation of Andromeda, orbiting the star HAT-P-6. This hot Jupiter planet orbits with a semi-major axis of about 7.832 gigameters, and takes 92 hours, 28 minutes, 17 seconds and 9 deciseconds to orbit the star. It has true mass of 5.7% greater than Jupiter and a radius 33% greater than Jupiter, corresponding to a density of 0.45 g/cm3, which is less than water. This planet was found by Noyes et al. on October 15, 2007.
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 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 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.
- 1 2 3 4 Noyes, R. W.; et al. (2008). "HAT-P-6b: A Hot Jupiter Transiting a Bright F Star". The Astrophysical Journal Letters. 673 (1): L79–L82. arXiv:0710.2894. Bibcode:2008ApJ...673L..79N. doi:10.1086/527358.
External links
- "HAT-P-6 b". Exoplanets.
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