HAT-P-6b
| Exoplanet | List of exoplanets | |
|---|---|---|
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| Parent star | ||
| Star | HAT-P-6 | |
| Constellation | Andromeda | |
| Right ascension | (α) | 23h 39m 05.8061s |
| Declination | (δ) | +42° 27′ 57.513″ |
| Distance | approx. 650 ly (approx. 200 pc) | |
| Spectral type | F | |
| Orbital elements | ||
| Semi-major axis | (a) | 0.05235 ± 0.00087 AU |
| Periastron | (q) | 0.05235 AU |
| Apastron | (Q) | 0.05235 AU |
| Eccentricity | (e) | 0 |
| Orbital period | (P) | 3.852985 ± 5e-6 d (0.01054871 y) |
| Orbital speed | (υ) | 148.3 km/s |
| Time of transit | (Tt) | 2,454,035.67575 ± 0.00028 JD |
| Physical characteristics | ||
| Mass | (m) | 1.057 ± 0.119 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 | |
| Database references | ||
| Extrasolar Planets Encyclopaedia | data | |
| SIMBAD | data | |
| Exoplanet Archive | data | |
| Open Exoplanet Catalogue | data | |
HAT-P-6b is a transiting extrasolar planet[1] 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.
See also
References
- ↑ 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
Media related to HAT-P-6 b at Wikimedia Commons
- "HAT-P-6 b". Exoplanets.
Coordinates:
23h 39m 05.8061s, +42° 27′ 57.513″
This article is issued from Wikipedia - version of the Friday, December 19, 2014. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.
