HAT-P-8b
Exoplanet | List of exoplanets | |
---|---|---|
| ||
Parent star | ||
Star | GSC 02757-01152 | |
Constellation | Pegasus | |
Right ascension | (α) | 22h 52m 09.862s |
Declination | (δ) | +35° 26′ 49.59″ |
Apparent magnitude | (mV) | 10.17 |
Distance | 750 ± 50 ly (230 ± 15 pc) | |
Orbital elements | ||
Semi-major axis | (a) | 0.0487 ± 0.00026 AU |
Eccentricity | (e) | ~0 |
Orbital period | (P) | 3.07632 ± 0.000004 d |
Orbital speed | (υ) | 173 km/s |
Inclination | (i) | 87.5+1.9 −0.9° |
Time of transit | (Tt) | 2,454,437.67582 ± 0.00034 JD |
Physical characteristics | ||
Mass | (m) | 1.52+0.18 −0.16 MJ |
Radius | (r) | 1.5+0.08 −0.06 RJ |
Discovery information | ||
Discovery date | December 5, 2008 | |
Discoverer(s) | HATNet Project | |
Discovery method | Transit | |
Discovery status | Unpublished | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HAT-P-8b is an extrasolar planet located approximately 750 light years away in the constellation of Pegasus, orbiting the 10th magnitude star GSC 02757-01152. This planet was discovered by transit on December 5, 2008. Despite the designation as HAT-P-8b, it is the 11th planet discovered by the HATNet Project. The mass of the planet is 50% more than Jupiter while the radius is also 50% more than Jupiter. The mass of this planet is exact since the inclination of the orbit is known, typical for transiting planets. This is a so-called “hot Jupiter” because this Jupiter-like gas giant planet orbits in a really close torch orbit around the star, making this planet extremely hot (in the order of a thousand kelvins). The distance from the star is roughly 20 times smaller than that of Earth from the Sun, which places the planet roughly 8 times closer to its star than Mercury is from the Sun. The “year” on this planet lasts only 3 days, 1 hour, 49 minutes, and 54 seconds, compared with Earth's 365 days, 6 hours, 9 minutes, and 10 seconds in a sidereal year.[1]
See also
References
- ↑ Latham, David W.; et al. (2009). "Discovery of a Transiting Planet and Eight Eclipsing Binaries in HATNet Field G205". The Astrophysical Journal. 704 (2): 1107–1119. arXiv:0812.1161. Bibcode:2009ApJ...704.1107L. doi:10.1088/0004-637X/704/2/1107.
External links
Media related to HAT-P-8 b at Wikimedia Commons
- "HAT-P-8b light curve using differential photometry". Exoplanets.
- "HAT-P-8 b". Exoplanets.
Coordinates: 22h 52m 09.862s, +35° 26′ 49.59″