HD 102272 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 102272 | |
Constellation | Leo | |
Right ascension | (α) | 11h 46m 23.5351s[1] |
Declination | (δ) | +14° 07′ 26.350″[1] |
Apparent magnitude | (mV) | 8.71[1] |
Distance | 1200±300 ly (360±90[2] pc) | |
Spectral type | K0[3] | |
Orbital elements | ||
Semi-major axis | (a) | 0.614 ± 0.001[3] AU |
Eccentricity | (e) | 0.05 ± 0.04[3] |
Orbital period | (P) | 127.58 ± 0.30[3] d |
Argument of periastron |
(ω) | 118 ± 58[3]° |
Time of periastron | (T0) | 2452146 ± 64[3] JD |
Semi-amplitude | (K) | 155.5 ± 5.6[3] m/s |
Physical characteristics | ||
Mass | (m) | >5.9 ± 0.2[3] MJ |
Discovery information | ||
Discovery date | 18 June 2008 | |
Discoverer(s) | Niedzielski et al. | |
Discovery method | Radial velocity | |
Discovery site | McDonald Observatory, USA | |
Discovery status | Published[3] |
HD 102272 b is an extrasolar planet approximately 1,200 light-years away in the constellation of Leo. The planet was discovered orbiting the K-type giant star HD 102272 in 2008. The planet was discovered by the radial velocity method, using the Hobby-Eberly Telescope. Another planet, HD 102272 c, was also discovered orbiting the same star. The discovery was announced in June 2008. HD 102272 b orbits at an average of 0.614 astronomical units away from its star, with a mass at least 5.9 ± 0.2 times that of Jupiter.[3]
See also
References
- 1 2 3 HD 102272, entry, SIMBAD. Accessed on line June 18, 2008.
- ↑ "Notes for star HD 102272". The Extrasolar Planets Encyclopaedia. Retrieved 2008-07-01.
- 1 2 3 4 5 6 7 8 9 10 Niedzielski, A.; et al. (2009). "A Planet in a 0.6 AU Orbit Around the K0 Giant HD 102272". The Astrophysical Journal 693 (1): 276–280. arXiv:0810.1710. Bibcode:2009ApJ...693..276N. doi:10.1088/0004-637X/693/1/276.
External links
- "Notes for planet HD 102272 b". The Extrasolar Planets Encyclopaedia. Retrieved 2008-07-01.
- "HD 102272 b". Exoplanets. Retrieved 2008-11-09.
Coordinates: 11h 46m 23.5351s, +14° 07′ 26.350″
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