Astronomy:HD 102272 b
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Discovery | |
---|---|
Discovered by | Niedzielski et al. |
Discovery site | McDonald Observatory, United States |
Discovery date | 18 June 2008 |
Radial velocity | |
Orbital characteristics | |
0.614 ± 0.001 AU (91,850,000 ± 150,000 km)[1] | |
Eccentricity | 0.05 ± 0.04[1] |
Orbital period | 127.58 ± 0.30[1] d |
astron|astron|helion}} | 2452146 ± 64[1] |
118 ± 58[1] | |
Semi-amplitude | 155.5 ± 5.6[1] |
Star | HD 102272 |
Physical characteristics | |
Mass | >5.9 ± 0.2[1] |♃|J}}}}}} |
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.[1]
See also
References
External links
- "Notes for planet HD 102272 b". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/hd_102272_b--485/. Retrieved 2008-07-01.
- "HD 102272 b". Exoplanets. http://media4.obspm.fr/exoplanets/base/planete.php?etoile=HD+102272&planete=b. Retrieved 2008-11-09.
Coordinates: 11h 46m 23.5351s, +14° 07′ 26.350″
Original source: https://en.wikipedia.org/wiki/HD 102272 b.
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