Puli
Sign in to saveHAT-P-12b, formally named Puli, is an extrasolar planet approximately 468 light years away from Earth, orbiting the 13th magnitude K-type star HAT-P-12, which is located in Canes Venatici constellation. It is a transiting hot Jupiter that was discovered by the HATNet Project on April 29, 2009.
Key facts
- Planet.name
- HAT-P-12b / Puli
- Planet.image
- Clear to cloudy hot Jupiters.jpg
- Planet.caption
- Artist’s Impression of hot Jupiters (Puli is bottom left)
- Planet.discoverer
- Hartman et al.
- Planet.discovery_site
- Cambridge, Massachusetts
- Planet.discovered
- April 29, 2009
- Planet.discovery_method
- Transit
- Planet.alt_names
- Puli
- Planet.apsis
- astron
- Planet.eccentricity
- 0 (assumed)
- Planet.period
- 3.2130598 ± 0.0000021 d
- Planet.inclination
- 89.0 ± 0.4
- Planet.star
- HAT-P-12
- Planet.mean_radius
- 0.959 ± 0.029
- Planet.mass
- 0.211 ± 0.012
via Wikipedia infobox
Article
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HAT-P-12b, formally named Puli, is an extrasolar planet approximately 468 light years away from Earth, orbiting the 13th magnitude K-type star HAT-P-12, which is located in Canes Venatici constellation. It is a transiting hot Jupiter that was discovered by the HATNet Project on April 29, 2009.
HAT-P-12b is a H/He-dominated gas giant planet with a core mass of 11.3 M and is moderately irradiated by its low-metallicity host star. Therefore, HAT-P-12b is most likely an H/He-dominated planet with a core of perhaps ~10 M, and a total metal fraction of ~15%. This makes HAT-P-12b the least massive H/He-dominated gas giant planet found to date; the previous record holder was Saturn.