HAT-P-12b

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 / Puli
Size comparison of HAT-P-12b with Jupiter.
Discovery
Discovered byHartman et al.
Discovery siteCambridge, Massachusetts
Discovery dateApril 29, 2009
Transit
Designations
Puli
Orbital characteristics
0.0384 ± 0.0003 AU (5,745,000 ± 45,000 km)
Eccentricity0 (assumed)
3.2130598 ± 0.0000021 d
Inclination89.0 ± 0.4
StarHAT-P-12
Physical characteristics
Mean radius
0.959 ± 0.029 RJ
Mass0.211 ± 0.012 MJ
Mean density
295 ± 25 kg/m3 (497 ± 42 lb/cu yd)

    HAT-P-12b is a H/He-dominated gas giant planet with a core mass of 11.3+2.6
    2.1
    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.

    In 2020, the obtained transmission spectra have revealed that the atmosphere of HAT-P-12b is cloudy, with haze above cloud tops. Water was detected. The prevalence of clouds and hazes in planetary atmosphere was disputed in 2021 though.

    In August 2022, this planet and its host star were included among 20 systems to be named by the third NameExoWorlds project. The approved names, proposed by a team from Hungary, were announced in June 2023. HAT-P-12b is named Puli and its host star is named Komondor, after the Hungarian Puli and Komondor dog breeds.

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