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  • 21 Aug, 2019

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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 is a H/He-dominated gas giant planet with a core mass of 11.3
−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.

Comparison of "hot Jupiter" exoplanets (artist concept).
From top left to lower right: WASP-12b, WASP-6b, WASP-31b, WASP-39b, HD 189733b, HAT-P-12b, WASP-17b, WASP-19b, HAT-P-1b and HD 209458b.

References

  1. ^ Hartman, J. D.; et al. (2009). "HAT-P-12b: A Low-density sub-Saturn mass planet transiting a metal-poor K dwarf". The Astrophysical Journal. 706 (1): 785–796. arXiv:0904.4704. Bibcode:2009ApJ...706..785H. doi:10.1088/0004-637X/706/1/785. S2CID 14540643.
  2. ^ "2022 Approved Names". nameexoworlds.iau.org. IAU. Retrieved 7 June 2023.
  3. ^ Lee, Jae Woo; Youn, Jae-Hyuck; Kim, Seung-Lee; Lee, Chung-Uk; Hinse, Tobias Cornelius (2012). "THE SUB-SATURN MASS TRANSITING PLANET HAT-P-12b". The Astronomical Journal. 143 (4): 95. arXiv:1201.6419. Bibcode:2012AJ....143...95L. doi:10.1088/0004-6256/143/4/95. S2CID 118610109.
  4. ^ Yan, F.; Espinoza, N.; Molaverdikhani, K.; Henning, Th.; Mancini, L.; Mallonn, M.; Rackham, B. V.; Apai, D.; Jordán, A.; Mollière, P.; Chen, G.; Carone, L.; Reiners, Ansgar (2020), "LBT transmission spectroscopy of HAT-P-12b: confirmation of a cloudy atmosphere with no significant alkali features", Astronomy & Astrophysics, A98: 642, arXiv:2007.15485, Bibcode:2020A&A...642A..98Y, doi:10.1051/0004-6361/201937265, S2CID 220870755
  5. ^ Wong, Ian; Benneke, Björn; Gao, Peter; Knutson, Heather A.; Chachan, Yayaati; Henry, Gregory W.; Deming, Drake; Kataria, Tiffany; Lee, Graham K. H.; Nikolov, Nikolay; Sing, David K.; Ballester, Gilda E.; Baskin, Nathaniel J.; Wakeford, Hannah R.; Williamson, Michael H. (2020). "Optical to near-infrared transmission spectrum of the warm sub-Saturn HAT-P-12b". The Astronomical Journal. 159 (5): 234. arXiv:2004.03551. Bibcode:2020AJ....159..234W. doi:10.3847/1538-3881/ab880d. S2CID 215238620.
  6. ^ Jiang, C.; Chen, G.; Pallé, E.; Murgas, F.; Parviainen, H.; Yan, F.; Ma, Y. (2021), "Evidence for stellar contamination in the transmission spectra of HAT-P-12b", Astronomy & Astrophysics, 656: A114, arXiv:2109.11235, Bibcode:2021A&A...656A.114J, doi:10.1051/0004-6361/202141824, S2CID 237604976
  7. ^ "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.

Media related to HAT-P-12b at Wikimedia Commons


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