Bibcode
Kuzuhara, Masayuki; Fukui, Akihiko; Livingston, John H.; Caballero, José A.; de Leon, Jerome P.; Hirano, Teruyuki; Kasagi, Yui; Murgas, Felipe; Narita, Norio; Omiya, Masashi; Orell-Miquel, Jaume; Palle, Enric; Changeat, Quentin; Esparza-Borges, Emma; Harakawa, Hiroki; Hellier, Coel; Hori, Yasunori; Ikuta, Kai; Ishikawa, Hiroyuki Tako; Kodama, Takanori; Kotani, Takayuki; Kudo, Tomoyuki; Morales, Juan C.; Mori, Mayuko; Nagel, Evangelos; Parviainen, Hannu; Perdelwitz, Volker; Reiners, Ansgar; Ribas, Ignasi; Sanz-Forcada, Jorge; Sato, Bun'ei; Schweitzer, Andreas; Tabernero, Hugo M.; Takarada, Takuya; Uyama, Taichi; Watanabe, Noriharu; Zechmeister, Mathias; Abreu García, Néstor; Aoki, Wako; Beichman, Charles; Béjar, Víctor J. S.; Brandt, Timothy D.; Calatayud-Borras, Yéssica; Carleo, Ilaria; Charbonneau, David; Collins, Karen A.; Currie, Thayne; Doty, John P.; Dreizler, Stefan; Fernández-Rodríguez, Gareb; Fukuda, Izuru; Galán, Daniel; Geraldía-González, Samuel; González-Garcia, Josafat; Hayashi, Yuya; Hedges, Christina; Henning, Thomas; Hodapp, Klaus; Ikoma, Masahiro; Isogai, Keisuke; Jacobson, Shane; Janson, Markus; Jenkins, Jon M.; Kagetani, Taiki; Kambe, Eiji; Kawai, Yugo; Kawauchi, Kiyoe; Kokubo, Eiichiro; Konishi, Mihoko; Korth, Judith; Krishnamurthy, Vigneshwaran; Kurokawa, Takashi; Kusakabe, Nobuhiko; Kwon, Jungmi; Laza-Ramos, Andrés; Libotte, Florence; Luque, Rafael; Madrigal-Aguado, Alberto; Matsumoto, Yuji; Mawet, Dimitri; McElwain, Michael W.; Meni Gallardo, Pedro Pablo; Morello, Giuseppe; Muñoz Torres, Sara; Nishikawa, Jun; Nugroho, Stevanus K.; Ogihara, Masahiro; Peláez-Torres, Alberto; Rapetti, David; Sánchez-Benavente, Manuel; Schlecker, Martin; Seager, Sara; Serabyn, Eugene; Serizawa, Takuma; Stangret, Monika; Takahashi, Aoi; Teng, Huan-Yu; Tamura, Motohide; Terada, Yuka; Ueda, Akitoshi et al.
Bibliographical reference
The Astrophysical Journal
Advertised on:
6
2024
Journal
Citations
3
Refereed citations
2
Description
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation is still small, limiting our ability to understand the diversity of the atmospheric composition and climates of temperate terrestrial planets. We report the discovery of an Earth-sized planet transiting the nearby (12 pc) inactive M3.0 dwarf Gliese 12 (TOI-6251) with an orbital period (P orb) of 12.76 days. The planet, Gliese 12 b, was initially identified as a candidate with an ambiguous P orb from TESS data. We confirmed the transit signal and P orb using ground-based photometry with MuSCAT2 and MuSCAT3, and validated the planetary nature of the signal using high-resolution images from Gemini/NIRI and Keck/NIRC2 as well as radial velocity (RV) measurements from the InfraRed Doppler instrument on the Subaru 8.2 m telescope and from CARMENES on the CAHA 3.5 m telescope. X-ray observations with XMM-Newton showed the host star is inactive, with an X-ray-to-bolometric luminosity ratio of $\mathrm{log}{L}_{{\rm{X}}}/{L}_{\mathrm{bol}}\approx -5.7$ . Joint analysis of the light curves and RV measurements revealed that Gliese 12 b has a radius of 0.96 ± 0.05 R ⊕, a 3σ mass upper limit of 3.9 M ⊕, and an equilibrium temperature of 315 ± 6 K assuming zero albedo. The transmission spectroscopy metric (TSM) value of Gliese 12 b is close to the TSM values of the TRAPPIST-1 planets, adding Gliese 12 b to the small list of potentially terrestrial, temperate planets amenable to atmospheric characterization with JWST.
Related projects

Very Low Mass Stars, Brown Dwarfs and Planets
Our goal is to study the processes that lead to the formation of low mass stars, brown dwarfs and planets and to characterize the physical properties of these objects in various evolutionary stages. Low mass stars and brown dwarfs are likely the most numerous type of objects in our Galaxy but due to their low intrinsic luminosity they are not so
Rafael
Rebolo López

Exoplanets and Astrobiology
The search for life in the universe has been driven by recent discoveries of planets around other stars (known as exoplanets), becoming one of the most active fields in modern astrophysics. The growing number of new exoplanets discovered in recent years and the recent advance on the study of their atmospheres are not only providing new valuable
Enric
Pallé Bago