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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…

地球与行星天体物理 · 物理学 2024-05-24 M. Kuzuhara , A. Fukui , J. H. Livingston , J. A. Caballero , J. P. de Leon , T. Hirano , Y. Kasagi , F. Murgas , N. Narita , M. Omiya , Jaume Orell-Miquel , E. Palle , Q. Changeat , E. Esparza-Borges , H. Harakawa , C. Hellier , Yasunori Hori , Kai Ikuta , H. T. Ishikawa , T. Kodama , T. Kotani , T. Kudo , J. C. Morales , M. Mori , E. Nagel , H. Parviainen , V. Perdelwitz , A. Reiners , I. Ribas , J. Sanz-Forcada , B. Sato , A. Schweitzer , H. M. Tabernero , T. Takarada , T. Uyama , N. Watanabe , M. Zechmeister , N. Abreu García , W. Aoki , C. Beichman , V. J. S. Béjar , T. D. Brandt , Y. Calatayud-Borras , I. Carleo , D. Charbonneau , K. A. Collins , T. Currie , J. P. Doty , S. Dreizler , G. Fernández-Rodríguez , I. Fukuda , D. Galán , S. Geraldía-González , J. González-Garcia , Y. Hayashi , C. Hedges , T. Henning , K. Hodapp , M. Ikoma , K. Isogai , S. Jacobson , M. Janson , J. M. Jenkins , T. Kagetani , E. Kambe , Y. Kawai , K. Kawauchi , E. Kokubo , M. Konishi , J. Korth , V. Krishnamurthy , T. Kurokawa , N. Kusakabe , J. Kwon , A. Laza-Ramos , F. Libotte , R. Luque , A. Madrigal-Aguado , Y. Matsumoto , D. Mawet , M. W. McElwain , P. P. Meni Gallardo , G. Morello , S. Mu~noz Torres , J. Nishikawa , S. K. Nugroho , M. Ogihara , A. Pel'aez-Torres , D. Rapetti , M. S'anchez-Benavente , M. Schlecker , S. Seager , E. Serabyn , T. Serizawa , M. Stangret , A. Takahashi , H. Teng , M. Tamura , Y. Terada , A. Ueda , T. Usuda , R. Vanderspek , S. Vievard , D. Watanabe , J. N. Winn , M. R. Zapatero Osorio

Small temperate planets are prime targets for exoplanet studies due to their possible similarities with the rocky planets in the Solar System. M dwarfs are promising hosts since the planetary signals are within our current detection…

M dwarf stars, which have masses less than 60 per cent that of the Sun, make up 75 per cent of the population of the stars in the Galaxy [1]. The atmospheres of orbiting Earth-sized planets are observationally accessible via transmission…

While JWST has provided us with the opportunity to probe the atmospheres of potentially-habitable planets, observations of the TRAPPIST-1 system have shown us that active stars severely complicate efforts at studying their planets. GJ 12b…

Gliese 436 is an M dwarf with a mass of 0.45 Msun and hosts the extrasolar planet GL 436b [3, 6, 7, 2], which is currently the least massive transiting planet with a mass of ~23.17 Mearth [10], and the only planet known to transit an M…

We report on the discovery of WASP-12b, a new transiting extrasolar planet with $R_{\rm pl}=1.79 \pm 0.09 R_J$ and $M_{\rm pl}=1.41 \pm 0.1 M_J$. The planet and host star properties were derived from a Monte Carlo Markov Chain analysis of…

In the age of JWST, temperate terrestrial exoplanets transiting nearby late-type M dwarfs provide unique opportunities for characterising their atmospheres, as well as searching for biosignature gases. We report here the discovery and…

We report the discovery of the transiting planet GJ 238 b, with a radius of $0.566\pm0.014$ R$_{\oplus}$ ($1.064\pm0.026$ times the radius of Mars) and an orbital period of 1.74 day. The transit signal was detected by the TESS mission and…

TOI-2285 b is a sub-Neptune-sized planet orbiting a nearby M dwarf, discovered through the TESS photometric survey and ground-based follow-up observations. The planet was initially reported to have an orbital period of 27.27 d, making it…

地球与行星天体物理 · 物理学 2025-05-29 Akihiko Fukui

One focus of modern astronomy is to detect temperate terrestrial exoplanets well-suited for atmospheric characterisation. A milestone was recently achieved with the detection of three Earth-sized planets transiting (i.e. passing in front…

We report the discovery of TrES-4, a hot Jupiter that transits the star GSC 02620-00648 every 3.55 days. From high-resolution spectroscopy of the star we estimate a stellar effective temperature of Teff = 6100 +/- 150 K, and from…

We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission. The host star is located $33$ pc away with a radius of…

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