Trifonov, T, Caballero, JA, Morales, JC, Seifahrt, A, Ribas, I, Reiners, A, Bean, JL, Luque, R, Parviainen, H, Pallé, E, Stock, S, Zechmeister, M, Amado, PJ, Anglada-Escudé, G, Azzaro, M, Barclay, T, Béjar, VJS, Bluhm, P, Casasayas-Barris, N, Cifuentes, C, Collins, KA, Collins, KI, Cortés-Contreras, M, de Leon, J, Dreizler, S, Dressing, CD, Esparza-Borges, E, Espinoza, N, Fausnaugh, M, Fukui, A, Hatzes, AP, Hellier, C ORCID: https://orcid.org/0000-0002-3439-1439, Henning, T, Henze, CE, Herrero, E, Jeffers, SV, Jenkins, JM, Jensen, ELN, Kaminski, A, Kasper, D, Kossakowski, D, Kürster, M, Lafarga, M, Latham, DW, Mann, AW, Molaverdikhani, K, Montes, D, Montet, BT, Murgas, F, Narita, N, Oshagh, M, Passegger, VM, Pollacco, D, Quinn, SN, Quirrenbach, A, Ricker, GR, Rodríguez López, C, Sanz-Forcada, J, Schwarz, RP, Schweitzer, A, Seager, S, Shporer, A, Stangret, M, Stürmer, J, Tan, TG, Tenenbaum, P, Twicken, JD, Vanderspek, R and Winn, JN (2021) A nearby transiting rocky exoplanet that is suitable for atmospheric investigation. Science, 371 (6533). 1038 - 1041.

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Abstract

Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. We detect a transiting rocky planet with an orbital period of 1.467 days around the nearby red dwarf star Gliese 486. The planet Gliese 486 b is 2.81 Earth masses and 1.31 Earth radii, with uncertainties of 5%, as determined from RV data and photometric light curves. The host star is at a distance of ~8.1 parsecs, has a J-band magnitude of ~7.2, and is observable from both hemispheres of Earth. On the basis of these properties and the planet's short orbital period and high equilibrium temperature, we show that this terrestrial planet is suitable for emission and transit spectroscopy.

Item Type: Article
Additional Information: The final version of this accepted manuscript and all relevant information related to it, including copyrights, can be found online at; https://science.sciencemag.org/content/371/6533/1038
Subjects: Q Science > Q Science (General)
Q Science > QB Astronomy
Q Science > QB Astronomy > QB460 Astrophysics
Q Science > QB Astronomy > QB600 Planets. Planetology
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 30 Apr 2021 14:42
Last Modified: 30 Apr 2021 14:42
URI: https://eprints.keele.ac.uk/id/eprint/9477

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