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GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star

Lam, KWF; Csizmadia, S; Astudillo-Defru, N; Bonfils, X; Gandolfi, D; Padovan, S; Esposito, M; ... Vezie, M; + view all (2021) GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star. Science , 374 (6572) pp. 1271-1275. 10.1126/science.aay3253. Green open access

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Abstract

Ultrashort-period (USP) exoplanets have orbital periods shorter than 1 day. Precise masses and radii of USP exoplanets could provide constraints on their unknown formation and evolution processes. We report the detection and characterization of the USP planet GJ 367b using high-precision photometry and radial velocity observations. GJ 367b orbits a bright (V-band magnitude of 10.2), nearby, and red (M-type) dwarf star every 7.7 hours. GJ 367b has a radius of 0.718 ± 0.054 Earth-radii and a mass of 0.546 ± 0.078 Earth-masses, making it a sub-Earth planet. The corresponding bulk density is 8.106 ± 2.165 grams per cubic centimeter—close to that of iron. An interior structure model predicts that the planet has an iron core radius fraction of 86 ± 5%, similar to that of Mercury’s interior.

Type: Article
Title: GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star
Open access status: An open access version is available from UCL Discovery
DOI: 10.1126/science.aay3253
Publisher version: https://doi.org/10.1126/science.aay3253
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10141172
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