
Judith Korth
Postdoc

GJ 367b : A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star
Author
Summary, in English
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.
Publishing year
2021-12-03
Language
English
Pages
1271-1275
Publication/Series
Science
Volume
374
Issue
6572
Document type
Journal article
Publisher
American Association for the Advancement of Science (AAAS)
Status
Published
ISBN/ISSN/Other
- ISSN: 0036-8075