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. 2021 Dec 3;374(6572):1271-1275.
doi: 10.1126/science.aay3253. Epub 2021 Dec 2.

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

Kristine W F Lam #  1   2 Szilárd Csizmadia #  2 Nicola Astudillo-Defru  3 Xavier Bonfils  4 Davide Gandolfi  5 Sebastiano Padovan  2   6 Massimiliano Esposito  7 Coel Hellier  8 Teruyuki Hirano  9 John Livingston  10 Felipe Murgas  11   12 Alexis M S Smith  2 Karen A Collins  13 Savita Mathur  11   12 Rafael A Garcia  14   15 Steve B Howell  16 Nuno C Santos  17   18 Fei Dai  19 George R Ricker  20 Roland Vanderspek  20 David W Latham  13 Sara Seager  20   21   22 Joshua N Winn  23 Jon M Jenkins  16 Simon Albrecht  24 Jose M Almenara  4 Etienne Artigau  4 Oscar Barragán  25 François Bouchy  26 Juan Cabrera  4 David Charbonneau  13 Priyanka Chaturvedi  7 Alexander Chaushev  1 Jessie L Christiansen  27 William D Cochran  28 José R De Meideiros  29 Xavier Delfosse  4 Rodrigo F Díaz  30 René Doyon  31 Philipp Eigmüller  2 Pedro Figueira  17   32 Thierry Forveille  4 Malcolm Fridlund  33   34 Guillaume Gaisné  4 Elisa Goffo  5   7 Iskra Georgieva  33 Sascha Grziwa  35 Eike Guenther  7 Artie P Hatzes  7 Marshall C Johnson  36 Petr Kabáth  37 Emil Knudstrup  24 Judith Korth  35   38 Pablo Lewin  39 Jack J Lissauer  16   40 Christophe Lovis  26 Rafael Luque  11   12 Claudio Melo  32 Edward H Morgan  20 Robert Morris  16   41 Michel Mayor  26 Norio Narita  11   42   43   44 Hannah L M Osborne  45 Enric Palle  11   12 Francesco Pepe  26 Carina M Persson  33 Samuel N Quinn  13 Heike Rauer  1   2   46 Seth Redfield  47 Joshua E Schlieder  48 Damien Ségransan  26 Luisa M Serrano  5 Jeffrey C Smith  16   41 Ján Šubjak  37   49 Joseph D Twicken  16   41 Stéphane Udry  26 Vincent Van Eylen  45 Michael Vezie  20
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Free article

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

Kristine W F Lam et al. Science. .
Free article

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.

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