Publicated:
2 December 2021.
Authors:
K. W. F. Lam, Sz. Csizmadia, N. Astudillo-Defru et al.
Summary:
Ultra-short-period (USP) exoplanets have orbital periods shorter than one day. Precise masses and radii of USPs 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.
Here you can find the link to the paper on arXiv and here from the magazine Science.
