Nature Astronomy, Published online: 12 April 2024; doi:10.1038/s41550-024-02252-5

An outstanding discrepancy between observations and models of stellar limb darkening is resolved here by the inclusion of stellar surface magnetism in models. This will enable an improved characterization of transiting exoplanets.

—————
Free Secure Email – Transcom Sigma
Transcom Hosting
Transcom Premium Domains