Image Details
Caption: Figure 3.
Predicted RV amplitude for a Mars-mass exoplanet as a function of incident flux, where the vertical dotted line indicates the incident flux for Mars (∼0.43 F⊕). The calculations are shown for host stars with a mass of 0.3, 0.7, and 1.0 M⊕.
© 2026. The Author(s). Published by the American Astronomical Society.