Moderately misaligned orbit of the warm sub-Saturn HD 332231 b
Measurements of exoplanetary orbital obliquity angles for different classes of planets are an essential tool in testing various planet formation theories. Measurements for those transiting planets on relatively large orbital periods (P > 10 d) present a rather difficult observational challenge. Here we present the obliquity measurement for the warm
Sedaghati, E. et al.
Fecha de publicación:
3
2022