September 09, 2022 updates Posted on September 9, 2022September 9, 2022 by Doug Loss Three types of planets orbit red dwarfs https://www.science.org/doi/10.1126/science.add7175 Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars https://www.science.org/doi/10.1126/science.abl7164 The Study of Atmosphere of Hot Jupiters and Their Host Stars https://arxiv.org/abs/2209.03669 Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudyhttps://arxiv.org/abs/2209.03677 Mass Production of 2021 KMTNet Microlensing Planets III: Analysis of Three Giant Planetshttps://arxiv.org/abs/2209.03886 CHEOPS finds KELT-1b darker than expected in visible light: Discrepancy between the CHEOPS and TESS eclipse depthshttps://arxiv.org/abs/2209.03890 A direct N-body integrator for modelling the chaotic, tidal dynamics of multi-body extrasolar systems: TIDYMESShttps://arxiv.org/abs/2209.03955