The habitability of planets orbiting M-dwarf stars - eScholarship
Abstract Planetary material accreted by white dwarfs provides critical insights re- garding the composition of planetary material. The analysis of polluted ...
GAUSS - genesis of asteroids and evolution of the solar systemExoplanet searches have found that roughly half of all Sun-like stars have one or more planets with radii of 1?4 Earth radii and orbital periods. Planets and AstrobiologyThe atmospheric substellar absorption of M-dwarf radiation on an Earth-like planet is stronger than for F- or G-dwarf instellation (Shields ... The Habitability of Planets Orbiting M-dwarf Stars - SciSpaceFrom our joint analysis, we found the host TOI-6894 to be a M5. 0 ± 0.5 dwarf star with a radius of 0.2276 ± 0.0057 R? and a mass of 0.207 ± 0.011 M?, a very ...
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