Water contents of Earth-mass planets around M dwarfs

By F. Tian, Shigeru Ida. 2015

140 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d588b275abfaabd5114c2b893462d79df221789f

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In Astronomy and Astrophysics

Citations in the corpus

Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs (2017, background): “The validity of this assumption can be debated, particularly for planets in the HZ of M dwarf stars, due to their high pre-main-sequence luminosity (Ramirez & Kaltengger 2014; Luger & Barnes 2015; Tian & Ida 2015), or atmospheric erosion due to high X-ray and UV fluxes (Airapetian et al. 2017).”
THE MUSCLES TREASURY SURVEY. I. MOTIVATION AND OVERVIEW (2016, background): “Recent works suggest that the influences of early evolution of low mass stars and XUV heating could lead to a bi-modal distribution of water fractions on Earth-mass planets in the HZ of M dwarfs (Tian & Ida 2015).”
ABIOTIC O2 LEVELS ON PLANETS AROUND F, G, K, AND M STARS: POSSIBLE FALSE POSITIVES FOR LIFE? (2015, background): “Luger & Barnes (2015) (see also Ramirez & Kaltenegger (2014) and Tian & Ida (2015)) have shown that because of the long, highly luminous, pre-main-sequence lifetime of M stars, planets orbiting within their habitable zones could lose most or all of their water early in their histories, with…”
How to Characterize Habitable Worlds and Signs of Life (2017, background): “…that are later located in the MS HZ receive stellar incident fluxes during the star’s initial pre-MS phase that exceed the runaway greenhouse threshold, and thus may lose a substantial part of the water initially delivered to them (Ramirez & Kaltenegger 2014, Luger & Barnes 2015, Tian & Ida 2015).”