The high-energy radiation environment around a 10 Gyr M dwarf: habitable at last?

The high-energy radiation environment around a 10 Gyr M dwarf: habitable at last?

Recent work has demonstrated that high levels of X-ray and UV activity on young M dwarfs may drive rapid atmospheric escape on temperate, terrestrial planets orbiting within the habitable zone. However, secondary atmospheres on planets orbiting older, less active M dwarfs may be stable and present m...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: France, K, Duvvuri, G, Egan, H, Koskinen, T, Wilson, DJ, Youngblood, A, Froning, CS, Brown, A, Alvarado-Gomez, J, Berta-Thompson, ZK, Drake, JJ, Garraffo, C, Kaltenegger, L, Kowalski, AF, Linsky, JL, Loyd, ROP, Mauas, PJD, Miguel, Y, Pineda, JS, Rugheimer, S, Schneider, PC, Tian, F, Vieytes, M
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: American Astronomical Society 2020

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