How Hospitable Are Space Weather Affected Habitable Zones? The Role of Ion Escape

Atmospheres of exoplanets in the habitable zones around active young G-K-M stars are subject to extreme X-ray and EUV (XUV) fluxes from their host stars that can initiate atmospheric erosion. Atmospheric loss affects exoplanetary habitability in terms of surface water inventory, atmospheric pressure...

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Veröffentlicht in:	Astrophysical journal. Letters Jg. 836; H. 1; S. L3
Hauptverfasser:	Airapetian, Vladimir S., Glocer, Alex, Khazanov, George V., Loyd, R. O. P., France, Kevin, Sojka, Jan, Danchi, William C., Liemohn, Michael W.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Goddard Space Flight Center The American Astronomical Society 10.02.2017 The American Astonomical Society
Schlagworte:	Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Atmospheric models Atmospherics COSMIC X-RAY BURSTS COSMIC X-RAY SOURCES EROSION Extrasolar planets EXTREME ULTRAVIOLET RADIATION Geophysics GREENHOUSES HARD X RADIATION HYDRODYNAMICS HYDROGEN IRRADIATION MAGNETIC FIELDS NITROGEN Oxygen OXYGEN IONS Planetary atmospheres PLANETS planets and satellites: atmospheres planets and satellites: magnetic fields radiation mechanisms: general Red dwarf stars SATELLITE ATMOSPHERES SATELLITES SPACE STARS stars: activity stars: late-type Stellar atmospheres SURFACES VOLCANISM Planets And Satellites Hydrodynamics Radiation Mechanisms Atmospheres Magnetic Fields Stars
ISSN:	2041-8205, 2041-8213
Online-Zugang:	Volltext
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