EUV-driven mass-loss of protoplanetary cores with hydrogen-dominated atmospheres: the influences of ionization and orbital distance

We investigate the loss rates of the hydrogen atmospheres of terrestrial planets with a range of masses and orbital distances by assuming a stellar extreme ultraviolet (EUV) luminosity that is 100 times stronger than that of the current Sun. We apply a 1D upper atmosphere radiation absorption and hy...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2016-08, Vol.460 (2), p.1300-1309
Hauptverfasser: Erkaev, N. V., Lammer, H., Odert, P., Kislyakova, K. G., Johnstone, C. P., Güdel, M., Khodachenko, M. L.
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Sprache:eng
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