Water Loss from Young Planets

Autor(en)
Feng Tian, Manuel Güdel, Colin P. Johnstone, Helmut Lammer, Rodrigo Luger, Petra Odert
Abstrakt

Good progress has been made in the past few years to better understand the XUV evolution trend of Sun-like stars, the capture and dissipation of hydrogen dominant envelopes of planetary embryos and protoplanets, and water loss from young planets around M dwarfs. This chapter reviews these recent developments. Observations of exoplanets and theoretical works in the near future will significantly advance our understanding of one of the fundamental physical processes shaping the evolution of solar system terrestrial planets.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Tsinghua University, Österreichische Akademie der Wissenschaften (ÖAW), University of Washington
Journal
Space Science Reviews
Band
214
Anzahl der Seiten
19
ISSN
0038-6308
DOI
https://doi.org/10.1007/s11214-018-0490-9
Publikationsdatum
04-2018
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/9b852b9b-e66c-402f-bdd3-915715d82146