Skip to main content
SearchLogin or Signup

EUV influences on exoplanet atmospheric stability and evolution

Published onMay 31, 2019
EUV influences on exoplanet atmospheric stability and evolution
·

Abstract

EUV photons (100-912 Å) drive atmospheric mass loss, and an accurate accounting of the EUV in a planet's energy budget is essential. Direct EUV observations of exoplanet host stars would require a new, dedicated observatory. Archival observations from EUVE and models are insufficient to accurately characterize EUV spectra of exoplanet host stars.

The full text of this article is only available in PDF format:



Comments
0
comment

No comments here