Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008a%26a...477..309p&link_type=abstract
Astronomy and Astrophysics, Volume 477, Issue 1, January I 2008, pp.309-314
Astronomy and Astrophysics
Astrophysics
33
Planetary Systems, Stars: Activity, X-Rays: Stars, Star: Coronae
Scientific paper
Aims:We investigate the influence of high-energy stellar radiation at close-in orbits on atmospheric mass loss during the stellar evolution of a G-type star. Methods: High-energy stellar luminosity varies over a wide range for G field stars. The X-ray luminosity distributions from the Pleiades, the Hyades, and the field are used to derive a scaling law for the evolution of the stellar X-ray luminosity distribution. A modified energy-limited escape approach is taken for calculating atmospheric mass loss for a broad range of planetary parameters. Results: We show that the evolution of close-in exoplanets strongly depends on the detailed X-ray luminosity history of their host stars, which varies over several orders-of-magnitude for G stars. Stars located in the high-energy tail of the luminosity distribution can evaporate most of its planets within 0.5 AU, while a significant fraction of planets can survive if exposed to a moderate X-ray luminosity. We show the change on an initial planetary mass distribution caused by atmospheric escape.
Lammer Helmut
Micela Giuseppina
Penz Thomas
No associations
LandOfFree
Influence of the evolving stellar X-ray luminosity distribution on exoplanetary mass loss does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Influence of the evolving stellar X-ray luminosity distribution on exoplanetary mass loss, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Influence of the evolving stellar X-ray luminosity distribution on exoplanetary mass loss will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1587811