The Mg I line: a new probe of the atmospheres of evaporating exoplanets

被引:22
作者
Bourrier, V. [1 ,2 ,3 ]
des Etangs, A. Lecavelier [1 ,2 ]
Vidal-Madjar, A. [1 ,2 ]
机构
[1] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France
[2] Univ Paris 06, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France
[3] Observ Univ Geneve, CH-1290 Sauverny, Switzerland
关键词
surveys; planets and satellites: atmospheres; methods: numerical; HOT JUPITERS; HD; 209458B; MASS-LOSS; STAR; ABSORPTION; HD209458B; RADIATION; MAGNESIUM; EXOSPHERE; TRANSITS;
D O I
10.1051/0004-6361/201323266
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Transit observations of HD 209458b in the UV revealed signatures of neutral magnesium escaping the planet's upper atmosphere. The absorption detected in the Mg I line provides unprecedented information on the physical conditions at the altitude where the atmospheric blow-off takes place. Here we use a 3D model of atmospheric escape to estimate the transit absorption signatures in the Mg I line of their host stars. The detectability of these signatures depends on the brightness of the star and the escape rate of neutral magnesium. We identify a sample of potentially evaporating exoplanets that covers a wide range of stellar and planetary properties, and whose extended exospheres might be detected through Mg I line observations with current UV facilities, allowing further steps in comparative exoplanetology.
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页数:4
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