The evaporation of planetary atmospheres

0585506 - ASÚ 2025 RIV SK eng J - Článek v odborném periodiku
Guenther, E.W. - Fossati, L. - Kabáth, Petr
The evaporation of planetary atmospheres.
Contributions of the Astronomical Observatory Skalnaté Pleso. Roč. 54, č. 2 (2024), s. 157-163. ISSN 1335-1842. E-ISSN 1336-0337
Institucionální podpora: RVO:67985815
Klíčová slova: planet * atmosphere * star
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 0.5, rok: 2022
Způsob publikování: Open access

In recent years the focus of exoplanet research has shifted from the mere detection to detailed characterization. Precise measurements of the masses and radii of transiting planets have shown that some low-mass planets have extended atmospheres while others are bare rocks. Hybrid atmospheres consisting of a mixture of Hydrogen and large amount of heavy elements have also been detected. A key factor in explaining this diversity of planetary atmospheres is the erosion by the X-ray and EUV-radiation (XUV) from the host-star. The evaporation through XUV-radiation has already been measured for a few exoplanets.The apparent weakness of the Ca II HK and the Mg II h&k emission cores has been interpreted as evidence for the evaporation of planetary atmospheres. The interpretation is that the evaporating material from the planet forms a thick torus which absorbs the Ca II HK and the Mg II h&k lines from the host star. In this contribution a new way how to prove, or disprove this hypothesis by observations is proposed. It is furthermore shown that there are enough bright targets already known that can be observed, and more will be found with the PLATO mission.
Trvalý link: https://hdl.handle.net/11104/0353189