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Neutral atmospheric escape in the Solar and extrasolar planetary systems

Published online by Cambridge University Press:  13 January 2020

Dmitry V. Bisikalo  and
Valery I. Shematovich Open the ORCID record for Valery I. Shematovich [Opens in a new window]
Dmitry V. Bisikalo
Affiliation:
Institute of astronomy RAS, Moscow, Russia email: bisikalo@inasan.ru
Valery I. Shematovich*
Affiliation:
Institute of astronomy RAS, Moscow, Russia email: shematov@inasan.ru
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Abstract

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New data obtained by space missions to various objects in the Solar system and observations of the outer Solar system and exoplanets by space and ground-based telescopes allowed us to conclude that the atmospheric escape plays an important role in the evolution of the terrestrial planets in the Solar system. We present the recent results of application of the kinetic approach to the problem of neutral escape from planetary atmospheres. As an example, the recent measurements by Mars Express and MAVEN spacecraft are compared with the calculations of neutral escape with the aim to understand the atmospheric loss at Mars. Also the recent calculations of the mass-loss rates of the hot Neptune and Jupiter atmospheres are presented.

Keywords

stars: flareplanets and satellites: formationultraviolet: solar systemetc
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 168 - 171
Copyright
© International Astronomical Union 2020 

References

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