P007
Cool Stars and Their Influence on (Exo)Planetary Habitability

Session ID#: 158764

Session Description:
The presence of strong stellar winds and/or extreme stellar particle events as well as coronal mass ejections may destroy atmospheric biosignatures and could prevent the creation and development of life. Thus, detailed knowledge of the astrospheric particle- and radiation environment and its impact on exoplanetary atmospheres is mandatory to study exoplanetary habitability.

The session brings together scientists from all fields of research that are related to solar, astrophysical, and exoplanetary sciences. It will allow the sharing of expertise amongst researchers working on different aspects of this interdisciplinary scientific field, allowing showcases of recent advancements in the field of specialization. The session aims to stimulate discussions on how individual disciplines can share their knowledge and benefit from each other.

We solicit contributions related but not limited to:

  • Modeling stellar astrospheres and the corresponding energy-dependent CR flux
  • Modeling the environment of close-in exoplanets around cool stars, in particular, modeling of mass-loss rates, angular momentum loss rates, the magnetic field configuration and the density and velocity of the stellar winds of G-, K- and M-stars
  • Modeling stellar CMEs
  • Evaluation and quantification of the solar UV-, X-ray, and energetic particle flux relationships and their extension to G-, K-, and M-dwarfs
  • The imprint of the stellar radiation field by modeling the magnetospheric transport and particle interactions within (exo)planetary atmospheres
  • Atmospheric modeling studies of climate and (biosignature) photochemistry and the influence of stellar activity
Index Terms:

2104 Cosmic rays [INTERPLANETARY PHYSICS]
5210 Planetary atmospheres, clouds, and hazes [PLANETARY SCIENCES: ASTROBIOLOGY]
6296 Extra-solar planets [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
7984 Space radiation environment [SPACE WEATHER]


Primary Convener:  Konstantin Herbst, University of Kiel, Kiel, Germany
Conveners:  L Grenfell, German Aerospace Center DLR Berlin, Institute of Planetary Research, Berlin, Germany and Athanasios Papaioannou, National Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, Athens, Greece
 
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