On the protection of extrasolar Earth-like planets around K/M stars against galactic cosmic rays
J.-M. Grie{\ss}meier (1, 2), A. Stadelmann (3), J. L. Grenfell (4, and 5), H. Lammer (6), U. Motschmann (3) ((1) LESIA, Observatoire de, Paris, Meudon, France, (2) Netherlands Institute for Radio Astronomy,, Dwingeloo, The Netherlands, (3) Technische Universit\"at Braunschweig,

TL;DR
This study investigates how the magnetic properties and composition of Earth-like exoplanets around M/K stars affect their protection against galactic cosmic rays, emphasizing the limited role of stellar wind variations.
Contribution
It demonstrates that planetary magnetic moment, influenced by mass and composition, is the key factor in cosmic ray shielding, rather than stellar wind effects.
Findings
Magnetic moment reduction weakens cosmic ray shielding.
Planetary mass alone does not guarantee better protection.
Composition significantly impacts magnetic shielding efficiency.
Abstract
Previous studies have shown that extrasolar Earth-like planets in close-in habitable zones around M-stars are weakly protected against galactic cosmic rays (GCRs), leading to a strongly increased particle flux to the top of the planetary atmosphere. Two main effects were held responsible for the weak shielding of such an exoplanet: (a) For a close-in planet, the planetary magnetic moment is strongly reduced by tidal locking. Therefore, such a close-in extrasolar planet is not protected by an extended magnetosphere. (b) The small orbital distance of the planet exposes it to a much denser stellar wind than that prevailing at larger orbital distances. This dense stellar wind leads to additional compression of the magnetosphere, which can further reduce the shielding efficiency against GCRs. In this work, we analyse and compare the effect of (a) and (b), showing that the stellar wind…
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