Simulations show that a single-hemisphere, high-latitude-polarity-inversion magnetic topology on a moderately rotating M dwarf would produce mostly high-latitude CMEs and only mild CME-driven pressure enhancements at equatorial exoplanet orbits.
Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone
1 Pith paper cite this work. Polarity classification is still indexing.
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Pith paper citing it
abstract
Observations of highly irradiated gas giant exoplanets have shown helium escaping from their atmospheres. There is limited evidence for atmospheres on rocky exoplanets, perhaps because they have already escaped. We report spectroscopic observations of LHS 1140b, a rocky exoplanet that orbits in the habitable zone of a nearby low-mass star. The near-infrared transit spectra show absorption by helium escaping from the planet's atmosphere. Helium absorption is detected in 2024 but not in 2025, indicating time-variable atmospheric escape. We interpret these results as indicating an upper atmosphere dominated by helium and depleted in hydrogen, with other volatile species trapped at lower altitudes, consistent with atmospheric fractionation models. No helium absorption is detected for LHS 1140c, a smaller and more heavily irradiated exoplanet in the same system.
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Intense but Harmless: Exo-Space Weather Around an M Dwarf with a Single-Hemisphere Dynamo
Simulations show that a single-hemisphere, high-latitude-polarity-inversion magnetic topology on a moderately rotating M dwarf would produce mostly high-latitude CMEs and only mild CME-driven pressure enhancements at equatorial exoplanet orbits.