V1005 Ori Archives

The magnetopause standoff distance of a planet orbiting our stellar sample. The theoretical decay of the Parker model (blue) and that measured in the solar system (red) are used in the estimations for Case 1 (left panels) and for Case 3, fast wind (right panels). In the upper (bottom) panels the planet is orbiting the outer (inner) radius of the HZ. The gray dashed line represents Earth’s early magnetosphere. The results of Vidotto et al. (2013) were added for comparison. -- astro-ph.SR

Habitable Zones, Imaging & Spectroscopy, Origin & Evolution of Life, Radiation, Space Weather & Heliophysics, Status Report

The Impact Of Stellar Winds And Tidal Locking Effects On The Habitability Of Earth-like Exoplanets Around M Dwarf Stars

by Keith CowingOctober 28, 2025October 28, 2025

We present an assessment of the effects of stellar wind magnetic and mechanical components on the habitability of Earth-like exoplanets orbiting the inner and outer radii of the habitable zone […]

V1005 Ori

The Impact Of Stellar Winds And Tidal Locking Effects On The Habitability Of Earth-like Exoplanets Around M Dwarf Stars

Complex Water Systems Revealed On Early Mars

An Accidental Impact Crater Discovery

The Nancy Grace Roman Space Telescope Coronagraph Community Participation Program

Unveiling Microbial Communities And Biogeochemical Cycles In Antarctic Colored Snow

NASA Spaceline Current Awareness List #1,217 21 September 2026 (Space Life Science Research Results)