The time evolution of the ultraviolet habitable zone
R. Spinelli, F. Borsa, G. Ghirlanda, G. Ghisellini, F. Haardt, F., Rigamonti

TL;DR
This study explores how the ultraviolet habitable zone around stars evolves over time and intersects with the circumstellar habitable zone, highlighting implications for the potential emergence of life on exoplanets, especially around M-dwarfs.
Contribution
It provides the first analysis of the time evolution of the ultraviolet habitable zone and its intersection with the habitable zone using observational data and stellar models.
Findings
Intersection of CHZ and UHZ varies over time for different stars.
Hotter M-dwarfs have longer periods where UHZ and CHZ overlap.
Proxima Centauri shows a prolonged CHZ-UHZ intersection, making it a prime target.
Abstract
For stars hosting Circumstellar Habitable Zone (CHZ) exoplanets, we investigate the time-evolution of their ultraviolet habitable zone (UHZ), the annular region around a star where an exoplanet could experience a suitable ultraviolet environment for the presence and emergence of life, and the possible intersection of the UHZ with the CHZ. To estimate their UV luminosity evolution, and therefore the evolution of their UHZ, we analyse Swift-UV/Optical telescope observations and adopt the near-UV luminosity evolutionary tracks derived using GALEX observations of young moving groups. We find that an intersection between CHZ and UHZ could exist (or have existed) around all stars of our sample at different epochs, except for the coldest M-dwarfs (temperature < 2800 K, e.g. Trappist-1). For hotter M-dwarfs the formation of RNA precursors through cyanosulfidic chemistry triggered by near-UV…
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