Impacts of UV Radiation from an AGN on Planetary Atmospheres and Consequences for Galactic Habitability
Kendall I. Sippy, Jake K. Eager-Nash, Ryan C. Hickox, Nathan J. Mayne,, McKinley C. Brumback

TL;DR
This study investigates how ultraviolet radiation from active galactic nuclei affects planetary atmospheres and potential habitability, highlighting the protective role of atmospheric oxygen and the varying impact across galaxy types.
Contribution
It introduces a model analyzing AGN UV effects on planetary atmospheres and assesses the habitability implications across different galaxy environments.
Findings
Thicker ozone layers form with initial oxygen, reducing UV damage.
Compact galaxies like red nugget relics are more affected by AGN UV radiation.
Atmospheric composition influences planetary resilience to AGN UV exposure.
Abstract
We present a study of the effects of ultraviolet (UV) emission from active galactic nuclei (AGN) on the atmospheric composition of planets and potential impact on life. It is expected that all supermassive black holes, which reside at galactic centers, have gone through periods of high AGN activity in order to reach their current masses. We examine potential damaging effects on lifeforms on planets with different atmosphere types and receiving different levels of AGN flux, using data on the sensitivity of various species' cells to UV radiation to determine when radiation becomes "dangerous". We also consider potential chemical changes to planetary atmospheres as a result of UV radiation from AGN, using the PALEO photochemical model. We find the presence of sufficient initial oxygen (surface mixing ratio ) in the planet's atmosphere allows a thicker ozone…
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Taxonomy
TopicsAstro and Planetary Science
