SIMBAD references

2019MNRAS.485.5598O - Mon. Not. R. Astron. Soc., 485, 5598-5603 (2019/June-1)

Lessons from early Earth: UV surface radiation should not limit the habitability of active M star systems.

O'MALLEY-JAMES J.T. and KALTENEGGER L.

Abstract (from CDS):

The closest potentially habitable worlds outside our Solar system orbit a different kind of star than our Sun: smaller red dwarf stars. Such stars can flare frequently, bombarding their planets with biologically damaging high-energy UV radiation, placing planetary atmospheres at risk of erosion and bringing the habitability of these worlds into question. However, the surface UV flux on these worlds is unknown. Here we show the first models of the surface UV environments of the four closest potentially habitable exoplanets: Proxima-b, TRAPPIST-1e, Ross-128b, and LHS-1140b assuming different atmospheric compositions, spanning Earth-analogue to eroded and anoxic atmospheres and compare them to levels for Earth throughout its geological evolution. Even for planet models with eroded and anoxic atmospheres, surface UV radiation remains below early Earth levels, even during flares. Given that the early Earth was inhabited, we show that UV radiation should not be a limiting factor for the habitability of planets orbiting M stars. Our closest neighbouring worlds remain intriguing targets for the search for life beyond our Solar system.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): astrobiology - planets and satellites: atmospheres - planets and satellites: surfaces

Simbad objects: 11

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2019MNRAS.485.5598O and select 'bookmark this link' or equivalent in the popup menu


2021.06.23-23:54:48

© Université de Strasbourg/CNRS

    • Contact