Assessments for possible habitability in Martian polar environments: Fundaments based in ice screening of UV radiation

C Cordoba-Jabonero* (Corresponding Author), MR Patel, MP Zorzano, CS Cockell, RA Harris (Editor), L Ouwehand (Editor)

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

We present a study of the solar UV radiation in Martian high latitude environments covered by ice, where the UV propagation through the polar cover depends on the ice radiative properties (layers of H2O or CO2 ice). But also we will investigate the changes in the subsurface UV levels induced by the seasonal variations of solar UV flux on the surface, as well as by the seasonal freezing-thawing and related CO2 sublimation processes. The biological dose relative to DNA-damage will be also estimated for biological implication assessments. All these studies will be compared with the biological dose received in the Antarctic snow-ice covered environment which is seasonally exposed to high UV radiation levels (formation of "ozone hole"), where the environmental conditions could be similar to those present on Mars (Cockell et al., 2002; Cockell and Córdoba-Jabonero, 2004).
Original languageEnglish
Title of host publicationProceedings of the III European Workshop on Exo-Astrobiology
Subtitle of host publicationMars: The Search for Life
EditorsR. A. Harris, L. Ouwehand
Place of PublicationNoordwijk, Netherlands
PublisherESA Publications Division
Pages187-188
Number of pages2
ISBN (Print)92-9092-856-5
Publication statusPublished - 2004
EventThe Third European Workshop on Exo-Astrobiology - Madrid, Spain
Duration: 18 Nov 200320 Nov 2003

Conference

ConferenceThe Third European Workshop on Exo-Astrobiology
Country/TerritorySpain
CityMadrid
Period18/11/0320/11/03

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