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dc.contributor.authorMuller, C.
dc.contributor.authorMoreau, D.
dc.date2001
dc.date.accessioned2017-05-04T09:31:05Z
dc.date.available2017-05-04T09:31:05Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5252
dc.descriptionThe radiative and chemical conditions at the surface in different Martian possible habitats are computed at various seasons combining a 2D photochemical model and radiation simulations. In most situations, the solar UV B and C radiations reach the surface however, a thin layer of deposited dust can constitute an effective UV shield, the protection presented by the atmosphere and airborne particles will also be characterized. This life favorable hypothesis is discussed for several Martian analogues.
dc.languageeng
dc.relation.ispartofseriesESA SP
dc.titleBiological role of Martian airborne and deposited dust
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleESA-SP 496: Proceedings of the First European Workshop on Exo-/astro-biology
dc.source.issue496
dc.source.page375-378
Orfeo.peerreviewedNo
dc.identifier.scopus2-s2.0-0034749166


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