Photochemical model of impact-produced lunar atmosphere

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dc.creatorBerezhnoi, A. A.
dc.creatorKlumov, B. A.
dc.date2002-01-31
dc.date.accessioned2026-07-07T02:02:35Z
dc.date.available2026-07-07T02:02:35Z
dc.descriptionThe Lunar Prospector mission detected hydrogen-containing compounds in the lunar polar regions. We have considered the comet hypothesis of the origin of polar volatiles on the Moon. In the present paper we use our model of a comet impact with photochemical processes to be included to estimate chemical composition of volatiles which can be captured by the cold traps.
dc.descriptionCurrent addreess of Dr. A.A. Berezhnoi is INAOE, Puebla, Mexico
dc.identifierhttps://arxiv.org/abs/astro-ph/0201546
dc.identifierhttp://arxiv.org/abs/astro-ph/0201546
dc.identifierProceedings of the Fourth International Conference on the Exploration and Utilisation of the Moon, p. 175 - 178, the Netherlands, Noordwijk, 10-14 July 2000
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4090
dc.subjectAstrophysics
dc.titlePhotochemical model of impact-produced lunar atmosphere
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