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Mars: Occurrence of Liquid Water

Ingersoll, Andrew P. (1970) Mars: Occurrence of Liquid Water. Science, 168 (3934). pp. 972-973. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20130219-094150339

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Abstract

In the absence of juvenile liquid water, condensation of water vapor to ice and subsequent melting of ice are the only means of producing liquid water on the martian surface. However, the evaporation rate is so high that the available heat sources cannot melt pure ice. Liquid water is therefore limited to concentrated solutions of strongly deliquescent salts.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.168.3934.972 DOIArticle
http://www.sciencemag.org/content/168/3934/972PublisherArticle
ORCID:
AuthorORCID
Ingersoll, Andrew P.0000-0002-2035-9198
Additional Information:© 1970 American Association for the Advancement of Science. Received 2 February 1969; revised 17 November 1969. Contribution No. 1614 of the Division of Geological Sciences, California Institute of Technology, Pasadena.
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological Sceinces1614
Issue or Number:3934
Record Number:CaltechAUTHORS:20130219-094150339
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130219-094150339
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36975
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Feb 2013 23:53
Last Modified:03 Oct 2019 04:43

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