Global warming and climate forcing by recent albedo changes on Mars
Lori K. Fenton (),
Paul E. Geissler () and
Robert M. Haberle
Additional contact information
Lori K. Fenton: Carl Sagan Center,
Paul E. Geissler: US Geological Survey, Flagstaff, Arizona 86001, USA
Robert M. Haberle: NASA Ames Research Center, Moffett Field, California 94035, USA
Nature, 2007, vol. 446, issue 7136, 646-649
Abstract:
Shadow dancing on Mars The surface albedo patterns on Mars, caused by local variation in the ratio of light reflected to light received, are constantly changing. A Mars global circulation model has been used to establish whether these changes contribute to climate change, and the answer is yes. Large swaths of the martian surface have darkened over the past three decades as they were swept free of dust. Climate modelling indicates that these changes caused elevated air temperatures, increased wind stresses and 'dust devil' production, creating a positive feedback loop between dust erosion and albedo. These conditions are consistent with observed polar cap erosion, and may even influence the triggering of large dust storms.
Date: 2007
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/nature05718 Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:446:y:2007:i:7136:d:10.1038_nature05718
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/nature05718
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().