New perspectives on ancient Mars

Science

Volumn 307, Issue 5713, 2005, Pages 1214-1220

  Solomon, Sean C ^a   Aharonson, Oded ^b   Aurnou, Jonathan M ^c   Banerdt, W Bruce ^d   Carr, Michael H ^e   Dombard, Andrew J ^f   Frey, Herbert V ^g   Golombek, Matthew P ^d   Hauck II, Steven A ^h   Head III, James W ⁱ   Jakosky, Bruce H ^j   Johnson, Catherine L ^k   McGovern, Patrick J ^l   Neumann, Gregory A ^m   Phillips, Roger J ^f   Smith, David E ^g   Zuber, Maria T ^m  

^a GEOPHYSICAL LABORATORY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e U S GEOLOGICAL SURVEY   (United States)

^f WASHINGTON UNIVERSITY   (United States)

^g NASA GODDARD SPACE FLIGHT CENTER   (United States)

^h CASE WESTERN RESERVE UNIVERSITY   (United States)

ⁱ BROWN UNIVERSITY   (United States)

^j UNIVERSITY OF COLORADO   (United States)

^k UNIVERSITY OF CALIFORNIA   (United States)

^l LUNAR AND PLANETARY INSTITUTE   (United States)

^m MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

CARBON DIOXIDE; CLIMATE CHANGE; COOLING; EARTH ATMOSPHERE; EROSION; MAGNETIZATION; MARTIAN SURFACE ANALYSIS; SEDIMENT TRANSPORT; SOLAR SYSTEM; WATER; WIND;

CLIMATE WARMING; CRUSTAL MAGNETIZATION; MAGNETIC DYNAMO; SOLAR WIND;

PLANETS;

CARBON DIOXIDE; WATER;

CORE (PLANETARY); CRUST; MANTLE; MARS; PLANETARY EVOLUTION; VOLCANISM;

ASTRONOMY; ATMOSPHERE; CLIMATE CHANGE; MAGNETISM; PRIORITY JOURNAL; REVIEW; SEDIMENT TRANSPORT; SEDIMENTATION; SOLAR ENERGY; WARMING; WIND;

ATMOSPHERE; CLIMATE; EXTRATERRESTRIAL ENVIRONMENT; MAGNETICS; MARS; TEMPERATURE; WATER;

EID: 20044367442     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1101812     Document Type: Review

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107. This paper began as a series of scientific discussions held at meetings of the Mars Orbiting Laser Altimeter team on the Mars Global Surveyor mission. We thank J. Dickson, L. Montesi, and J. Roark for assistance with figure preparation. Support for this paper has been provided by NASA, through the Mars Exploration Program, the Planetary Geology and Geophysics Program, and the NASA Astrobiology Institute.