New perspectives on ancient Mars

被引:231
作者
Solomon, SC
Aharonson, O
Aurnou, JM
Banerdt, WB
Carr, MH
Dombard, AJ
Frey, HV
Golombek, MP
Hauck, SA
Head, JW
Jakosky, BM
Johnson, CL
McGovern, PJ
Neumann, GA
Phillips, RJ
Smith, DE
Zuber, MT
机构
[1] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[2] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[3] Univ Calif Los Angeles, Dept Earth & Space Sci, Los Angeles, CA 90095 USA
[4] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[5] US Geol Survey, Menlo Pk, CA 94025 USA
[6] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[7] NASA, Terr Phys Lab, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[8] Case Western Reserve Univ, Dept Geol Sci, Cleveland, OH 44106 USA
[9] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[10] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80309 USA
[11] Univ Colorado, Dept Geol Sci, Boulder, CO 80309 USA
[12] Univ Calif San Diego, Scripps Inst Oceanog, Inst Geophys & Planetary Phys, La Jolla, CA 92093 USA
[13] Lunar & Planetary Inst, Houston, TX 77058 USA
[14] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
关键词
D O I
10.1126/science.1101812
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Mars was most active during its first billion years. The core, mantle, and crust formed within similar to50 million years of solar system formation. A magnetic dynamo in a convecting fluid core magnetized the crust, and the global field shielded a more massive early atmosphere against solar wind stripping. The Tharsis province became a focus for volcanism, deformation, and outgassing of water and carbon dioxide in quantities possibly sufficient to induce episodes of climate warming. Surficial and near-surface water contributed to regionally extensive erosion, sediment transport, and chemical alteration. Deep hydrothermal circulation accelerated crustal cooling, preserved variations in crustal thickness, and modified patterns of crustal magnetization.
引用
收藏
页码:1214 / 1220
页数:7
相关论文
共 104 条
[1]   Global distribution of crustal magnetization discovered by the Mars Global Surveyor MAG/ER experiment [J].
Acuña, MH ;
Connerney, JEP ;
Ness, NF ;
Lin, RP ;
Mitchell, D ;
Carlson, CW ;
McFadden, J ;
Anderson, KA ;
Rème, H ;
Mazelle, C ;
Vignes, D ;
Wasilewski, P ;
Cloutier, P .
SCIENCE, 1999, 284 (5415) :790-793
[2]   Lead isotopic ages of chondrules and calcium-aluminum-rich inclusions [J].
Amelin, Y ;
Krot, AN ;
Hutcheon, ID ;
Ulyanov, AA .
SCIENCE, 2002, 297 (5587) :1678-1683
[3]   Primary centers and secondary concentrations of tectonic activity through time in the western hemisphere of Mars [J].
Anderson, RC ;
Dohm, JM ;
Golombek, MP ;
Haldemann, AFC ;
Franklin, BJ ;
Tanaka, KL ;
Lias, J ;
Peer, B .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2001, 106 (E9) :20563-20585
[4]   Water and the martian landscape [J].
Baker, VR .
NATURE, 2001, 412 (6843) :228-236
[5]   A global view of Martian surface compositions from MGS-TES [J].
Bandfield, JL ;
Hamilton, VE ;
Christensen, PR .
SCIENCE, 2000, 287 (5458) :1626-1630
[6]  
Banerdt W.A., 2001, LUNAR PLANET SCI, VXXXII
[7]  
Banerdt W.B., 2000, LUNAR PLANET SCI, V31, P2038
[8]   Perennial water ice identified in the south polar cap of Mars [J].
Bibring, JP ;
Langevin, Y ;
Poulet, F ;
Gendrin, A ;
Gondet, B ;
Berthé, M ;
Soufflot, A ;
Drossart, P ;
Combes, M ;
Bellucci, G ;
Moroz, V ;
Mangold, N ;
Schmitt, B .
NATURE, 2004, 428 (6983) :627-630
[9]   Constraints on Martian differentiation processes from Rb-Sr and Sm-Nd isotopic analyses of the basaltic shergottite QUE 94201 [J].
Borg, LE ;
Nyquist, LE ;
Taylor, LA ;
Wiesmann, H ;
Shih, CY .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1997, 61 (22) :4915-4931
[10]   The age of Dar al Gani 476 and the differentiation history of the martian meteorites inferred from their radiogenic isotopic systematics [J].
Borg, LE ;
Nyquist, LE ;
Wiesmann, H ;
Shih, CY ;
Reese, Y .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2003, 67 (18) :3519-3536