Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator

被引:126
作者
Murray, JB
Muller, JP
Neukum, G
Werner, SC
van Gasselt, S
Hauber, E
Markiewicz, WJ
Head, JW
Foing, BH
Page, D
Mitchell, KL
Portyankina, G
机构
[1] Open Univ, Dept Earth Sci, Milton Keynes MK7 6AA, Bucks, England
[2] UCL, Dept Geomat Engn, London WC1E 6BT, England
[3] Free Univ Berlin, Inst Geosci, D-12249 Berlin, Germany
[4] DLR, Inst Planetenforsch, D-12489 Berlin, Germany
[5] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
[6] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[7] European Space Agcy, Res & Sci Support Dept, ESTEC, SCISR, NL-2200 AG Noordwijk, Netherlands
[8] Nat Hist Museum, Dept Mineral, London SW7 5PB, England
[9] Univ Lancaster, Dept Environm Sci, Lancaster LA1 4YQ, England
关键词
D O I
10.1038/nature03379
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
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water floods(1,2-4) two to ten million years ago(1,2,5). Evidence for the resulting lava plains has been identified in eastern Elysium(1,2,4,6 - 8), but seas and lakes from these fissures and previous water flooding events were presumed to have evaporated and sublimed away(9-11). Here we present High Resolution Stereo Camera images from the European Space Agency Mars Express spacecraft that indicate that such lakes may still exist. We infer that the evidence is consistent with a frozen body of water, with surface pack-ice, around 5 degrees north latitude and 150 degrees east longitude in southern Elysium. The frozen lake measures about 800 x 900 km in lateral extent and may be up to 45 metres deep - similar in size and depth to the North Sea. From crater counts, we determined its age to be 5 +/- 2 million years old. If our interpretation is confirmed, this is a place that might preserve evidence of primitive life, if it has ever developed on Mars.
引用
收藏
页码:352 / 356
页数:5
相关论文
共 28 条
[1]  
BAKER VR, 1992, MARS, P493
[2]   Recent fluvial, volcanic, and tectonic activity on the cerberus plains of Mars [J].
Berman, DC ;
Hartmann, WK .
ICARUS, 2002, 159 (01) :1-17
[3]   Repeated aqueous flooding from the Cerberus Fossae: Evidence for very recently extant, deep groundwater on Mars [J].
Burr, DM ;
Grier, JA ;
McEwen, AS ;
Keszthelyi, LP .
ICARUS, 2002, 159 (01) :53-73
[4]   STABILITY OF STREAMS AND LAKES ON MARS [J].
CARR, MH .
ICARUS, 1983, 56 (03) :476-495
[5]   D/H ON MARS EFFECTS OF FLOODS, VOLCANISM, IMPACTS, AND POLAR PROCESSES [J].
CARR, MH .
ICARUS, 1990, 87 (01) :210-227
[6]   Oceans on Mars: An assessment of the observational evidence and possible fate [J].
Carr, MH ;
Head, JW .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2003, 108 (E5)
[7]   The evolution of the Martian hydrosphere: Implications for the fate of a primordial ocean and the current state of the northern plains [J].
Clifford, SM ;
Parker, TJ .
ICARUS, 2001, 154 (01) :40-79
[8]   A MODEL FOR THE HYDROLOGIC AND CLIMATIC BEHAVIOR OF WATER ON MARS [J].
CLIFFORD, SM .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1993, 98 (E6) :10973-11016
[9]   Amazonis Planitia: The role of geologically recent volcanism and sedimentation in the formation of the smoothest plains on Mars [J].
Fuller, ER ;
Head, JW .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2002, 107 (E10)
[10]  
Garvin J. B., 2003, 6 INT C MARS PAS CA