Risks threatening viable transfer of microbes between bodies in our solar system

被引:28
作者
Mileikowsky, C [1 ]
Cucinotta, FA
Wilson, JW
Gladman, B
Horneck, G
Lindegren, L
Melosh, J
Rickman, H
Valtonen, M
Zheng, JQ
机构
[1] KTH Royal Inst Technol, Stockholm, Sweden
[2] NASA, Lyndon B Johnson Space Ctr, Houston, TX 77058 USA
[3] NASA, Langley Space Res Ctr, Newport News, VA USA
[4] Observ Cote Azur, F-06003 Nice, France
[5] DLR, Cologne, Germany
[6] Univ Lund, Lund Observ, S-22100 Lund, Sweden
[7] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[8] Univ Turku, Observ, SF-20500 Turku, Finland
[9] Univ Uppsala, Astron Observ, S-75105 Uppsala, Sweden
关键词
D O I
10.1016/S0032-0633(00)00085-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A fraction of the number of ejecta expelled from a planet by comet or asteroid impacts end up landing on another planet. If microorganisms were living in the ground before impact, they would be transported inside ejecta to the target planet. During that perilous trip, they would be subject to four main categories of threat to their survival: dynamical stress, excess temperature, radiation, chemical attack and vacuum. The effect of these, in the form of survival fractions as a function of time, as well as approximate numbers of arriving ejecta with viable flight times, have been investigated in a quantitative study we have made. The result shows that viable transfer from Mars to Earth and vice versa was highly probable during the first 0.5 Ga, and also probable, but with lower frequency, thereafter. Here we follow up with considerations about the consequences of the result regarding the question of whether the ancestor cell of all life on Earth must have originated on Earth, or whether it could have originated on Mars, its descendants thereafter moving to Earth. Some other possible consequences are also discussed. (C) 2000 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:1107 / 1115
页数:9
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