Microbial habitability of the Hadean Earth during the late heavy bombardment

被引:156
作者
Abramov, Oleg [1 ]
Mojzsis, Stephen J. [1 ]
机构
[1] Univ Colorado, Dept Geol Sci, Boulder, CO 80309 USA
关键词
SUPRACRUSTAL ROCKS; LUNAR CATACLYSM; WEST GREENLAND; ORIGIN; LIFE; METEORITE; ZIRCONS; AGE; EVOLUTION; HISTORY;
D O I
10.1038/nature08015
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
Lunar rocks(1,2) and impact melts(3), lunar(4) and asteroidal meteorites(5), and an ancient martian meteorite(6) record thermal metamorphic events with ages that group around and/or do not exceed 3.9 Gyr. That such a diverse suite of solar system materials share this feature is interpreted to be the result of a post-primary-accretion cataclysmic spike in the number of impacts commonly referred to as the late heavy bombardment (LHB)(1-7). Despite its obvious significance to the preservation of crust and the survivability of an emergent biosphere, the thermal effects of this bombardment on the young Earth remain poorly constrained. Here we report numerical models constructed to probe the degree of thermal metamorphism in the crust in the effort to recreate the effect of the LHB on the Earth as a whole; outputs were used to assess habitable volumes of crust for a possible near-surface and subsurface primordial microbial biosphere. Our analysis shows that there is no plausible situation in which the habitable zone was fully sterilized on Earth, at least since the termination of primary accretion of the planets and the postulated impact origin of the Moon. Our results explain the root location of hyperthermophilic bacteria in the phylogenetic tree for 16S small-subunit ribosomal RNA(8), and bode well for the persistence of microbial biospheres even on planetary bodies strongly reworked by impacts.
引用
收藏
页码:419 / 422
页数:4
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