On the Effect of Planetary Stable Isotope Compositions on Growth and Survival of Terrestrial Organisms

被引:9
|
作者
Xie, Xueshu [1 ]
Zubarev, Roman A. [1 ]
机构
[1] Karolinska Inst, Div Physiol Chem 1, Dept Med Biochem & Biophys, Stockholm, Sweden
来源
PLOS ONE | 2017年 / 12卷 / 01期
基金
瑞典研究理事会;
关键词
HEAVY-WATER; RESONANCE HYPOTHESIS; BIOLOGICAL PROCESSES; ESCHERICHIA-COLI; DEUTERIUM; SPECIFICITY; REPLACEMENT; BACTERIA; D2O;
D O I
10.1371/journal.pone.0169296
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
Isotopic compositions of reactants affect the rates of chemical and biochemical reactions. Usually it is assumed that heavy stable isotope enrichment leads to progressively slower reactions. Yet the effect of stable isotopes may be nonlinear, as exemplified by the "isotopic resonance" phenomenon. Since the isotopic compositions of other planets of Solar system, including Mars and Venus, are markedly different from terrestrial (e.g., deuterium content is and X100 times higher, respectively), it is far from certain that terrestrial life will thrive in these isotopic conditions. Here we found that Martian deuterium content negatively affected survival of shrimp in semi-closed biosphere on a year-long time scale. Moreover, the bacterium Escherichia coli grows slower at Martian isotopic compositions and even slower at Venus's compositions. Thus, the biological impact of varying stable isotope compositions needs to be taken into account when planning interplanetary missions.
引用
收藏
页数:9
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