The upper temperature limit for life is a key parameter for delimiting when and where life might have evolved on a hot, early Earth; the depth to which life exists in the Earth's subsurface; and the potential for life in hot, extraterrestrial environments. A combination of geological and microbiological evidence suggests that electron transport to Fe(III) may have been the first form of microbial respiration as life evolved (1–3). Geological evidence suggests that microorganisms that use Fe(III) as an electron acceptor are key components of the deep, hot biosphere (1, 4). Furthermore, the accumulation of Fe(III) in hot sediments around marine hydrothermal vents might have led to Fe(III) reduction being an important process in modern hydrothermal environments.
具体描述
读后感
用户评价
相关图书
本站所有内容均为互联网搜索引擎提供的公开搜索信息，本站不存储任何数据与内容，任何内容与数据均与本站无关，如有需要请联系相关搜索引擎包括但不限于百度，google,bing,sogou 等
© 2025 onlinetoolsland.com All Rights Reserved. 本本书屋 版权所有