Garcia Amanda K, Schopf J William, Yokobori Shin-Ichi, Akanuma Satoshi, Yamagishi Akihiko
Center for the Study of Evolution and the Origin of Life, University of California, Los Angeles, CA 90095;
Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095.
Proc Natl Acad Sci U S A. 2017 May 2;114(18):4619-4624. doi: 10.1073/pnas.1702729114. Epub 2017 Apr 17.
Paleotemperatures inferred from the isotopic compositions (δO and δSi) of marine cherts suggest that Earth's oceans cooled from 70 ± 15 °C in the Archean to the present ∼15 °C. This interpretation, however, has been subject to question due to uncertainties regarding oceanic isotopic compositions, diagenetic or metamorphic resetting of the isotopic record, and depositional environments. Analyses of the thermostability of reconstructed ancestral enzymes provide an independent method by which to assess the temperature history inferred from the isotopic evidence. Although previous studies have demonstrated extreme thermostability in reconstructed archaeal and bacterial proteins compatible with a hot early Earth, taxa investigated may have inhabited local thermal environments that differed significantly from average surface conditions. We here present thermostability measurements of reconstructed ancestral enzymatically active nucleoside diphosphate kinases (NDKs) derived from light-requiring prokaryotic and eukaryotic phototrophs having widely separated fossil-based divergence ages. The ancestral environmental temperatures thereby determined for these photic-zone organisms--shown in modern taxa to correlate strongly with NDK thermostability--are inferred to reflect ancient surface-environment paleotemperatures. Our results suggest that Earth's surface temperature decreased over geological time from ∼65-80 °C in the Archean, a finding consistent both with previous isotope-based and protein reconstruction-based interpretations. Interdisciplinary studies such as those reported here integrating genomic, geologic, and paleontologic data hold promise for providing new insight into the coevolution of life and environment over Earth history.
从海洋燧石的同位素组成(δO和δSi)推断出的古温度表明,地球海洋温度从太古宙时期的70±15°C降至目前的约15°C。然而,由于海洋同位素组成、同位素记录的成岩或变质重置以及沉积环境等方面存在不确定性,这种解释一直受到质疑。对重建的祖先酶热稳定性的分析提供了一种独立的方法,用于评估从同位素证据推断出的温度历史。尽管先前的研究已经证明,重建的古细菌和细菌蛋白质具有极端的热稳定性,与早期炎热的地球环境相符,但所研究的分类群可能栖息于与平均地表条件有显著差异的局部热环境中。我们在此展示了对源自需光原核生物和真核光合生物的重建祖先核苷二磷酸激酶(NDK)的热稳定性测量,这些光合生物具有基于化石的广泛分离的分歧年龄。由此确定的这些光合带生物的祖先环境温度(在现代分类群中显示与NDK热稳定性密切相关)被推断反映了古代地表环境的古温度。我们的结果表明,在地质时间内,地球表面温度从太古宙时期的约65 - 80°C下降,这一发现与先前基于同位素和基于蛋白质重建的解释一致。像本文报道的这种整合基因组、地质和古生物学数据的跨学科研究,有望为深入了解地球历史上生命与环境的共同演化提供新的见解。