Processes on the Young Earth and the Habitats of Early Life

In press. International audience Conditions at the surface of the young (Hadean and early Archean) Earth were suitable for the emergence and evolution of life. After an initial hot period, surface temperatures in the late Hadean may have been clement beneath an atmosphere containing greenhouse gases...

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Main Authors: Arndt, Nicholas T., Nisbet, Euan
Other Authors: Géochimie, Institut des Sciences de la Terre (ISTerre), Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Department of Earth Sciences Egham, Royal Holloway University of London (RHUL)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2012
Subjects:
Online Access:https://insu.hal.science/insu-00683529
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spelling ftunivsavoie:oai:HAL:insu-00683529v1 2024-04-28T08:21:53+00:00 Processes on the Young Earth and the Habitats of Early Life Arndt, Nicholas T. Nisbet, Euan Géochimie Institut des Sciences de la Terre (ISTerre) Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS) Department of Earth Sciences Egham Royal Holloway University of London (RHUL) 2012 https://insu.hal.science/insu-00683529 en eng HAL CCSD Annual Reviews insu-00683529 https://insu.hal.science/insu-00683529 ISSN: 0084-6597 EISSN: 0084-6597 Annual Review of Earth and Planetary Sciences https://insu.hal.science/insu-00683529 Annual Review of Earth and Planetary Sciences, 2012, 40, pp [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology info:eu-repo/semantics/article Journal articles 2012 ftunivsavoie 2024-04-11T00:16:41Z In press. International audience Conditions at the surface of the young (Hadean and early Archean) Earth were suitable for the emergence and evolution of life. After an initial hot period, surface temperatures in the late Hadean may have been clement beneath an atmosphere containing greenhouse gases over an ocean-dominated planetary surface. Plate tectonics probably started early, and had produced voluminous continental crust by late Hadean, but ocean volumes may have been sufficient to submerge much of this crust. In the Hadean and early Archean, hydrothermal systems around abundant komatiitic volcanism may have provided suitable sites for hosting the earliest living communities, and for the evolution of key enzymes. Evidence from the Isua belt, Greenland, suggests life was present by 3.8 Ga ago, and by mid-Archean the geological record both in the Pilbara in Western Australia and the Barberton Mountain Land in South Africa shows that microbial life was abundant, probably using anoxygenic photosynthesis. By late Archean oxygenic photosynthesis had evolved, transforming the atmosphere and permitting the evolution of eukaryotes. Article in Journal/Newspaper Greenland Université Savoie Mont Blanc: HAL
institution Open Polar
collection Université Savoie Mont Blanc: HAL
op_collection_id ftunivsavoie
language English
topic [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
spellingShingle [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
Arndt, Nicholas T.
Nisbet, Euan
Processes on the Young Earth and the Habitats of Early Life
topic_facet [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology
description In press. International audience Conditions at the surface of the young (Hadean and early Archean) Earth were suitable for the emergence and evolution of life. After an initial hot period, surface temperatures in the late Hadean may have been clement beneath an atmosphere containing greenhouse gases over an ocean-dominated planetary surface. Plate tectonics probably started early, and had produced voluminous continental crust by late Hadean, but ocean volumes may have been sufficient to submerge much of this crust. In the Hadean and early Archean, hydrothermal systems around abundant komatiitic volcanism may have provided suitable sites for hosting the earliest living communities, and for the evolution of key enzymes. Evidence from the Isua belt, Greenland, suggests life was present by 3.8 Ga ago, and by mid-Archean the geological record both in the Pilbara in Western Australia and the Barberton Mountain Land in South Africa shows that microbial life was abundant, probably using anoxygenic photosynthesis. By late Archean oxygenic photosynthesis had evolved, transforming the atmosphere and permitting the evolution of eukaryotes.
author2 Géochimie
Institut des Sciences de la Terre (ISTerre)
Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut Français des Sciences et Technologies des Transports, de l'Aménagement et des Réseaux (IFSTTAR)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement IRD : UR219-PRES Université de Grenoble-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)
Department of Earth Sciences Egham
Royal Holloway University of London (RHUL)
format Article in Journal/Newspaper
author Arndt, Nicholas T.
Nisbet, Euan
author_facet Arndt, Nicholas T.
Nisbet, Euan
author_sort Arndt, Nicholas T.
title Processes on the Young Earth and the Habitats of Early Life
title_short Processes on the Young Earth and the Habitats of Early Life
title_full Processes on the Young Earth and the Habitats of Early Life
title_fullStr Processes on the Young Earth and the Habitats of Early Life
title_full_unstemmed Processes on the Young Earth and the Habitats of Early Life
title_sort processes on the young earth and the habitats of early life
publisher HAL CCSD
publishDate 2012
url https://insu.hal.science/insu-00683529
genre Greenland
genre_facet Greenland
op_source ISSN: 0084-6597
EISSN: 0084-6597
Annual Review of Earth and Planetary Sciences
https://insu.hal.science/insu-00683529
Annual Review of Earth and Planetary Sciences, 2012, 40, pp
op_relation insu-00683529
https://insu.hal.science/insu-00683529
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