The Paleomineralogy of the Hadean Eon Revisited

A preliminary list of plausible near-surface minerals present during Earth’s Hadean Eon (>4.0 Ga) should be expanded to include: (1) phases that might have formed by precipitation of organic crystals prior to the rise of predation by cellular life; (2) minerals associated with large...

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Main Authors: Shaunna M. Morrison, Simone E. Runyon, Robert M. Hazen
Format: Article
Language:English
Published: MDPI AG 2018-12-01
Series:Life
Subjects:
Online Access:https://www.mdpi.com/2075-1729/8/4/64
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spelling doaj-507d5548c8bd4d57882574626f8d0cbb2020-11-24T20:44:37ZengMDPI AGLife2075-17292018-12-01846410.3390/life8040064life8040064The Paleomineralogy of the Hadean Eon RevisitedShaunna M. Morrison0Simone E. Runyon1Robert M. Hazen2Geophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, DC 20015, USAGeophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, DC 20015, USAGeophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, DC 20015, USAA preliminary list of plausible near-surface minerals present during Earth’s Hadean Eon (>4.0 Ga) should be expanded to include: (1) phases that might have formed by precipitation of organic crystals prior to the rise of predation by cellular life; (2) minerals associated with large bolide impacts, especially through the generation of hydrothermal systems in circumferential fracture zones; and (3) local formation of minerals with relatively oxidized transition metals through abiological redox processes, such as photo-oxidation. Additional mineral diversity arises from the occurrence of some mineral species that form more than one ‘natural kind’, each with distinct chemical and morphological characteristics that arise by different paragenetic processes. Rare minerals, for example those containing essential B, Mo, or P, are not necessary for the origins of life. Rather, many common minerals incorporate those and other elements as trace and minor constituents. A rich variety of chemically reactive sites were thus available at the exposed surfaces of common Hadean rock-forming minerals.https://www.mdpi.com/2075-1729/8/4/64mineral evolutionphoto-oxidationimpactspaleomineralogyHadean Eon
collection DOAJ
language English
format Article
sources DOAJ
author Shaunna M. Morrison
Simone E. Runyon
Robert M. Hazen
spellingShingle Shaunna M. Morrison
Simone E. Runyon
Robert M. Hazen
The Paleomineralogy of the Hadean Eon Revisited
Life
mineral evolution
photo-oxidation
impacts
paleomineralogy
Hadean Eon
author_facet Shaunna M. Morrison
Simone E. Runyon
Robert M. Hazen
author_sort Shaunna M. Morrison
title The Paleomineralogy of the Hadean Eon Revisited
title_short The Paleomineralogy of the Hadean Eon Revisited
title_full The Paleomineralogy of the Hadean Eon Revisited
title_fullStr The Paleomineralogy of the Hadean Eon Revisited
title_full_unstemmed The Paleomineralogy of the Hadean Eon Revisited
title_sort paleomineralogy of the hadean eon revisited
publisher MDPI AG
series Life
issn 2075-1729
publishDate 2018-12-01
description A preliminary list of plausible near-surface minerals present during Earth’s Hadean Eon (>4.0 Ga) should be expanded to include: (1) phases that might have formed by precipitation of organic crystals prior to the rise of predation by cellular life; (2) minerals associated with large bolide impacts, especially through the generation of hydrothermal systems in circumferential fracture zones; and (3) local formation of minerals with relatively oxidized transition metals through abiological redox processes, such as photo-oxidation. Additional mineral diversity arises from the occurrence of some mineral species that form more than one ‘natural kind’, each with distinct chemical and morphological characteristics that arise by different paragenetic processes. Rare minerals, for example those containing essential B, Mo, or P, are not necessary for the origins of life. Rather, many common minerals incorporate those and other elements as trace and minor constituents. A rich variety of chemically reactive sites were thus available at the exposed surfaces of common Hadean rock-forming minerals.
topic mineral evolution
photo-oxidation
impacts
paleomineralogy
Hadean Eon
url https://www.mdpi.com/2075-1729/8/4/64
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