Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars

Sulphate-rich sediments have been taken as evidence of surface water on Mars. Here, the authors show that cryo-concentrated brines chemically weather olivine minerals forming sulfate minerals at up to −60 °C, showing that cryogenic weathering and sulfate formation can occur under current Martian con...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Paul B. Niles, Joseph Michalski, Douglas W. Ming, D. C. Golden
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2017
Materias:
Q
Acceso en línea:https://doaj.org/article/869f51d4c7044d1681fc64975790d012
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:869f51d4c7044d1681fc64975790d012
record_format dspace
spelling oai:doaj.org-article:869f51d4c7044d1681fc64975790d0122021-12-02T17:06:01ZElevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars10.1038/s41467-017-01227-72041-1723https://doaj.org/article/869f51d4c7044d1681fc64975790d0122017-10-01T00:00:00Zhttps://doi.org/10.1038/s41467-017-01227-7https://doaj.org/toc/2041-1723Sulphate-rich sediments have been taken as evidence of surface water on Mars. Here, the authors show that cryo-concentrated brines chemically weather olivine minerals forming sulfate minerals at up to −60 °C, showing that cryogenic weathering and sulfate formation can occur under current Martian conditions.Paul B. NilesJoseph MichalskiDouglas W. MingD. C. GoldenNature PortfolioarticleScienceQENNature Communications, Vol 8, Iss 1, Pp 1-5 (2017)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
Paul B. Niles
Joseph Michalski
Douglas W. Ming
D. C. Golden
Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
description Sulphate-rich sediments have been taken as evidence of surface water on Mars. Here, the authors show that cryo-concentrated brines chemically weather olivine minerals forming sulfate minerals at up to −60 °C, showing that cryogenic weathering and sulfate formation can occur under current Martian conditions.
format article
author Paul B. Niles
Joseph Michalski
Douglas W. Ming
D. C. Golden
author_facet Paul B. Niles
Joseph Michalski
Douglas W. Ming
D. C. Golden
author_sort Paul B. Niles
title Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
title_short Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
title_full Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
title_fullStr Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
title_full_unstemmed Elevated olivine weathering rates and sulfate formation at cryogenic temperatures on Mars
title_sort elevated olivine weathering rates and sulfate formation at cryogenic temperatures on mars
publisher Nature Portfolio
publishDate 2017
url https://doaj.org/article/869f51d4c7044d1681fc64975790d012
work_keys_str_mv AT paulbniles elevatedolivineweatheringratesandsulfateformationatcryogenictemperaturesonmars
AT josephmichalski elevatedolivineweatheringratesandsulfateformationatcryogenictemperaturesonmars
AT douglaswming elevatedolivineweatheringratesandsulfateformationatcryogenictemperaturesonmars
AT dcgolden elevatedolivineweatheringratesandsulfateformationatcryogenictemperaturesonmars
_version_ 1718381740795363328