VOLATILE ELEMENT ABUNDANCE PATTERNS AND AN EARLY LIQUID WATER OCEAN ON EARTH

dc.contributor.author	Kramers J.D.
dc.date.accessioned	2022-02-19T06:47:05Z
dc.date.available	2022-02-19T06:47:05Z
dc.date.issued	2003
dc.identifier	https://elibrary.ru/item.asp?id=13930865
dc.identifier.citation	Precambrian Research, 2003, 126, 3-4, 379-394
dc.identifier.issn	0301-9268
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/35536
dc.description.abstract	The abundances of the elements H, C, N, Ne, primordial Ar, Cl, Br, Kr, I and Xe, in the atmo-hydrosphere, continental crust and MORB-source mantle (termed the outer Earth reservoirs (OER)) are examined and compared with solar matter and an average of carbonaceous chondrites (CC). The aim is to assess the likelihood of various possible sources for these volatile elements now on Earth, and discuss and possibly quantify processes whereby volatiles were lost, in order to narrow down scenarios for the earliest terrestrial environment.
dc.subject	Terrestrial volatiles
dc.subject	Atmosphere loss
dc.subject	Hadean ocean
dc.subject	Hydrodynamic escape
dc.title	VOLATILE ELEMENT ABUNDANCE PATTERNS AND AN EARLY LIQUID WATER OCEAN ON EARTH
dc.type	Статья

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