FIRST DATA ON THE ISOTOPIC COMPOSITION OF HYDROGEN IN THE EARLY SOLAR SYSTEM

dc.contributor.author	Ul'yanov A.A.
dc.contributor.author	Devirts A.L.
dc.contributor.author	Lagutina Ye.P.
dc.contributor.author	Korovkin M.A.
dc.contributor.author	Shukolyukov Yu.A.
dc.contributor.author	Barsukov V.L.
dc.date.accessioned	2020-10-09T08:55:41Z
dc.date.available	2020-10-09T08:55:41Z
dc.date.issued	1989
dc.identifier	https://elibrary.ru/item.asp?id=31128463
dc.identifier.citation	Transactions (Doklady) of the USSR Academy of Sciences. Earth Science Sections, 1989, , 5, 235-237
dc.identifier.issn	0891-5571
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/17845
dc.description.abstract	A fine-grained oval 5 x 7 mm inclusion (designated ALD-03) from the Allende meteorite was analyzed. A delta D value of -75 per mil was determined which may characterize the composition of hydrogen in other silicate and hydrosilicate mineral phases that occurred at the early stage of solar-system evolution. If the accretion of the terrestrial planets occurred on the basis of such material, the value detla D = -75 per mil can also characterize the primordial isotopic composition of water-containing mineral phases of the primordial earth.
dc.title	FIRST DATA ON THE ISOTOPIC COMPOSITION OF HYDROGEN IN THE EARLY SOLAR SYSTEM
dc.type	Статья

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