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

dc.contributor.authorUl'yanov A.A.
dc.contributor.authorDevirts A.L.
dc.contributor.authorLagutina Ye.P.
dc.contributor.authorKorovkin M.A.
dc.contributor.authorShukolyukov Yu.A.
dc.contributor.authorBarsukov V.L.
dc.date.accessioned2020-10-09T08:55:41Z
dc.date.available2020-10-09T08:55:41Z
dc.date.issued1989
dc.description.abstractA 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.identifierhttps://elibrary.ru/item.asp?id=31128463
dc.identifier.citationTransactions (Doklady) of the USSR Academy of Sciences. Earth Science Sections, 1989, , 5, 235-237
dc.identifier.issn0891-5571
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/17845
dc.titleFIRST DATA ON THE ISOTOPIC COMPOSITION OF HYDROGEN IN THE EARLY SOLAR SYSTEM
dc.typeСтатья

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