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Part of book or chapter of book . 1988 . Peer-reviewed

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Chemical Abundances in Meteorites

Name: Chemical Abundances in Meteorites
Creator: Herbert Palme
Keywords: 13. Climate action

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 1988Publisher:Springer Berlin Heidelberg

Authors: Herbert Palme;

doi: 10.1007/978-3-642-74188-3_2

Chemical Abundances in Meteorites

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Abstract

Some 4.6 billion years ago contraction and subsequent collapse of an interstellar cloud led to the formation of the solar system. The ratio of heavy elements to hydrogen, increasing continuously in interstellar material, due to the addition of freshly synthesized material from stars, was frozen in for the solar system at this point of time.

Related Organizations

Max Planck Society
Germany

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	19
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average