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Halogens in chondritic meteorites and terrestrial accretion

Halogens in chondritic meteorites and terrestrial accretion

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1970640469

Halogens in chondritic meteorites and terrestrial accretion

About this item

Full title

Halogens in chondritic meteorites and terrestrial accretion

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2017-11, Vol.551 (7682), p.614-618

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

Halogen abundances in chondrites are 6 to 37 times lower than previously reported, which is consistent with the low abundances of these elements found in Earth.
An Earthly halogen history
The heavy halogens chlorine (Cl), bromine (Br) and iodine (I) are key tracers of accretion during the formation of Earth owing to their high volatility and...

Alternative Titles

Full title

Halogens in chondritic meteorites and terrestrial accretion

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1970640469

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1970640469

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature24625

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