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  4. Combined element (H and C) stable isotope ratios of methane in carbonaceous chondrites
 
research article

Combined element (H and C) stable isotope ratios of methane in carbonaceous chondrites

Butterworth, A. L.
•
Aballain, O.
•
Chappellaz, J.
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January 21, 2004
Monthly Notices of the Royal Astronomical Society

We have performed the first ever combined-element stable isotopic measurements of extraterrestrial molecules. Methane from two carbonaceous chondrites, Murchison and Cold Bokkeveld, was measured for its hydrogen and carbon isotopic compositions. The combined isotopic composition of meteoritic methane reveals information about the indigenous nature of volatile aliphatic organic matter in meteorites and its probable extraterrestrial source environment. Deuterium enrichments relative to the solar nebula 4.6 Gyr ago reflect a contribution from low-temperature chemical reactions in interstellar space. Similar carbon but different hydrogen isotopic compositions for methane in the two meteorite samples probably represent comparable primary origins but varying levels of secondary processing and exchange with isotopically light hydrogen. Our high precision laboratory-obtained measurements provide valuable reference points for observational spectroscopists undertaking astronomical investigations of the stable isotopic composition of extraterrestrial methane.

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Type
research article
DOI
10.1111/j.1365-2966.2004.07251.x
Web of Science ID

WOS:000187960000014

Author(s)
Butterworth, A. L.
Aballain, O.
Chappellaz, J.
Sephton, M. A.
Date Issued

2004-01-21

Publisher

Oxford University Press (OUP)

Published in
Monthly Notices of the Royal Astronomical Society
Volume

347

Issue

3

Start page

807

End page

812

Subjects

Carbon

•

Hydrogen

•

Isotopes

•

Methane

•

Molecules

•

Solar power generation

•

Temperature

•

Astrochemistry

•

Carbonaceous chondrites

•

Combined element

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Hydrogen isotopic composition

•

ISM:molecules

•

Meteor, meteoroid

•

Methods:laboratory

•

Molecular data

•

Solar system formation

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Stable isotope ratios

•

Meteorites

Editorial or Peer reviewed

REVIEWED

Written at

OTHER

EPFL units
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Available on Infoscience
November 23, 2022
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/192610
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