12C/ 13C Ratio in ethane on titan and implications for methane's replenishment
- Donald E. Jennings,
- Paul N. Romani,
- Gordon L. Bjoraker,
- ,
- Conor A. Nixon,
- Allen W. Lunsford
Research Output: Contribution to journal Article Peer-review
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9
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65
Abstract
The 12C/13C abundance ratio in ethane in the atmosphere of Titan has
been measured at 822 cm-1 from high spectral resolution ground-based
observations. The value, 89(8), coincides with the telluric standard and
also agrees with the ratio seen in the outer planets. It is almost
identical to the result for ethane on Titan found by the composite
infrared spectrometer (CIRS) on Cassini. The 12C/13C ratio for ethane is
higher than the ratio measured in atmospheric methane by Cassini/Huygens
GCMS, 82.3(1), representing an enrichment of 12C in the ethane that
might be explained by a kinetic isotope effect of approximately 1.1 in
the formation of methyl radicals. If methane is being continuously
resupplied to balance photochemical destruction, then we expect the
isotopic composition in the ethane product to equilibrate at close to
the same 12C/13C ratio as that in the supply. The telluric value of the
ratio in ethane then implies that the methane reservoir is primordial.
Publication Information
Output type
Research Output: Contribution to journal Article Peer-review
Original language
EnglishPages from-to (Number of pages)
Pages 11101-11106 (6 pages)Journal (Volume, Issue Number)
Journal of Physical Chemistry A (Volume 113, Issue 42)Publication milestones
- Published - 22/10/2009
Publication status
Published - 22/10/2009
ISSN
1089-5639Publication IDs
- Scopus: 70350137100
- WOS: 000270670700003
