Ground-based IR observation of oxygen isotope ratios in the Venus atmosphere
Authors:
Iwagami et al
Abstract:
The oxygen isotope ratios 17O/16O and 18O/16O in the Venus atmosphere were measured simultaneously by ground-based IR spectroscopy. The CO2 absorption lines in the 2648 cm−1 (for 17O/18O) and 4582 cm−1 (for 18O/16O) regions were observed using the IRTF/CSHELL spectrometer. The deviations of the isotope fractions are found to be δ17O=+92±158‰ and δ18O=−42±85‰ as compared to the terrestrial standard (HITRAN 2012) where the uncertainties include both random and systematic errors. Such combination agrees with the Earth-Moon fractionation line within the errors. This is consistent to the fact that the proto-Venus matter was also well mixed with the proto-Earth-Moon matter.
Friday, December 05, 2014
Based in Oxygen Isotope Ratios, Venus Originated From the Same Portion of the Protoplanetary Nebula as Earth, Moon (and Theia)
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