The 16OH/18OH and OD/OH isotope ratios in comet C/2002 T7 (LINEAR)
D. Hutsemekers, J. Manfroid, E. Jehin, J.-M. Zucconi, C. Arpigny

TL;DR
This study measures isotope ratios in comet C/2002 T7 (LINEAR) using ground-based UV observations, finding ratios similar to Earth's and other comets, and estimates the D/H ratio in water.
Contribution
It provides new measurements of 16O/18O and OD/OH isotope ratios in a specific comet using UV spectroscopy, contributing to understanding of cometary composition.
Findings
16O/18O ratio is 425 +/- 55, close to terrestrial value.
D/H ratio in water is 2.5 +/- 0.7 x 10^-4, consistent with other comets.
Results support similarity between cometary and terrestrial isotope ratios.
Abstract
The 16OH/18OH and OD/OH isotope ratios are measured in the Oort-Cloud comet C/2002 T7 (LINEAR) through ground-based observations of the OH ultraviolet bands at 3063 A (0,0) and 3121 A (1,1) secured with the Very Large Telescope (VLT) feeding the Ultraviolet-Visual Echelle Spectrograph (UVES). From the 16OH/18OH ratio, we find 16O/18O = 425 +/- 55, equal within the uncertainties to the terrestrial value and to the ratio measured in other comets, although marginally smaller. We also estimate OD/OH from which we derive D/H = 2.5 +/- 0.7 10-4 in water. This value is compatible with the water D/H ratios evaluated in other comets and marginally higher than the terrestrial value.
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