HO and O Absorption in the Coma of Comet 67P/Churyumov-Gerasimenko Measured by the Alice Far-Ultraviolet Spectrograph on Rosetta
arXiv:1706.01948 · doi:10.1093/mnras/stx1426
Abstract
We have detected HO and O absorption against the far-UV continuum of stars located on lines of sight near the nucleus of Comet 67P/Churyumov-Gerasimenko using the Alice imaging spectrograph on Rosetta. These stellar appulses occurred at impact parameters of -20 km, and heliocentric distances ranging from to 2.3 AU (negative values indicate pre-perihelion observations). The measured HO column densities agree well with nearly contemporaneous values measured by VIRTIS-H. The clear detection of O independently confirms the initial detection by the ROSINA mass spectrometer; however, the relative abundance of O/HO derived from the stellar spectra (11%-68%, with a median value of 25%) is considerably larger than published values found by ROSINA. The cause of this difference is unclear, but potentially related to ROSINA measuring number density at the spacecraft position while Alice measures column density along a line of sight that passes near the nucleus.
arXiv comment21 pages, accepted by MNRAS
References in corpus (9)
- The SIMBAD astronomical database
- Alice: The Rosetta Ultraviolet Imaging Spectrograph
- Measurements of the Near-Nucleus Coma of Comet 67P/Churyumov-Gerasimenko with the Alice Far-Ultraviolet Spectrograph on Rosetta
- Evolution of CO, CH, and OCS abundances relative to HO in the coma of comet 67P around perihelion from Rosetta/VIRTIS-H observations
- A primordial origin for molecular oxygen in comets: A chemical kinetics study of the formation and survival of O ice from clouds to disks
- Origin of molecular oxygen in Comet 67P/Churyumov-Gerasimenko
- Molecular Oxygen in Oort Cloud Comet 1P/Halley
- Detection of exposed HO ice on the nucleus of comet 67P/Churyumov-Gerasimenko
- The Nature and Frequency of the Gas Outbursts in Comet 67P/Churyumov-Gerasimenko observed by the Alice Far-ultraviolet Spectrograph on Rosetta
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