Physics
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jgre..107.5096m&link_type=abstract
Journal of Geophysical Research (Planets), Volume 107, Issue E11, pp. 6-1, CiteID 5096, DOI 10.1029/2002JE001863
Physics
12
Planetology: Solar System Objects: Comets, Planetology: Comets And Small Bodies: Composition, Planetology: Comets And Small Bodies: Atmospheres-Composition And Chemistry
Scientific paper
Spectral emission from HCN in C/1996 B2 Hyakutake was detected on UT 1996 March 24.4 (rh = 1.06 AU, Δ = 0.106 AU), using the CSHELL infrared spectrometer at the NASA Infrared Telescope Facility. A Boltzmann analysis of eight ro-vibrational lines in the ν3 band returned a rotational temperature (83 +/- 9 K) for a region centered on the nucleus. The global HCN production rate was (4.50 +/- 0.81) × 1026 molecules s-1. The HCN abundance relative to water is then (0.18 +/- 0.04)%, based on direct measurements of H2O made on the same night with the same instrument and reduced with the same data processing algorithms. The measured spatial distribution for HCN is consistent with its release at the nucleus; no significant contribution from a distributed source is required within ~600 km of the nucleus. We use these data to obtain insights regarding the origin of HCN in this comet.
Dello Russo Neil
DiSanti Michael A.
Magee-Sauer Karen
Mumma Michael J.
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