Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Airborne infrared spectroscopy of Comet Wilson (1986l) and comparisons with Comet Halley

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/167260· OSTI ID:6062738
H/sub 2/O and possibly CH/sub 4/ have been detected in near-infrared spectra of Comet Wilson (1986l). The observed number and relative intensities of cometary H/sub 2/O lines in the nu3 band at 2.65 microns were consistent with fluorescent excitation pumped by solar infrared photons. The H/sub 2/O production rate in Comet Wilson was approximately 3 x 10 to the 29th/s at R = 1.2 AU; no pronounced temporal variability was observed. Lines in the nu3 band of CH/sub 4/ at 3.3 microns were possibly detected at the 3 sigma confidence level. The CH/sub 4/ abundance is in the range CH/sub 4//H/sub 2/O = 0.014-0.045; the uncertainty is due primarily to the assumed effective excitation temperature of CH/sub 4/. The CH/sub 4/ abundance in this dynamically 'new' comet is similar to that observed in P/Halley. These values are low for equilibrium compositional models and very high for disequilibrium condensation in the solar nebula. 35 references.
Research Organization:
Arizona Univ., Tucson (USA); Arizona Univ., Tucson (USA); Space Telescope Science Institute, Baltimore, MD (USA); NASA, Goddard Space Flight Center, Greenbelt, MD (USA); Max-Planck-Institut fuer extraterrestrische Physik, Garching (Germany, F.R.)
OSTI ID:
6062738
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 338; ISSN ASJOA
Country of Publication:
United States
Language:
English