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Placing the Deep Impact Mission into context: Two decades of observations of 9P/Tempel 1 from McDonald Observatory |
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| Authors: | AL Cochran ES Barker J Györgey-Ries |
| Institution: | a McDonald Observatory, University of Texas, 1 University Station, C1402, Austin, TX 78712, USA b NASA Johnson Space Center, KX/Orbital Debris Program Office, 2101 NASA Pkwy, Houston, TX 77058, USA c Georgia Institute of Technology, Center for Nonlinear Science and School of Physics, Georgia Institute of Technology, Atlanta, GA 30332, USA |
| Abstract: | We report on low-spectral resolution observations of Comet 9P/Tempel 1 from 1983, 1989, 1994 and 2005 using the 2.7 m Harlan J. Smith telescope of McDonald Observatory. This comet was the target of NASA's Deep Impact mission and our observations allowed us to characterize the comet prior to the impact. We found that the comet showed a decrease in gas production from 1983 to 2005, with the decrease being different factors for different species. OH decreased by a factor 2.7, NH by 1.7, CN by 1.6, C3 by 1.8, CH by 1.4 and C2 by 1.3. Despite the decrease in overall gas production and these slightly different decrease factors, we find that the gas production rates of OH, NH, C3, CH and C2 ratioed to that of CN were constant over all of the apparitions. We saw no change in the production rate ratios after the impact. We found that the peak gas production occurred about two months prior to perihelion. Comet Tempel 1 is a “normal” comet. |
| Keywords: | Comet Tempel 1 Comets composition Spectroscopy |
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