McDonald Obs. observations of 9P/Tempel 1 by A. Cochran

 
Citation Cochran, A. L., Barker, E. S., Caballero, M. D., and Gyorgey-Ries, J., McDonald Observatory 9P/Tempel 1 Data V1.0. EAR-C-LCS-5-9PTMPL1-SPECTRA-V1.0. NASA Planetary Data System, 2009.
Digital Object Identifier (DOI) 10.26007/pc41-b661
Data Set Abstract We report on low-spectral resolution observations of comet 9P/Tempel 1 from 1983, 1989, 1994 and 2005 using the 2.7m 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. In the published paper, we showed that the comet decreased 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 found that the ratios of the gas production rates of OH, NH, C3, CH and C2 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. This data set represents the integrated fluxes and column densities, mentioned in the published paper, which were used to derive the production rates in the paper.
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    Additional Information
    Mission Information SUPPORT ARCHIVES
    Data Set Information EAR-C-LCS-5-9PTMPL1-SPECTRA-V1.0
    Instrument Host Information MCD27
    Instrument Information LCS
    Target Information 9P/TEMPEL 1 (1867 G1)