DPS Pasadena Meeting 2000, 23-27 October 2000
Session 41. Comets Posters - Coma, Tails, Solar Wind Interaction
Displayed, 1:00pm, Monday - 1:00pm, Friday, Highlighted Tuesday and Thursday, 3:30-6:30pm, C101-C105, C211

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[41.19] Spectroscopy of comets Lee and LINEAR S4 in the 3 micron region using NIRSPEC

K. Magee-Sauer (Rowan Univ.), M.J. Mumma (NASA GSFC), M.A. DiSanti, N. Dello Russo (NASA GSFC / CUA), T.W. Rettig (Notre Dame), R. Novak (Iona)

We present results of spectroscopic observations of C/1999 H1 Lee on UT August 21.6, 1999 and C/1999 LINEAR S4 on UT July 13.4, 2000. The data were obtained using the NIRSPEC instrument at the Keck II telescope atop of Mauna Kea, HI. The NIRSPEC instrument is a cross-dispersed cryogenic infrared spectrometer which permits a nearly complete high-dispersion survey of the 2.9 - 3.7 \mum region. The 3 \mum region (3335 cm-1 - 3285 cm-1) includes emission from HCN, C2H2, OH, NH2, and strong lines that are preliminarily consistent with the 2\nu1 - \nu1 band of H2O.

Thirteen lines of HCN were detected in comet Lee, permitting an accurate determination of its rotational temperature (72 ± 8 K) and production rate (2.9 ± 0.2) x 1026 molecules/sec. This production rate corresponds to a relative abundance to water of (0.23 ± 0.02)%. Three lines of C2H2 were also detected corresponding to a production rate of (3.4 ± 0.3) x 1026 molecules/second and a C2H2/H2O relative abundance of (0.27 ± 0.3)%.

Comet LINEAR S4 was observed under high humidity. Thus, many lines that normally would have been clear of absorption, fell in regions of low atmospheric transmittance. A few relative strong emission lines were detected in the spectrum, but do not correspond with HCN or C2H2. A full analysis of this spectrum will be presented.

This research is supported by NSF grant no. 9619461 through the Research at Undergraduate Institutions Program.

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