Circular No. 5010 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN COMET AUSTIN (1989c1) D. J. Sahnow, P. D. Feldman, S. R. McCandliss, and M. E. Martinez, Johns Hopkins University, report obtaining long-slit ultraviolet spectra of comet Austin from a sounding rocket experiment launched from White Sands Missile Range, NM, on Apr. 21.43 UT. The wavelength range was 125-185 nm at a spectral resolution of 0.7 nm along an 8".25 slit. Emissions of O I, C I, S I, and CO were detected. The CO production rate derived from a radial outflow model is 1-2 x 10E27 sE-1, indicating an abundance of CO relative to water of about 2 percent. V3890 SAGITTARII B. A. Skiff, Lowell Observatory, reports the following position that is a mean of measurements from two plates taken 1990 May 9.4 UT with the 0.33-m Lowell astrograph: R.A. = 18h27m39s.976, Decl. = -24 03'18.23 (equinox 1950.0; standard deviations +/- 0".64 in R.A., +/- 0".52 in Decl.). W. Liller, Vina del Mar, Chile, reports his independent discovery of the outburst of this object, and provides the following magnitudes from 2415 film images: Apr. 25.39 UT, [12; 29.14, 8.8; 30.15, 8.6. 1990 HA Improved orbital elements from MPC 16438: T = 1990 Feb. 24.784 ET Peri. = 307.469 e = 0.66772 Node = 184.770 1950.0 q = 0.79369 AU Incl. = 3.795 a = 2.38863 AU n = 0.266981 P = 3.69 years 1990 ET R.A. (1950) Decl. Delta r V May 9 13 44.67 - 1 04.5 0.334 1.321 16.1 19 13 51.90 - 2 47.9 29 13 59.09 - 4 18.1 0.587 1.519 17.8 June 8 14 07.03 - 5 43.3 18 14 15.85 - 7 05.7 0.887 1.711 19.0 28 14 25.59 - 8 26.2 July 8 14 36.19 - 9 44.6 1.230 1.894 20.0 1990 May 11 (5010) Daniel W. E. Green
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