Circular No. 2002 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Cable Address: SATELLITES, NEWYORK Western Union: RAPID SATELLITE CAMBMASS SUPERNOVA IN NGC 3389 Dr. F. Bertola, Osservatorio Astronomico, Padova, writes as follows: "After the announcement of the discovery of Chuadze of the supernova in NGC 3389, I secured a spectrum with the 122-cm Asiago reflector on March 4-5. The spectrum exhibits the features characteristic of a Type I supernova near maximum. The supernova is present on a plate taken for a search of blue objects with the Asiago 90-65-cm Schmidt telescope on March 2-3, and the resulting U - B color index is close to zero." A cable from Dr. L. Detre, Director of the Konkoly Observatory, Budapest, reports the independent discovery by Lovas on March 10 of this supernova, 1' northwest of the nuclues of NGC 3389, with the magnitude given as 14. PERIODIC COMET TUTTLE (1967a) B. Milet, Nice Observatory, provides the following positions: 1967 UT R.A. (1950) Decl. Jan. 24.84319 23 48 30.89 +35 46 06.1 26.75549 23 56 03.85 +35 01 51.1 Feb. 1.75167 0 19 29.42 +32 39 19.7 1.76279 0 19 31.84 +32 39 02.5 6.75716 0 39 14.44 +30 32 54.2 6.76824 0 39 17.57 +30 32 37.6 17.75397 1 22 28.15 +25 32 18.5 17.76217 1 22 29.92 +25 32 04.1 18.77314 1 26 26.40 +25 02 58.9 27.77734 2 00 54.63 +20 33 32.2 BD +26 870 Mr. C. Y. Shao, Harvard College Observatory, writes: "Examination of yellow (103a-G) and red (103a-E) patrol plates taken at the Agassiz Station by Mr. W. Black on January 30.0 showed that BD +26 870 was definitely fainter than the nearby star 121 Tau (mv = 5.2, B3V)." 1967 March 14 (2002) Owen Gingerich
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