Circular No. 2229 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 COMET BENNETT (1969i) The following precise positions have been reported: 1970 UT R. A. (1950) Decl. Mag. Observer Jan. 6.04075 0 31 07.06 -64 31 49.1 Potter 11.05195 0 14 44.98 -63 29 47.1 " 12.07907 0 11 46.85 -63 16 35.8 " 13.04437 0 08 52.65 -63 03 03.3 " 14.05062 0 06 02.31 -62 49 12.2 " 15.04441 0 03 18.76 -62 35 17.7 " 16.08039 0 00 32.91 -62 20 33.4 " 18.04512 23 55 31.81 -61 52 05.4 " 29.03548 23 31 30.74 -59 01 04.2 " 31.04113 23 27 40.48 -58 27 44.8 " Feb. 1.03932 23 25 48.38 -58 10 51.3 " 2.03308 23 23 58.04 -57 53 52.2 " 3.03379 23 22 08.37 -57 36 29.7 " 4.03451 23 20 19.71 -57 18 55.0 " 6.02902 23 16 45.46 -56 43 04.1 " 7.02975 23 14 58.72 -56 24 35.2 " 8.02701 23 13 12.72 -56 05 52.7 " 9.02910 23 11 26.48 -55 46 42.2 " 10.02840 23 09 40.41 -55 27 10.2 " 11.02772 23 07 54.30 -55 07 08.5 " 12.02982 23 06 07.43 -54 46 34.6 " 13.02846 23 04 20.50 -54 25 32.6 " 14.02778 23 02 32.81 -54 03 53.2 " 15.02641 23 00 44.45 -53 41 34.8 " 16.02649 22 58 54.90 -53 18 27.2 " 17.02575 22 57 04.55 -52 54 31.9 " 18.02508 22 55 12.99 -52 29 41.2 " Mar. 18.40017 22 04 24.52 -20 44 57.8 0.5 Rodriguez 18.40090 22 04 24.29 -20 44 50.3 " 21.38762 22 03 56.71 -12 46 58.5 0.5 Pereyra 21.38831 22 03 56.69 -12 46 50.5 " 21.38900 22 03 56.82 -12 46 44.0 " 22.83698 22 04 32.1 - 8 34 19 -0.5 Seki 22.84398 22 04 32.6 - 8 33 06 " H. Potter and A. Lokalov (National Observatory, Santiago). Cerro El Roble station; Maksutov astrograph. Measurer: C. Torres; Computer: H. Wroblewski. J. J. Rodriguez and Z. M. Pereyra (Cordoba Observatory for the CNEGH). 33-cm astrograph. Measurer: Miss B. Oviedo. Objective prism spectra of both head and tail show strong continuum and emission. The curved dust tail, 10o long, shows filaments extending along the prolongation of the radius vector. T. Seki (Kochi Observatory). 22-cm f/5 camera. Tail > 5o. Mr. J. C. Bennett, Pretoria, writes that on March 20.1 the tail could be traced with the naked eye to at least 11o; on March 28.1 the tail was traced to more than 6o in spite of poor conditions. On March 22.1 the magnitude of the central condensation was estimated as 1.0, and in an 8-cm refractor (magnification up to 227 x) short faint jets were seen radiating from it on the sunward side. A guided 20-min exposure taken at the same time by K. J. Sterling shows a straight gas tail that is almost as prominent as the dust tail and which can be followed for some 20o. Mr. K. Simmons, Jacksonville, Florida, writes that on March 25.5 the magnitude (7 x 50 binoculars) was 1.6. A central condensation, of magnitude 6.0, and 0'.2 to 0'.4 in diameter, was observed with a 21-cm reflector; the coma was 5' in diameter, the brightest portion about 2'.5. A fan-shaped tail, 2o.5 long as seen with the naked eye, curved to p.a. 225o (near the coma in p.a. 215-220o); there was a 2' counter tail at p.a. 90o and jets at p.a. 75o and 105o. Mr. D. Li, Honolulu, describes orange "pin-wheel" streamers that on March 26.6 appeared to come out of the western arc of the head envelope and sweep around to the east. The comet's total magnitude was 0.0, a magnitude fainter than the previous morning. Mr. J. E. Bortle, Mount Vernon, New York, reports that on March 28.4 the comet was of magnitude 0.5, with a brilliant central condensation of magnitude 1.7. The curved tail extended about 5o in the brightly moonlit sky. Fountain-type jets extended from the nucleus, and the appearance was very similar to that of comet 1861 II, as depicted by Secchi and by Schmidt. SUPERNOVA IN IC 3476 Mr. K. Locher, Wetzikon, Switzerland, sends the following visual estimates (from comparison with nearby MVSO sequences): 1970 UT V Mar. 28.88 13.6 +/- 0.2 30.85 13.8 +/- 0.2 1970 April 6 (2229) Brian G. Marsden
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