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IAUC 2279: SN IN NGC 1533; SN IN NGC 7619; 1970g; Occn OF beta Sco BY JUPITER

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                                                  Circular No. 2279
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 1533
     Mr. Robert Evans, Boolaroo, New South Wales, reports that he
discovered on July 1 a supernova close to the nucleus of NGC 1533
(R. A. 4h08m.8, Decl. -56o15', equinox 1950.0).  The visual magnitude
was 11.8.  Other magnitude estimates follow: July 6, 12.6; 8, 12.1;
11, 12.4; 13, 12.2; 17, 12.7.  The object was no longer visible in
his 25-cm reflector on July 29.  Comparison with other supernovae
suggests that the magnitude may still be as bright as 16, and
photographic confirmation would be most desirable.


SUPERNOVA IN NGC 7619
     Dr. L. Rosino, Asiago Astrophysical Observatory, reports the
discovery of a supernova in NGC 7619 (R. A. 23h17m.7, Decl. +7o55'
equinox 1950.0), 27" west and 30" south of the nucleus.  On Sept.
24 the photographic magnitude was 14.5.


COMET ABE (1970g)
     The following precise positions have been reported:

     1970 UT             R. A. (1950) Decl.        Observer
     Aug.  1.99438     2 14 04.66   +39 19 11.9    Petrovicova
           4.97840     2 10 52.82   +41 54 40.7      "
           5.97456     2 09 33.58   +42 50 29.8      "
           6.96652     2 08 05.87   +43 48 00.6      "
          13.95963     1 51 50.68   +51 39 05.6      "
          14.99561     1 48 08.60   +52 59 25.3      "
          17.91700     1 34 47.50   +57 00 41.4    Waterfield
          17.94315     1 34 39.62   +57 02 55.5    Rutter
          25.91557     0 11 54.11   +69 05 11.0    Petrovicova
          26.04798     0 09 27.17   +69 16 31.7    Chareton
          26.88905    23 52 37.03   +70 25 36.8    Petrovicova
          26.91005    23 52 10.78   +70 27 16.7    Waterfield
          27.93544    23 28 13.61   +71 43 38.5    Petrovicova
          28.92348    23 01 26.52   +72 45 57.8      "
          30.89289    21 57 46.86   +74 03 02.6      "
          31.88351    21 22 19.67   +74 11 36.5      "
    Sept.  2.83871    20 13 18.37   +73 22 32.3    Chareton
           2.91049    20 10 54.63   +73 19 03.3    Mrkos
           7.89748    18 09 36.88   +66 09 49.9      "
           8.79751    17 56 07.24   +64 28 27.5      "
          12.87024    17 13 57.53   +56 29 28.7    South
          14.83935    17 00 53.24   +52 41 43.2    Chareton
          16.86285    16 50 26.74   +48 56 42.3      "
          17.89636    16 46 00.27   +47 06 19.3    Considere
          18.02448    16 45 29.27   +46 52 48.5      "
          18.89572    16 42 10.18   +45 22 46.8    Chareton
          19.87886    16 38 47.01   +43 44 07.8    Hilaire

R. Petrovicova and A. Mrkos (Klet Observatory).
R. L. Waterfield, G. H. Rutter and R. South (Woolston Observatory).
   Measurer: R. L. Waterfield.
Chareton, Considere and Hilaire (Besancon Observatory).


OCCULTATION OF beta SCORPII BY JUPITER
     Mr. G. E. Taylor writes: "On 1971 May 13 Jupiter will occult
the bright spectroscopic binary beta Sco, and also two nearby stars of
magnitudes 5 and 9, respectively. One or both phases of the occultations
will be visible for most of the inhabited regions of the
world except for North and South America and western Europe.  Predictions
are given in Handbk Br. astr. Assoc. for 1971 as follows:

                      Area of      Station      Disappears    Reappears
1971     Star         Visibility                 UT  p.a.      UT  p.a.
May  13  S.A.O.       Australia    Mt. Stromlo  17.8 267      20.0 115
         159683       New Zealand  Wellington   17.8 266       low
          (5.1)       Asia         Tokyo        17.8 274      20.1 109
                      Europe       Abastuman    17.9 272      20.2 110
                      Africa       Cape         17.9 264      20.2 118
May  13  beta Sco     Australia    Mt. Stromlo  18.4 222      19.6 158
          (2.9)       New Zealand  Wellington   18.5 220      low
                      Asia         Tokyo        18.3 233      19.8 149
                      Europe       Abastuman    18.4 232      20.0 150
                      Africa       Cape         18.7 218      19.8 161

The star of magnitude 9 is 0".8 distant from beta Sco in p.a. 106o and
will be occulted a few minutes earlier than beta Sco itself.  A little
earlier in the day, on about May 13.3-13.4, satellite III will pass
very close to beta Sco, and this event will be visible from North
America (except the eastern part), the Pacific, New Zealand and Australia
(except the western part).  Although it seems likely that satellite
III will pass about 3" north of the star (geocentrically), it
is suggested that observers keep careful watch in case of an occultation.
The farther north the observer is, the greater the chance
of an occultation."  Mr. Taylor would be glad to receive observations
at the address: H.M. Nautical Almanac Office, Royal Greenwich
Observatory, Herstmonceux Castle, Hailsham, Sussex, England.


1970 September 29              (2279)              Brian G. Marsden

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