Circular No. 2221 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 TRANSIT OF MERCURY P. M. Janiczek and A. D. Fiala communicate: "We request observations of the transit of Mercury on May 9. The primary interest is in series of photographs taken between second and third contacts, bracketing the time of conjunction. Observations with equatorial refractors and photoheliographs of focal length greater than 3 meters are especially encouraged. Times should be recorded to ls (UT) or better, and the orientations of the images should be indicated by wires or fiducial marks. We are prepared to measure and reduce the plates. Meridian observations and visual timings of the contacts are also of interest. The location of the instrument, aperture used, focal length, and seeing conditions should be specified. For questions on detail write to us at: U.S. Nautical Almanac Office, U.S. Naval Observatory, Washington, D.C. 20390, U.S.A." AGK2-AGK3 P. Lacroute and A. Valbousquet write: "L'Observatoire de Strasbourg, 11 rue de l'Universite, Strasbourg, France, can prepare magnetic tapes with the AGK2-AGK3 as determined at Hamburg and refined at Strasbourg using overlapping plates. The data furnished are: the AG and BD numbers, the coordinates at epochs 1930.0 and 1958.0 and their uncertainties, the proper motions and their uncertainties, the magnitude, the spectral type and the number of observations used in each mean. The tapes are in the IBM 360 operating system. They can be in seven tracks at 800 b.p.i. or nine tracks at 1600 b.p.i. The data available at present extend from the north pole to +40o declination, inclusive. They can be contained on one 1200-foot reel provided that it is: 1) in nine tracks at 1600 b.p.i.; 2) in binary, IBM 360 system; 3) with a large block size (of the order of 6000 to 7000). Shortly we shall be able to furnish data for the exact mean epochs of observations. Then the data will be extended toward lower declinations, when we have received the material. Some plates, especially between declinations +52o and +60o, are in the course of remeasurement at Hamburg; thus the current solution is not completely definitive. Some chance uncertainties will be somewhat diminished, but the system will not be modified." [Translation from the French.] 1970 March 5 (2221) Brian G. Marsden
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