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ASTROMETRIC UPDATE:
OCCULTATION BY (451) PATIENTIA - 1999 JULY 6

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[Prediction by Edwin Goffin]

[Prediction using OCCULT software]

Both the Goffin and OCCULT predictions suggest a very favourable path across southern New Zealand.


UPDATE: 2 July 1999

This prediction update is supplied by Jan Manek of the Stefanik Observatory, Prague, and is based on USNO/Flagstaff and Table Mountain astrometry for the minor planet and the GSC 1.2 star position.

Note that the accuracy of the star position in the GSC 1.2 catalog is 0.3". The photographic magnitude of 12.05 given in Goffin's prediction is in fact a visual magnitude. Therefore the brightness drop at occultation will be only about 0.5 magnitudes, which is right on the limit of reliable visual detection. Notwithstanding this, the path is exceptionally well-placed for many of the photometric observatories within New Zealand

Summary:

The update astrometry gives a path very much in accord with both the Goffin and OCCULT predictions, with a time approximately 30 seconds later than Goffin's.

Although this will be a difficult event for visual observers, it is quite within the reach of photometric instruments. At present, the update path directly crosses photometric sites at Mt John, Christchurch, Blenheim and Wellington, New Zealand, with the Auckland Observatory less than one track width away. (Track uncertainty is ~3 track widths). All photometric observatories are encouraged to monitor this event.

  • Approx time for Auckland: 14h 59m UT
  • Approx time for Wellington/Blenhem: 14h 59.5m UT
  • Approx time for Christchurch/Mt John: 15h 00m UT

    THE EVENT AT ONE GLIMPSE:

    The Occultation Path: Data for the target star: Data for the minor planet: Data for the event:

    Patientia Update (July 6)

    IMPORTANT NOTE!

    Astrometric updates such as these should not be taken as definitive, but rather only as an indication of where the true track may lie relative to the original predicted track. Observers must bear in mind that later astrometry, in which the target star is measured in the same field as the asteroid, may still reveal substantial changes to the predicted track and time of the event. For this reason it is most important that observers far from the predicted track still monitor the event.

    Use these links for further information:
    [Planetary Occultations] [Using the Predictions]
    [Observing Details] [Timing Details] [Reporting Details] [Report Form]
    [Asteroid Occultation Results]


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