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ASTROMETRIC UPDATE:
OCCULTATION BY (76) FREIA - 2002 JANUARY 14

[Prediction by Edwin Goffin]

[Prediction using OCCULT software]

The prediction given by Goffin shows a path just missing the far northern tip of New Zealand at low altitude before running from southeastern Queensland to the Kimberley area of Western Australia. The path given by Occult using the TAC star position lies only a fraction of a path width to the south.


UPDATE: 8 JANUARY 2002

THE UPDATED PATH

Freia Update

This updated path lies around 0.4 of a path width to the south of that given by Goffin and around 40 seconds later. Due to twilight and low altitude (sun = 7 degrees below horizon and star altitude = 18 degrees), observation from the far northern tip of the North Island may not be practical. Across the Tasman Sea, the path covers the Queensland coastline between central Brisbane and Hervey Bay at 17:04 UT. Further west, the path crosses Tennant Creek in the Northern Territory around 17:07 UT before leaving the Australian mainland around the King Sound area at 17:08 UT.

The error margin on this calculation is such that all of Brisbane stands a good chance of seeing an occultation and observations will be worthwhile between Coff's Harbour in New South Wales and Mackay in central Queensland.

Calculation Source

This prediction update has been computed by Steve Preston of Medina, Washington (state) in the United States based on astrometry from Ron Stone of the US Naval Observatory - Flagstaff Station supplemented with data from the AstDys database. The UCAC position of the target star has been used combined with proper motion data from Tycho 2.

Additional details of this and other events are available at Steve Preston's website at
http://www.oz.net/~stevepr/Asteroids/asteroid.htm

EVENT DETAILS SUMMARY:

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

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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