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ASTROMETRIC UPDATE:
OCCULTATION BY (238) HYPATIA - 1999 DECEMBER 7

THIS UPDATE REPLACES THE PREVIOUS UPDATE OF 2 DECEMBER.


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[Prediction by Edwin Goffin]

[Prediction using OCCULT software]

Goffin's prediction suggests a path across southern Australia from around Brisbane through to Perth. The OCCULT path lies to the south with Canberra on the northern limit and Melbourne on the southern limit.


NEW UPDATE: 4 December 1999

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

Summary:

This calculation gives ~0.7" south shift and time ~3 seconds later compared to Goffin's nominal path.

Path runs over very SE Australia and twilight will make the observations hard on the Pacific coast and east part of Victoria. Melbourne lies near the centre line of the updated path. However due to uncertain star position observers within 2.5 path widths may observe an occultation. This would include Sydney, Canberra and northern Tasmania.

The TAC gives a star magnitude of 11.3 (vis) giving a predicted brighness drop is 1.3 magnitudes - enough for visual observers. But the star magnitude is also uncertain by about 0.5 magnitude. Stephen Kerr has made a ROUGH visual estimate of the stars brightness (3 December). It would appear to be around magnitude 11.6 making the brightness drop less than predicted and close to the threshold for visual observation. This combined with the absolute faintness of the star will make this observation difficult with small telescopes (< 10cm) notwithstanding the impending twilight.

THE EVENT AT ONE GLIMPSE:

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

Hypatia Update No 2 (December 7)

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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