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Jan Manek of the Stefanik Observatory has attempted to compute an update for this event. The results of these calculations show that the asteroid will pass as far as 48" north (from geocentric view) of the target star around 00:47 UT which is 6.5 hours earlier than predicted. As a result, no occultation will be visible from any point on Earth.
This calculation is consistant with the views expressed elsewhere on these webpages (click here for reference) and also with calculations performed in OCCULT and Guide 7. As a general visualisation of the situation, attached below is a star chart generated in Guide 7 showing the path of the asteroid relative to the target star. This chart covers around 40' by 30' with a magnitude limit around 13.5.
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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