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Updated: 2006 JUL 18, 18:50 UT
Event Rank : 52
(The event Rank is a measure of the likelihood of observing an event, and is equal to the probability of at least one successful observation by a team of two observers spaced 1/8 path width just inside opposite sides of the predicted path. An event rank of 100 indicates that the prediction is expected to be very accurate).
THE UPDATED PATH
Note: The duration given in the line below is the interval during which the occultation shadow sweeps across the Earth - please see the minute markers on the map to determine the approximate time for your location.
On 2006 Aug 19 UT, the 22 km diameter asteroid (1584) Fuji will occult a 9.5 mag star in the constellation Andromeda for observers along a path across Cape York Peninsula and central Queensland.
In the case of an occultation, the combined light of the asteroid and the star will drop by 5.7 mag to 15.2 mag (the magnitude of the asteroid) for at most 1.5 seconds.
This update is based on UNSO/Flagstaff astrometry for the asteroid kindly provided by Ron Stone, historical astrometry from the MPC files (via AstDys), and the following catalogs for the star position: UCAC.
Additional details of this and other events are available at Steve Preston's website at http://www.asteroidoccultation.com/
EVENT DETAILS SUMMARY :Important Note regarding Accuracy:
The uncertainty interval in path widths given above (and shown as a 1-sigma uncertainty ellipse on the plot) refers to RMS deviation and is applied as a +/- range. In other words, a path uncertainty of 1.0 path widths means that the actual center of the asteroid's shadow path should fall within plus or minus 1 path width of the plotted path center. However path errors larger than 1 sigma have been observed so observers should be alert for primary occultations within plus or minus 3 sigma of the updated path.
Further, almost all asteroidal satellites discovered so far have been found within 10 diameters of the asteroid (since this distance is deep enough within the gravitational well to be stable over long timescales). Therefore, if monitoring for secondary events, observing out to about 10 path-widths either side of the predicted track remains worthwhile.
We therefore recommend that you monitor for events if your observing location is up to +/- 10 path-widths from the predicted track. If not monitoring for occultations by secondary bodies you should observe from locations within 3 sigma of the nominal path.
In terms of time, the predictions are now usually accurate to about +/- 0.3 minute so you should be most attentive during the predicted minute of the event. However if intending to catch a potential satellite occultation you should start observing at least 10 times the predicted central duration before the predicted closest approach time for your location, and continue for a similar period afterwards.
Centre Star Star Sun Path Limit1 Path Limit2 Error Limit1 Error Limit2
E. Longitude Latitude U.T. Alt Az Alt
o ' " o ' " h m s o o o o ' " o ' " o ' " o ' " o ' " o ' " o ' " o ' "
Longitude Latitude Longitude Latitude Longitude Latitude Longitude Latitude
147 52 58 -28 15 26 20 0 4 11 327 -9 147 40 11 -28 7 54 148 5 56 -28 23 12 147 10 3 -27 50 28 148 38 15 -28 42 57
145 19 3 -23 37 42 20 0 14 16 328 -10 145 9 1 -23 33 4 145 29 10 -23 42 25 144 45 1 -23 22 10 145 53 57 -23 54 11
143 36 43 -20 2 29 20 0 25 20 329 -11 143 27 48 -19 59 1 143 45 41 -20 6 0 143 6 23 -19 50 51 144 7 33 -20 14 42
142 18 50 -16 58 30 20 0 35 23 329 -12 142 10 33 -16 55 43 142 27 9 -17 1 20 141 50 37 -16 49 5 142 47 23 -17 8 20
141 15 43 -14 14 12 20 0 45 26 329 -12 141 7 51 -14 11 50 141 23 36 -14 16 35 140 48 54 -14 6 14 141 42 48 -14 22 29
140 22 38 -11 43 44 20 0 55 29 329 -12 140 15 4 -11 41 41 140 30 14 -11 45 48 139 56 48 -11 36 49 140 48 41 -11 50 55
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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