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Updated: 2004 DEC 30, 04:24 UT
Event Rank : 75
(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 2005 Jan 30 UT, the 57 km diameter asteroid (611) Valeria will occult a 11.8 mag star in the constellation Cetus for observers along a path across New Zealand.
In the case of an occultation, the combined light of the asteroid and the star will drop by 2.6 mag to 14.2 mag (the magnitude of the asteroid) for at most 4.3 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 Limits Error Limits
E. Longitude Latitude U.T. Alt Az Alt Limit 1 Limit 2 Limit 3 Limit 4
o ' " o ' " h m s o o o o ' " o ' " o ' " o ' "
Longitude Longitude Longitude Longitude
153 3 56 -62 0 0 10 46 17 19 324 -2 154 34 44 151 35 18 156 57 27 149 24 18
153 47 5 -61 0 0 10 46 25 19 323 -3 155 16 4 152 20 15 157 35 57 150 11 55
154 33 26 -60 0 0 10 46 33 20 322 -4 156 0 51 153 8 8 158 18 20 151 2 8
155 22 53 -59 0 0 10 46 41 20 320 -5 156 49 0 153 58 54 159 4 30 151 54 53
156 15 26 -58 0 0 10 46 49 21 319 -6 157 40 29 154 52 31 159 54 23 152 50 10
157 11 3 -57 0 0 10 46 58 21 318 -7 158 35 16 155 49 0 160 48 0 153 48 0
158 9 48 -56 0 0 10 47 7 22 317 -8 159 33 26 156 48 23 161 45 22 154 48 25
159 11 45 -55 0 0 10 47 17 22 316 -9 160 35 2 157 50 45 162 46 35 155 51 31
Latitude Latitude Latitude Latitude
160 0 0 -54 15 21 10 47 24 22 314 -10 -55 33 42 -53 4 10 -57 53 31 -51 26 5
161 0 0 -53 22 7 10 47 33 22 313 -11 -54 36 37 -52 13 53 -56 47 7 -50 39 10
162 0 0 -52 31 15 10 47 42 22 312 -12 -53 42 25 -51 25 35 -55 45 18 -49 53 53
163 0 0 -51 42 33 10 47 50 22 311 -13 -52 50 50 -50 39 11 -54 47 21 -49 10 13
164 0 0 -50 55 54 10 47 59 22 309 -14 -52 1 38 -49 54 35 -53 52 44 -48 28 5
165 0 0 -50 11 10 10 48 7 22 308 -15 -51 14 38 -49 11 41 -53 1 3 -47 47 28
166 0 0 -49 28 15 10 48 15 22 307 -16 -50 29 42 -48 30 27 -52 12 2 -47 8 17
167 0 0 -48 47 4 10 48 23 22 306 -17 -49 46 42 -47 50 47 -51 25 26 -46 30 32
168 0 0 -48 7 34 10 48 31 22 305 -18 -49 5 34 -47 12 40 -50 41 5 -45 54 10
169 0 0 -47 29 40 10 48 39 22 304 -19 -48 26 10 -46 36 3 -49 58 50 -45 19 9
170 0 0 -46 53 20 10 48 46 21 303 -20 -47 48 28 -46 0 52 -49 18 33 -44 45 28
171 0 0 -46 18 30 10 48 54 21 301 -21 -47 12 24 -45 27 6 -48 40 9 -44 13 6
172 0 0 -45 45 7 10 49 1 21 300 -22 -46 37 53 -44 54 44 -48 3 31 -43 42 0
173 0 0 -45 13 11 10 49 8 20 299 -22 -46 4 54 -44 23 42 -47 28 36 -43 12 10
174 0 0 -44 42 39 10 49 15 20 298 -23 -45 33 24 -43 54 1 -46 55 20 -42 43 36
175 0 0 -44 13 28 10 49 21 20 297 -24 -45 3 20 -43 25 37 -46 23 39 -42 16 14
176 0 0 -43 45 38 10 49 27 19 296 -25 -44 34 40 -42 58 31 -45 53 30 -41 50 5
177 0 0 -43 19 6 10 49 34 19 295 -25 -44 7 23 -42 32 40 -45 24 52 -41 25 9
178 0 0 -42 53 52 10 49 40 18 294 -26 -43 41 27 -42 8 3 -44 57 40 -41 1 23
179 0 0 -42 29 55 10 49 45 18 294 -27 -43 16 50 -41 44 41 -44 31 54 -40 38 47
180 0 0 -42 7 12 10 49 51 17 293 -27 -42 53 31 -41 22 30 -44 7 31 -40 17 20
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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