Updated: 2009 JUL 08, 13:38 UT
Event Rank : 33
(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 2009 Jul 20 UT, the 21 km diameter asteroid (2259) Sofievka will occult a 11.1 mag star in the constellation Scorpius for observers along a path that may graze the east coast of New Zealand.
In the case of an occultation, the combined light of the asteroid and the star will drop by 4.2 mag to 15.3 mag (the magnitude of the asteroid) for at most 6.0 seconds.
This update is based on UNSO/Flagstaff astrometry for the asteroid kindly provided by Alice Monet, 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 173 18 43 -47 11 6 14 38 44 18 256 -53 172 53 12 -47 13 48 173 44 35 -47 8 15 171 13 55 -47 23 5 175 32 34 -46 54 55 173 50 18 -46 28 53 14 39 3 17 255 -53 173 24 27 -46 31 50 174 16 33 -46 25 45 171 44 1 -46 42 4 176 6 23 -46 11 10 174 24 10 -45 45 52 14 39 22 17 254 -53 173 57 53 -45 49 7 174 50 53 -45 42 25 172 16 1 -46 0 25 176 43 1 -45 26 23 175 0 34 -45 1 55 14 39 41 16 254 -53 174 33 44 -45 5 30 175 27 52 -44 58 6 172 50 5 -45 18 0 177 22 53 -44 40 22 175 39 50 -44 16 52 14 40 1 15 253 -53 175 12 20 -44 20 51 176 7 52 -44 12 38 173 26 27 -44 34 45 178 6 31 -43 52 52 176 22 24 -43 30 32 14 40 20 14 252 -53 175 54 4 -43 35 0 176 51 20 -43 25 48 174 5 25 -43 50 30 178 54 37 -43 3 35 177 8 51 -42 42 40 14 40 39 14 252 -53 176 39 27 -42 47 41 177 38 56 -42 37 19 174 47 21 -43 5 6 179 48 13 -42 12 2 177 59 56 -41 52 53 14 40 58 13 251 -52 177 29 11 -41 58 36 178 31 32 -41 46 47 175 32 44 -42 18 19 -179 11 8 -41 17 33 178 56 49 -41 0 42 14 41 18 12 250 -52 178 24 16 -41 7 18 179 30 25 -40 53 37 176 22 11 -41 29 53 -178 0 57 -40 19 0 -179 58 47 -40 5 20 14 41 37 11 249 -52 179 26 11 -40 13 8 -179 22 22 -39 56 55 177 16 36 -40 39 23 -176 36 39 -39 14 23 -178 44 3 -39 5 34 14 41 56 9 248 -51 -179 22 42 -39 15 2 -178 3 22 -38 55 10 178 17 16 -39 46 16 -174 47 51 -37 59 8 Uncertainty in time = +/- 14 secs Prediction of 2009 Jul 8.0
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