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Updated: 2009 AUG 20, 18:09 UT
Event Rank : 49
(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 Sep 02 UT, the 77 km diameter asteroid (61) Danae will occult a 13.3 mag star in the constellation Scorpius for observers along a path across Australia, from Princess Charlotte Bay across western Queensland and central South Australia Ceduna, and across New Guinea near Lae.
In the case of an occultation, the combined light of the asteroid and the star will drop by 0.4 mag to 12.5 mag (the magnitude of the asteroid) for at most 6.1 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 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
152 21 30 3 0 0 11 30 7 35 216 -53 152 45 37 151 57 25 153 49 29 150 54 2
151 48 49 2 0 0 11 30 1 36 216 -53 152 12 51 151 24 49 153 16 31 150 21 37
151 16 28 1 0 0 11 29 55 37 216 -53 151 40 26 150 52 31 152 43 55 149 49 28
150 44 24 0 0 0 11 29 49 38 216 -53 151 8 20 150 20 31 152 11 40 149 17 36
150 12 38 - 1 0 0 11 29 42 40 216 -52 150 36 31 149 48 47 151 39 44 148 45 58
Latitude Latitude Latitude Latitude
149 0 0 - 3 18 53 11 29 27 42 217 -51 - 4 4 52 - 2 33 7 - 6 7 29 - 0 33 19
148 0 0 - 5 15 9 11 29 13 44 217 -51 - 6 1 38 - 4 28 55 - 8 5 31 - 2 27 54
147 0 0 - 7 12 32 11 28 59 46 218 -50 - 7 59 26 - 6 25 52 -10 4 27 - 4 23 45
146 0 0 - 9 10 41 11 28 45 49 218 -49 - 9 57 57 - 8 23 39 -12 3 57 - 6 20 34
145 0 0 -11 9 16 11 28 30 51 219 -48 -11 56 51 -10 21 56 -14 3 40 - 8 18 2
144 0 0 -13 7 57 11 28 14 53 220 -47 -13 55 46 -12 20 22 -16 3 13 -10 15 49
143 0 0 -15 6 20 11 27 58 55 220 -45 -15 54 19 -14 18 35 -18 2 13 -12 13 35
142 0 0 -17 4 5 11 27 42 57 222 -44 -17 52 10 -16 16 15 -20 0 17 -14 10 57
141 0 0 -19 0 50 11 27 25 59 223 -43 -19 48 56 -18 12 58 -21 57 5 -16 7 35
140 0 0 -20 56 14 11 27 8 62 224 -42 -21 44 17 -20 8 24 -23 52 15 -18 3 8
139 0 0 -22 49 57 11 26 51 64 226 -40 -23 37 52 -22 2 14 -25 45 27 -19 57 15
138 0 0 -24 41 40 11 26 35 66 228 -39 -25 29 23 -23 54 9 -27 36 24 -21 49 39
137 0 0 -26 31 7 11 26 18 67 230 -38 -27 18 33 -25 43 52 -29 24 50 -23 40 1
136 0 0 -28 18 3 11 26 1 69 232 -37 -29 5 9 -27 31 8 -31 10 30 -25 28 7
135 0 0 -30 2 16 11 25 45 71 235 -35 -30 48 58 -29 15 44 -32 53 14 -27 13 41
134 0 0 -31 43 34 11 25 28 73 238 -34 -32 29 50 -30 57 29 -34 32 52 -28 56 34
133 0 0 -33 21 51 11 25 12 74 242 -33 -34 7 37 -32 36 15 -36 9 17 -30 36 35
132 0 0 -34 56 59 11 24 57 76 247 -32 -35 42 13 -34 11 55 -37 42 25 -32 13 36
131 0 0 -36 28 55 11 24 42 77 252 -30 -37 13 34 -35 44 25 -39 12 13 -33 47 33
130 0 0 -37 57 36 11 24 27 78 258 -29 -38 41 39 -37 13 41 -40 38 40 -35 18 22
129 0 0 -39 23 1 11 24 12 79 266 -28 -40 6 27 -38 39 44 -42 1 47 -36 46 0
128 0 0 -40 45 12 11 23 58 80 274 -27 -41 27 59 -40 2 32 -43 21 35 -38 10 27
Uncertainty in time = +/- 8 secs
Prediction of 2009 Aug 21.0
Use these links for further information:
[Planetary Occultations]
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[Observing Details]
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