This event is going to take place during the evening of Wednesday, 25th January,
a few days before Saturn's 2006 opposition, and should be quite spectacular
telescopically, particularly as SAO 98054, at m(v) 7.9 is a little brighter than
Titan. The occultation presents an interesting challenge for both amateurs who use
CCD's for imaging, and also for those who sketch what they see. It is of course
reasonably rare for a star of this magnitude to be occulted by the Saturnian System,
and I do hope that you will want to take up the challenge.
The occultation had been noted last summer by Dr Tolis Christou of the Armagh
Observatory in Northern Ireland, but very little information has been distributed
as yet.
My own predicted data relating to the event for central UK (using Guide 8 software)
is as follows:
Occultation by Ring A: 18h 50m (all times = UT).
Reappearance in Cassini's Division: 19h 01m.
Disappearance behind Ring B: 19h 06m.
Possible brief reappearance in Cassini's Division prior to occultation by Saturn's disk: 20h 03m.
Reappearance from behind the disk in the vicinity of Saturn's South Pole (PA = 166°): 20h 50m.
I am encouraging all members of the SPA to attempt observing this interesting occultation,
and hopefully some of you may try imaging it, especially during the Cassini "window"
around 19h 01m - 19h 06m.
The following information is from David Herald, Canberra, Australia:
This is a known event, but there hasn't been much publicity about it. The following
are predictions from winOccult for a range of locations in Europe. The predictions
below are topocentric. Note that the ring numbers are the edges of the various rings,
with ring 4 and ring 3 defining the Cassini gap. Also, ring events that occur when
the star is behind Saturn have not been excluded, and for many locations 'reappearance'
events of the star through the ring structure occur before the occultation by the planet.
The occultation by Saturn will be visible from Europe, Africa and Asia - although
South Africa will get a miss. There are no occultations by the rings after the
planetary occultation, but an extensive passage through the rings before the occultation.
That passage will occur at low altitude in Europe, but will also be visible in Japan
and Australia.
One of the challenges for this event will be in detecting the star. At Mv=7.9, Mp=8.1,
the star is only marginally brighter than Titan (mag 8.4 on that date). Note that the
surface brightness of Titan is about the same as the planet and rings A and B, Note
that passage through Ring C might be more readily visible, but the star does not pass
through Ring C for any location on the Earth. The greater challenge will be to get a
decent recording of the event - and appropriate filtering might be highly desirable.
|
Location
|
Ring 5 |
Ring 4 |
Ring 3 |
Ring 2 |
Ring 1 |
D |
R |
Ring 1 |
Ring 2 |
Ring 3 |
Ring 4 |
Ring 5 |
| Aberdeen |
18h 45.0m |
18h 57.0m |
19h 1.6m |
- |
- |
20h 6.9m |
20h 51.2m |
- |
- |
20h 9.7m |
20h 14.3m |
20h 26.3m |
| Belfast |
18h 45.2m |
18h 57.3m |
19h 1.9m |
- |
- |
20h 7.4m |
20h 51.1m |
- |
- |
20h 9.4m |
20h 14.0m |
20h 26.1m |
| Birmingham |
18h 45.3m |
18h 57.5m |
19h 2.2m |
- |
- |
20h 7.8m |
20h 50.7m |
- |
- |
20h 8.7m |
20h 13.3m |
20h 25.5m |
| Bristol |
18h 45.3m |
18h 57.6m |
19h 2.3m |
- |
- |
20h 7.9m |
20h 50.7m |
- |
- |
20h 8.5m |
20h 13.2m |
20h 25.4m |
| Dublin |
18h 45.3m |
18h 57.4m |
19h 2.1m |
- |
- |
20h 7.6m |
20h 51.0m |
- |
- |
20h 9.1m |
20h 13.8m |
20h 25.9m |
| Glasgow |
18h 45.1m |
18h 57.2m |
19h 1.8m |
- |
- |
20h 7.1m |
20h 51.2m |
- |
- |
20h 9.6m |
20h 14.1m |
20h 26.2m |
| Liverpool |
18h 45.2m |
18h 57.4m |
19h 2.1m |
- |
- |
20h 7.6m |
20h 50.9m |
- |
- |
20h 8.9m |
20h 13.6m |
20h 25.7m |
| London |
18h 45.3m |
18h 57.6m |
19h 2.3m |
- |
- |
20h 7.9m |
20h 50.5m |
- |
- |
20h 8.3m |
20h 13.0m |
20h 25.3m |
| Newcastle upon Tyne |
18h 45.1m |
18h 57.3m |
19h 1.9m |
- |
- |
20h 7.3m |
20h 51.0m |
- |
- |
20h 9.2m |
20h 13.8m |
20h 25.9m |
| Plymouth |
18h 45.4m |
18h 57.7m |
19h 2.4m |
- |
- |
20h 8.1m |
20h 50.6m |
- |
- |
20h 8.3m |
20h 13.0m |
20h 25.3m |
All times are UT.
Click on the preview images below to see the full size version
Note about BY Cancri ( SAO 98054)
This star lies at the edge of the 'Beehive Open Cluster' M44, and is is is a
Delta Scuti type variable star, with a small amplitude of only 0.01. It is a
white star of spectral type A5, and so should show up nicely against the dusky
tint of Saturn's South Polar region after the star's reappearance at 20h 03m.
Please visit the UK's definitive site for lunar and asteroidal occultations:
www.asterocc.org.uk