Occultation of BY Cancri (SAO 98054) by Saturn and its ring system

25th January 2006 (18h 05 UT - 20h 50m UT)

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

Occ. Start Occ. Finish
BY Cancri Occultation BY Cancri Occultation BY Cancri Occultation

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

Jon Harper
Email: occultation@popastro.com
Address in Popular Astronomy


Maintained by Jeff Stevens. Last modified 23rd December 2005.