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First Occultation of Kuiper Belt Object 31 Dec 2005
- eansbro
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- Red Giant
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19 years 1 week ago #20868
by eansbro
First Occultation of Kuiper Belt Object 31 Dec 2005 was created by eansbro
First ever occultation of an Edgeworth Kuiper Belt Object called 20000 Varuna since the Pluto/Charon occultation will occur on 31 December, 2005. Varuna will occult star UCAC - 40675770 RA 7h 11m 6.9s, dec +25 9.51m from 6h 16m to 6h 23m UT. The star is actually 6 degrees from Castor in the constellation Gemini. The duration of the occultation is 35 seconds.
Varuna was discovered in recent times and was one of the biggest EKBOs with a diameter of 900 km. However, recent albedo observations from Chile suggests that it may be alot bigger at around 1500 km. This would make Varuna one of the 3 biggest EKBOs known. There has never been an occultation within the annals, hence the importance of this one.
This is going to be the first occultation of an EKBO and in particular one of the largest ones makes this an exciting challenge to record/time this event. The reason to record this event by accurate timing is to obtain a diameter. Albedo observations have a weaker determination as compared to a timing of an occultation. It is quite possible that if an accurate timing is successfully done the diameter could even be bigger than the other two.
It was only yesterday that final orbital calculations indicates that even with a degree of uncertainty the occultation path will go through Ireland. I did some calculations which indicate that we have a 12% of a probable certainty of this event throughout Ireland. However, if the diameter is 1500 km the certainty will be improved to 20%.
Nevertheless for the observers using integrating video or CCD
windowing, the 40 ±5 ? s expected occultation could be detected
by pushing the integration time to 3, 5 or even 10 sec., depending
on the telescope size.
If you are using a Meade 10 inch or C11 telescope and a Watec 120N or similar video camera (integrating camera) could detect V= 15.7 (probably R~ 15.1) with 3 sec. integrations with average 3 secs arc seeing in Ireland used the f/10 focus, i.e. no focal reducer. Using 10 sec integration will get down to 16.5 mag.
If anybody is interested I have some field charts for the area.
Good luck and clear skies
Eamonn A
Varuna was discovered in recent times and was one of the biggest EKBOs with a diameter of 900 km. However, recent albedo observations from Chile suggests that it may be alot bigger at around 1500 km. This would make Varuna one of the 3 biggest EKBOs known. There has never been an occultation within the annals, hence the importance of this one.
This is going to be the first occultation of an EKBO and in particular one of the largest ones makes this an exciting challenge to record/time this event. The reason to record this event by accurate timing is to obtain a diameter. Albedo observations have a weaker determination as compared to a timing of an occultation. It is quite possible that if an accurate timing is successfully done the diameter could even be bigger than the other two.
It was only yesterday that final orbital calculations indicates that even with a degree of uncertainty the occultation path will go through Ireland. I did some calculations which indicate that we have a 12% of a probable certainty of this event throughout Ireland. However, if the diameter is 1500 km the certainty will be improved to 20%.
Nevertheless for the observers using integrating video or CCD
windowing, the 40 ±5 ? s expected occultation could be detected
by pushing the integration time to 3, 5 or even 10 sec., depending
on the telescope size.
If you are using a Meade 10 inch or C11 telescope and a Watec 120N or similar video camera (integrating camera) could detect V= 15.7 (probably R~ 15.1) with 3 sec. integrations with average 3 secs arc seeing in Ireland used the f/10 focus, i.e. no focal reducer. Using 10 sec integration will get down to 16.5 mag.
If anybody is interested I have some field charts for the area.
Good luck and clear skies
Eamonn A
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- DaveGrennan
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19 years 1 week ago #20870
by DaveGrennan
Regards and Clear Skies,
Dave.
J41 - Raheny Observatory.
www.webtreatz.com
Equipment List here
Replied by DaveGrennan on topic Re: First Occultation of Kuiper Belt Object 31 Dec 2005
I saw this circular and have been thinking of how I could do this with my modified webcam or DSLR. I can get down to mag 16 easy with both but I'll have to do some tests to see how quickly I can get that deep. If I can get that deep in say 15-20 seconds then I could use the autoguider to nudge the scope every 15 secs about 3 arcsecs that would have the effect of causing the star to draw a line and record any dimming.
All depends on the weather of course!
All depends on the weather of course!
Regards and Clear Skies,
Dave.
J41 - Raheny Observatory.
www.webtreatz.com
Equipment List here
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- johnflannery
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- Super Giant
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19 years 1 week ago #20873
by johnflannery
Replied by johnflannery on topic Re: First Occultation of Kuiper Belt Object 31 Dec 2005
I'm holding out for an occultation of a magnitude 6.5 star in Aquarius by a binary Trans-Neptunian Object - 1999 RZ253 - on October 4th, 2007. Alas, it's in daylight for Irish observers but one worth travelling somewhere for I think, considering its a once in a millenium event!
John
John
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