resonant behaviour of comet halley & the orionid stream

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Resonant Behaviour of Comet Halley & the Orionid Stream Aswin Sekhar & David Asher Armagh Observatory United Kingdom EPSC 2012, Madrid

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Resonant Behaviour of Comet Halley & the Orionid Stream. Aswin Sekhar & David Asher Armagh Observatory United Kingdom. EPSC 2012, Madrid. Brief Background to the History of Comet 1P/Halley. * Observational records date back to 240 B. C. (Yeomans & Kiang 1981). - PowerPoint PPT Presentation

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Page 1: Resonant Behaviour of Comet Halley & the Orionid Stream

Resonant Behaviour of Comet Halley & the Orionid Stream

Aswin Sekhar & David Asher

Armagh Observatory

United Kingdom

EPSC 2012, Madrid

Page 2: Resonant Behaviour of Comet Halley & the Orionid Stream

Brief Background to the History of Comet 1P/Halley

* Observational records date back to 240 B. C. (Yeomans & Kiang 1981)

(Credit: MPS Germany/H. U. Keller)(Credit: W. Liller, International Halley Watch, 8 March 1986)

• Accurate orbital elements from 1404 B. C. (Yeomans & Kiang 1981)

• Physical life-time assumed to be about 200 revolutions (Whipple 1951)

* Dynamical life time of the order of 100,000 years (Hughes 1985, Hadjuk 1986, Steel 1987, Bailey & Emel’yanenko 1996)

Page 3: Resonant Behaviour of Comet Halley & the Orionid Stream

Brief Introduction to the Interesting Observations of Orionids

(Credit: S. Quirk)

•Orionids outbursts in 1993 and 2006 were unexpected

* Previous works explained the outburst in 2006 using 1:6 mean motion resonance with Jupiter (Rendtel 2007, Sato & Watanabe 2007)

Page 4: Resonant Behaviour of Comet Halley & the Orionid Stream

Our Present Work

•Halley itself was 1:6 resonant from about 1404 B.C. to 690 B.C.

Starting epoch here is 1404 B.C.

Page 5: Resonant Behaviour of Comet Halley & the Orionid Stream

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* Halley itself was 2:13 resonant from about 240 B.C. to 1700 A.D.

Starting epoch here is 240 B.C.

Page 6: Resonant Behaviour of Comet Halley & the Orionid Stream

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•Our present calculations show enhanced activity in 1916,1993 & 2070 due to 2:13 resonance mechanism and outbursts in 1436-1440, 1933-1938 & 2006-2010 from 1:6 resonance mechanism

• The simulations match the observational records for 1993 (Rendtel & Betlem 1993), 1916 (Olivier 1921), 2006-2010 (Rendtel 2008, IMO records), 1933-1938 (Lovell 1954) & 1436-1440 (Imoto & Hasegawa 1958) very well.

Page 7: Resonant Behaviour of Comet Halley & the Orionid Stream

•Halley’s orbit was substantially different about 12,000 years back

History of Comet’s Orbit

Starting epoch here is 240 B.C.

Page 8: Resonant Behaviour of Comet Halley & the Orionid Stream

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Page 9: Resonant Behaviour of Comet Halley & the Orionid Stream

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* This sudden change in orbit was due to close encounters with Jupiter

Starting epoch is 240 B.C.

Page 10: Resonant Behaviour of Comet Halley & the Orionid Stream

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Orbit positions 12,000 years back

Page 11: Resonant Behaviour of Comet Halley & the Orionid Stream

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Present Orbit

Page 12: Resonant Behaviour of Comet Halley & the Orionid Stream

Intended Future Work

• To develop an ejection model to populate meteoroids from 12,000 years in the past

Enough of interesting open problems to keep anyone occupied till 2061 (next apparition of Halley)

• To constrain the orbit of the comet using the ancient & present day meteor records

• Meteor showers can be an interesting source to tell us the positions of the comet beyond its recorded observations

• Look for diminished meteor rates in some years and treat them with same priority

* Negative observations could prove as valuable as enhanced meteor activity possibly

Page 13: Resonant Behaviour of Comet Halley & the Orionid Stream

THANK YOU