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Dust Production of Comet 21P/Giacobini Zinner Using Broadband PhotometryComet 21P/Giacobini-Zinner is a Jupiter family comet that was discovered in December of 1900 by the French astronomer Michel Giacobini, and rediscovered two orbits later by German astronomer Ernst Zinner in 1913. 21P is approximately 2 km in diameter, and is the parent of the Draconids, a meteor shower known to undergo dramatic outbursts. In 1933 and 1946, up to 10,000 meteors per hour were reported for the Draconids; and 2011 saw a minor Draconid outburst. As meteor stream modeling/ forecasting is a primary focus for the NASA Meteoroid Environment Office, it was decided to monitor 21P for three purposes: firstly to find the apparent and absolute magnitude with respect to heliocentric distance; second to calculate Af(rho), a quantity that describes the dust production rate and is used in models to predict the activity of the Draconids; thirdly to detect possible increases in cometary activity, which could correspond to future Draconid meteor outbursts. Giacobini-Zinner is unique in several ways. It was the first comet to have measurements made in situ. Comet 21P was visited by ICE (International Cometary Explorer) in 1985 to study the interaction of the cometary atmosphere with the flowing solar-wind plasma. It is a carbon-depleted comet, and most studies show that it peaks in gas and dust production pre-perihelion, specifically in two very studied passages; 1985 and 1998. A prior study was conducted by Pittichova et al (2008) for 21P during its 2004-2006 close approach to the Sun. Apparent and absolute magnitudes were measured at various heliocentric distances as well as the dust production. At 2.32 AU from the Sun, 21P exhibited an apparent magnitude of 17.05 and Af of 83 cm, and an apparent magnitude of 15.91/Af(rho) of 130.66 cm at 1.76 AU. Another such study performed by Lara et al.on 21P s 1998 apparition found values of Af(rho) of 1010 cm when 1.05 AU from the Sun, two weeks before perihelion, and 669 cm at perihelion, when 1.03 AU from the Sun
Document ID
20120014971
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Blaauw, Rhiannon
(Dynetics, Inc. Huntsville, AL, United States)
Suggs, Robert M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cooke, William
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 26, 2013
Publication Date
May 16, 2012
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
M12-1690
Report Number: M12-1690
Meeting Information
Meeting: Asteroids, Comets, Meteors (ACM) 2012
Location: Niigata
Country: Japan
Start Date: May 16, 2012
End Date: May 20, 2012
Sponsors: Lunar and Planetary Inst.
Funding Number(s)
CONTRACT_GRANT: NNM10AA03C
Distribution Limits
Public
Copyright
Public Use Permitted.
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