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Dust Production of Comet 21P/Giacobini-Zinner using Broadband PhotometryPresented here are results from photometric analysis on broadband images taken of Comet 21P/Giacobini-Zinner from May 24, 2011 to October 24, 2011. As the parent body of the Draconids, a meteor shower known for outbursting, 21P was studied for its dust production activity, Afrho, focusing on how it changes with heliocentric distance. An expected increase in dust production with a decrease in heliocentric distance was observed. The comet went from heliocentric distance of 3.05 AU to 1.77 AU during the observed time that corresponded to an apparent magnitude of 19.61 to 15.72 and Afrho of 16.48 cm to 284.17 cm. These values can be extrapolated to estimate a peak Afrho value at perihelion of 3824 cm. The images were obtained using a 0.5-meter f/8.1 Ritchey-Chretien telescope located in Mayhill, New Mexico.
Document ID
20130013031
Acquisition Source
Marshall Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Blaauw, Rhiannon C.
(Dynetics Technical Services Huntsville, AL, United States)
Suggs, Robert M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cooke, William J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 27, 2013
Publication Date
January 1, 2012
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
M12-2124
Report Number: M12-2124
Funding Number(s)
CONTRACT_GRANT: NNM10AA03C
Distribution Limits
Public
Copyright
Public Use Permitted.
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