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Using Dust Shed from Asteroids as Microsamples to Link Remote Measurements with Meteorite ClassesGiven the diversity of asteroids, it is impossible to consider returning samples from each one• Dust particles are abundant around asteroids• Primary minerals and organic materials can be measured by in situ dust detectorinstruments• These particles can be used to classify the parent body as an ordinary chondrite,basaltic achondrite, or other class of meteorite• Such instruments could provide direct links to known meteorite groups withoutreturning the samples to terrestrial laboratories
Document ID
20190000494
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
Cohen, B. A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Richardson, J. A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Szalay, J. R.
(Princeton Univ. Princeton, NJ, United States)
Rivkin, A. S.
(Johns Hopkins Univ. Laurel, MD, United States)
Kilma, R. E.
(Johns Hopkins Univ. Laurel, MD, United States)
Ernst, C. M.
(Johns Hopkins Univ. Laurel, MD, United States)
Chabot, N. L.
(Johns Hopkins Univ. Laurel, MD, United States)
Sternovsky, Z.
(Colorado Univ. Boulder, CO, United States)
Horanyi, M.
(Colorado Univ. Boulder, CO, United States)
Date Acquired
February 9, 2019
Publication Date
December 14, 2018
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN64415
Meeting Information
Meeting: American Geophysical Union (AGU) Fall Meeting
Location: Washington, DC
Country: United States
Start Date: December 10, 2018
End Date: December 14, 2018
Sponsors: American Geophysical Union (AGU)
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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