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Contrasting Size Distributions of Chondrules and Inclusions in Allende CV3There are several leading theories on the processes that led to the formation of chondrites, e.g., sorting by mass, by X-winds, turbulent concentration, and by photophoresis. The juxtaposition of refractory inclusions (CAIs) and less refractory chondrules is central to these theories and there is much to be learned from their relative size distributions. There have been a number of studies into size distributions of particles in chondrites but only on relatively small scales primarily for chondrules, and rarely for both Calcium Aluminum-rich Inclusions (CAIs) and chondrules in the same sample. We have implemented macro-scale (25 cm diameter sample) and high-resolution microscale sampling of the Allende CV3 chondrite to create a complete data set of size frequencies for CAIs and chondrules.
Document ID
20140012796
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Fisher, Kent R.
(Cincinnati Univ. OH, United States)
Tait, Alastair W.
(Monash Univ. Clayton, Australia)
Simon, Jusin I.
(NASA Johnson Space Center Houston, TX, United States)
Cuzzi, Jeff N.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
October 2, 2014
Publication Date
March 17, 2014
Subject Category
Geophysics
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-30403
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 17, 2014
End Date: March 21, 2014
Sponsors: Universities Space Research Association, NASA Johnson Space Center, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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