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Microstructures of Hibonite From an ALH A77307 (CO3.0) CAI: Evidence for Evaporative Loss of CalciumHibonite is a comparatively rare, primary phase found in some CAIs from different chondrite groups and is also common in Wark-Lovering rims [1]. Hibonite is predicted to be one of the earliest refractory phases to form by equilibrium condensation from a cooling gas of solar composition [2] and, therefore, can be a potential recorder of very early solar system processes. In this study, we describe the microstructures of hibonite from one CAI in ALH A77307 (CO3.0) using FIB/TEM techniques in order to reconstruct its formational history.
Document ID
20140010679
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Han, Jangmi
(Lunar and Planetary Inst. Houston, TX, United States)
Brearley, Adrian J.
(New Mexico Univ. Albuquerque, NM, United States)
Keller, Lindsay P.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 15, 2014
Publication Date
January 1, 2014
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-31840
Report Number: JSC-CN-31840
Meeting Information
Meeting: Annual Meeting of the Meteoritical Society
Location: Casablanca
Country: Morocco
Start Date: September 7, 2014
End Date: September 12, 2014
Sponsors: Meteoritical Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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