The formation and evolution of Asteroids
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The formation and evolution of Asteroids
CoPED ID
f434b1cd-8a2a-484a-9461-d77dc0ec45aa
Status
Closed
Value
No funds listed.
Start Date
Sept. 30, 2016
End Date
Sept. 29, 2020
Description
The aim of this project is to characterise the mineralogical and chemical properties of the thermally altered CI and CM chondrites. The project will use X-ray diffraction (XRD), thermogravimetric analysis (TGA) and trace element abundance measurements. Results will be placed in the context of hydration and dynamic heating experiments aimed at understanding the timescales for the mineralogical changes. In addition, the student will measure the infrared signatures associated with altered and un-altered samples under Earth-like and asteroid-like conditions.
University of Oxford | LEAD_ORG |
Sara Russell | SUPER_PER |
Helena Bates | STUDENT_PER |
Subjects by relevance
- Measurement
- Measuring methods
Extracted key phrases
- Trace element abundance measurement
- Mineralogical change
- Dynamic heating experiment
- Aim
- Project
- Chemical property
- Cm chondrite
- Formation
- Infrared signature
- Ray diffraction
- Thermogravimetric analysis
- Asteroids