In situ geochronology as a mission-enabling technology
Abstract
Although there are excellent estimates of ages of terrains on Mars from crater counting, even a few absolute ages would serve to validate the calibration. Results with uncertainties, although much larger than those that could be achieved in labs on Earth, would be extremely valuable. While there are other possibilities for in situ geochronology instruments, we describe here two alternative technologies, being developed in JPL. There are two common features of both. The first is analysis by means of miniature mass spectrometer. The second is use of laser sampling to reduce or avoid sample handling, preparation and pre-treatment and equally importantly, to allow analysis of individual, texturally resolved minerals in coarse-grained rocks. This textural resolution will aid in selection of grains more or less enriched in the relevant elements and allow construction of isochrons for more precise dating. Either of these instruments could enable missions to Mars and other planetary bodies.
Additional Information
© 2012 IEEE. This work was carried out at the Jet Propulsion Laboratory (JPL), California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA), supported in part by both The Keck Institute for Space Studies and the JPL Research and Technology Development programs.Attached Files
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Additional details
- Eprint ID
- 64922
- DOI
- 10.1109/AERO.2012.6187053
- Resolver ID
- CaltechAUTHORS:20160301-135518164
- Keck Institute for Space Studies (KISS)
- JPL Research and Technology Development Fund
- NASA/JPL/Caltech
- Created
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2016-03-02Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Keck Institute for Space Studies