Evaluating changes in the elemental composition of micrometeorites during entry into the earth`s atmosphere
DRS at CSIR-National Institute of Oceanography
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Title |
Evaluating changes in the elemental composition of micrometeorites during entry into the earth`s atmosphere
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Creator |
Rudraswami, N.G.
ShyamPrasad, M. Dey, S. Plane, J.M.C. Feng, W. Taylor, S. |
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Subject |
CHEMISTRY AND BIOGEOCHEMISTRY
GEOLOGY AND GEOPHYSICS |
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Description |
We evaluate the heating of extraterrestrial particles entering the atmosphere using the comprehensive chemical ablation model (CABMOD). This model predicts the ablation rates of individual elements in a particle with a defined size, composition, entry velocity, and entry angle with respect to the zenith (ZA). In the present study, bulk chemical analyses of 1133 Antarctica micrometeorites (collected from the south pole water well) are interpreted using CABMOD. The marked spread in Fe/Si values in unmelted, partially melted, and melted micrometeorites is explained by the loss of relatively volatile Fe during atmospheric entry. The combined theoretical modeling and elemental composition of the micrometeorites (Mg/Si ratios) suggest that ~85% of particles have a provenance of carbonaceous chondrites, the remaining ~15% are either ordinary or enstatite chondrites. About 65% of the micrometeorites have undergone 11–21 km s-1
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Date |
2016-01-08T06:48:33Z
2016-01-08T06:48:33Z 2015 |
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Type |
Journal Article
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Identifier |
The Astrophysical Journal, vol.814; 2015; no.78 doi: 10.1088/0004-637X/814/1/78
no http://drs.nio.org/drs/handle/2264/4891 |
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Language |
en
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Relation |
Astrophys_J_814_1.jpg
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Rights |
Copyright [2015] The American Astronomical Society. An edited version of this paper was published by the Society. All efforts have been made to respect the copyright to the best of our knowledge. Inadvertent omissions, if brought to our notice, stand for correction and withdrawal of document from this repository.
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Publisher |
The American Astronomical Society
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