Core dynamo in mantle-stripped asteroids
Date Issued
2018
Author(s)
•
Federico, Costanzo
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•
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Abstract
Core dynamo is one of the most efficient mechanism to produce magnetic field in the planetary bodies as well as in the minor bodies of the solar system. It is interesting to study and to evaluate how the thickness and composition of the overlying rocky lid influences the thermal convective evolution of the core.
Coverage
European Planetary Science Congress 2018
Start page
EPSC2018-740
Conferenece
European Planetary Science Congress 2018
Conferenece place
Berlin, Germany
Conferenece date
16–21 September, 2018
Ads BibCode
2018EPSC...12..740F
Rights
open.access
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EPSC2018-740.pdf
Description
abstract
Size
94.09 KB
Format
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