On the asteroidal conductivities as inferred from meteorites

W. H. Ip, F. Herbert

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

Solar wind interactions with planetary bodies without intrinsic magnetic fields depend to a large extent on the electrical conductivities of the objects in question. If the combined (i.e., ionospheric and interior) electrical conductivities are large, as in the case of Venus, the solar wind interaction is strong due to the generation of a large electrical current flow. It is suggested here that a similar interaction may occur at some asteroids, if their interior conductivity can be approximated by the conductivities of carbonaceous or iron-bearing meteorites. This interaction, in turn, can be used as a tool for remote sensing of the asteroidal interior properties in a spacecraft mission to asteroids.

Original languageEnglish
Pages (from-to)43-47
Number of pages5
JournalThe Moon and the Planets
Volume28
Issue number1
DOIs
StatePublished - Feb 1983

Fingerprint

Dive into the research topics of 'On the asteroidal conductivities as inferred from meteorites'. Together they form a unique fingerprint.

Cite this