NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The Viking magnetic properties experiment - Primary mission resultsThree permanent magnet arrays were mounted on each Viking lander: a strong array fixed on a photometric reference test chart on top of the landers; and two arrays, one strong and one weak, incorporated into the backhoe of the surface sampler. Some or all of the magnetic particles detected could be highly magnetic unoxidized mineral grains (metallic Fe, magnetite, pyrrhotite) forming the core beneath a reddish coating of limonite or hematite; or grains composed of gamma-Fe2O3, with and without other iron oxides; or igneous rock (or mineral particles) which consist of an admixture of unweathered silicate material or minerals with a significant fraction of highly magnetic phase, again with a reddish coating; they could be also igneous rock or mineral particles, intrinsically nonmagnetic, but having a reddish coating containing gamma-Fe2O3; or clay mineral particles which contain and/or are coated with Fe2O3, of which a substantial fraction is in the gamma-Fe2O3 form.
Document ID
19780027532
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hargraves, R. B.
(Princeton University Princeton, N.J., United States)
Collinson, D. W.
(Newcastle-upon-Tyne, University Newcastle-upon-Tyne, United Kingdom)
Arvidson, R. E.
(Washington University St. Louis, Mo., United States)
Spitzer, C. R.
(NASA Langley Research Center Hampton, Va., United States)
Date Acquired
August 9, 2013
Publication Date
September 30, 1977
Publication Information
Publication: Journal of Geophysical Research
Volume: 82
Subject Category
Lunar And Planetary Exploration
Accession Number
78A11441
Funding Number(s)
CONTRACT_GRANT: NAS1-9705
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available