An Approach to Magnetic Cleanliness for the Psyche Mission M. de Soria-Santacruz J. Ream K. Ascrizzi (
[email protected]), (
[email protected]), (
[email protected]) M. Soriano R. Oran University of Michigan Ann Arbor (
[email protected]), (
[email protected]), 500 S State St O. Quintero B. P. Weiss Ann Arbor, MI 48109 (
[email protected]), (
[email protected]) F. Wong Department of Earth, Atmospheric, (
[email protected]), and Planetary Sciences S. Hart Massachusetts Institute of Technology (
[email protected]), 77 Massachusetts Avenue M. Kokorowski Cambridge, MA 02139 (
[email protected]) B. Bone (
[email protected]), B. Solish (
[email protected]), D. Trofimov (
[email protected]), E. Bradford (
[email protected]), C. Raymond (
[email protected]), P. Narvaez (
[email protected]) Jet Propulsion Laboratory, California Institute of Technology 4800 Oak Grove Drive Pasadena, CA 91109 C. Keys C. Russell L. Elkins-Tanton (
[email protected]), (
[email protected]), (
[email protected]) P. Lord University of California Los Angeles Arizona State University (
[email protected]) 405 Hilgard Avenue PO Box 871404 Maxar Technologies Inc. Los Angeles, CA 90095 Tempe, AZ 85287 3825 Fabian Avenue Palo Alto, CA 94303 Abstract— Psyche is a Discovery mission that will visit the fields. Limiting and characterizing spacecraft-generated asteroid (16) Psyche to determine if it is the metallic core of a magnetic fields is therefore essential to the mission. This is the once larger differentiated body or otherwise was formed from objective of the Psyche’s magnetics control program described accretion of unmelted metal-rich material.