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Elkins-Tanton LT, Asphaug E, Bell JF, Bierson CJ, Bills BG, Bottke WF, Courville SW, Dibb SD, Jun I, Lawrence DJ, Marchi S, McCoy TJ, Merayo JMG, Oran R, O’Rourke JG, Park RS, Peplowski PN, Prettyman TH, Raymond CA, Weiss BP, Wieczorek MA, Zuber MT. Distinguishing the Origin of Asteroid (16) Psyche. SPACE SCIENCE REVIEWS 2022; 218:17. [PMID: 35431348 PMCID: PMC9005435 DOI: 10.1007/s11214-022-00880-9] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/06/2021] [Accepted: 03/16/2022] [Indexed: 06/02/2023]
Abstract
The asteroid (16) Psyche may be the metal-rich remnant of a differentiated planetesimal, or it may be a highly reduced, metal-rich asteroidal material that never differentiated. The NASA Psyche mission aims to determine Psyche's provenance. Here we describe the possible solar system regions of origin for Psyche, prior to its likely implantation into the asteroid belt, the physical and chemical processes that can enrich metal in an asteroid, and possible meteoritic analogs. The spacecraft payload is designed to be able to discriminate among possible formation theories. The project will determine Psyche's origin and formation by measuring any strong remanent magnetic fields, which would imply it was the core of a differentiated body; the scale of metal to silicate mixing will be determined by both the neutron spectrometers and the filtered images; the degree of disruption between metal and rock may be determined by the correlation of gravity with composition; some mineralogy (e.g., modeled silicate/metal ratio, and inferred existence of low-calcium pyroxene or olivine, for example) will be detected using filtered images; and the nickel content of Psyche's metal phase will be measured using the GRNS.
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Affiliation(s)
- Linda T. Elkins-Tanton
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | - Erik Asphaug
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092 USA
| | - James F. Bell
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | - Carver J. Bierson
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | | | | | - Samuel W. Courville
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | - Steven D. Dibb
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | - Insoo Jun
- Jet Propulsion Laboratory, Pasadena, CA 91109 USA
| | - David J. Lawrence
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA
| | | | - Timothy J. McCoy
- Smithsonian National Museum of Natural History, Washington, DC 20013 USA
| | - Jose M. G. Merayo
- National Space Institute, Danish Technical University, Lyngby, Denmark
| | - Rona Oran
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA
| | - Joseph G. O’Rourke
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA
| | - Ryan S. Park
- Jet Propulsion Laboratory, Pasadena, CA 91109 USA
| | | | | | | | - Benjamin P. Weiss
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA
| | - Mark A. Wieczorek
- Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Université Côte d’Azur, Nice, France
| | - Maria T. Zuber
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA
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