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Distinguishing the Origin of Asteroid (16) Psyche.
Elkins-Tanton, Linda T; Asphaug, Erik; Bell, James F; Bierson, Carver J; Bills, Bruce G; Bottke, William F; Courville, Samuel W; Dibb, Steven D; Jun, Insoo; Lawrence, David J; Marchi, Simone; McCoy, Timothy J; Merayo, Jose M G; Oran, Rona; O'Rourke, Joseph G; Park, Ryan S; Peplowski, Patrick N; Prettyman, Thomas H; Raymond, Carol A; Weiss, Benjamin P; Wieczorek, Mark A; Zuber, Maria T.
Afiliación
  • Elkins-Tanton LT; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Asphaug E; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092 USA.
  • Bell JF; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Bierson CJ; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Bills BG; Jet Propulsion Laboratory, Pasadena, CA 91109 USA.
  • Bottke WF; Southwest Research Institute, Boulder, CO 80302 USA.
  • Courville SW; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Dibb SD; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Jun I; Jet Propulsion Laboratory, Pasadena, CA 91109 USA.
  • Lawrence DJ; Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
  • Marchi S; Southwest Research Institute, Boulder, CO 80302 USA.
  • McCoy TJ; Smithsonian National Museum of Natural History, Washington, DC 20013 USA.
  • Merayo JMG; National Space Institute, Danish Technical University, Lyngby, Denmark.
  • Oran R; Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.
  • O'Rourke JG; School of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
  • Park RS; Jet Propulsion Laboratory, Pasadena, CA 91109 USA.
  • Peplowski PN; Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
  • Prettyman TH; Planetary Science Institute, Tucson, AZ 85719 USA.
  • Raymond CA; Jet Propulsion Laboratory, Pasadena, CA 91109 USA.
  • Weiss BP; Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.
  • Wieczorek MA; Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Université Côte d'Azur, Nice, France.
  • Zuber MT; Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.
Space Sci Rev ; 218(3): 17, 2022.
Article en En | MEDLINE | ID: mdl-35431348
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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Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2022 Tipo del documento: Article

Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2022 Tipo del documento: Article