Evidence map›Paper›PMID 35431348›Full record

ReviewSpace science reviews2022

Distinguishing the Origin of Asteroid (16) Psyche.

Linda T Elkins-Tanton, Erik Asphaug, James F Bell, Carver J Bierson, Bruce G Bills, William F Bottke, Samuel W Courville, Steven D Dibb, Insoo Jun, David J Lawrence and 12 more

Abstract readReview
In one paragraph

Review in Space science reviews, 2022. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 11 papers.

0numbers the graph read from it
0cells of the map it votes in
11citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

11 citing papers in PubMed.

  1. Article
  2. Article
  3. Review
  4. Review
  5. Review
  6. The Psyche Light Elements Investigation.Space science reviews · 2025
    Review
  7. Article
  8. The Psyche Magnetometry Investigation.Space science reviews · 2023
    Review
  9. Review
  10. Article
  11. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

22 authors.

Linda T Elkins-TantonSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Erik AsphaugLunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092 USA.
James F BellSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Carver J BiersonSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Bruce G BillsJet Propulsion Laboratory, Pasadena, CA 91109 USA.
William F BottkeSouthwest Research Institute, Boulder, CO 80302 USA.
Samuel W CourvilleSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Steven D DibbSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Insoo JunJet Propulsion Laboratory, Pasadena, CA 91109 USA.
David J LawrenceJohns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
Simone MarchiSouthwest Research Institute, Boulder, CO 80302 USA.
Timothy J McCoySmithsonian National Museum of Natural History, Washington, DC 20013 USA.
Jose M G MerayoNational Space Institute, Danish Technical University, Lyngby, Denmark.
Rona OranDepartment of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.
Joseph G O'RourkeSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 86387-2001 USA.
Ryan S ParkJet Propulsion Laboratory, Pasadena, CA 91109 USA.
Patrick N PeplowskiJohns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
Thomas H PrettymanPlanetary Science Institute, Tucson, AZ 85719 USA.
Carol A RaymondJet Propulsion Laboratory, Pasadena, CA 91109 USA.
Benjamin P WeissDepartment of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.
Mark A WieczorekObservatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Université Côte d'Azur, Nice, France.
Maria T ZuberDepartment of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139-4307 USA.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

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.

Indexed as

AsteroidMeteoritePlanetesimalPsycheSpace exploration

Identifiers

PMID35431348
PMCPMC9005435

What OpenQuestion holds

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LicenceCC BY
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Registered trials

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.