Evidence map›Paper›PMID 41235094›Full record

ReviewSpace science reviews2025

The Psyche Light Elements Investigation.

Thomas H Prettyman, David W Mittlefehldt, Erik I Asphaug, Richard P Binzel, Samuel W Courville, Linda T Elkins-Tanton, David J Lawrence, Simone Marchi, José M G Merayo, Timothy J McCoy and 1 more

Abstract readReview
In one paragraph

Review in Space science reviews, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing 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

1 citing paper in PubMed.

  1. Review
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

11 authors.

Thomas H PrettymanPlanetary Science Institute, Tucson, AZ USA.ORCID 0000-0003-0072-2831
David W MittlefehldtLunar and Planetary Institute, Universities Space Research Association, Houston, TX USA.
Erik I AsphaugLunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA.
Richard P BinzelDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA USA.
Samuel W CourvilleSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ USA.
Linda T Elkins-TantonSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ USA.
David J LawrenceJohns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
Simone MarchiSouthwest Research Institute, Boulder, CO USA.
José M G MerayoDTU Space, Technical University of Denmark, Lyngby, Denmark.
Timothy J McCoySmithsonian National Museum of Natural History, Washington, DC USA.
Benjamin P WeissDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA USA.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Light elements, such as C, S, Si, O, C, and H, are thought to be present in Earth's liquid-Fe outer core. These elements lower melting temperatures, thereby allowing the core to remain in liquid state at high pressure and influencing magnetic and geodynamic processes. However, the identity and abundance of the light elements in the cores of terrestrial planets and how they were delivered to these cores is not well known. The NASA Psyche mission will travel to and explore (16) Psyche, which may be the metal-rich core of a differentiated planetesimal exposed by collisional stripping. If so, the Psyche mission could provide a direct assessment of the light element content of an asteroidal core, allowing comparisons to the inferred composition of planetary cores and the parent bodies of the magmatic iron group meteorites. In particular, Earth's high-pressure core formed gradually (over ∼100 Myr), in a multistage process, under increasingly oxidizing conditions, whereas the cores of planetesimals formed quickly (within 10 Myr) at low pressure, likely in chemical equilibrium with their mantles. The trace element systematics and mineral composition of magmatic iron meteorites indicate the presence of C, P, and S in planetesimal cores prior to solidification. Such elements would have played a role in core dynamics, including dynamo generation. Their low solubility combined with the immiscibility of their mineral precipitates would have resulted in their separation from Fe upon crystallization and their eruption onto the surface of a stripped core (via ferrovolcanism). The Psyche spacecraft will detect their elemental, mineral, and magnetic signatures with the payload instruments, which include a Gamma Ray and Neutron Spectrometer, a Multispectral Imager, and a Magnetometer. Additional constraints on interior composition and processes influenced by light elements will be provided by Psyche's gravity and geomorphology investigations. We provide a brief introduction to the topic of light elements along with prospects for (16) Psyche. While we emphasize core formation processes, we also consider other possibilities for the origin and evolution of this metal-rich body.

Indexed as

Asteroid (16) PsycheFerrovolcanismIron meteoritesLight elementsMetal-rich chondrite meteoritesNASA Psyche missionPlanetary cores

Identifiers

PMID41235094
PMCPMC12605634

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LicenceCC BY-NC-ND
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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.