A numerical approach using a finite element model to constrain the possible interior layout of (16) Psyche
Yaeji Kim, Masatoshi Hirabayashi

TL;DR
This study uses a finite element model to numerically constrain the interior structure of asteroid (16) Psyche, suggesting a metallic core and layered silicate regions, based on density and pressure constraints.
Contribution
It introduces an inverse problem algorithm combining finite element modeling and pressure constraints to determine Psyche's interior layout, considering various layer configurations.
Findings
Smallest core radius likely 72 km
Silicate-rich layer up to 68 km thick
Core may occupy 34-40% of Psyche's size
Abstract
Asteroid (16) Psyche is notable for the largest M-type asteroid and has the high radar albedo among the main-belt asteroids. The object is likely a mixture of metal and silicates because of its lower bulk density than metallic materials and observations inferring the existence of silicate materials on the surface. Here, we numerically investigate the interior layout when the structure of Psyche consists of a spherical iron core and two types of silicate-rich layers (compressed and uncompressed ones resulting from the compaction process. We develop an inverse problem algorithm to determine the layout distribution by combining a Finite Element Model approach that accounts for density variations and constrains pressure-based crushing conditions. The results show that given the crushing limit of 10 MPa the smallest core size likely reaches 72 km in radius, and the silicate-rich layer,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Geological and Geochemical Analysis
