Exogenous origin of hydration on asteroid (16) Psyche: The role of hydrated asteroid families
C. Avdellidou, M. Delbo', A. Fienga

TL;DR
This study suggests that hydration features on asteroid Psyche likely originate from exogenous hydrated impactors, primarily from the Themis family, challenging the idea of a purely metallic core origin.
Contribution
The paper introduces a collisional model demonstrating that hydrated impactors from asteroid families can explain Psyche's hydration features, emphasizing the role of exogenous delivery.
Findings
Hydrated impactors from the Themis family can deliver significant water to Psyche.
The implanted hydrated mass on Psyche is estimated around 10^14 kg.
Hydration on Psyche is likely due to exogenous sources rather than its intrinsic composition.
Abstract
Asteroid (16) Psyche, that for long was the largest M-type with no detection of hydration features in its spectrum, was recently discovered to have a weak 3 micron band and thus it eventually was added to the group of hydrated asteroids. Its relatively high density in combination with the high radar albedo, led to classify the asteroid as a metallic object, possibly a core of a differentiated body, remnant of "hit-and-run" collisions. The detection of hydration is, in principle, inconsistent with a pure metallic origin of this body. Here we consider the scenario that the hydration on its surface is exogenous and was delivered by hydrated impactors. We show that impacting asteroids that belong to families whose members have the 3 m band can deliver the hydrated material to Psyche. We developed a collisional model with which we test all the dark carbonaceous asteroid families, which…
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