Mesosiderite formation on asteroid 4 Vesta by a hit-and-run collision

TL;DR

This study uses high-precision dating to link mesosiderite formation on asteroid Vesta to a specific hit-and-run collision event 4.525 billion years ago, shedding light on asteroid differentiation and meteorite origins.

Contribution

It provides the first precise age constraints on mesosiderite formation and directly links it to a collision event on Vesta, clarifying their origin and formation process.

Findings

Mesosiderite formation coincides with crust formation on Vesta.

A hit-and-run collision 4.525 billion years ago caused mesosiderite formation.

Vesta is confirmed as the parent body of mesosiderites.

Abstract

Collision and disruption processes of proto-planetary bodies in the early solar system are key to understanding the genesis of diverse types of main-belt asteroids. Mesosiderites are stony-iron meteorites that formed by mixing of howardite-eucrite-diogenite-like crust and molten core materials and provide unique insights into the catastrophic break-up of differentiated asteroids. However, the enigmatic formation process and the poorly constrained timing of metal-silicate mixing complicate the assignment to potential parent bodies. Here we report high-precision uranium-lead dating of mesosiderite zircons by isotope dilution thermal ionization mass spectrometry, revealing initial crust formation 4,558.5 +/- 2.1 million years ago and metal-silicate mixing at 4,525.39 +/- 0.85 million years. The two distinct ages coincide with the timing of crust formation and a large-scale reheating event on the eucrite parent body, likely the asteroid Vesta. This chronological coincidence corroborates that Vesta is the parent body of mesosiderite silicates. Mesosiderite formation on Vesta can be explained by a hit-and-run collision 4,525.4 million years ago that caused the thick crust observed by NASA's Dawn mission and explains the missing olivine in mesosiderites, howardite-eucrite-diogenite meteorites, and vestoids.