2006Open Research Online - ORO (The Open University)Requires access

Asteroidal differentiation processes deduced from ultramafic achondrite ureilite meteorites

Hilary Downes, David W. Mittlefehldt, Pierre Hudon, Christopher S. Romanek, I. A. Franchi

Open publisher page 0 citations

Abstract

Ureilite meteorites are partial melt residues of an asteroid-sized object. They record the differentiation process that transformed many asteroids during the earliest stages of solar system formation.

Open-access reader

About this research paper

What this paper is about

Ureilite meteorites are partial melt residues of an asteroid-sized object. They record the differentiation process that transformed many asteroids during the earliest stages of solar system formation.

Why it matters

A significance statement is not available in the OpenAlex record.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

Ureilite meteorites are partial melt residues of an asteroid-sized object. They record the differentiation process that transformed many asteroids during the earliest stages of solar system formation.

Key concepts: Achondrite, Meteorite, Planetary differentiation, Astrobiology, Geology, Geochemistry, Planetesimal, Formation and evolution of the Solar System

Related papers

Back to paper searchBrowse research topicsOriginal source
Asteroidal differentiation processes deduced from ultramafic achondrite ureilite meteorites — Research Paper | ScholarLens