Published In

Icarus

Document Type

Article

Publication Date

5-1-2026

Subjects

Asteroids -- Surfaces, Spectroscopy, Meteorites -- Composition, Experimental techniques

Abstract

Brachinite meteorites are typically linked to the olivine-rich A-type asteroids. In this study, however, they appear to exhibit unexpected spectral diversity. Spectroscopic analysis of seven meteorites from the brachinite clan reveals two distinct populations in band parameters, overlapping with both the A-type and S-complex asteroids. This dual association shows that a single meteorite group can originate from multiple asteroid taxonomies. Notably, one S-complex-like specimen, Northwest Africa (NWA) 14,635, displays band parameters similar to those of asteroid (65803) Didymos, the target of the European Space Agency's (ESA) ongoing Hera mission. These results underscore the value of spectroscopic characterization of poorly understood meteorite groups and identifying potential analogs that are highly relevant for current and future mission planning.

Rights

Copyright (c) 2025 The Authors Creative Commons License This work is licensed under a Creative Commons Attribution 4.0 International License.

DOI

10.1016/j.icarus.2026.116965

Persistent Identifier

https://archives.pdx.edu/ds/psu/44472

Publisher

Elsevier BV

Included in

Geology Commons

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