Morphological and surface micro-reflective features consistent with a CO-4 carbonaceous chondrite

A small carbonaceous chondrite specimen was investigated using exclusively non-destructive macroscopic, morphological, and surface microtextural methods. The specimen exhibits a thin, continuous fusion crust, ghost chondrules visible beneath the surface, weak magnetic response, and a bulk density consistent with CO carbonaceous chondrites. Its external morphology is markedly aerodynamically sculpted, with a flattened leading apex, flow-oriented fusion crust textures, and localized shock-related surface disruption. High-resolution imaging under oblique illumination reveals numerous discrete stellar micro-reflective features producing characteristic radial light spikes. These features are interpreted as specular reflections from ultrafine metallic phases or high-refractive-index silicate microlites exposed within an exceptionally thin fusion crust. The combined morphological and surface characteristics are consistent with moderate thermal metamorphism approaching petrologic type CO-4. Although definitive classification requires laboratory petrographic and chemical analyses, the non-destructive evidence presented here supports a robust provisional classification and highlights the scientific value of preserving rare aerodynamic morphologies that would be compromised by destructive sampling.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-12-26
DOI
https://doi.org/10.5281/zenodo.18010167
Primary Topic
Astro and Planetary Science
Type
article
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article

Morphological and surface micro-reflective features consistent with a CO-4 carbonaceous chondrite

Eduardo Brandão
Zenodo (CERN European Organization for Nuclear Research)
Astro and Planetary Science
article

Morphological and surface micro-reflective features consistent with a CO-4 carbonaceous chondrite

Eduardo Brandão
article en

Abstract

A small carbonaceous chondrite specimen was investigated using exclusively non-destructive macroscopic, morphological, and surface microtextural methods. The specimen exhibits a thin, continuous fusion crust, ghost chondrules visible beneath the surface, weak magnetic response, and a bulk density consistent with CO carbonaceous chondrites. Its external morphology is markedly aerodynamically sculpted, with a flattened leading apex, flow-oriented fusion crust textures, and localized shock-related surface disruption. High-resolution imaging under oblique illumination reveals numerous discrete stellar micro-reflective features producing characteristic radial light spikes. These features are interpreted as specular reflections from ultrafine metallic phases or high-refractive-index silicate microlites exposed within an exceptionally thin fusion crust. The combined morphological and surface characteristics are consistent with moderate thermal metamorphism approaching petrologic type CO-4. Although definitive classification requires laboratory petrographic and chemical analyses, the non-destructive evidence presented here supports a robust provisional classification and highlights the scientific value of preserving rare aerodynamic morphologies that would be compromised by destructive sampling.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 30%
Astro and Planetary Science
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