How to identify Meteoritic Breccia/Conglomerate (Thin Section)
Breccia or Conglomerate (likely meteorite) in thin section, viewed under plane-polarized light (PPL) and cross-polarized light (XPL)
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Open the appTo correctly identify Meteoritic Breccia/Conglomerate (Thin Section) (Breccia or Conglomerate (likely meteorite) in thin section, viewed under plane-polarized light (PPL) and cross-polarized light (XPL)), check each of these features in order. Many rocks and minerals look alike, so cross-reference multiple properties before deciding.
Step-by-step identification
- 1
Color
Overall color and any zoning or banding
Highly variable in PPL, depending on mineralogy. Silicates (olivine, pyroxene) are typically colorless to pale green/brown. Plagioclase is colorless. Opaque minerals (metal, troilite) are black. Matrix can be dark brown to black. In XPL, interference colors vary based on mineral composition and orientation.
- 2
Luster
How the surface reflects light: metallic, vitreous, dull
Not directly observable in thin section, but constituent minerals would have vitreous to sub-vitreous luster (silicates) or metallic luster (metal).
- 3
Texture
Grain size and surface feel: coarse, fine, glassy
Clastic, polymict, angular to sub-rounded fragments (clasts) embedded in a finer-grained matrix. Clasts can range from sub-millimeter to several millimeters. Chondritic textures (e.g., barred olivine, radial pyroxene chondrules) may be present. Shock metamorphic features (e.g., planar deformation features, mosaicism, maskelynite) are critical indicators.
- 4
Crystal Form
Shape of visible crystals or crystal faces
Individual mineral grains within clasts may show euhedral to anhedral forms. Chondrules exhibit characteristic spherical to sub-spherical shapes with internal textures (e.g., porphyritic, barred, radial).
- 5
Cleavage
How it breaks: flat cleavage planes vs irregular fracture
Observable in individual mineral grains within clasts. Olivine typically lacks cleavage. Pyroxenes show two cleavages at approximately 90 degrees (orthopyroxene) or 87/93 degrees (clinopyroxene). Plagioclase shows two cleavages at nearly 90 degrees.
- 6
Geological Environment
The rock formation and setting where it occurs
Extraterrestrial environments: asteroid parent bodies, lunar regolith, Martian surface. Formation involves high-velocity impacts, fragmentation, and subsequent lithification. Terrestrial occurrences are limited to impact sites where meteorites have fallen and been preserved, or where impactites (rocks formed by terrestrial impacts) are found, which may contain meteoritic components.
Key Facts
- Hardness
- Variable, depending on constituent minerals (e.g., olivine 6.5-7, pyroxene 5-6, metal 4-5).
- Specific Gravity
- Variable, typically higher than terrestrial rocks due to metal content (e.g., 3.0-3.8 for ordinary chondrites, higher for iron-rich meteorites).
- Crystal System
- Constituent minerals vary (e.g., orthorhombic for olivine/orthopyroxene, monoclinic for clinopyroxene, isometric for metal).
- Color
- Microscopically, variable in PPL (colorless, pale green, brown, black opaques).
- Luster
- Not applicable for thin section.
- Transparency
- Transparent to translucent for silicate minerals, opaque for metal and troilite.
- Fracture
- Conchoidal to uneven for silicates, hackly for metal.
- Cleavage
- Variable, depending on constituent minerals (e.g., good in pyroxene and plagioclase, absent in olivine).
- Composition
- Silicates (olivine, pyroxene, plagioclase), Fe-Ni metal (kamacite, taenite), sulfides (troilite), oxides (chromite), and sometimes carbonaceous material or high-pressure phases. The exact composition depends on the meteorite class (e.g., chondrite, achondrite).
Physical characteristics
- Crystal Habit: Granular, anhedral to subhedral grains within clasts; chondrules are spherical to sub-spherical.
- Cleavage Type: Perfect to good in pyroxenes and plagioclase; absent in olivine.
- Fracture Type: Conchoidal to uneven for silicates; hackly for metal.
- Tenacity: Brittle for silicates; ductile for metal.
- Luster Type: Not applicable for thin section; constituent minerals have vitreous to metallic luster.
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