4x/0.25, breccia, howardite, northwest africa, polarized, scope2, Tucsen C30 3MP sCMOS, zerene stacker

NWA 8595 Meteorite Thin Section

NWA 8595 Meteorite Thin Section

NWA 8595 Meteorite Thin Section

As a Howardite, the NWA 8595 meteorite called Vesta 4 home for billions of years — until an impact knocked this regolith breccia off its lonely host and on a trajectory for the more hospitable land of Morocco, Earth.

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4x/0.25, diogenite, northwest africa, polarized, scope2, Tucsen C30 3MP sCMOS, zerene stacker

NWA 2824 Meteorite Thin Section

NWA 2824 Meteorite Thin Section

NWA 2824 Meteorite Thin Section

Cross polarized thin section of NWA 2824, a diogenite with a multitude of white-gray needle like inclusions which, in their color and texture, resemble those found in the Ibitira Meteorite Thin Section. These are described as “Plagioclase recrystallized into complex spherulitic textures.”  See this link for more classification information on diogenites.

Impactika has nice close-up images of the the plagioclase textures: TS Image 1 and TS Image 2

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4x/0.25, achondrite, northwest africa, polarized, scope2, Tucsen C30 3MP sCMOS, zerene stacker

NWA 7325 Meteorite Thin Section

NWA 7325 Meteorite Thin Section

NWA 7325 Meteorite Thin Section

The ungrouped achondrite meteorite NWA 7325 originates from a differentiated parent body. Based on various analyses it has been determined that the meteorite shares characteristics with Mercury — or a parent body of similar composition to Mercury. The thin section displays several areas which have trails of bubbles preserved in the minerals at the time of crystallization. More scientific details about NWA 7325 can be found at Meteorite Studies.

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