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Section of Chassigny meteorite
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Section of Chassigny meteorite
Thin section of Chassigny in cross-polarized light, showing shocked and deformed olivine grains. The field of view is 3mm
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Media ID 8585019
© Mary Evans Picture Library 2015 - https://copyrighthub.org/s0/hub1/creation/maryevans/MaryEvansPictureID/10716572
Abstract Achondrite Bright Close Up Closeup Grain Igneous Intrusion Intrusive Intrusive Rock Mars Meteorite Mineral Nesosilicate Olivine Orthosilicate Section Silicate Silicate Mineral Space Stony Meteorite
EDITORS COMMENTS
In this image, a thin section of the Chassigny meteorite is illuminated under cross-polarized light, revealing a mesmerizing pattern of shocked and deformed olivine grains. The Chassigny meteorite, also known as Chassigny meteorite or Chassignite, is an olivine achondrite that originated from Mars and fell to Earth in 1815 in the village of Chassigny, France. The intriguing intrusive rock, classified as a dunite, is composed primarily of olivine, a silicate mineral, and displays a striking contrast of colors and textures. The olivine grains, appearing bright and colorful against the darker matrix, have been subjected to intense heat and pressure, resulting in their unique, elongated, and distorted shapes. These features are indicative of the meteorite's violent impact history and its origin from the Martian mantle. The intriguing abstract design showcased in this close-up view is a testament to the intriguing geological processes that shaped the Chassigny meteorite. The silicate minerals, including orthosilicates and nesosilicates, have been rearranged and recrystallized under extreme conditions, resulting in this captivating, otherworldly scene. This image serves as a reminder of the vastness and complexity of the universe and the wonders that can be discovered through scientific exploration. The Chassigny meteorite, with its intriguing composition and history, continues to captivate scientists and enthusiasts alike, offering valuable insights into the geological history of Mars and our solar system.
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