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  2. Weaubleau structure - Wikipedia

    en.wikipedia.org/wiki/Weaubleau_structure

    The Weaubleau structure is a probable meteorite impact site in western Missouri near the towns of Gerster, Iconium, Osceola, and Vista. It is believed to have been caused by a 1,200-foot (370 m) meteoroid between 335 and 340 million years ago [1] during the middle Mississippian Period (Latest Osagean to Earliest Meramecian).

  3. Meteorite - Wikipedia

    en.wikipedia.org/wiki/Meteorite

    It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater. [2]

  4. Widmanstätten pattern - Wikipedia

    en.wikipedia.org/wiki/Widmanstätten_pattern

    Widmanstätten patterns, also known as Thomson structures, are figures of long phases of nickel–iron, found in the octahedrite shapes of iron meteorite crystals and some pallasites. Iron meteorites are very often formed from a single crystal of iron-nickel alloy, or sometimes a number of large crystals that may be many meters in size, and ...

  5. Meteoric water - Wikipedia

    en.wikipedia.org/wiki/Meteoric_water

    Meteoric water, derived from precipitation such as snow and rain, includes water from lakes, rivers, and ice melts, all of which indirectly originate from precipitation.. The journey of meteoric water from the atmosphere to the Earth's surface is a critical component of the hydrologic cyc

  6. Meteoroid - Wikipedia

    en.wikipedia.org/wiki/Meteoroid

    A meteorite is a portion of a meteoroid or asteroid that survives its passage through the atmosphere and hits the ground without being destroyed. [22] Meteorites are sometimes, but not always, found in association with hypervelocity impact craters; during energetic collisions, the entire impactor may be vaporized, leaving no meteorites.

  7. Chondrite - Wikipedia

    en.wikipedia.org/wiki/Chondrite

    A chondrite / ˈ k ɒ n d r aɪ t / is a stony (non-metallic) meteorite that has not been modified by either melting or differentiation of the parent body. [a] [1] They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids.

  8. Carbonaceous chondrite - Wikipedia

    en.wikipedia.org/wiki/Carbonaceous_chondrite

    The presence of volatile organic chemicals and water indicates that they have not undergone significant heating (>200 °C) since they were formed, and their compositions are considered to be close to that of the solar nebula from which the Solar System condensed. Other groups of C chondrites, e.g., CO, CV, and CK chondrites, are relatively poor ...

  9. Asteroidal water - Wikipedia

    en.wikipedia.org/wiki/Asteroidal_water

    The planets, and to an extent the asteroid belt, were previously held to be static and unchanging; the belt was a former or stalled planet.. In the late 1860s, Hubert Newton and Giovanni Schiaparelli simultaneously showed that meteor showers (and by implication, meteorites) were comet debris.