Corvid meteoroids are ejecta from the Giordano Bruno impact

Physics

Scientific paper

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Ejecta, Lunar Craters, Meteorite Craters, Meteoroid Showers, Earth-Moon System, Meteorite Collisions, Orbital Mechanics, Solar Orbits, Space Observations (From Earth), Moon, Impact Craters, Meteoroids, Origin, Source, Giordano Bruno, Ejecta, Corvids, Parameters, Position (Location), Motion, Velocity, Meteor Shower, Hypotheses, Orbit, Geometry, Commensurability

Scientific paper

Attention is given to Corvid meteoroids, with reference to a Corvid meteor shower observed in late June of 1937. On June 18, 1178, the upper horn of a crescent moon was reported to have split, with fire and sparks emanating from the division point. This report was interpreted to be a description of events related to the formation of the lunar crater Giordano Bruno. Corvid meteoroids are judged to be Giordano Bruno ejecta fragments based on similarities in their heliocentric positions, directions of motion, and speeds. Commensurability relationships between meteoroid/ejecta and earth-moon system orbital periods enable definitive predictions of Corvid showers in the years 2003 and/or 2006.

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