Facts about Mice Galaxies
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Gravitational disruption from the Mice Galaxies collision has triggered widespread star formation, creating thousands of new massive stars within their tidal regions over the past 200 million years.
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Hubble Space Telescope imaging reveals that NGC 4676A and NGC 4676B are currently separated by approximately 20,000 light-years and approaching each other at relative velocities exceeding 1,000 kilometers per second.
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Each of the Mice Galaxies contains roughly 100 billion stars, making their collision one of the most massive galactic encounters observable in the nearby universe.
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In 1953, astronomer Fritz Zwicky first identified the Mice Galaxies as a classic example of galactic collision, demonstrating how gravitational forces reshape entire star systems.
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Observations of the Mice Galaxies reveal prominent tidal tails extending over 500,000 light-years, among the longest structures created by galactic interactions in the universe.
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The two colliding galaxies NGC 4676A and NGC 4676B, located 300 million light-years away, will eventually merge into a single elliptical galaxy over billions of years.