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  • Pluto's Demotion: The Story of How It Became a Dwarf Planet
    The story of Pluto's demotion to "dwarf planet" is complex and has to do with the definition of a planet, which changed in 2006.

    Here's a simplified timeline:

    * 1930: Clyde Tombaugh discovers Pluto and it's hailed as the ninth planet in our solar system.

    * Early 2000s: Astronomers begin discovering objects in the Kuiper Belt, a region beyond Neptune, that are comparable in size to Pluto. This raises questions about Pluto's planet status.

    * 2005: Eris, a Kuiper Belt object larger than Pluto, is discovered. This further fuels debate about Pluto's status.

    * 2006: The International Astronomical Union (IAU) defines a planet as a celestial body that:

    * Orbits the Sun.

    * Has enough mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape.

    * Has cleared the neighborhood around its orbit.

    * Pluto fails to meet the third criterion: Pluto shares its orbital space with other objects in the Kuiper Belt.

    * August 24, 2006: The IAU votes to reclassify Pluto as a "dwarf planet" along with Eris, Ceres, and Makemake.

    Therefore, Pluto was reclassified as a dwarf planet because it didn't meet the newly defined criteria for a full-fledged planet, particularly the requirement to have cleared its orbital neighborhood.

    This decision sparked controversy, but it ultimately led to a more scientific and accurate understanding of the diverse objects in our solar system.

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