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  • Pluto's Demotion: Understanding Dwarf Planet Classification
    Pluto was reclassified as a dwarf planet in 2006 due to the following reasons:

    1. It does not dominate its orbital region: The International Astronomical Union (IAU) defined a planet as a celestial body that orbits the Sun, is massive enough for its own gravity to make it round, and has cleared its neighborhood around its orbit. Pluto shares its orbital region with many other icy bodies in the Kuiper belt.

    2. Its orbit is highly eccentric and tilted: Pluto's orbit is highly elliptical and tilted at a significant angle compared to the other planets. This indicates that it did not form in the same way as the other planets.

    3. Discovery of similar objects: The discovery of Eris, a trans-Neptunian object larger than Pluto, raised questions about the definition of a planet. Eris, like Pluto, shares its orbital region with other objects.

    4. The need for a more comprehensive definition: The discovery of Eris and other similar objects highlighted the need for a more precise definition of a planet that could encompass the growing number of celestial objects being discovered.

    The IAU established a new definition for a dwarf planet:

    * Orbits the Sun

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

    * Has not cleared its neighborhood around its orbit

    * Is not a satellite

    In conclusion, Pluto's reclassification as a dwarf planet was a result of a more precise understanding of planetary formation and the discovery of similar objects in the Kuiper Belt. It reflects the ongoing evolution of our understanding of the Solar System and the need for a more robust definition of a planet.

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