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  2. Haumea - Wikipedia

    • The revised solution for Haumea's shape implies that it has a core of approximately 1,626 × 1,446 × 940 km, with a relatively high density of ≈ 2.68 g/cm 3, indicative of a composition largely of hydrated silicates such as kaolinite. The core is surrounded by an icy mantle that ranges in thickness from about 70 km at the poles to 170 km ...… See more

    Discovered byBrown et al. · Ortiz et al.
    Discovery date7 March 2003 (Ortiz) · 28 December 2004 (Brown)
    MPC designation(136108) Haumea
    Named afterHaumea
    Overview

    Haumea (minor-planet designation: 136108 Haumea) is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 by a team headed by Mike Brown of Caltech at the Palomar Observatory, and formally announce… See more

    History

    Two teams claim credit for the discovery of Haumea. A team consisting of Mike Brown of Caltech, David Rabinowitz of Yale University, and Chad Trujillo of Gemini Observatory in Hawaii discovered Haumea on 28 Dece… See more

     
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  2. Clay

    Water soaked into the rocky material at the center of Haumea and made it swell into a large core made of clay, which is less dense than rock. The larger core increased the moment of inertia and thus slowed Haumea’s spin to its current rate.
    spaceref.com/science-and-exploration/nasa-studies-origins-of-weird-solar-system-object-dwarf-planet-haumea/
    spaceref.com/science-and-exploration/nasa-studies-origins-of-weird-solar-syste…
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