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  2. Eris (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Eris_(dwarf_planet)

    Eris ( minor-planet designation: 136199 Eris) is the most massive and second-largest known dwarf planet in the Solar System. [ 22] It is a trans-Neptunian object (TNO) in the scattered disk and has a high- eccentricity orbit. Eris was discovered in January 2005 by a Palomar Observatory –based team led by Mike Brown and verified later that year.

  3. Dysnomia (moon) - Wikipedia

    en.wikipedia.org/wiki/Dysnomia_(moon)

    Dysnomia (formally (136199) Eris I Dysnomia) is the only known moon of the dwarf planet Eris and is the second-largest known moon of a dwarf planet, after Pluto I Charon. It was discovered in September 2005 by Mike Brown and the Laser Guide Star Adaptive Optics (LGSAO) team at the W. M. Keck Observatory. It carried the provisional designation ...

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Eris's discovery contributed to a ... Careful observations of the 1769 transit of Venus allowed astronomers to calculate the average Earth–Sun distance as ...

  5. Scientists discern internal structure of mysterious dwarf ...

    www.aol.com/news/scientists-discern-internal...

    Dwarf planet Eris, similar in size to its better-known cosmic cousin Pluto, has remained an enigma since being discovered in 2005 lurking in the solar system's far reaches. While Pluto was ...

  6. Makemake - Wikipedia

    en.wikipedia.org/wiki/Makemake

    Makemake was discovered on March 31, 2005, by a team at the Palomar Observatory, led by Michael E. Brown, [8] and was announced to the public on July 29, 2005. The team had planned to delay announcing their discoveries of the bright objects Makemake and Eris until further observations and calculations were complete, but announced them both on July 29 when the discovery of another large object ...

  7. Kuiper belt - Wikipedia

    en.wikipedia.org/wiki/Kuiper_belt

    [27] It is said that Kuiper was operating on the assumption, common in his time, that Pluto was the size of Earth and had therefore scattered these bodies out toward the Oort cloud or out of the Solar System; there would not be a Kuiper belt today if this were correct. [28] The hypothesis took many other forms in the following decades.

  8. Sedna (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Sedna_(dwarf_planet)

    1.83±0.05[14] 1.3[2] Sedna(minor-planet designation: 90377 Sedna) is a dwarf planetin the outermost reaches of the Solar System, orbiting the Sun beyond the orbit of Neptune. Discovered in 2003, the planetoid's surface is one of the reddestknown among Solar System bodies. Spectroscopyhas revealed Sedna's surface to be mostly a mixture of the ...

  9. Location of Earth - Wikipedia

    en.wikipedia.org/wiki/Location_of_Earth

    The average diameter of the orbit of the Earth relative to the Sun. Encompasses the Sun, Mercury and Venus. [18] Inner Solar System ~6.54 AU 9.78×10 8: 8.99: Encompasses the Sun, the inner planets (Mercury, Venus, Earth, Mars) and the asteroid belt. Cited distance is the 2:1 resonance with Jupiter, which marks the outer limit of the asteroid belt.