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  2. IAU definition of planet - Wikipedia

    en.wikipedia.org/wiki/IAU_definition_of_planet

    A separate "working" definition for extrasolar planets was, however, recommended by a working group of the IAU in 2003 [53] and includes the criterion: "The minimum mass/size required for an extrasolar object to be considered a planet should be the same as that used in the Solar System." [54]

  3. Definition of planet - Wikipedia

    en.wikipedia.org/wiki/Definition_of_planet

    However, acceptance of Eris as the tenth planet implicitly demanded a definition of planet that set Pluto as an arbitrary minimum size. Many astronomers, claiming that the definition of planet was of little scientific importance, preferred to recognise Pluto's historical identity as a planet by "grandfathering" it into the planet list. [47]

  4. Planet - Wikipedia

    en.wikipedia.org/wiki/Planet

    The eight planets of the Solar System with size to scale (up to down, left to right): Saturn, Jupiter, Uranus, Neptune (outer planets), Earth, Venus, Mars, and Mercury (inner planets) A planet is a large, rounded astronomical body that is generally required to be in orbit around a star, stellar remnant, or brown dwarf, and is not one itself. [1]

  5. The tiny planet-not-planet that could: Pluto was discovered ...

    www.aol.com/short-uneventful-life-pluto-planet...

    An icy dwarf only half the size of the United States, it was on average 3.7 billion miles from the sun. It also has a decidedly strange orbit that was highly elliptical and tilted. At times it is ...

  6. Pluto - Wikipedia

    en.wikipedia.org/wiki/Pluto

    The similarity in size of Charon and Pluto has prompted some astronomers to call it a double dwarf planet. [152] The system is also unusual among planetary systems in that each is tidally locked to the other, which means that Pluto and Charon always have the same hemisphere facing each other — a property shared by only one other known system ...

  7. Clearing the neighbourhood - Wikipedia

    en.wikipedia.org/wiki/Clearing_the_neighbourhood

    Also listed are Stern–Levison's Λ and Soter's μ; again, the planets are orders of magnitude greater than 1 for Λ and 100 for μ, and the dwarf planets are orders of magnitude less than 1 for Λ and 100 for μ. Also shown are the distances where Π = 1 and Λ = 1 (where the body would change from being a planet to being a dwarf planet).

  8. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    The size of solid bodies does not include an object's atmosphere. For example, Titan looks bigger than Ganymede, but its solid body is smaller. For the giant planets , the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure.

  9. Minimum mass - Wikipedia

    en.wikipedia.org/wiki/Minimum_mass

    In astronomy, minimum mass is the lower-bound calculated mass of observed objects such as planets, stars, binary systems, [1] nebulae, [2] and black holes. Minimum mass is a widely cited statistic for extrasolar planets detected by the radial velocity method or Doppler spectroscopy, and is determined using the binary mass function .