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Dwarf planets are all the celestial bodies in our solar system that:

  1. Directly orbit the Sun (this means that moons are excluded)
  2. are massive enough that their self-gravity has caused their shape (which means they generally are bigger than about 1000 km in diameter and their shape is more or less a sphere)
  3. have not cleared their orbit of all the other celestial bodies (which means there are other celestial bodies that orbit the Sun at more or less the same distance)

This system was established by the International Astronomical Union (IAU) in 2006 after the discovery of other celestial bodies that orbit the Sun at a similar distance to that with which Pluto does. One of these bodies, named Eris, is even bigger than Pluto itself. Instead of increasing the number of planets by all these new discoveries (and those that will be discovered in the future) the IAU decided to call Pluto and all similar objects dwarf planets. So, currently we are left with the eight planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune and the currently known dwarf planets Ceres (part of the asteroid belt), Pluto, Haumea, Makemake, and Eris (all trans-Neptunian objects). It is suspected that about one hundred known objects are dwarf planets. We still need to make sure that self-gravity has formed them into spherical bodies; otherwise they would just be classified as asteroids. Furthermore, astronomers believe that there are up to 200 dwarf planets in the Kuiper belt and up to another 10 000 dwarf planets in the region beyond the Kuiper belt.

Unfortunately we do not have detailed images of any of these dwarf planets yet; they are too small and too far away from Earth. But this will change soon when in February 2015 the Dawn spacecraft will arrive at Ceres and deliver crisp HD images of this dwarf planet. Then a few months later, in July 2015, we will add images of Pluto when the New Horizons spacecraft will fly-by Pluto. Until then we have to be satisfied with the images provided by the Hubble Space Telescope that can just give us a very basic idea of these objects.

The image below shows an artist's impression of the dwarf planets Eris (left centre), Ceres (centre), Pluto and its moon Charon (bottom) compared with the Earth and our moon (top).

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Veröffentlicht von Veröffentlicht oder zuletzt modifiziert am 14.01.2017