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Dwarf planets are objects in our solar system that are big enough to pull themselves into a rounded shape yet orbit the Sun in a "messy" neighbourhood (like the asteroid belt, or the Kuiper Belt beyond Neptune.) So far, the International Astronomical Union lists five dwarf planets: Ceres in the asteroid belt, and Pluto, Haumea, Makemake and Eris in the Kuiper Belt. However, it is highly likely that a LOT more objects out there in the Kuiper Belt are round and therefore dwarf planets - we just haven't been able to observe them closely enough to prove it. It's likely that by the time we have better pictures of everything we've discovered so far we'll have found dozens, perhaps even hundreds of dwarf planets out there. Some examples of things that are almost certainly dwarf planets but that the IAU doesn't list yet as their shape isn't proven are Ixion, Orcus, Varuna, Quaoar and Sedna. So bear in mind that any list of dwarf planets is bound to grow quickly and will be out of date soon!

If you believe dwarf planets are planets, you can remember the five dwarf planets in order from the sun with the mnemonic: "Can Planets Have Massive Eccentricity?"

If you don't believe dwarf planets are planets and that only the eight big ones count, you can use this one: "Counting Planets Here Means Eight!"

And if you want to remember the five dwarf planets alongside the eight other planets, use "My Very Easy Method Can't Just Speed Up Naming Planets, However Many Exist!"

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14y ago

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