
Dwarf planets are celestial bodies in the solar system that orbit the Sun and have enough mass for their gravity to make them nearly round in shape. However, unlike planets, they have not cleared their orbital paths of other debris. Notable examples include Pluto, Eris, Haumea, and Makemake. Dwarf planets are generally smaller than the eight main planets and are found mostly in the Kuiper Belt and beyond Neptune.

Dwarf planets are celestial bodies in the solar system that orbit the Sun and have enough mass for their gravity to make them nearly round in shape. However, unlike planets, they have not cleared their orbital paths of other debris. Notable examples include Pluto, Eris, Haumea, and Makemake. Dwarf planets are generally smaller than the eight main planets and are found mostly in the Kuiper Belt and beyond Neptune.
What is a dwarf planet?
A celestial body that orbits the Sun, is round enough to be shaped by gravity (hydrostatic equilibrium), but has not cleared its orbital neighborhood of other debris.
How does a dwarf planet differ from a regular planet?
A regular planet has cleared its orbit around the Sun, whereas a dwarf planet shares its orbital region with other objects of similar size and hasn’t cleared its neighborhood.
Can you name some examples of dwarf planets?
Pluto, Eris, Haumea, Makemake, and Ceres are well-known dwarf planets (Ceres sits in the asteroid belt; the others are in the Kuiper Belt or scattered disk).
How are dwarf planets identified by scientists?
Scientists check if a body orbits the Sun, has enough mass to be nearly round, has not cleared its neighborhood, and is not a natural satellite.