Dwarf planets are an intriguing classification of celestial bodies within our Solar System. To be considered a dwarf planet, an object must meet several specific criteria set by the IAU:
• The object must orbit the Sun
• It should be approximately spherical in shape due to its own gravity
• Unlike planets, it does not need to have cleared its orbit of other debris
• It is not a satellite of another body
These criteria distinguish dwarf planets from planets by acknowledging that they can be part of a crowded orbital zone.
- Pluto is the most famous example of a dwarf planet, having been reclassified from planet status following the establishment of these criteria.
- Other examples include Eris, Haumea, Makemake, and Ceres.
Dwarf planets play an essential role in helping astronomers understand the diversity and complexity of our Solar System's formation.