Why does it matter if Pluto is a planet or a dwarf planet?

 

“Comet,” “star” and “planet” are category names that immediately tell you something important about what they describe. 
Our solar system consists of the sun, planets (which orbit around the sun) and small bodies (which either orbit around the sun or planets). The “small bodies” category is divided up into even smaller categories, mostly depending on the shape and size of orbits. In 1801, astronomers discovered Ceres, which was initially categorized as a “planet.” Astronomers measured that it was much smaller than the other known planets. Soon, a lot of smaller objects were discovered on orbits very close to Ceres. These small bodies were categorized as “asteroids” and we have since discovered hundreds of thousands of these in the asteroid belt. 
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How planets form
A similar process of discovery and re-categorization happened for small bodies further out in the solar system. Agen Slot Terpercaya
Pluto was discovered in 1930 and was called the ninth planet in our solar system for many decades. But astronomers soon learned that Pluto was pretty different from the other eight planets: it’s on a tilted orbit and it’s way, way smaller than the other planets.
Over the years, astronomers discovered more and more small, planet-like objects that crossed Pluto’s orbit. These are now categorized as “Kuiper Belt objects.” It was looking more and more like Pluto might fit in better with the category of Kuiper Belt objects than with planets. In 2005, a new object was discovered in the outer solar system, Eris, that is even heavier than Pluto. This led astronomers to consider if both Eris and Pluto are planets or not. Astronomers thought this was an important enough decision that the International Astronomical Union voted on it in 2006. Astronomers decided that rather than demoting Pluto to a plain old Kuiper Belt object, they would make a new category of small body called a “dwarf planet.” Pluto and Eris would both be part of this new category.
Solar systems like ours form from big clouds of dust and gas that collapse into disks around young stars, but astronomers are still learning exactly how that process works. We use telescopes to look carefully at forming solar systems far away, but they are so far that it’s really hard to see the planets forming directly.
A planetesimal — a baby planet — first forms from clumps of dust in a disc orbiting a young star. Planetesimals then grab nearby pebbles, dust and sometimes even smaller planetesimals with their gravity, which gets stronger as they get bigger. When they get to be a few hundred kilometres across, they have enough gravity to pull themselves into a round shape, which is the definition of a dwarf planet.