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Kuiper Belt - Facts for Kids


The Kuiper Belt is similar to the asteroid belt, because they're both regions full of bits left over from the early Solar System.

It's easy to remember what we call objects in the Kuiper Belt. We call them Kuiper Belt Objects (KBOs). Although asteroids are rocks, KBOs are icy bodies made of frozen water and gases with some rock mixed in.

The Kuiper Belt is so far away that if you were there, the Sun would just look like a very bright star.

Astronomers don't measure Solar System distances in kilometers or miles. They use astronomical units (AU), where 1 AU is the distance from the Earth to the Sun. That's about 150 million km or 93 million miles. So when we say that the Kuiper Belt starts at Neptune's orbit 30 AU from the Sun, that is thirty times farther from the Sun than we are.

The Kuiper Belt is really big.

The Kuiper Belt starts at 30 AU, but it goes on for another 20 AU - that's 3 billion km (1.9 billion miles). If you'd like to see how it compares with the rest of the Solar System, have a look here. In order to fit the Kuiper Belt into the diagram, the "Sun" covers the orbits of Mercury, Venus and Earth. Mars and the asteroid belt aren't shown.

Pluto was the first KBO to be discovered, but they didn't know it then.

Astronomers didn't know there was a Kuiper Belt in 1930 when American astronomer Clyde Tombaugh discovered Pluto. However another American astronomer, named Frederick C. Leonard, suggested that instead of being a new planet, Pluto might the first of a new kind of Solar System object. Everyone else was too excited about a new planet to pay much attention to this idea.

So was there a faraway place full of icy stuff that didn't get made into planets? Over the next half century, more astronomers started to think so.

Gerard Kuiper was one of the astronomers that wrote about this belt of material. But since he also said that it didn't exist anymore, it was odd that it got named after him.

It took 48 years to discover Pluto's moon Charon and another twelve to find the next KBO.

Finding tiny objects a few billion kilometers away was never going to be easy. David Jewitt and Jane Luu hunted on and off for five years before they found one. This made other astronomers sit up and pay attention. Jewitt and Luu wanted to call their discovery Smiley, but it's listed as 1992 QB1.

There are three recognized dwarf planets in the Kuiper Belt.

Besides Pluto, the International Astronomical Union officially lists two other KBOs as dwarf planets: Haumea (how MAY ah) and Makemake (MAH kay MAH kay). The largest dwarf planet is Eris, but it's not in the Kuiper Belt. All of them are smaller than the Moon, including Ceres (SEER ees), the only dwarf planet in the Asteroid Belt.

There are at least 70,000 KBOs bigger than 100 km (62 miles) across, and millions of smaller ones.

Imagine zipping around the Kuiper Belt and picking up all the KBOs to make them into one planet. Sounds as though you'd have a biggie! But the total mass would be about that of Mars, which has only 10% of Earth's mass. Astronomers think there should be lots more mass, but no one knows what happened to it.

The Scattered Disk lies beyond the Kuiper Belt.

You might think that once you were at the far side of the Kuiper Belt you'd have reached the end of the Solar System. But no, because then there is still the Scattered Disk which goes out to about 100 AU. The dwarf planet Eris, which is a bit smaller than Pluto, but more massive, is a scattered disk object (SDO).
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Content copyright © 2013 by Mona Evans. All rights reserved.
This content was written by Mona Evans. If you wish to use this content in any manner, you need written permission. Contact Mona Evans for details.

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