Spiral galaxy facts for kids

Kids Encyclopedia Facts
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An example of a spiral galaxy, the Pinwheel Galaxy (also known as Messier 101 or NGC 5457)
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A barred spiral galaxy

A spiral galaxy is a kind of galaxy that looks like a flat, slowly rotating disk with a bulge in the centre. It contains stars, gas, dust, dark matter and a supermassive black hole at its centre.

Galaxies were first listed in the 18th century by William Herschel. The spiral galaxy as a type was first described by Edwin Hubble in his 1936 work The Realm of the Nebulae. They are named after their shape. The spiral arms are where young, hot stars are made, which is why they are brighter than the center of the galaxy. Some spiral galaxies have yellow, 'fossil' arms of older stars.

The barred spiral galaxy is an important and common type of spiral galaxy. There are three other kinds of spiral galaxies. Grand-design spiral galaxies have two well-shaped arms. Multiple-arm spiral galaxies have more arms. In flocculent spiral galaxies, it is hard to see the arms at all.

About 60% of galaxies in the universe near us (the 'local universe') are spiral and irregular galaxies. They are mostly found in low-density parts of the universe, and are rare in the centers of galaxy clusters.

Milky Way

Our own Milky Way has recently (in the 1990s) been confirmed to be a barred spiral galaxy, although the bar itself is difficult to observe from our position in the Galactic disk. The most convincing evidence for its existence comes from a recent survey, performed by the Spitzer Space Telescope, of stars in the Galactic center.

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Spiral galaxy Facts for Kids. Kiddle Encyclopedia.