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Types of Objects

Stars

With a telescope, you can see thousands of stars. Stars are giant balls of gas that use up hydrogen when they shine. When they run out of hydrogen, they can use other elements. Eventually, their fuel supply runs out and they die.

The Pleiades
Copyright Anglo-Australian Observatory / Royal Observatory, Edinburgh
Courtesy AAO Astronomical Images Gallery.

Stars are often found in clusters, hundreds together. The famous star cluster called The Pleiades is shown at the right.

Sometimes (as in the Pleiades picture) stars appear to have bright spikes or crosses through them. These aren't really part of the star - they're just an optical illusion that comes from the telescope.

Nebulae

Orion Nebula
Courtesy AAO Astronomical Images Gallery.

Nebulae (the plural of nebula) are places where new stars are born. They are collections of gas and dust that come together due to gravity to form stars.

Galaxies

Galaxies are huge collections of stars. Our galaxy, The Milky Way, may contain up to a trillion stars. No one is exactly sure how many. Other galaxies are even bigger. Some "dwarf" galaxies are much smaller.

Galaxies come in different shapes. The three types of galaxies are spiral, elliptical, and irregular. Examples of each type are shown below.

Elliptical galaxy

Spiral galaxy
(seen from the front)

Spiral galaxy
(seen from the side)

Irregular galaxy

Galaxies come in clusters, just like stars do. Some galaxies are so far away that they look like stars. Sometimes, galaxies pass close to each other. When they do, their gravity can cause them to warp. The galaxies can bend each other, making them look like the pair shown below.

A close pair of galaxies

Quasars

Quasar

Quasars are galaxies with active centers. They are so far away that they look like stars. They are very far away but they shine brightly: one quasar can be as bright as millions of regular galaxies. The red "star" shown to the right is actually a quasar.

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Sponsored by the National Science Foundation under Cooperative Agreement AST0122449 with
The Johns Hopkins University. Developed in collaboration with the International Virtual Observatory Alliance.

Last Modified: Wednesday, June 21, 2006 at 5:22:47 PM by Jordan Raddick
Revision 1.3