
“Where are the rest of the planets you talked about?
I can’t see any of them. I
can see the Moon, and earlier I saw the Sun.
So where’s the other planets?”
“Well, Io, you can’t see them because they are millions of miles away.
You can see the sun because it is gigantic.
It could fit all the planets inside of it many times.
The Moon isn’t very large. In
fact, it is smaller than most of the planets, but we can see it because it is so
close to us compared to the other planets and the stars. From Earth, planets look much like the distant stars because
they reflect our Sun’s light.
Early
astronomers used lenses to make the planets seem closer.
These lenses were put into tubes and called telescopes.
Before telescopes were invented,
it was difficult to see distant objects in the night sky. Therefore, astronomers
were limited in their progress. After the discovery of the telescope about 300
years ago, star gazing became easier, and we have found out much more about our
solar system, the Milky Way galaxy, and our universe.
The earliest telescopes were the refracting and reflecting telescopes. In the
1930’s came radio telescopes that didn’t need light to "see".
Today we have space telescopes, which are satellite telescopes located above the
Earth’s atmosphere."

When the Hubble Space Telescope was brought into space by the space shuttle
Discovery, it was supposed to get clearer pictures and collect better
information about things in space. The Hubble did all that and much more. Using
the Hubble, people have been able to find out many things about space. The
Hubble has expanded our understanding of star birth, star death, and galaxy
evolution. It has moved black holes from a theory to a fact. It has even
downloaded over 100,000 pictures of the universe in the last eight years.

Radio telescopes were first invented in the late 1930’s. An American
engineer named Grote Reber built the first one. Radio telescopes can produce
images of objects in space without requiring light to "see". Radio
telescopes use a bowl shaped reflector called a dish to collect radio waves in
space. The reflector focuses the waves onto an antenna that changes them into
electrical signals. A radio receiver amplifies these signals and records their
strength. The information is analyzed by the computer to draw a picture of the
source of the radio waves.

Galileo Galilee made the first refracting telescope that was used for looking
at space in 1609. Using it, he discovered 4 of Jupiter’s moons. He also used
the refracting telescope to map the surface of the moon. James Gregory invented
the reflecting telescope in 1663. He came up with the design for the telescope,
but Isaac Newton actually made the first one in 1688.

We've found some great videos that show how different kinds of telescopes
work. You will need shockwave on your computer to play them. Just
click on the telescope, and you will open up a new window to see the
video. When you're finished, just close the window and you come right back
here!
