Whenever you
look up at night you see what astronomers thousands of years ago saw.
This section tells some history, defines terms, explains telescopes
and other tools that astronomers use and gives observing hints. When
you are ready, click back to return to the Student Center or click below
to explore again.
History
For most of
recorded history the Earth was the center of the universe and never
moved. The constellations were named and stories were told about them.
The Greek Aristotle wrote in the third century BC that the Earth was
a sphere because different stars could be seen as you move north and
south and the shadow of the Earth on the moon during an eclipse was
curved. A hundred or so years later, Eratosthenes used the length of
the shadow cast by the sun to determine the circumference of the Earth.
In the second century AD Ptolemy gathered star catalogs and astronomical
writings. Astronomers were called astrologers at the time and tried
to predict events using the stars. Ptolemy proposed that the solar system
was like a huge carousel with the Earth as the center and the planets,
stars, sun and moon riding where the horses would be.
After about 1400 years Nicolaus Copernicus used mathematics to place
the sun in the center of the "carousel" to better allow for
how the sun, planets and stars appear to move. Johannes Kepler expanded
on the idea using elliptical orbits to predict planetary motion.
Soon after the invention of the refracting telescope, Galileo Galilei
used one to view craters on the moon and watch the moons of Jupiter
circle the planet. This validated the idea that the sun was in the center
of the solar system and the Earth orbiting it. In addition, Isaac Newton
invented the reflecting telescope that used a mirror instead of a glass
lens and proposed the Theory of Gravity which explained how the planets
were held in place. At about this time Gian Cassini measured the distances
between the planets using a method called parallax shift. This is similar
to watching the thumb on your outstretched arm "move" from
side to side when you close one eye and then the other.
This is, of course, a very brief and narrow view of history but will
give you a few clues for further study. There are many contributions
by women and non-European cultures that would make a great report project
and Internet search practice. See the links below.
Here is a list of other contributors to astronomy you may want to research.
Hipparchus, Tycho Brahe, Edmond Halley,
William and Caroline Herschel, Edwin Hubble,
Henrietta Swan Leavitt, Harlow Shapley, Percival Lowell,
Vesta Slipher and Albert Einstein.
Terms
Here are some
basic terms used in astronomy.
Asterism
A named group of stars that is part of
a constellation, the Big Dipper is one.
Asteroid
Small, rocky world. Most asteroids are
between the orbits of Mars and Jupiter.
Astronomical Unit
The average distance between Earth and
the sun, 1.5 x 108 km.
Aurora
The glowing light from solar particles
interact with Earth's magnetic field.
Celestial Equator
The imaginary line around the sky directly
above the Earth's equator.
Celestial Pole
Points above the Earth's north and south
poles.
Celestial Sphere
An imaginary sphere surrounding the Earth
where the sun, planets and stars are, a 3 dimensional map
of the universe.
Comet
One of the small, icy bodies that orbit
the sun that make tails of gas and dust when they get close to
the sun.
Constellation
A pattern of stars usually named after
animals or people in stories.
Ecliptic
The path the sun seems to follow in the
sky.
Emission Nebula
A cloud of glowing gas.
Globular Star Cluster
A group of stars that look like a shape
of a ball.
Light Pollution
Wasted light from city and outdoor lights
that makes it hard to see the stars at night.
Light-year
The distance light travels in a year.
Meteor
Small rocks or sand making a bright trail
through the sky as it burns in the atmosphere.
Meteorite
A meteor that has landed on the Earth.
Nebulae
A glowing clouds of gas or dust reflecting
the light of nearby stars.
Open Star Cluster
A group of stars that look close together
in the sky.
Orbit
The path an object takes as it moves around
another object.
Planetary Nebula
An expanding ring of gas around a star.
Reflecting Telescope
A telescope that uses a mirror to focus
light.
Reflection Nebula
Dust and gas reflecting light from stars
close by.
Refracting Telescope
A telescope that uses a lens to focus
light by bending it.
Rotation
An object spinning about its center.
SETI
The Search for Extra-Terrestrial Intelligence.
Solar Eclipse
The name of the event when the moon comes
between the sun and Earth.
Zenith
The point in the sky directly overhead.
Telescopes
Telescopes come in different sizes, designs and styles. The usefulness
of the power of the instrument is limited by the size of the lens or
primary mirror. The table below summarizes the three main types of optical
telescopes. Radio telescopes use the reflecting design, however, they
focus radio waves instead of light.
Galileo used the refracting type of telescope to discover the moons
of Jupiter. Most large observatories use the reflectors. These are sometimes
known as "Newtonian" telescopes named after the inventor Isaac
Newton.
Telescope
Types
Refracting

Reflecting

Combination
Telescope
Types
Refracting
The incoming light is focused by the objective lens and directed down
the tube to the eyepiece.
The focused image is then magnified by the eyepiece.
Reflecting
The incoming light is focused by the primary mirror and directed up
the tube to the secondary mirror. The light travels to the eyepiece.
The focused image is then magnified by the eyepiece.
Combination
The incoming light is adjusted by the corrector plate before it travels
down the tube. Then the light is focused by the primary mirror and directed
back up the tube to the secondary mirror. Finally, the light travels
back down the tube through a hole in the primary mirror to the eyepiece.
The focused image is then magnified by the eyepiece.
Telescopes are
attached to various types of mounts. Some are mounted on tripods like
a camera and some, called Dobsonian mounts, rest in boxes that move
up and down and around like a lazy susan. Equatorial mounts can be aligned
with the axis of the Earth to help keep an object centered in the eyepiece.
Some newer mounts have built-in electronics and computers to point to
any celestial object in the night sky.

From
left to right are the Dobsonian, Equatorial and Fork mounts.
The diameter of the telescope primary lense or mirror determines how
much light is focused in the eyepiece and how much detail you can see.
Telescopes as small as 60 mm in diameter with the right lenses can view
the craters of the moon, the rings of Saturn, cloud bands on Jupiter,
and split binary stars. Most observers, however, prefer 4 inch or more
in size.
Observing
Hints
There are a
number of things you should keep in mind when observing the night sky.
First, learn the sky using your eyes and binoculars. Find out where
each constellation is located and how to find out what time of year
they can be seen. Learn to estimate how big a constellation is in the
night sky. Learn the names of the brighter stars. This preparation makes
it easier to find objects because when you are looking through a telescope
you see only a small part of the sky.
Soon you can learn how to read star maps and how to find binary stars,
nebulae, galaxies and the planets. Keep a log of your adventure.
Dress for cooler temperatures, bring a chair or blanket to sit on and
let your eyes adjust to the darkness. Sometimes you can just lay on
your back and look for meteors, satellites and the aurora. Bring snacks
and beverages and make it a fun family time discovering the cosmos.
For more information on observing go to the Astronomical League pages
describing their viewing programs. The site below will open up in a
new window. Close the window to return to Kid's Cosmos.