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INTRODUCTION
Astronomy is a fascinating lifetime hobby enjoyed by young children
to centenarians, by people from all walks of life and with varied
interests.
You can observe or photograph the universe on a casual or serious
basis. Astronomy can be a fun and relaxing way to soothe our minds
and bodies from our hectic everyday life. It is a way to enjoy
nature, being outside and marveling at the night sky.
Astronomy is fun and easy to learn! You don't have to be a scholar
in physics or math to enjoy our universe. Besides binoculars or
a telescope you will need star maps or books listing the location
of various objects in the sky.
A telescope is an instrument designed for the observation of remote
objects. The term usually refers to optical telescopes, but there
are telescopes for most of the spectrum of electromagnetic radiation
and for other signal types like Radio and X-ray etc.
A telescope (optical) gathers and focuses light. Telescopes increase
the apparent angular size of distant objects, as well as their
apparent brightness. Telescopes work by using one or more curved
optical elements like lenses or mirrors, to gather light and bring
that light to a focus, where the image can be observed, photographed
or studied.
HISTORY OF TELESCOPE
The telescope was the first optical instrument and its origin
is surrounded by controversy. The most likely story puts it in
the shop of a Dutch spectacle maker named Hans Lippershey, about
1600. Two children were playing with his lens, put two together,
peered through them at a distant church tower and saw it wonderfully
magnified. Lippershey looked for himself and soon mounted lenses
together, creating his instrument called "looker." Unfortunately
the telescopes built on Lippershey's model had poor image quality,
caused by the bending of light though the glass lenses. (Glass
does not bend the different colors of light equally. Red light
is bent the least causing a colour distortion in the image.) Isaac
Newton eventually solved this problem in 1668 by making a telescope
that worked with mirrors in place of lenses.
Galileo Galilei was the first person to use the telescope to study
the heavenly bodies, in 1609. Galileo was able to see that the
moon was not smooth, but covered with huge valleys and craters.
He discovered four moons orbiting Jupiter and found out that Venus
has phases just like the moon. He realized that this must mean
that Venus, and the other planets, revolve around the sun not
around the earth, as many people believed at the time.
WHAT YOU CAN SEE WITH A TELESCOPE
Some of the types of celestial objects you can view are:
THE MOON ? Prepare for an awesome spectacle.
The moon's disk has a pastel-cream and gray background, streamers
of material from impact craters stretch halfway across the lunar
surface, river-like rilles wind for hundreds of miles, numerous
mountain ranges and craters are available for inspection. At
low or high power the moon is continually changing as it goes
through its phases. Occasionally you will be treated to a lunar
eclipse.
THE SUN - It is quite safe to view the Sun
by projecting image of sun on a sheet of paper. The Sun is fascinating
to inspect as you detect and watch the ever-changing sunspot
activity. If you are fortunate enough, and are willing to travel
to remote locations, you may at some point experience a solar
eclipse.
THE PLANETS - You will find views of the planets
through a telescope quite satisfying, and they will keep you
coming back for more. You can also observe planets from urban
areas, where there may be moderate to substantial light pollution.
With a small telescope (2-inch or 60-mm refractor, 4-inch or
100-mm reflector), you can see some details on the surfaces
of planets, but a larger telescope (3- to 4-inch or 75- to 100-mm
refractor, 6- to 10-inch or 15- to 25-cm reflector) will reveal
better detail. Generally, refractors provide crisper images
of planets, but lack the light gathering ability of reflectors.
Regardless of which type of telescope you use, observing planets
requires good seeing conditions -- steady, dry atmosphere with
little or no clouds -- and you should cool your telescope to
the outside temperature for about 30 minutes before observing.
Cooling the telescope reduces air currents inside the tube that
could produce fuzzy, blurring images.
Venus ? You won't see any surface detail on
Venus because it is covered with clouds. You can find something
interesting to look at, though, because Venus has phases just
like the moon, and you can easily see these phases with any
telescope. Also, Venus is one of the brightest objects in the
sky, and you can find it easily. Usually, Venus can be seen
above the horizon before or after sunset; you can see it referred
to in newspapers as "the morning star" or "the
evening star."
Mars ? Mars is a difficult but challenging
target, because of its distance and small size. In a 4-inch
(100-mm) rich-field, in a reflecting telescope, one can see
a small red disc with no surface detail. In an 8- to 10-inch
(20- to 25-cm) reflector, you could probably see the polar ice
caps and some dark surface features ("canals") depending
upon the seeing conditions. However, the face of Mars is constantly
changing. Using filters may help to enhance the viewing somewhat.
Jupiter ? This is about the size of the image
of Jupiter in a telescope.
Jupiter is one of the prettiest sights in a small telescope.
It is the largest planet in our solar system, and you can find
it easily. In a 4-inch reflector, one can see Jupiter as a small,
bright yellow disc, usually with two brown cloud bands on either
side of its equator. In a larger telescope (8- to 10-inch /
20- to 25-cm reflector), you could see more cloud bands and
the Great Red Spot. You can also see the moons of Jupiter (Galilean
satellites) -- Io, Europa, Callisto and Ganymede. The moons
orbit Jupiter in changing positions each night, and they are
interesting to watch over the course of many days. In a large
telescope (8 to 10 inch or 20 to 25 cm reflector), you can even
watch the shadow of a moon cross the disc of Jupiter!
Saturn ? Saturn is a favourite object for a
telescope because of its rings. The rings of Saturn change their
angle as seen from Earth as Saturn orbits the sun. So sometimes
the rings are highly visible, while other times you cannot see
them at all (viewed edge-on). Saturn is a bright object that
you can easily find. In a telescope, Saturn appears as a small,
bright yellow ball with the rings around it. one cannot see
any surface detail, or the gap between the rings called the
Cassini division. These features would probably be visible in
a larger telescope. Like Jupiter, Saturn has several moons --
Titan, Iapetus, Phoebe -- that change position. One may have
difficult time seeing Saturn's moons in a telescope, although
may be able to see one of them on a good night. However, a larger
telescope would probably reveal them much better.
Uranus, Neptune and Pluto ? Because of their
great distance from Earth, these planets are difficult to locate,
a challenge for any observer. In a larger telescope, it is likely
that these planets could still only appear as small discs
Asteroids ? Like the outer planets, asteroids
are difficult to see in small telescopes. Because they are so
small, they appear in a telescope as points of light, like stars.
Typically, to locate an asteroid, you find its position from
a chart and then look at the field of stars. The asteroid will
be a bright object that looks out of place when compared to
the chart. If you look at the same field on successive nights,
the asteroid will be the object that moves in the field. Finding
these objects takes patience! Some advanced observers will measure
the light intensities of asteroids over time, using photometers
or CCD/digital cameras attached to the telescopes. You can use
the changes in the light intensities to calculate the rate of
the asteroid's rotation.
STAR CLUSTERS - There are two types of star
clusters- (1) open star clusters (also called galactic clusters)
which are loosely arranged groups of stars, occasionally not
too distinctive from the background stars, and (2) globular
star clusters which are tightly packed groups of many millions
of stars.
NEBULAE - These are glowing clouds of gas falling
into two types- (1) planetary nebulae which are relatively small
ball-shaped clouds of expanding gases and are believed to be
the remnants of stellar explosions, and (2) diffuse nebulae
which are vast, irregularly-shaped clouds of gas and dust.
GALAXIES - These are vast, remote "island
universes," each composed of many billions of stars. Galaxies
exist in a variety of sizes with regular and irregular shapes.
COMETS - Magnificent comets are routinely visible
through telescopes.
DOUBLE (BINARY) STARS - These are pairs of
stars orbiting around a common center of gravity, often of different
and contrasting colors.
What you can see is dependent on a lot of factors. The most
important of these for astronomy is aperture. Other important
factors are optical quality, steadiness of your stand and mount,
seeing conditions, your location (city or rural), brightness
of the object and your experience. You won't see as much color
as you see in astrophotographs (photos of celestial objects)
because these utilize long exposure times which allow the light
and color to build up on the film.
Astrophotography is also a rich and rewarding experience. With
many telescopes it is relatively easy, but takes patience and
experience to produce excellent results. Taking your own astrophotographs
is a thrill as you can share the results with others.
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