Transcript File

Astronomy for beginners
Telescopes
By Aashman Vyas
What are Telescopes?
A telescope is an instrument designed for
the observation of remote objects by the
collection of Light
 A telescope’s diameter is measured in
inches, meters or centimeters
 Eg: A 6inch Telescope is bigger than a
4inch Telescope because it can collect
more light

How do Telescopes Work?
Telescopes work by using a system of
mirrors and lenses to refract, magnify or
bend light
 They can be used for terrestrial viewing
and deep-space viewing
 The main purpose of the Telescope is that
they make far away objects seem more
closer

Telescopic Words







Aperture: Aperture is the size of the main optical lens of the
Telescope
Counter weight: The thing that keeps the Telescope Balanced on it’s
Tripod
CCD Camera: A CCD Camera converts optical brightness into
electrical Signals that are sent to a Computer. (Otherwise known as
a Telescope image/video Camera)
Lens: An Eyepiece attached to a Telescope that lets you see stuff.
Magnitude: Magnitude of a celestial body is a measure of its
brightness as seen by an observer on Earth
Observatory: A type of domed house housing a large Telescope
Electromagnetic Spectrum: The Spectrum of Light with all the other
wavelengths
Types of Telescopes
There are many types of Telescopes
 Refractor
 Newtonian Reflector
 Schmidt-Cassegrain (falls under
Catadioptric category)

Refractor Telescope




The Refractor, is a telescope that
uses lenses to refract, (bend), the
light that it collects
This refraction causes parallel
light rays that converge at a focal
point at the opposite end, where
they can be magnified by an
eyepiece
The large lens at the front is called
the objective lens. The objective
lens is usually composed of two or
more individual lenses that are
bonded and or arranged together
to make up what is called the
objective lens cell
The glass material used can also
vary which will help in the overall
performance of the objective lens
Refractor Telescope
Advantages and Disadvantages
Advantages
-Little or no maintenance and is
easy to use
-Reliable due to the simplicity of
design
-Good for terrestrial viewing
-Objective lens is usually
permanently mounted and
aligned
-Sealed optical tube reduces
image degrading air currents
and protects the optics

Disadvantages
-Usually more expensive per inch
of aperture than Newtonians or
Catadioptrics
-Heavier, longer and bulkier than
equivalent aperture
Newtonians or Catadioptrics
-Less suited for observation of
deep sky objects such as
distant galaxies and nebulae
because of practical aperture
limitations

Newtonian Reflector


The Newtonian Reflector,
is a telescope which uses
a spherical or concave
parabolic primary mirror
to collect, reflect and
focus the light onto a flat
secondary mirror
This secondary mirror in
turn reflects the light out
of an opening in the side
of the tube and into an
eyepiece for focus and
magnification
Newtonian Reflector
Advantages and Disadvantages
Advantages
-Excellent for faint deep sky
objects such as remote
galaxies, nebulae and star
clusters due to the generally
fast focal ratios
-Reasonably compact and
portable up to focal lengths of
1000mm
-Low in optical abnormalities and
deliver very bright images

Disadvantages
-Requires regular alignment
(collimation) of optics in order
to perform at its best. Badly
aligned optics can make the
image quality suffer quite
dramatically.
-The open nature of the tube
assembly could mean more
complicated cleaning of mirror
surfaces when compared to
telescopes of other designs
-Generally not suited for terrestrial
applications
-Slight light loss due to secondary
(diagonal) obstruction when
compared with refractors

Schmidt-Cassegrain




In Schmidt Cassegrain designs
the light enters a thin aspheric
Schmidt correcting lens
The light then strikes the
primary mirror and is reflected
back up to the secondary
mirror that reflects the light out
an opening in the rear of the
instrument
Schmidt's usually have shorter
focal lengths thus making them
more suitable for fainter deep
sky objects
The thinner corrector plate
means the Schmidt is faster to
reach thermal stability
Schmidt-Cassegrain
Advantages and Disadvantages
Advantages
 -Best all-around, all-purpose
telescope design. Combines
the optical advantages of both
lenses and mirrors while
canceling their disadvantages
-Excellent for deep sky observing
or astrophotography with fast
films or CCD's
-Very good for lunar, planetary
and binary star observing or
photography

Disadvantages
-More expensive than Newtonians
of equal aperture
-It is not what people expect a
telescope to look like
-May suffer from image shift when
focusing due to focus design
moving the entire primary
mirror

Bibliography
The big book of Stars and Planets by
Robin Kerrod
 Google Images
 www.aoe.com.au/telescope_types.html
 Ask an Astronomer.com
 Bluebird Book’s Tell me how

Thank You For
Watching!!!