Telescope Basics - Celestron XLT series Instruction Manual

Omni xlt series telescopes
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A telescope is an instrument that collects and focuses light. The nature of the optical design determines how the light is focused.
S
ome tele opes, known as re
sc
fractors, use lenses. Other
S
chmidt-
Ca
ssegrai elescop
n t
e uses both mirrors and len
D
evelope in the early 1600s,
d
in
coming ght rays
li
. The refractor uses a l
designs used single element lenses. However, the single len
r
ainbow, a phenomenon known as chromatic aberration. To
w
as introduced. Each element has a different index of refraction allowing two different wavelengths of light to be focused at the
same point. Most two-element lenses, usually made of crown and flint glasses, are corrected for red and green light. Blue lig
may still be focused at a slightly different point.
A
A
A
New
tonian reflector uses a single concave mirror as its primary. Light enters the tube traveling to the mirror at
th
e back end. There light is bent forward in the tube to a single point, its focal point. Since putting your head in
front of the telescope to look at the image with an eyepiece would keep the reflector from working, a flat mirror
called a diagonal intercepts the light and points it out the side of the tube at right angles to the tube. The eyepiece
p
laced there for easy viewing.
Newtonian Reflector telescopes replace heavy lenses with mirrors to collect and focus the light, providing much
more light-gathering power for the dollar. Because the light path is intercepted and reflected out to the side, yo
have focal lengths up to 1000mm and still enjoy a telescope that is relatively compact and portable. A Newtonian
Reflector telescope offers such impressive light-gathering characteristics you can take a serious interest in deep
space astronomy even on a modest budget. Newtonian Reflector telescopes do require more care and maintenance
because the primary mirror is exposed to air
te
lescope's popularity with those who want an economical telescope that can still resolve faint, distant objects.
telescopes, known as reflectors (Newtonians), use mirrors. Then, the
ses. Each optical design is briefly discussed below:
the refractor
is the oldest telescope design. It derives its name from the method it uses to focus
ens to bend or refra
s acts like a prism and breaks light down into the colors of the
Figure 3-1
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and dust. However, this small drawback does not hamper this type of
ct incoming light rays, hence the name (see Figure 4-1). Early
get around this problem, a two-element lens, known as an achromat,
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Omni xlt 102Omni xlt 120Omni xlt 150Omni xlt 127

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