Barlow Lens
An auxiliary lens that increases the power by a factor.
For example, a 2x Barlow doubles the magnification
of the telescope.
Erecting Lens
Lens used with a refractor telescope when viewing
land-based objects to correct the normally upside-down
image provided by an astronomical telescope.
Finderscope
On most astronomical telescopes a lower powered
finderscope with a wider field-of-view lets the
user quickly locate the object to be viewed by
the high-magnification main telescope. There
are two types of finderscopes, optical and red
dot.
Focal Length
The measured light path of the optical system (tube
length), typically measured in millimeters.
Focusing Knob
Controls the rack and pinion focusing system. Permits
smooth movement of eyepiece for precise, sharp
images.
Objective Lens Size (or Aperture)
The second number in the formula (100x4.5")
is the
diameter of the objective lens or mirror. The aperture
relates directly to how bright images will appear
and how much detail is revealed. The larger the
objective lens, the better. The size of the telescope's
objective lens, or aperture, limits the amount
of power that can be used effectively. As the
magnification of an object increases, the brightness
of the image decreases. This is because the light
gathered by
the telescope is being spread over a larger area.
Aperture also limits the clarity of an image at
increased magnification. When magnified beyond
an aperture’s recommended power, the image
dims and becomes fuzzy.
Magnification (Power)
Telescopes are often referred to by two numbers
separated by an "x". For example:
100x4.5".
The first number is the power or magnification
of the telescope. With a 100x4.5" telescope,
the object being viewed appears to be 100 times
closer than you would see it with the
unaided eye. The magnification of a telescope is
determined by dividing its focal length by the
focal length of the eyepiece being used. For example,
a 500mm telescope with a 5mm eyepiece would magnify
objects 100x. Thus, a telescope can provide nearly
any magnification required depending on the focal
length of the eyepiece used. Since most objects
in the sky are rather large, high magnification
isn't necessary. Rather, a telescope that
gathers lots of light is needed to make dim objects
appear brighter and sharper. The power or magnification
contributes to the overall size and bulk of the
telescope. This is because as the power increases,
so must the physical size of the objective lens.
Penta Mirror Technology*
This patented Bushnell® technology breakthrough
allows for left-to-right correct view of the stars
(not backwards – as in most telescope models)
taking the guesswork out of where to move the telescope.
This feature provides unparalleled ease of use
for finding and tracking objects with a 90 degree
viewing angle and 1.25" eyepiece adapter.
Resolution
Resolution, or definition, is the ability of a
telescope to
distinguish fine detail and retain clarity.
Rotary Power Turret*
This patented Bushnell feature allows for magnification
and accessory changes to occur through a simple
twist of the
turret or accessory dial. Accessories are incorporated
into the telescope so there are no loose parts,
and magnification and accessory changes can be
made instantaneously to suit
viewing conditions. |