T
ELE
SCO
PE
T
E
R
M
INO
L
OGY
O
BJECTIVE
- The objective is the front lens of a telescope. The measurement listed for objec-
tive lenses is the diameter of the lens. A larger objective allows more light to enter a telescope
and provides a brighter image. The objective diameter is also sometimes referred to as the
aperature of a telescope.
F
OCAL
L
ENGTH
- The focal length of a telescope is the distance from the point where light
enters a telescope (the objective) to the point where the image is in focus. In telescopes
with the same size objective, a longer focal length will provide higher magnification and a
smaller field of view.
M
AGNIFICATION
- The magnification of a telescope is determined by the relationship between
the focal length of the telescope and the focal length of the eyepiece used. The greater the
difference in focal lengths, the greater the magnification. A telescope has a maximum use-
ful magnification of about 60 times the diameter of the objective in inches. Magnification
beyond the maximum useful magnification will provide dim, low-contrast images.
F
OCAL
R
ATIO
- The focal ratio of a telescope describes the ratio between the focal length
and objective size of a telescope. Visually, the smaller the focal ratio (also called f-stop) of a
telescope, the wider the field of view. Photographically, the lower the f-stop, the shorter the
exposure time needed to capture an object on film.
L
IMITING
M
AGNITUDE
- The limiting magnitude of a telescope describes the faintest object
you can see with a telescope. The magnitude of a star describes its brightness. The larger the
magnitude of an object, the fainter it appears to be. The brightest stars have a magnitude
of 0 or less.
R
ESOLVING
P
OWER
- The resolving power, or Dawes’ Limit, of a telescope is the ability
to view closely spaced objects through a telescope. The resolving power of a telescope is
measured in seconds of arc. The smaller the resolving power, the better you will be able to
separate binary stars when viewing through your telescope.
A
BERRATION
- Aberrations are degradations in image which may occur due to optical system
design or improper alignment of optical system components. The most common types
of aberration are chromatic aberration, spherical abberation, coma, astigmatism, and field
curvature.
C
OLLIMATION
- Collimation is the alignment of optical components within an optical system.
Improper collimation will distort an image and may result in abberations present in the im-
age. Most reflector telescopes have collimation adjustments which can be made in order to
reduce aberrations and image distortion.
Summary of Contents for Tycho
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