Fig. 15: 25mm and 9mm eyepieces.
DEFINITION:
A capital "X" is used to denote an eye- piece's (or a Barlow's) power or magnification. For example, "40X" is read as
image) has been aligned to the main telescope. Fig. 13B shows these same images after the viewfinder and main telescope are aligned.
5.Check this alignment on a celestial object, such as the Moon or a bright star, and make any necessary refinements.
Choosing an Eyepiece
A telescope’s eyepiece magnifies the image formed by the telescope’s main optics. Each eye- piece has a focal length, expressed in millimeters, or “mm.” The smaller the focal length, the higher the magnification. For example, an eyepiece with a focal length of 9mm has a higher magnification than an eyepiece with a focal length of 25mm.
Your telescope comes supplied with a
Low power eyepieces offer a wide field of view, bright,
NOTE: Viewing conditions vary widely from
The power, or magnification of a telescope is determined by the focal length of the telescope and the focal length of the eyepiece being used. To calculate eyepiece power, divide the tele- scope's focal length by the eyepiece's focal length. For example, you may wish to use a 25mm eyepiece with the
Telescope focal length divided by Eyepiece focal length = Eyepiece power
1000 25 = 40
The eyepiece power, or magnification is therefore 40X (approximately).
The Barlow Lens
Some Meade telescopes include a power multiplier called a Barlow lens. Consisting of a lens mounted in a
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