Barlow lens
A diverging lens, placed in front of the focal point of a telescope, that
increases both magnification and eye
relief when used in conjunction with an eyepiece.
The magnification is typically doubled, though at the cost of a fainter
image. Invented in 1834 by the English engineer and mathematician Peter
Barlow (1776–1862), the lens is used
commonly by amateur astronomers.
Related categories
OPTICS
AND OPTICAL PHENOMENA TELESCOPE
EQUIPMENT AND TECHNIQUES
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