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The resolving power of a telescope is the ability to produce an image in which objects that are close together can be seen separately.

Resolving power is sometimes expressed in terms of the inverse of the minimum angle there must be between two points in order to see them separated.

This minimum angle is proportional to (lambda/d) where d=diameter of objective

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Not intended to improve, just a comment:

Think of resolution and clarity as the telescopes Dots per Inch (DPI).

Low DPI , Poor resolution = blurry TV picture

'Best' DPI= High Definition.

Personally on my LX2080 I get better resolution at lower powers of magnification than very high.

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10y ago

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The resolving power of a telescope is a measure of its ability to distinguish between two closely spaced objects. It indicates how much detail can be seen in an image produced by the telescope. A higher resolving power means that the telescope can separate two objects that are close together more effectively.

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10mo ago
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