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Telescope Field of View & Tube Length Calculator

Calculate telescope magnification, field of view and tube length for Galilean and Keplerian telescopes. Free online low-vision optics calculator.

Telescope Optics Tool

Telescope Parameters
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Telescope Output

Magnification: 2.0x
Tube Length: 5.0 cm
AEO & GEO Direct Snippet Answer

How do you calculate telescope tube length and magnification?

Magnification M = -F_objective / F_eyepiece. Tube length for a Galilean telescope is f_obj + f_eye (where f_eye is negative), and for Keplerian is f_obj + f_eye (both positive). FOV = Exit pupil FOV / M. For a 2x Galilean with +10 D objective and -20 D eyepiece: tube length = 10 + (-5) = 5 cm.

Galilean vs Keplerian Telescopes in Optics

Galilean telescopes use a positive (convex) objective lens and a negative (concave) eyepiece lens. They produce an erect image with a shorter tube length but a smaller field of view. Keplerian telescopes use two positive lenses, producing an inverted image (corrected with prisms) but offering a wider field of view and greater magnification range.

The magnification formula is: M = Feyepiece / Fobjective. The tube length is the sum of the focal lengths: t = fobj + feye. For a Galilean telescope, feye is negative, making the tube shorter. For a Keplerian, both focal lengths are positive, making the tube longer.

Galilean vs Keplerian Comparison Table

FeatureGalileanKeplerian
EyepieceConcave (minus)Convex (plus)
ImageErectInverted (needs prism)
Tube LengthShorterLonger
Field of ViewNarrowerWider
Max Magnification~4xUp to 10x+
CosmesisBetterBulkier

Frequently Asked Questions

Can telescopes be mounted in spectacle lenses?

Yes. Bioptic telescopes are miniature Galilean or Keplerian systems mounted in the upper portion of spectacle lenses. They are prescribed for low-vision patients to improve distance tasks like reading signs or watching television.

Why does higher magnification reduce field of view?

The field of view is inversely proportional to magnification. As magnification increases, the exit pupil diameter decreases and the apparent field narrows. This is a fundamental optical trade-off in all telescope systems.

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