Telescope Magnification Calculator

Magnification and true field of view from your telescope's focal length and any eyepiece.

mm
mm
°
Magnification (×)
36
  1. Magnification (×)36
  2. True field of view (°)1.39
  3. Full Moons that fit across the view2.7
Inputs used
  • Telescope focal length900 mm
  • Eyepiece focal length25 mm
  • Eyepiece apparent field of view50 °

About this calculator

Magnification is simply the telescope's focal length divided by the eyepiece's: a 900 mm telescope with a 25 mm eyepiece gives 36×, and swapping in a 10 mm eyepiece raises that to 90×. Shorter eyepiece, higher power.

Higher isn't automatically better. Divide the eyepiece's apparent field of view by the magnification to get the true field — the patch of sky you actually see. At 36× with a 50° eyepiece you get 1.4°, nearly three full Moons wide and great for star clusters; at 180× you're down to 0.28°, a tight crop suited to planets and double stars.

A practical ceiling: about 2× per millimetre of aperture (a 130 mm telescope tops out near 260×). Beyond that, the image grows dimmer and blurrier without revealing anything new — the atmosphere usually caps useful power at 150–250× anyway.

Quick reference

Magnification by eyepiece and telescope focal length

Common eyepiece sizes against popular telescope focal lengths (mm).

Eyepiece focal length650 mm900 mm1,200 mm2,000 mm
4 mm163225300500
6 mm108150200333
10 mm6590120200
15 mm436080133
25 mm26364880
32 mm20283863

Frequently asked questions

How do I calculate telescope magnification?

Divide the telescope's focal length by the eyepiece's focal length, both in millimetres. A 1200 mm telescope with a 10 mm eyepiece gives 1200 ÷ 10 = 120×.

What magnification do I need to see Saturn's rings?

The rings become visible around 25–30× and look clearly ring-shaped at 100× or more, seeing conditions permitting. Steady air matters more than raw power — a crisp 120× beats a wobbly 250× every night.

Why does everything look dimmer at high magnification?

The telescope gathers a fixed amount of light, and magnifying spreads it over a larger apparent area. Doubling the magnification makes the view four times dimmer per unit of sky — one reason faint galaxies are hunted at low power.

Results are informational only — not financial, medical or legal advice.