Telescope Magnification Calculator
Enter your telescope's objective focal length and eyepiece focal length — get magnification instantly in your browser
Showing example: 1200 mm telescope + 25 mm eyepiece = 48×. Enter your own values to get your result.
Telescope Parameters
Result
- Magnification
- 48.0×
How Telescope Magnification Works
The Magnification Formula
Magnification = Objective Focal Length ÷ Eyepiece Focal Length. A 1200 mm telescope with a 25 mm eyepiece yields 48×. Shorter eyepiece focal lengths produce higher magnification — a 10 mm eyepiece on the same telescope gives 120×.
Sky & Telescope: Magnification GuideUseful Magnification Limits
Every telescope has practical limits. Minimum useful magnification ≈ Aperture(mm) ÷ 7 (limited by the eye's pupil). Maximum ≈ Aperture(mm) × 2 (limited by atmospheric seeing). Pushing beyond maximum yields a blurry, empty image.
Cloudy Nights: Magnification LimitsChoosing the Right Eyepiece
Low-power eyepieces (25-40 mm) are ideal for large deep-sky objects and star clusters. Medium-power (10-20 mm) works for general observing. High-power (4-8 mm) is best for planetary detail and double stars — when seeing conditions allow.
Sky & Telescope: Choosing EyepiecesEyepiece Barrel Sizes
Eyepieces come in 1.25″ and 2″ formats. 2″ eyepieces allow wider true fields of view at low magnification — essential for large nebulae and galaxies. Most telescopes accept 1.25″ eyepieces; check your focuser before buying 2″.
Cloudy Nights Equipment ForumsFrequently Asked Questions
- How do I calculate telescope magnification?
- Magnification = Objective (Telescope) Focal Length ÷ Eyepiece Focal Length. Both values are usually printed on the telescope and eyepiece. Enter them above and this calculator computes the result instantly — no manual math needed.
- What magnification do I need to see planets?
- For Jupiter's cloud bands and Saturn's rings, aim for 100-150×. For Mars polar caps and surface detail, 150-250× is ideal — but only when the atmosphere is steady (good 'seeing'). Lunar craters show well at 80-200×. Remember that maximum useful magnification is approximately 2× per millimetre of aperture.
- Why does a higher magnification show a dimmer image?
- Doubling the magnification spreads the same amount of light over 4× the area, reducing surface brightness to 25%. The exit pupil (Eyepiece FL ÷ f/ratio) also shrinks. For bright objects like the Moon and planets this is acceptable; for faint deep-sky objects, stay at lower magnifications (larger exit pupil) to preserve brightness.
- Can I use a Barlow lens to increase magnification?
- Yes. A 2× Barlow lens doubles the effective focal length of your telescope, which doubles magnification with any eyepiece. For example, a 1200 mm telescope with a 2× Barlow becomes effectively 2400 mm — a 25 mm eyepiece then yields 96× instead of 48×. A Barlow effectively doubles your eyepiece collection.
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Free, browser-only telescope magnification calculator. Enter objective focal length and eyepiece focal length — magnification is computed instantly in your browser. No upload, no server, no data transmitted. · All calculations execute client-side — zero network requests. · Magnification formula verified: standard optical textbook formula. No approximation error for valid input values. · Formula: standard telescope optics (Carroll & Ostlie, Ch.6) · Methodology v1.0.0