Telescope Magnification Calculator

Find angular magnification M = f_o / f_e for normal adjustment

Parameters

cmⓘ
cmⓘ
Show Trail

Controls

xⓘ

Calculated Values

Magnification:
10.00;×10.00;×
Tube Length (approx):
110.00;cm110.00;cm

Examples

f_o=100, f_e=10

10× telescope.

    Visualization

    Telescope Angular Magnification

    An astronomical refracting telescope in normal adjustment (relaxed eye, final image at infinity) has angular magnification M = f_o/f_e, where f_o is objective focal length and f_e is eyepiece focal length.

    Large M requires long objective (high f_o) and short eyepiece (small f_e). Tube length L ≈ f_o + f_e. Objective diameter sets light-gathering and resolution, not M directly.

    Example: f_o = 100 cm, f_e = 2 cm → M = 50×. Field of view decreases as M increases. Terrestrial telescopes add erecting prisms; magnification formula may include sign conventions.

    Reflecting telescopes use curved mirrors with same M concept for eyepiece combination. Newtonian, Cassegrain designs fold optical path.

    Magnifying glass alone: M ≈ 1 + D/f_e (D = near point). Compound microscope uses different formula M ≈ (L/f_o)(D/f_e).

    Key Concepts

    • M = f_o/f_e
    • Normal adjustment L ≈ f_o + f_e
    • Large f_o → high M
    • Objective sets brightness/resolution
    • Eyepiece sets magnification

    Real-World Applications

    • Astronomical telescopes
    • Binoculars (with prisms)
    • Spotting scopes
    • Class 12 optical instruments
    • Amateur astronomy

    Explore Further

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    • Thin Lens Equation

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    • Spherical Mirror Equation

      Calculate image position and magnification for concave and convex mirrors.

    • Lens Power

      Convert focal length to diopters and combine thin lens powers.

    • Critical Angle

      Find critical angle for total internal reflection between two media.

    Physics Equations

    Magnification:
    M=fofeM = \frac{f_o}{f_e}

    Step-by-Step Solution

    See how the main results are calculated.

    1

    Step 1: Angular Magnification

    Equation:

    M=fofeM = \frac{f_o}{f_e}

    Explanation:

    Astronomical telescope in normal adjustment.

    2

    Step 2: Focal Lengths

    Result:

    fo=100cm,fe=10cmf_o = 100 cm, f_e = 10 cm
    3

    Step 3: Magnification

    Calculation:

    M=10010=10.0000M = \frac{100}{10} = 10.0000

    Result:

    M=10.00×M = 10.00×
    4

    Step 4: Tube Length

    Equation:

    L≈fo+feL \approx f_o + f_e

    Calculation:

    L≈110cmL \approx 110 cm

    Explanation:

    Normal adjustment: final image at infinity.

    5

    Step 5: Brightness

    Magnification reduces field of view.

    Explanation:

    Large f_o improves light gathering.

    6

    Step 6: Terrestrial Telescope

    Uses erecting prism; different M formula.

    Explanation:

    This tool is for simple astronomical layout.

    Frequently Asked Questions (FAQ)

    Maximum practical M?

    Limited by atmosphere, vibration, and field; very high M dims and blurs.

    Binoculars 10×50?

    10× magnification, 50 mm objective diameter.

    Practice MCQs

    1. Telescope M =
    2. To increase M:
    3. Normal adjustment means:
    4. f_o=80 cm, f_e=4 cm → M =
    5. Objective diameter affects:
    6. Microscope M differs because: