Focalyard

Eyepiece Calculator: Field of View and Exit Pupil

mm
mm
°
mm
Barrel
mm
Simulated view: the full Moon in the eyepiece fieldA 1.08° circle with the 0.52° Moon drawn to scale.
Simulated view · SVG Field 1.08° wide; the Moon (0.52°) fits 2.1 times across.

Inside the useful range.

Magnification
48.0x
True field
1.08°
Exit pupil
4.2 mm
Max useful
406x

A 25 mm eyepiece in a 1200 mm telescope gives 48x. Divide 1200 by 25.

The aperture behind that focal length is 203 mm (8 in). Exit pupil is 4.23 mm, from 203 ÷ 48.

At 52° apparent, true field of view is 1.08°, or 2.1 Moon widths at 0.52°. The calculator above opens on these numbers. Sky & Telescope's formulas, checked Oct 17, 2026.

Simulated view: the Moon in four true fields on one angular scale, from the default eyepiece to the barrel caps and high powerSimulated view · SVG · one scale, 1° = 76 px · Moon 0.52° · 1,200 mm tube1.08° · 48x at 52°Moon is 48% of the width1.29° · 27 mm stop1.25 in barrel cap2.20° · 46 mm stop2 in barrel cap0.26° · 200xMoon wider than the fielddashed: Moon limb outside the 0.26° fieldSimulated view: the Moon in four true fields on one angular scale, from the default eyepiece to the barrel caps and high powerSimulated view · one scale, 1° = 64 px · Moon 0.52°1.08°48x at 52°Moon is 48% of the width1.29°27 mm stop1.25 in barrel cap2.20°46 mm stop2 in barrel cap0.26°200xMoon wider than fieldDashed: Moon limb outside the 0.26° field
Fig. 01Simulated view. One scale for a 0.52° Moon: 1.08° at 48x and 52°, the 1.29° and 2.20° barrel caps on 1200 mm, and 0.26° at 200x, where the Moon is wider than the field.

How the numbers work

Magnification is telescope focal length divided by eyepiece focal length. On the default, 1200 ÷ 25 = 48x. The magnification calculator is the page for a separate power check.

A 60 mm (2.4 in) department-store refractor box often says 675x. That is 900 mm × 3 (the 3x Barlow in the box) ÷ 4 mm. The ceiling for 60 mm is 2 × 60 = 120x, so 675x is unusable, about 5.6 times past it.

The table below works the same four inputs by hand. Magnification = focal length ÷ eyepiece. Exit pupil = aperture ÷ magnification, and also eyepiece ÷ focal ratio. Here 1200 ÷ 203 = f/5.91, so 25 ÷ 5.91 = 4.23 mm. True field ≈ apparent field ÷ magnification = 52 ÷ 48 = 1.08°. A field stop is a separate sum: 57.3 × stop mm ÷ focal length mm.

Default inputs: 203 mm aperture, 1200 mm focal length, apparent field 52°. Moon widths use a 0.52° disk. The 32 mm row is capped by a 1.25 in stop.
EyepieceMagnificationExit pupilTrue fieldMoon widthsCheck
32 mm37.5x5.41 mm1.29° (stop cap; 1.39° by 52 ÷ 37.5)2.51.25 in barrel
25 mm48x4.23 mm1.08°2.1Between 0.5 mm and 7 mm
10 mm120x1.69 mm0.43°0.8Middle of a three-eyepiece set
6 mm200x1.02 mm0.26°0.5Moon wider than the field
2 mm600x0.34 mm0.09°0.2Under 0.5 mm and past 406x

Exit pupil is the beam diameter leaving the eyepiece. Divide aperture by magnification. On the default, 203 ÷ 48 = 4.23 mm.

The second path divides eyepiece focal length by focal ratio. Here 1200 ÷ 203 = f/5.91. The tube's f/6 label is the round number.

Then 25 ÷ 5.91 = 4.23 mm. Both exit-pupil paths agree. Use the millimeters on the tube, and keep the f/ label off the inputs.

Divide 25 by a rounded f/6 and the beam comes out 4.17 mm. That 0.06 mm gap is the label, not a second optic.

Light path of the default telescope and eyepiece, with the exit-pupil disk and the two beam limits drawn to one scaleFocal length 1,200 mmEyepiece 25 mm203 mm apertureFocusExit pupil203 ÷ 48 = 4.23 mm1,200 ÷ 25 = 48xBeam diameter to one scale, 1 mm = 10 px0.5 mmflag below this4.23 mmdefault beam7 mmflag above thisLight path of the default telescope and eyepiece, with the exit-pupil disk and the two beam limits drawn to one scaleFocal length 1,200 mmEyepiece 25 mm203 mm aperture1,200 ÷ 25 = 48xExit pupil203 ÷ 48 = 4.23 mmBeam to one scale, 1 mm = 8 px0.5 mmflag below4.23 mmdefault7 mmflag above
Fig. 02Exit pupil of the default. 1200 mm ÷ 25 mm = 48x. The beam is 203 ÷ 48 = 4.23 mm, between the 0.5 mm and 7 mm lines.

We flag an exit pupil under 0.5 mm. You are past the useful ceiling, which is about 2× the aperture in millimeters.

On this 203 mm default, 2 × 203 = 406x. A 2 mm eyepiece forces 1200 ÷ 2 = 600x. Then 203 ÷ 600 = 0.34 mm.

That 2 mm row fails both checks: power is past 406x and the beam is under 0.5 mm. The calculator shows the ceiling warning. The field at 52° shrinks to 0.09°.

We also flag an exit pupil over 7 mm. Minimum useful power is aperture ÷ 7, the 7 mm planning pupil in the Sky & Telescope notes.

On the default, 203 ÷ 7 = 29x. A 7 mm beam wants about a 41 mm eyepiece (a 2 in barrel), because 7 × 5.91 = 41.4.

The spill shows up on a faster tube. Take a 130 mm (5.1 in) f/5. Focal length is 650 mm. Fit a 40 mm eyepiece.

Power is 650 ÷ 40 = 16.25x, listed as 16.3x. Exit pupil is 40 ÷ 5 = 8.0 mm. The floor is 130 ÷ 7 = 18.6x, so 16.3x sits under it.

Exit pupil for seven eyepieces on the default telescope, with lines at the two beam flags203 mm aperture, 1,200 mm focal length · exit pupil = 203 ÷ power32 mm · 37.5x5.41 mm25 mm · 48x4.23 mm15 mm · 80x2.54 mm10 mm · 120x1.69 mm6 mm · 200x1.02 mm4 mm · 300x0.68 mm3 mm · 400x0.51 mm01234567mm0.5 mm flag7 mm flagExit pupil for seven eyepieces on the default telescope, with lines at the two beam flags203 mm, 1,200 mm · 203 ÷ power32 mm · 37.5x5.41 mm25 mm · 48x4.23 mm15 mm · 80x2.54 mm10 mm · 120x1.69 mm6 mm · 200x1.02 mm4 mm · 300x0.68 mm3 mm · 400x0.51 mmDashed lines: 0.5 mm and 7 mm flags
Fig. 03Exit pupil by eyepiece. On 203 mm and 1200 mm, from 5.41 mm at 32 mm down to 0.51 mm at 3 mm. Lines mark 0.5 mm and 7 mm.

True field of view is the sky patch, in degrees. Apparent field is the angle at the eyepiece glass. Divide before you compare them.

A 52° eyepiece at 48x covers 52 ÷ 48 = 1.08°. Type 82° on the 1.25 in barrel and the calculator caps that 48x view at 1.29°, not 82 ÷ 48 = 1.71°. Switch the barrel to 2 in and 1.71° fits under the 46 mm cap.

82° is the apparent field, the angle you see at the eyepiece. In a 1.25 in barrel the 27 mm stop holds that 48x view to 1.29°.

The calculator caps a 1.25 in barrel at 27 mm and a 2 in barrel at 46 mm, and it says so under the result. A printed field stop, typed in millimeters, is used as-is.

Tele Vue lists a 27 mm maximum stop for a 1.25 in barrel, and 46 mm for a 2 in barrel. We checked that note on Oct 17, 2026.

On 1200 mm, 57.3 × 27 ÷ 1200 = 1.29°. The 46 mm stop gives 57.3 × 46 ÷ 1200 = 2.20°. Those are barrel caps, not a guess for one model.

A 32 mm Plössl at 52° claims 52 ÷ 37.5 = 1.39°, and 1200 ÷ 32 = 37.5x. The 27 mm stop pulls the sky patch back to 1.29°. The calculator shows 1.29° and the cap note.

A real 32 mm Plössl prints about 48°–50° because the 27 mm stop allows no more. At 48°, 48 ÷ 37.5 = 1.28°, inside the cap.

52° is the calculator's default, the number many low-cost Plössls print. Tele Vue's Plössl class is 50°. Then 50 ÷ 48 = 1.04°.

1. Type focal length, eyepiece focal length, apparent field, and aperture.

2. Read power, exit pupil, and true field. Check 0.5 mm and 7 mm.

3. If the maker prints a field stop, type it. The calculator uses 57.3 × stop ÷ focal length and skips the barrel cap. Sky & Telescope calls apparent field ÷ power rough. With no printed stop, pick the barrel: 27 mm for 1.25 in, or 46 mm for 2 in.

Our assumptions

Aperture rows use 203 mm for 8 in, 152 mm for 6 in, 102 mm for 4 in, 127 mm for a 5 in Mak, and 130 mm for the f/5 spill case.

Focal lengths are 1200 mm, 663 mm, 1500 mm, and 650 mm. Working focal ratio is focal length ÷ aperture, so the 1200 mm tube is f/5.91.

Apparent field stays 52° until you replace it. A printed stop is typed in and used as 57.3 × stop ÷ focal length, with no barrel cap. With no printed stop, the barrel caps the field: 27 mm at 1.25 in, or 46 mm at 2 in.

The Moon disk is 0.52°. Las Cumbres lists about 31 arcmin, which is 0.52°, checked Oct 17, 2026. The calculator uses that same diameter.

Max useful power is 2 × 203 = 406x. The inch form is 50 × 8 = 400x. Min useful power is aperture ÷ 7, from the 7 mm pupil. The field calculator shows the max, not the min.

The Suburban sky and dark sky section below uses Bortle 6–7 for suburban and Bortle 3–4 for dark.

Focal length, eyepiece, and the field

One focal length, 1200 mm. Seven eyepieces. The 203 mm column and the 152 mm column share every power. Power ignores aperture.

1200 mm focal length, 52° apparent field. Exit pupil uses 203 mm or 152 mm. Moon widths use a 0.52° disk. A 1.25 in barrel still caps the field at 1.29°.
EyepieceMagnificationExit pupil, 203 mmExit pupil, 152 mmTrue field at 52°Moon widths
32 mm37.5x5.41 mm4.05 mm1.29° (stop cap; 1.39° by 52 ÷ 37.5)2.5
25 mm48x4.23 mm3.17 mm1.08°2.1
15 mm80x2.54 mm1.90 mm0.65°1.3
10 mm120x1.69 mm1.27 mm0.43°0.8
6 mm200x1.02 mm0.76 mm0.26°0.5
4 mm300x0.68 mm0.51 mm0.17°0.3
3 mm400x0.51 mm0.38 mm0.13°0.3

The 32 mm row is the low end of a 1.25 in set. You get 37.5x. The beam on 203 mm is 5.41 mm, from 203 ÷ 37.5.

The 52° shortcut gives 1.39°. The 27 mm stop gives 1.29°. On this 1200 mm tube, keep 1.29° for a 1.25 in barrel.

The 10 mm row is the middle of three. You are at 120x, with a 1.69 mm beam and a 0.43° field. A 0.52° Moon no longer fits whole.

The 6 mm row is the high one. You get 200x, a 1.02 mm beam, and a 0.26° field. That circle covers 0.26 ÷ 0.52 = 0.50 of the Moon's width.

The 3 mm row is 400x and 0.51 mm. You are on the 0.5 mm line, just under the 406x ceiling.

On the 152 mm column, powers match the 203 mm column. Focal length is still 1200 mm. Beams shrink. At 48x you get 3.17 mm, from 152 ÷ 48.

The 152 mm ceiling is 304x, from 2 × 152. A 4 mm eyepiece at 300x is on that line, with a 0.51 mm beam. The 6-inch page uses this aperture.

Same 48x, same 1.08° field, two beams. That is why the calculator asks for aperture.

Area scales with the square of field diameter. A 2.20° stop against a 1.29° stop is 1.71 across. Square that and the sky area is about 2.9 times.

25 mm eyepiece, 52° apparent field. Stop fields use 57.3 × stop ÷ focal length. The 127 mm Mak row has no 46 mm stop: its back is 1.25 in. Max useful is 2 × aperture mm. Min useful is aperture ÷ 7.
TelescopeFocal lengthFocal ratio25 mm powerExit pupilTrue field at 52°Max / min27 mm stop46 mm stop
102 mm (4 in)663 mmf/6.5026.5x3.85 mm1.96°204x / 14.6x2.33°3.98°
152 mm (6 in)1200 mmf/7.8948x3.17 mm1.08°304x / 21.7x1.29°2.20°
203 mm (8 in)1200 mmf/5.9148x4.23 mm1.08°406x / 29x1.29°2.20°
127 mm (5 in) Mak1500 mmf/11.860x2.12 mm0.87°254x / 18.1x1.03°n/a (1.25 in rear port)
130 mm f/5650 mmf/526x5.00 mm2.00°260x / 18.6x2.38°4.06°

The 102 mm f/6.5 refractor is the 663 mm row. A 25 mm eyepiece gives 26.5x, from 663 ÷ 25. The beam is 3.85 mm. The 52° field is 1.96°.

Its 46 mm stop opens 3.98°, from 57.3 × 46 ÷ 663. That clears a 3° target. The 27 mm stop stops at 2.33°.

The 127 mm Mak at 1500 mm goes the other way. A 25 mm eyepiece gives 60x and 0.87°, and its 1.25 in back holds the field near the 1.03° stop cap.

The 130 mm f/5 at 650 mm is the wide fast case. At 25 mm you get 26x, a 5.00 mm beam, and 2.00°. The 46 mm stop reaches 4.06°.

Swap to a 10 mm eyepiece and the tubes split. On 663 mm you get 66.3x, a 1.54 mm beam, and 0.78°.

On 1500 mm that same 10 mm eyepiece gives 150x, a 0.85 mm beam, and 0.35°. Focal length did the splitting.

One eyepiece on four focal lengths: true field at the default apparent field and at the two-inch stop cap25 mm eyepiece · 52° field = 52 ÷ power · stop field = 57.3 × stop ÷ focal length130 mm f/5 · 650 mm27 mm stop 2.38°52° field 2.00°46 mm stop 4.06°102 mm f/6.5 · 663 mm27 mm stop 2.33°52° field 1.96°46 mm stop 3.98°152 or 203 mm · 1,200 mm27 mm stop 1.29°52° field 1.08°46 mm stop 2.20°127 mm Mak · 1,500 mm1.25 in back52° field 0.87°27 mm stop 1.03°0°1°2°3°4°dashed: 3° targetOne eyepiece on four focal lengths: true field at the default apparent field and at the two-inch stop cap25 mm eyepiece · true field in degrees130 mm f/5 · 650 mm52° field2.00°46 mm stop4.06°102 mm f/6.5 · 663 mm52° field1.96°46 mm stop3.98°152/203 mm · 1,200 mm52° field1.08°46 mm stop2.20°127 mm Mak · 1.25 in back52° field0.87°27 mm stop1.03°Dashed: 3° target27 mm stop: 2.38°, 2.33°, 1.29°, 1.03°
Fig. 04Stop cap by focal length. 25 mm eyepiece, 52° apparent field. Each tube shows the 52° true field and the 46 mm cap where the tube takes a 2 in eyepiece. The 127 mm Mak row stops at the 1.25 in back. The dashed line is a 3° target length.

Suburban sky and dark sky

From a Bortle 6–7 yard the Moon and planets carry the night. At 48x the 0.52° disk fills 0.48 of the 1.08° circle.

Planets want about 20x to 30x per inch of aperture. On an 8 in tube that band is 160x to 240x. Sky & Telescope gives that range for planetary work.

On 1200 mm, 160x needs a 7.5 mm eyepiece, and 240x needs 5 mm. At 160x the beam is 1.27 mm and a 52° field is 0.33°.

At 240x the beam is 0.85 mm and the field is 0.22°. A 40″ Jupiter at 240x looks about 2.7° wide, roughly 1/20 of the 52° view.

A Bortle 3–4 sky does not widen the optic. Andromeda's length is six Moon diameters, or 3°, in the NASA note.

The 2.20° stop on the 1200 mm tube covers 2.20 ÷ 3 = 73% of that length. The 1.08° field covers 1.08 ÷ 3 = 36%.

The 3.98° field on the 663 mm tube covers that 3° length and still has margin. You want the whole galaxy, so you shorten the focal length.

Simulated view: the Andromeda Galaxy's length inside three true fields on one angular scaleSimulated view · SVG · one scale, 1° = 54 px · dashed = M31 length 3°1.08° · 1,200 mm25 mm at 52° · 36% of the length2.20° · 1,200 mm46 mm stop · 73% of the length3.98° · 663 mm46 mm stop · whole length fitsSimulated view: the Andromeda Galaxy's length inside three true fields on one angular scaleSimulated view · 1° = 30 pxDashed = M31 length 3°1.08°1,200 mm · 25 mm at 52°36% of the length2.20°1,200 mm · 46 mm stop73% of the length3.98°663 mm · 46 mm stopwhole length fits
Fig. 05Simulated view. M31's 3° length, dashed, inside 1.08° and 2.20° fields on the 1200 mm tube and a 3.98° field on the 663 mm tube, drawn to one scale.

Five misses

Carton power first. A 60 mm box says 675x. On that lens, 675x is unusable, about 5.6 times past the 120x ceiling.

Apparent field second. That angle is at the glass. Divide by magnification before you name a sky patch.

Barrel third. A 1.25 in eyepiece on a 1200 mm tube tops out at 1.29°. A printed 82° still has to pass that 27 mm stop.

Fourth miss: adding a 2× Barlow and keeping the old field. The 1.08° patch becomes 0.54°. The 4.23 mm beam becomes 2.11 mm.

Fifth miss: eye relief. If you keep glasses on for astigmatism, Tele Vue suggests at least 15–20 mm of eye relief (checked Oct 17, 2026). A 21 mm Baader Hyperion lists 20 mm, the top of that range. Below it, the field edge starts to vignette.

The calculator does not compute eye relief. Compare the printed millimeters after the power and field match. The eyepiece guide sorts the surviving focal lengths into a low, mid, and high set.

Common Questions

How do you calculate true field of view?

Divide apparent field by magnification. A 52° eyepiece at 48x covers 52 ÷ 48, which is 1.08°. That is 2.1 Moon widths if you take the Moon as 0.52°.

A printed field stop is the real sky patch: 57.3 × stop ÷ focal length. The calculator uses that number and skips the barrel cap. Sky & Telescope calls apparent field ÷ power rough. With no printed stop, pick 1.25 in (27 mm) or 2 in (46 mm).

What exit pupil is worth using?

Divide aperture in millimeters by magnification. At 203 mm and 48x the beam is 4.23 mm. We flag a result under 0.5 mm or over 7 mm.

Under 0.5 mm you are past about 2× the aperture, 406x on this tube. The view gets dimmer without new detail.

Over 7 mm, part of the beam misses a 7 mm pupil. A 40 mm eyepiece on an f/5 tube is an 8.0 mm beam.

Does a wide apparent field show more sky?

Only after you divide, and after the barrel. An 82° eyepiece at 48x is 82 ÷ 48 = 1.71° before the cap. On 1.25 in the calculator shows 1.29°. On 2 in, 1.71° fits under the 46 mm cap.

A 2 in stop near 46 mm is 2.20° on that same focal length.

Why do equal powers still give different exit pupils?

Magnification uses focal length only. A 152 mm telescope and a 203 mm telescope, both at 1200 mm, both give 48x with a 25 mm eyepiece. At 52° they also share the 1.08° true field.

Exit pupil uses aperture. You get 3.17 mm from 152 ÷ 48, and 4.23 mm from 203 ÷ 48. The smaller optic also tops out sooner, at 304x instead of 406x.

What should you read for glasses?

If you keep glasses on for astigmatism, Tele Vue suggests at least 15–20 mm of eye relief (checked Oct 17, 2026). A 21 mm Baader Hyperion lists 20 mm, the top of that range. Below it, the field edge starts to vignette. Nearsighted or farsighted only? Take the glasses off and refocus.

The calculator leaves eye relief alone. Compare the printed millimeters after power and field match, such as 48x and 1.08°.

An open foam-lined case of telescope eyepieces on a weathered picnic table at dusk, a red flashlight beside it and a small Dobsonian behind

Read next

Sources

  1. Sky & Telescope, Simple Formulas for the Telescope Owner (checked Oct 17, 2026): skyandtelescope.org. Magnification = telescope focal length ÷ eyepiece focal length. Exit pupil = aperture ÷ magnification, and also eyepiece focal length ÷ focal ratio. Notes beams under about 0.5 mm and the 7 mm pupil.
  2. Sky & Telescope, A Pupil Primer (checked Oct 17, 2026): skyandtelescope.org. Exit pupil = aperture ÷ power. The 0.5 mm beam matches the 50×-per-inch ceiling. Lowest useful power tracks pupil diameter.
  3. Sky & Telescope, How to Choose Your Telescope's Magnification (checked Oct 17, 2026): skyandtelescope.org. Planetary planning band of about 20x to 30x per inch. A 7 mm pupil as the low-power reference. Apparent field ÷ power is only a rough true field.
  4. Sky & Telescope, Telescope Calculator (checked Oct 17, 2026): skyandtelescope.org. Max useful magnification about 50× aperture in inches, or twice aperture in millimeters. Apparent field is an input.
  5. Tele Vue Optics, Choosing Eyepieces (Basic) (checked Oct 17, 2026): televue.com. Magnification = telescope focal length ÷ eyepiece focal length. True field = field stop ÷ telescope focal length × 57.3. Plössl class listed at 50° apparent. If you keep glasses on for astigmatism: at least 15 mm to 20 mm of eye relief, to limit vignetting.
  6. Baader Planetarium, Hyperion 21 mm 68° eyepiece spec (checked Oct 23, 2026): baader-planetarium.com. Focal length 21 mm, apparent field 68°, eye relief 20 mm.
  7. Tele Vue Optics, Ethos 17 mm package note (checked Oct 17, 2026): televue.com. Maximum field stop about 27 mm in a 1.25 in barrel and about 46 mm in a 2 in barrel.
  8. Las Cumbres Observatory, Using angles to describe sizes (checked Oct 17, 2026): lco.global. Moon about 31 arcmin, which is 0.52°.
  9. NASA Science, Messier 31 (checked Oct 17, 2026): science.nasa.gov. Andromeda's angular size is about six times the full Moon's diameter. Public-domain agency page. We do not use a NASA image on this page.

Formula log and check method: How we research.