Free Astro Pixel Scale Calculator

Image scale = 206.265 × pixel size (µm) ÷ focal length (mm). The result, in arcseconds per pixel, tells you whether your seeing, tracking, and optics are matched to your sensor.

Your setup

Result

Pixel scale
arcsec / pixel
Seeing sampling
pixels per seeing disk
Verdict
for sharp round stars
🔭 The 1–2″/px rule: most amateur setups land between 1 and 2 arcseconds per pixel — a good match for typical seeing (2″) and common mounts. Below ~0.5″/px you're oversampling (huge files, no new detail, tracking demands explode); above ~4″/px you're undersampling (blocky stars, wasted resolution).

Why pixel scale matters

Pixel scale determines how much sky each pixel covers. It's the single best number for judging whether a camera + lens/telescope pairing makes sense before you buy:

Rule of thumb: pixel scale ≈ seeing ÷ 3 gives near-critical sampling. With 2″ seeing that's ~0.67″/px — most hobbyists choose slightly coarser to keep guiding easy.

Pixel scale FAQ

What's the formula for pixel scale?

Pixel scale (″/px) = 206.265 × pixel size (µm) ÷ focal length (mm). Example: a camera with 3.8 µm pixels behind a 400 mm lens gives 206.265 × 3.8 ÷ 400 ≈ 1.96″/px.

Is smaller pixel scale always better?

No. Below the seeing limit you're oversampling — more pixels per star than the atmosphere delivers. The result is larger files, longer exposures for the same signal, and stricter guiding for zero real resolution gain.

How do I find my camera's pixel size?

Pixel size = sensor height (mm) × 1000 ÷ vertical resolution. ShutterMath stores this for every camera in the list automatically — just pick your camera.