500 Rule & NPF Calculator

Star-sharp exposure time for astrophotography

Camera & Lens
Stars near the pole move less, so you can expose longer
Longest exposure without star trails (NPF rule)
22.7 s
500 rule (lower-resolution cameras)35.7 s
300 rule (high-resolution cameras)21.4 s
Pixel pitch6.00 µm
Full-frame equivalent14mm

The 500 rule dates from film and low-resolution sensors; at 100% view on modern cameras stars look elongated. Use the NPF value for pixel-sharp stars.

Max Shutter Speed by Focal Length
Lens500 rule300 ruleNPF
Starting Settings
SituationApertureISOShutter
Milky Way, dark sitef/1.8~2.83200~6400NPF value
Starry landscape, moonlightf/2.8~41600~320010–20 s
Star trails (stacked)f/2.8~4400~160020–30 s × many frames
Milky Way Season
MonthsMilky Way core (Northern Hemisphere)
Feb–AprBriefly before dawn in the east
May–AugMost of the night in the south — best season
Sep–OctEarly evening in the southwest
Nov–JanMostly hidden (behind the Sun)

Plan around the new moon and dark skies — check the moon phase calculator.

Formulas & Sources
🔭 Wikipedia — Astrophotography
Last reviewed: 2026-10-19
FAQ
What is the 500 rule?
Divide 500 by (focal length × crop factor) to get the longest exposure before stars trail. A 14 mm lens on full frame gives about 35 s; on 1.5× APS-C about 24 s.
How is the NPF rule different?
NPF also accounts for pixel size and aperture, so stars stay pinpoint on high-resolution sensors. A 24 MP full-frame camera at 14 mm f/2.8 aimed at the Milky Way core gets about 23 s.
When is Milky Way season?
In the Northern Hemisphere the core is best from May to August, visible before dawn from February and in the early evening into October. Shoot near the new moon.
What ISO should I use for the Milky Way?
Start around ISO 3200–6400 at f/2.8 from a dark site. Stack several frames to reduce noise.
Why can I expose longer near Polaris?
Stars circle the celestial pole, so those near it move less across the sensor. Pick a declination to scale the exposure.

How to find the right shutter speed for stars

Because the Earth rotates, long exposures turn stars into short lines. The classic 500 rule is easy but too long for modern high-megapixel cameras, so this calculator also gives the NPF rule, which uses pixel pitch and aperture.

Enter your sensor, megapixels, lens, aperture and the part of the sky you're shooting to get the longest exposure for sharp stars and the nearest shutter setting.

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