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Capture thePerfect Night Sky

Professional-grade astrophotography calculators and planning tools. Get sharp stars, perfect exposures, and plan your sessions like a pro.

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Why Use NPF Calculator?

Built by astrophotographers, for astrophotographers. No gimmicks, just tools that work.

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All tools are completely free and work instantly in your browser

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Once loaded, calculators work without an internet connection

All Camera Brands

Presets for Sony, Canon, Nikon, Fujifilm, and custom settings

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Use in the field on your phone or tablet while shooting

NPF Rule Calculator

Calculate the maximum shutter speed for perfectly sharp stars

Camera Settings

Lens Settings

Advanced Settings

Most conservative - perfectly round stars

-90° (South Pole)0°+90° (North Pole)

Maximum Shutter Speed

11.5s
(11.5 seconds)
500 Rule Result:20.8s
Difference:+82%

⚠️ The 500 rule would result in 82% more star trailing than NPF

Your Settings

Camera:Custom
Pixel Pitch:5.9 μm
Focal Length:24mm
Aperture:f/2.8
Tolerance:sharp

Pro Tips

  • • Use a sturdy tripod and remote shutter release
  • • Shoot at your lens's sharpest aperture (usually f/2.8-f/4)
  • • Higher ISO allows shorter exposures for sharper stars
  • • Stack multiple exposures for better noise reduction
  • • Check your histogram to avoid overexposure

What is the NPF Rule? Complete Guide to Astrophotography Exposure

The NPF Rule is the most accurate method for calculating the maximum shutter speed in astrophotography before stars begin to trail. Unlike the older "500 Rule" or "600 Rule," the NPF formula takes into account your camera's sensor resolution (pixel pitch) and lens aperture, making it essential for modern high-resolution cameras.

The NPF Formula Explained

NPF = (35 × Aperture + 30 × Pixel Pitch) ÷ Focal Length

Where Aperture is your f-number (e.g., 2.8), Pixel Pitch is in micrometers (μm), and Focal Length is in millimeters (mm). The result is your maximum shutter speed in seconds.

Why NPF is More Accurate Than the 500 Rule

The 500 Rule (shutter speed = 500 ÷ focal length) was developed for film cameras and early digital sensors. Modern cameras with 40-60+ megapixels require shorter exposures to avoid star trailing.

  • Accounts for sensor resolution: A 61MP Sony A7R V needs much shorter exposures than a 12MP Sony A7S III at the same focal length.
  • Considers aperture: Wider apertures (f/1.4-f/2.8) create larger star images on the sensor, making slight movement less visible.
  • More precise results: The 500 Rule can overestimate safe shutter speeds by 50-100% for modern cameras, resulting in oblong stars.

Understanding Pixel Pitch for Your Camera

Pixel pitch is the distance between the centers of adjacent pixels on your camera's sensor, measured in micrometers (μm). Here's how pixel pitch relates to megapixels:

  • Large pixel pitch (6-8μm): Lower resolution sensors (12-24MP full frame) - longer exposures possible
  • Medium pixel pitch (4-6μm): Standard resolution sensors (24-33MP full frame) - moderate exposure times
  • Small pixel pitch (3-4μm): High resolution sensors (45-61MP full frame, APS-C) - shorter exposures needed

Best Settings for Milky Way Photography

  • Focal length: 14-24mm for wide Milky Way shots
  • Aperture: f/1.4-f/2.8 for maximum light gathering
  • ISO: 1600-6400 depending on your camera's high ISO performance
  • Shutter speed: Use this NPF calculator for your exact settings
  • Focus: Manual focus at infinity, verify with live view magnification

Tips for Getting Sharp Stars Every Time

  • Use a sturdy tripod - carbon fiber dampens vibrations better than aluminum
  • Turn off image stabilization - it can cause blur on a tripod
  • Use a remote shutter release or your camera's 2-second timer
  • Focus manually using live view at 10x magnification on a bright star
  • Use the "Sharp" accuracy setting for critical work and large prints
  • Consider image stacking - combine 10-20 shorter exposures for better noise and sharpness

Celestial Declination and Star Movement

Not all stars move at the same apparent speed. Stars near the celestial equator (declination 0°, including most of the Milky Way core) move fastest across the sky. Stars near the celestial poles (Polaris in the north, Sigma Octantis in the south) appear nearly stationary, allowing longer exposures.

Pro tip: When shooting circumpolar star trails, you can ignore the NPF rule entirely and use exposures of several minutes to capture beautiful star trail circles.

Frequently Asked Questions

Everything you need to know about the NPF Rule and astrophotography

Frequently Asked Questions

The NPF Rule is a formula for calculating the maximum shutter speed before stars begin to trail in astrophotography. Unlike the simpler 500 Rule, NPF accounts for your camera's sensor resolution (pixel pitch) and lens aperture, making it significantly more accurate for modern high-megapixel cameras. The formula is: NPF = (35 × Aperture + 30 × Pixel Pitch) ÷ Focal Length.