Pixel Scale Calculator

Resolution Analysis

Calculate the pixel scale of your astrophotography setup to optimize image resolution and quality. This essential tool helps determine how much sky detail each pixel captures and whether your setup matches seeing conditions.

How to Use the Pixel Scale Calculator

  1. Enter your telescope or lens focal length.
  2. Enter your camera's pixel size or select a preset.
  3. Adjust binning if applicable.
  4. See pixel scale and resolution analysis results.

Pixel Scale Guidelines

Application Recommended Pixel Scale Notes
Wide Field (Milky Way) 3-6 arcsec/pixel Good balance of detail and coverage
Deep Sky (General) 1-3 arcsec/pixel Standard for most deep-sky objects
Small Objects/Planets 0.3-1 arcsec/pixel High resolution for small targets
Excellent Seeing (<1") 0.3-0.7 arcsec/pixel Take advantage of good conditions
Average Seeing (2-3") 1-2 arcsec/pixel Optimal for typical conditions
Poor Seeing (>3") 2-4 arcsec/pixel Avoid oversampling in poor seeing

Understanding Pixel Scale

The Formula

Pixel scale is calculated using: Pixel Scale = 206.265 × pixel_size / focal_length

Where pixel size is in micrometers, focal length is in millimeters, and the result is in arcseconds per pixel.

Key Concepts

Practical Applications

Illustration showing pixel scale relationship between telescope focal length and camera sensor
Calculate precise pixel scale for astrophotography — optimize resolution and image quality for your telescope and camera setup.

FAQ

  • What is pixel scale in astrophotography?

    Pixel scale measures how much sky each camera pixel covers, expressed in arcseconds per pixel. It determines the resolution and detail level of your images.

  • What's a good pixel scale for astrophotography?

    Generally, 1-2 arcsec/pixel provides a good balance. Smaller values give higher resolution but may be limited by seeing conditions, while larger values reduce detail but improve signal-to-noise.

  • How does pixel scale relate to telescope resolution?

    Pixel scale should ideally be 2-3 times smaller than your telescope's resolution limit to properly sample the image without losing detail (Nyquist sampling).

  • Why is pixel scale important?

    Pixel scale determines how much detail you can capture, affects file sizes, and helps plan whether your setup matches seeing conditions and target requirements.