Pixel Scale Formula:
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Pixel scale represents the angular size of each pixel in an imaging system, typically measured in arcseconds per pixel. It's a crucial parameter in astronomy and photography that determines the field of view and resolution of an imaging system.
The calculator uses the pixel scale formula:
Where:
Explanation: The formula calculates how much sky or scene is covered by each pixel in your imaging system, which is essential for determining resolution and field of view.
Details: Proper pixel scale calculation is essential for optimizing imaging systems, matching telescope/camera combinations, achieving optimal sampling for astrophotography, and ensuring appropriate resolution for scientific measurements.
Tips: Enter the pixel size of your camera sensor in micrometers (μm) and the focal length of your optical system in millimeters (mm). Both values must be positive numbers.
Q1: What is the ideal pixel scale for astrophotography?
A: For deep-sky astrophotography, a pixel scale of 1-3 arcseconds per pixel is generally recommended, while planetary imaging benefits from smaller scales (0.1-0.5 arcseconds per pixel).
Q2: How does pixel scale affect image quality?
A: Pixel scale determines the resolution and field of view. Smaller pixel scales provide higher resolution but narrower field of view, while larger scales offer wider fields with lower resolution.
Q3: What is the 206265 constant in the formula?
A: This is the number of arcseconds in one radian (3600 arcseconds/degree × 180/π ≈ 206265), used to convert from linear measurement to angular measurement.
Q4: Can I use this calculator for terrestrial photography?
A: Yes, though the angular measurement (arcseconds) is more relevant for astronomical applications. For terrestrial use, you might want to calculate angular field of view instead.
Q5: How does binning affect pixel scale?
A: Binning combines adjacent pixels, effectively increasing the pixel size and thus increasing the pixel scale (larger arcseconds per pixel).