Quick guide
How to use this calculator
- Choose the astronomical relationship and solve direction first, then keep angles, distances, wavelengths, magnitudes, fluxes, and motion units explicit.
- Use exact geometry where supplied and compare it with the small-angle or classical approximation rather than assuming every astronomical scale uses the same model.
- Use the companion outputs to reconcile the result, then retain the stated observational and model limits before interpreting a theoretical value as a measured physical property.
Calculation method
How the angular size, physical size and distance calculator works
Keep the exact tangent geometry and the commonly used small-angle relationship together so visitors can see when the approximation is material.
Exact full-angle geometry is physical size = 2 × distance × tan(angle/2). The small-angle approximation is physical size ≈ distance × angle in radians; reverse modes rearrange the exact relationship.
Worked example
Angular Size, Physical Size and Distance example
A 3,474.8 km object at 384,400 km subtends about 0.518° using the exact relationship.
Exact full-angle geometry is physical size = 2 × distance × tan(angle/2). The small-angle approximation is physical size ≈ distance × angle in radians; reverse modes rearrange the exact relationship.
Supported inputs
Precision and limits
Astronomy and model boundary
This is transverse Euclidean geometry using a single distance. It does not infer projection, cosmology, gravitational lensing, extended-object depth, atmosphere, image distortion, or whether an observed boundary represents the physical diameter of interest.
Precision and reporting
Calculations retain working precision and round only for display. Very small and large nonzero values use scientific notation; displayed digits cannot create accuracy, traceability, or observational certainty absent from the entered data.
Category ownership
This collection owns unit-aware astronomy and extreme-scale measurement relationships. Calendar astronomy, orbital dynamics, cosmology, telescope equipment selection, and professional astrometric reduction require separate models and tools.
Privacy
Entered values and results stay in this browser and are not sent to analytics or third parties.
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