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Angular Size Formula

Calculate the angular size of any object using its physical size and distance.
Includes the small angle approximation and examples with planets and the Moon.

The Formula

θ = 2 × arctan(d / 2D)

Angular size (also called angular diameter) is the angle subtended by an object as seen from the observer. It depends on both the object's physical size and its distance — a small nearby object can appear larger than a huge distant one. This formula applies to any object: planets, galaxies, telescope fields of view, or everyday objects.

Small Angle Approximation

θ ≈ d / D    (in radians, when θ is small)

For small angles (less than about 10°), the approximation θ ≈ d/D is excellent and much easier to compute. Converting to arcseconds: θ″ = 206,265 × (d / D).

Variables

SymbolMeaningUnit
θAngular size (angular diameter)radians, degrees, or arcseconds
dPhysical diameter of the objectany unit (km, m, AU, ly)
DDistance from observer to objectsame unit as d

Example 1 — The Moon

Moon diameter = 3,474 km, distance = 384,400 km

θ = 3,474 / 384,400 = 0.009036 radians

Convert: 0.009036 × (180/π) = 0.518°

θ ≈ 0.52° or about 31 arcminutes — roughly the same as the Sun

Example 2 — Jupiter through a Telescope

Jupiter diameter = 139,820 km, distance at opposition = 628,000,000 km

θ = 139,820 / 628,000,000 = 2.226 × 10⁻⁴ radians

In arcseconds: 2.226 × 10⁻⁴ × 206,265 = 45.9″

θ ≈ 46 arcseconds at closest approach — visible disc in small telescope

Example 3 — Rearranged for Distance

A galaxy has angular size 0.5° and known diameter of 100,000 light-years. How far is it?

θ in radians = 0.5 × π/180 = 0.008727 rad

D = d / θ = 100,000 / 0.008727

D ≈ 11,460,000 light-years ≈ 11.5 million light-years

When to Use It

  • Predicting how large planets and nebulae will appear through a telescope
  • Calculating the field of view needed for astrophotography
  • Estimating distances to objects of known size (standard rulers)
  • Describing apparent sizes of craters, star clusters, and galaxies in star atlases
  • Camera and lens selection — calculating image scale in photography

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