Paritian

Science

Angular Size Calculator (Apparent Size of the Moon, a Building, a Star)

How big an object looks, as an angle in degrees and arcminutes, from its real size and distance — or the real size from the angle it covers.

Results

Angular size in degrees 0.5178 °
Angular size in arcminutes 31.07 ′
Angular size in arcseconds 1864 ″
Size of an object that covers that angle —

What this tool does

Angular size is the angle an object covers in your view: θ = 2 × atan(s ÷ 2d). For small angles this is close to s ÷ d radians, so 57.3 × s ÷ d gives degrees. The Moon is about 3,474 km across and 384,400 km away on average, so it covers roughly 0.52° (31 arcminutes) — almost exactly what the Sun covers, which is why total eclipses happen. As a rough guide, a fist at arm's length spans about 10° and a finger about 1°. Run it backwards to find the real size of something whose distance and apparent angle you know; use the same unit for size and distance.

Formula

θ = 2 × atan(s ÷ 2d) · s = 2 d × tan(θ ÷ 2)

Variables

SymbolMeaningUnit
szSize of the object (any unit)—
ddDistance to the object (same unit as the size)—
anAngular size you know (degrees)°
TDAngular size in degrees°
TMAngular size in arcminutes′
TSAngular size in arcseconds″
SZSize of an object that covers that angle—

Worked example

  • Size of the object (any unit)3474
  • Distance to the object (same unit as the size)384,400
  • Angular size in degrees0.5178 °
  • Angular size in arcminutes31.07 ′
  • Angular size in arcseconds1864 ″

Limitations

  • Mixing units is the most common source of error. Convert every input to the units shown next to each field before calculating.
  • The calculation runs at full precision and only the display is rounded. If you copy an intermediate value and retype it, small differences can appear.