Radar Horizon Calculator

Find how far you can see with a radar with our radar horizon calculator.

Clear
Distance to the horizon24.0483 km14.9429 miles, 12.9851 nautical miles
Geometric distance19.5515 kmrefraction extends the horizon by 23%, because the atmosphere bends light downwards around the curve
Observer height30 m
Angle below horizontal0.17583°how far down the horizon sits — small, but real, and measurable with a sextant
Drop over the horizon distance30 mequal to your own height, by the geometry — the horizon is where the surface has curved away by exactly your eye height
Horizon distance for a 50 m object31.0463 km
Maximum distance you could see it55.0946 kmthe two horizon distances ADD — which is why a ship's mast appears before its hull, and why radio masts are built tall at both ends
How much of it is hidden at 24 kmnone — that is your own horizonbeyond your horizon the hidden height grows roughly as the square of the excess distance
At 4× the height48.097 km2× further — the distance goes as the SQUARE ROOT of height, so doubling your altitude gains only 41%
At 100× the height240.511 km10× further — the distance goes as the SQUARE ROOT of height, so doubling your altitude gains only 41%
Height needed to double this horizon120 mfour times the height, for twice the distance

The formula

d = √(2Rh + h²); radar horizon multiplies by about 1.23

Square root, so height buys less than you expect

The distance to the horizon goes as the square root of the observer's height. Doubling your altitude extends the horizon by only 41%; quadrupling it doubles the distance. At eye level on a beach the horizon is about 4.7 km away, and from a 100 m cliff still only about 36 km.

A tidy piece of geometry: the surface drops away by exactly your own eye height over the horizon distance. That is what defines the horizon — the point where the curve has fallen by however high you are standing.

Two elevated points see each other much further than either sees the horizon, because the two horizon distances simply add. This is why a ship's masts appear over the horizon before its hull, why radio links raise antennas at both ends, and why lookout positions were placed as high as possible.

The atmosphere bends light downwards, following the curve slightly and extending the visible horizon by about 6% under standard conditions. Radio waves refract more strongly, roughly 23%, which is the origin of the 4/3-Earth-radius approximation used in radio path planning. Both figures vary with temperature gradient, and a strong inversion can produce genuine looming or mirage effects.