Horizon Dip Calculator
Enter your eye height above sea level to find the horizon dip correction and distance.
Result
How it is calculated
From the height of eye h in metres, the tool computes the dip of the sea horizon in arcminutes as dip = 1.758 × √h, converts it to degrees by dividing by 60, and gives the distance to the horizon as d = 3.57 × √h kilometres. Both grow with the square root of height, so quadrupling the height only doubles them. These are the usual navigation formulas for normal atmospheric refraction, with the horizon taken as open sea level. Height must be above zero and no more than 100,000 m (the small-angle approximation is not meant beyond that); anything else shows no result. It is the height of your eye above the water, not the height of the ship or the deck. Dip is the angle you subtract from a sextant altitude measured to the visible horizon.
Worked example
Suppose the observer's eye is 10 m above sea level. √10 ≈ 3.1623. Dip: 1.758 × 3.1623 ≈ 5.56 arcminutes, shown as 5.56 arcmin, and 5.56 ÷ 60 ≈ 0.09 degrees. Distance: 3.57 × 3.1623 ≈ 11.29 km. So from 10 m up the visible sea horizon lies about 11.29 km away, and a sextant sight of a star must be corrected by about 5.56 arcminutes for dip.
Common mistakes
- Entering the height of the deck, mast or the ship instead of the height of the observer's eye above the water.
- Entering feet while the field expects metres. A 33 ft eye height typed as 33 gives a dip of about 10.1 arcminutes instead of the correct 5.6 for 10 m.
- Confusing dip (an angle, in arcminutes) with the distance to the horizon (kilometres). The tool gives both and they are separate numbers.
- Trying very large heights, such as those of an aircraft or a rocket. Anything above 100,000 m, and zero or negative heights, give no result; even at 100,000 m the straight square-root rule is only a rough guide.
- Expecting the distance to tell how far you can see a tall object. It is only the distance to the sea horizon for an observer at that height; a ship's hull or a lighthouse is visible beyond it.
About this calculator
Because the Earth curves away beneath an observer, the true sea horizon appears slightly below the astronomical horizontal — this angle is the horizon dip. For an eye height h in meters, the standard approximation (accounting for normal atmospheric refraction) is dip ≈ 1.76 × √h arcminutes, growing with the square root of height.
The same geometry gives the distance to the horizon, roughly d ≈ 3.57 × √h kilometers (or 1.17 × √h nautical miles for h in feet), the range at which the sea surface itself drops out of sight.
Navigators use dip as a standard correction when taking a sextant altitude of a star, the Sun, or the Moon above the visible horizon — it must be subtracted from the observed altitude, alongside refraction and semi-diameter corrections, before the sight can be reduced to a usable position line in celestial navigation.
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Comments (1)
Muy útil para la navegación astronómica, muchas gracias 🔥🔥