Claim status
Global plane not supported
In the record
Geoid and horizon in modern surveying practice
Testable
Horizon distance for measured observer and target heights
Method
Tangent geometry on a sphere, without atmospheric refraction
FLAT EARTH / CASE FILE

Horizon distance: 5,048 m to water, 16.34 km to a mast

From the default eye height the water horizon lies 5,048 m away, and an elevated target adds 11,288 m, giving a shared sightline of 16.34 km.

A calm sea looks level, and the horizon can look like a straight division between water and sky. Neither observation requires an infinite plane. The interesting test begins when the observer changes height: the visible boundary moves farther away, and an elevated target can remain visible beyond the observer’s own sea-level horizon.

Run the calculation
An engraved circular map with red horizon measurement linesA claim about the world should fit the whole world.
01 / THE CLAIM

Local level is extended across the world

The claim is that water seeks its level, so a large body of water must form a single flat surface. Its immediate evidence is familiar: the sea does not look like a mound from the beach. The step requiring examination is the extension of a local horizontal into a plane that stays horizontal everywhere.

Level depends on the direction of gravity where it is measured. A local tangent plane can be horizontal at one location and cease to be horizontal elsewhere on a curved surface. Keeping this distinction allows water to be locally level all along a surface whose direction changes gradually with position.

02 / THE CASE

The observer stands above the surface being viewed

Surveyors describe the gravity-related reference for global mean sea level as the geoid. It is curved and gently irregular because Earth’s shape and mass distribution are irregular. Remove tides and currents from the ocean and its equilibrium surface follows that gravity field. The geoid is also extended through land to provide a reference for elevations.

For the horizon calculation, replace that detailed surface with a sphere. The last unobstructed straight ray from an elevated eye just touches it. The touching point is the geometric horizon. An eye above the water therefore looks slightly downward toward that boundary, even though the nearby surface is locally level.

A distant target can also extend above its own horizon. Seeing the upper part of a lighthouse or a mast beyond the distance to the observer’s water horizon is not an exception to the geometry. Both endpoint heights matter. A claim based only on the camera height has omitted a measurable part of the sightline.

03 / THE COMPUTATION

Two heights determine the available sightline

A radius drawn to a tangent point meets the sightline at a right angle. For Earth radius R and observer height h, the right triangle gives the straight distance d = √[h(2R + h)]. The same calculation applies to the target’s height. At the limiting shared sightline, those two tangent distances add together.

The opening assumptions place the eye 2 metres above the water and the target’s top 10 metres above it. With JPL’s mean Earth radius, the observer’s tangent distance is about 5.05 kilometres. The target contributes about 11.29 kilometres. The maximum unobstructed straight sightline between those heights is therefore about 16.34 kilometres.

The larger combined result is not a claim that the observer can see water itself that far away. The target stands above the water. Set its height to zero to recover the distance to a point on the surface. Raise either endpoint and more distance becomes available; at heights small compared with Earth’s radius, quadrupling one height approximately doubles that endpoint’s horizon distance.

These are straight-ray distances over a smooth sphere. For an actual observation, use the height above the intervening water, including the local water level, and account for any terrain. Atmospheric refraction bends the light path and can change the visible range. A photograph taken through an unknown near-water temperature profile does not supply a measured straight ray.

RUN THE NUMBERS

How far can these two heights see?

Enter eye height and target-top height above the same water surface. The calculation uses straight light rays over a smooth sphere and reports line-of-sight lengths.

Calculation inputs
m

Your height assumption. Raising the eye extends its horizon; at low heights, four times the height gives about twice the range.

m

Your target-height assumption. A taller target can remain visible farther beyond the observer’s water horizon. Set zero for a water-level point.

Maximum shared straight sightline16.34km

The two tangent lengths combined; refraction and intervening obstructions are absent from this geometry.

Observer’s water-horizon distance5,048 m

Straight distance from the eye to the tangent point on the water.

Range contributed by target height11,288 m

An elevated target contributes its own tangent distance.

Working tape
  1. Twice Earth’s radius6,371,008.4 × 2 = 12,742,016.8
  2. Earth diameter + eye height12,742,016.8 + 2 = 12,742,018.8
  3. Eye height × adjusted diameter2 × 12,742,018.8 = 25,484,037.6
  4. Observer tangent distance√(25,484,037.6) = 5,048.171709
  5. Earth diameter + target height12,742,016.8 + 10 = 12,742,026.8
  6. Target height × adjusted diameter10 × 12,742,026.8 = 127,420,268
  7. Target tangent distance√(127,420,268) = 11,288.058646
  8. Add the two tangent distances5,048.171709 + 11,288.058646 = 16,336.230355
  9. Convert the sightline to kilometres16,336.230355 ÷ 1,000 = 16.33623
04 / THE FINDING

The boundary is close because the observer is low

For an eye 2 metres above the water, the geometric water horizon is about 5.05 kilometres away. A target standing 10 metres above the same surface extends the available straight sightline to about 16.34 kilometres. Its height accounts for the extra range beyond the observer’s own water horizon.

The nearby horizon gives a low observer a small view of a large curved surface. Raising either endpoint extends that view while the water remains locally level under gravity. Comparing an observation with these distances requires both endpoint heights and the light path: refraction changes the path, while a taller target changes the geometry.

All Flat Earth
Parallel-arc length compared with polar projection radius

Flat Earth map distortion

A southern parallel of 7,076 km is drawn 23,580 km long on a north-polar disk, a 3.33× stretch. Move the latitude and watch the error grow with it.

Orthographic projection of an ideal circular disk

Flat disk eclipse shadow

A tilted disk throws an oval shadow 100 cm by 50 cm, an axis ratio of 0.5. A sphere casts a circle at every angle. Set the tilt and compare the edges.