Shows the formula
Every step of the distance formula with your numbers.
Enter two points to get the straight-line distance, with the distance formula worked out, the exact answer as a simplified square root, the midpoint and more. Switch to map mode for latitude and longitude.
Use decimal degrees: north and east are positive, south and west are negative. The example is London to New York.
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Every step of the distance formula with your numbers.
Whole-number inputs give a simplified square root like 2√13.
Flat 2D, 3D space, or real places on Earth.
The distance between (x₁, y₁) and (x₂, y₂) comes from Pythagoras' theorem: the horizontal and vertical differences are the two short sides of a right triangle, so d = √((x₂ − x₁)² + (y₂ − y₁)²). In 3D you add the squared z-difference under the same square root.
On the Earth's surface, straight lines become great circles. The haversine formula gives the shortest distance over a sphere using latitudes and longitudes, which is accurate to within about half a percent for the real, slightly flattened Earth.
The average of the coordinates: ((x₁ + x₂)/2, (y₁ + y₂)/2).
The sum of absolute differences, like walking a city grid.
The compass direction to start in when travelling from point 1 to point 2.
d = √((x₂ − x₁)² + (y₂ − y₁)²) in 2D, and d = √((x₂ − x₁)² + (y₂ − y₁)² + (z₂ − z₁)²) in 3D.
No. The differences are squared, so swapping the points gives the same distance.
The largest perfect square is taken out of the square root. For example √52 = √(4 × 13) = 2√13.
The haversine result is the shortest path over the Earth's surface. Roads, flight paths and terrain make real routes longer.
The mean radius of 6,371.0088 km recommended by the International Union of Geodesy and Geophysics.
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