3D Distance Calculator
Calculate the Euclidean distance between two points in 3D space, plus midpoint, direction cosines, direction angles, and 2D projection comparisons.
Calculate the distance between two points in 2D space using Euclidean, Manhattan, or Chebyshev metrics. Also computes midpoint, slope, and component breakdown.
| Metric | Formula | Distance | Ratio to Euclidean |
|---|---|---|---|
| Euclidean | √(Δx² + Δy²) | 5.0000 | 1.0000 |
| Manhattan | |Δx| + |Δy| | 7.0000 | 1.4000 |
| Chebyshev | max(|Δx|, |Δy|) | 4.0000 | 0.8000 |
| From | To | Euclidean | Manhattan |
|---|---|---|---|
| (0,0) | (1,0) | 1 | 1 |
| (0,0) | (1,1) | 1.4142 | 2 |
| (0,0) | (3,4) | 5 | 7 |
| (0,0) | (5,12) | 13 | 17 |
| (0,0) | (8,15) | 17 | 23 |
| (0,0) | (7,24) | 25 | 31 |
| (1,2) | (4,6) | 5 | 7 |
| (−3,−4) | (0,0) | 5 | 7 |
The **2D Distance Calculator** finds the straight-line (Euclidean) distance between any two points on a coordinate plane and also offers Manhattan and Chebyshev distance metrics for comparison. Enter the coordinates of Point A and Point B, and the tool returns the distance, midpoint, slope, and component breakdown.
Calculating distances in two dimensions is a foundational skill in analytic geometry, physics, computer science, and data science. The classic distance formula, derived from the Pythagorean theorem, measures the length of the hypotenuse of a right triangle formed by the horizontal and vertical displacements between the two points. Manhattan distance (also called taxicab distance) sums the absolute differences along each axis, modelling movement restricted to a grid. Chebyshev distance takes the maximum of the two axis differences, useful for chessboard-king movement and certain optimization problems.
This calculator goes beyond a raw number — it breaks out Δx and Δy visually so you can see which component dominates, computes the midpoint and line slope, and provides a comparison table of all three metrics side by side. Eight presets cover classic examples such as the 3-4-5 right triangle and diagonal grid traversals, letting you compare different scenarios quickly.
Whether you are plotting paths on a map, analysing k-nearest-neighbor distances in machine learning, or solving a high-school geometry problem, the page keeps the metric comparison, midpoint, slope, and component breakdown together so you can judge the geometry from more than a single distance value.
Distance problems often depend on which metric you mean, not just on the coordinates. This calculator keeps Euclidean, Manhattan, and Chebyshev distance side by side so you can compare the straight-line answer with grid-based and max-axis alternatives.
It is also useful when the geometry around the distance matters. Midpoint, slope, and the Δx/Δy breakdown help confirm whether the coordinate pair was entered correctly and whether the result fits the picture you expect.
Euclidean: d = √((x₂−x₁)² + (y₂−y₁)²). Manhattan: d = |x₂−x₁| + |y₂−y₁|. Chebyshev: d = max(|x₂−x₁|, |y₂−y₁|). Midpoint: M = ((x₁+x₂)/2, (y₁+y₂)/2). Slope: m = (y₂−y₁)/(x₂−x₁).Result: Euclidean distance = 5
Using x1=0, y1=0, x2=3, y2=4, the calculator returns Euclidean distance = 5. This example mirrors the calculator's live computation flow and is useful for checking manual steps and unit handling.
This page is designed for point-to-point distance problems where you want both the main answer and the geometric context around it. It compares three common 2D metrics and also reports midpoint, slope, and coordinate differences from the same pair of points.
Start with the Euclidean distance if you want the straight-line result. Then compare Manhattan and Chebyshev distance to see how the same coordinate pair behaves under grid-based or max-step movement rules.
Work one example manually with the distance formula, then compare the Euclidean result with the two alternate metrics. After that, try a horizontal, vertical, and diagonal pair of points to see how each metric responds to different geometry.
Last updated:
Euclidean distance is the straight-line length between two points. Manhattan distance sums the absolute horizontal and vertical differences, modelling travel along grid lines.
Chebyshev distance is useful when diagonal movement costs the same as horizontal or vertical movement, such as king moves in chess or certain warehouse routing problems.
Yes. The calculator works for any real-valued coordinates, including negative values that place points in other quadrants of the coordinate plane.
All three distance metrics return zero, the midpoint equals the point itself, and the slope is undefined (0/0).
The midpoint M is the average of the two x-coordinates and the average of the two y-coordinates: M = ((x₁+x₂)/2, (y₁+y₂)/2).
Yes. By the triangle inequality, the straight-line distance never exceeds the sum of axis-aligned segments. Manhattan ≥ Euclidean ≥ Chebyshev always holds.
Calculate the Euclidean distance between two points in 3D space, plus midpoint, direction cosines, direction angles, and 2D projection comparisons.
Find a missing side of a triangle using the Law of Cosines, Law of Sines, Pythagorean Theorem, or subtract known sides from the perimeter. Select a method, enter known values, and get the unknown s...
Solve right triangles with the Pythagorean theorem. Find any side, angles, area, perimeter, altitude, inradius, circumradius, and detect special triples.