Distance Between Points Calculator
Calculate the distance between two points in 2D, 3D, or N-dimensional space. Enter values for instant results with step-by-step formulas.
Reviewed by Manoj Kumar, Mathematics Educator
Formula
d = sqrt((x2-x1)^2 + (y2-y1)^2 + (z2-z1)^2)
The Euclidean distance formula is derived from the Pythagorean theorem. For 2D, it uses the square root of the sum of squared differences in x and y coordinates. For 3D, a z-component is added. The formula generalizes to N dimensions by adding additional squared difference terms under the radical.
Worked Examples
Example 1: 2D Distance Between Two Points
Problem:Find the distance between points A(1, 2) and B(4, 6).
Solution:d = sqrt((x2 - x1)^2 + (y2 - y1)^2)\nd = sqrt((4 - 1)^2 + (6 - 2)^2)\nd = sqrt(3^2 + 4^2)\nd = sqrt(9 + 16)\nd = sqrt(25) = 5.0 units\nMidpoint: ((1+4)/2, (2+6)/2) = (2.5, 4.0)\nSlope: (6-2)/(4-1) = 4/3 = 1.333\nManhattan distance: |3| + |4| = 7
Result:Euclidean: 5.0 | Manhattan: 7 | Midpoint: (2.5, 4.0)
Example 2: 3D Distance Between Two Points
Problem:Find the distance between points P(2, 3, 1) and Q(5, 7, 4).
Solution:d = sqrt((x2-x1)^2 + (y2-y1)^2 + (z2-z1)^2)\nd = sqrt((5-2)^2 + (7-3)^2 + (4-1)^2)\nd = sqrt(3^2 + 4^2 + 3^2)\nd = sqrt(9 + 16 + 9)\nd = sqrt(34) = 5.831 units\nMidpoint: (3.5, 5.0, 2.5)\nManhattan distance: 3 + 4 + 3 = 10\nChebyshev distance: max(3, 4, 3) = 4
Result:Euclidean: 5.831 | Manhattan: 10 | Chebyshev: 4
Frequently Asked Questions
What is the distance formula and how is it derived from the Pythagorean theorem?
The distance formula is a direct application of the Pythagorean theorem extended to coordinate geometry. For two points (x1, y1) and (x2, y2) in a plane, the horizontal distance is |x2 - x1| and the vertical distance is |y2 - y1|, forming the two legs of a right triangle. The distance between the points is the hypotenuse: d = sqrt((x2-x1)^2 + (y2-y1)^2). This formula was first formalized by Rene Descartes when he unified algebra and geometry in the 17th century, creating analytic geometry. The same principle extends to three dimensions by adding a z-component: d = sqrt((x2-x1)^2 + (y2-y1)^2 + (z2-z1)^2). The formula generalizes to N dimensions by adding additional squared difference terms.
What is the difference between Euclidean distance, Manhattan distance, and Chebyshev distance?
These three distance metrics measure separation between points in fundamentally different ways. Euclidean distance is the straight-line distance, representing the shortest possible path between two points in space. Manhattan distance, also called taxicab distance or L1 norm, measures the sum of absolute differences along each axis, representing the distance traveled on a grid where you can only move horizontally or vertically. Chebyshev distance, also called chessboard distance or L-infinity norm, is the maximum absolute difference along any single axis, representing the minimum number of moves a king needs on a chess board. For points (1,2) and (4,6): Euclidean = 5, Manhattan = 7, Chebyshev = 4. Each metric is useful in different applications.
How do you calculate the distance between two points in 3D space?
The 3D distance formula extends the 2D version by adding a z-coordinate component. For points (x1, y1, z1) and (x2, y2, z2), the distance equals sqrt((x2-x1)^2 + (y2-y1)^2 + (z2-z1)^2). This works because you can form a right triangle in 3D: first calculate the 2D distance in the xy-plane, then use that as one leg and the z-difference as the other leg of a new right triangle. The hypotenuse of this second triangle gives the full 3D distance. For example, the distance from (1, 2, 3) to (4, 6, 8) equals sqrt(9 + 16 + 25) = sqrt(50) = 7.071 units. This formula is essential in physics, engineering, computer graphics, and any field dealing with spatial measurements.
What is the midpoint formula and how does it relate to the distance formula?
The midpoint formula finds the exact center point between two given points by averaging their coordinates. For points (x1, y1) and (x2, y2), the midpoint is ((x1+x2)/2, (y1+y2)/2). In 3D, it extends to ((x1+x2)/2, (y1+y2)/2, (z1+z2)/2). The midpoint is equidistant from both original points, and the distance from the midpoint to either point equals exactly half the total distance between them. This property makes the midpoint formula valuable in geometry for bisecting line segments, finding centers of circles, and constructing perpendicular bisectors. In practical applications, the midpoint helps find the geographic center between two locations, the balanced center of mass, or the optimal meeting point between two positions.
References
Reviewed by Manoj Kumar, Mathematics Educator · Editorial policy