Manhattan Distance Formula:
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The Manhattan Distance, also known as Taxicab Distance or L₁ Distance, is a measure of the distance between two points in a grid-based system where movement is restricted to horizontal and vertical paths only, much like navigating the streets of Manhattan.
The calculator uses the Manhattan Distance formula:
Where:
Explanation: The distance is calculated by summing the absolute differences of their Cartesian coordinates.
Details: Manhattan Distance is widely used in computer science (pathfinding algorithms), data analysis (clustering), image processing, and urban planning.
Tips: Enter the coordinates of two points in 2D space. The calculator will compute the Manhattan Distance between them. All values can be positive or negative real numbers.
Q1: How is Manhattan Distance different from Euclidean Distance?
A: Manhattan Distance sums absolute differences (grid path), while Euclidean Distance uses straight-line distance (Pythagorean theorem).
Q2: Can this be extended to higher dimensions?
A: Yes, for n-dimensional points, sum absolute differences across all dimensions: \( \sum_{i=1}^n |x_i - y_i| \).
Q3: Why is it called "Manhattan" Distance?
A: It resembles the path a taxi would take in Manhattan's grid-like street layout, unable to cut diagonally through buildings.
Q4: What's the maximum Manhattan Distance between two points?
A: In a bounded area, it depends on the grid size. For a square of side length L, maximum distance is 2L (between opposite corners).
Q5: When should I use Manhattan vs Euclidean Distance?
A: Use Manhattan when movement is grid-constrained (like chess), Euclidean when straight-line distance is possible (like flying).