Manhattan Distance Formula:
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The Manhattan distance (also called taxicab distance or city block distance) is a metric that measures the distance between two points in a grid-based system by summing the absolute differences of their coordinates. It's called "Manhattan distance" because it resembles the path a taxi would take in a grid-like city like Manhattan.
The calculator uses the Manhattan distance formula:
Where:
Explanation: The formula calculates the sum of the absolute differences between the x-coordinates and y-coordinates of the two points.
Details: Manhattan distance is widely used in computer science (pathfinding algorithms), data analysis (clustering), and any application where movement is restricted to grid-like paths.
Tips: Enter the coordinates of two points in any unit system (the distance will be in the same units). The calculator works with both positive and negative coordinate values.
Q1: How is Manhattan distance different from Euclidean distance?
A: Euclidean distance measures the straight-line distance between points, while Manhattan distance measures the sum of the absolute differences of their coordinates.
Q2: Can Manhattan distance be used in 3D space?
A: Yes, the formula extends to: \( d = |x_2 - x_1| + |y_2 - y_1| + |z_2 - z_1| \)
Q3: When should I use Manhattan distance instead of Euclidean?
A: Use Manhattan distance when movement is constrained to grid-like paths (like city streets), or when outliers should have less impact.
Q4: Is Manhattan distance always greater than Euclidean distance?
A: Yes, for any two points in the same space, Manhattan distance will always be equal to or greater than Euclidean distance.
Q5: Can Manhattan distance be negative?
A: No, distance is always a non-negative value as it's the sum of absolute differences.