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===Straight-line or Euclidean distance=== {{main|Euclidean distance}} The distance between two points in physical [[space]] is the [[length]] of a [[line segment|straight line]] between them, which is the shortest possible path. This is the usual meaning of distance in [[classical physics]], including [[Newtonian mechanics]]. Straight-line distance is formalized mathematically as the [[Euclidean distance]] in [[two-dimensional Euclidean space|two-]] and [[three-dimensional space]]. In [[Euclidean geometry]], the distance between two points {{mvar|A}} and {{mvar|B}} is often denoted <math>|AB|</math>. In [[Cartesian coordinate system|coordinate geometry]], Euclidean distance is computed using the [[Pythagorean theorem]]. The distance between points {{math|(''x''<sub>1</sub>, ''y''<sub>1</sub>)}} and {{math|(''x''<sub>2</sub>, ''y''<sub>2</sub>)}} in the plane is given by:<ref name=":0">{{Cite web|last=Weisstein|first=Eric W.|title=Distance|url=https://mathworld.wolfram.com/Distance.html|access-date=2020-09-01|website=mathworld.wolfram.com|language=en}}</ref><ref>{{Cite web|title=Distance Between 2 Points|url=https://www.mathsisfun.com/algebra/distance-2-points.html|access-date=2020-09-01|website=www.mathsisfun.com}}</ref> <math display="block">d=\sqrt{(\Delta x)^2+(\Delta y)^2}=\sqrt{(x_2-x_1)^2+(y_2-y_1)^2}.</math> Similarly, given points (''x''<sub>1</sub>, ''y''<sub>1</sub>, ''z''<sub>1</sub>) and (''x''<sub>2</sub>, ''y''<sub>2</sub>, ''z''<sub>2</sub>) in three-dimensional space, the distance between them is:<ref name=":0" /> <math display="block">d=\sqrt{(\Delta x)^2+(\Delta y)^2+(\Delta z)^2}=\sqrt{(x_2-x_1)^2+(y_2-y_1)^2+(z_2-z_1)^2}.</math> This idea generalizes to higher-dimensional [[Euclidean space]]s. ==== Measurement ==== {{main|Distance measurement}} There are many ways of [[measuring]] straight-line distances. For example, it can be done directly using a [[ruler]], or indirectly with a [[radar]] (for long distances) or [[interferometry]] (for very short distances). The [[cosmic distance ladder]] is a set of ways of measuring extremely long distances.
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