quantity

length

length — from formula anatomy
1 related articles · 6 formulas

Description

Length is a measure of the spatial extent of an object or the distance between two points. In physics, it is one of the seven base quantities in the International System of Units (SI), with the meter as its unit. Length appears in nearly every formula, from simple kinematics (distance = speed × time) to the wavelength of light and the size of a system in thermodynamics.

History

Length measurement is as old as civilization; the meter was introduced during the French Revolution (1790s) as a fraction of the Earth's meridian. The current definition based on the speed of light was adopted in 1983.

How it works

Length is defined operationally: it is what a ruler measures. In modern physics, the meter is defined by the distance light travels in a vacuum in 1/299,792,458 of a second, tying length to the speed of light. In geometry and calculus, length can be generalized to arc length along curves, computed via integrals.

In practice

Essential for engineering, construction, navigation, and all experimental physics — from measuring particle trajectories to astronomical distances.

Fun fact

The Planck length (about 1.6 × 10⁻³⁵ meters) is the smallest meaningful length in quantum gravity, below which our current laws of physics break down.

Concept graph →

Formulas

$$V(r) = -g \frac{e^{-r/\lambda}}{r}$$
Potential decaying exponentially with distance.
What is in the formula
VvariablePotential energy — potential energy joule
rvariableRadial distance from source — distance metre
gvariableCoupling strength (not a universal constant) joule metre
λvariableScreening length (range of interaction) — length metre
$$\Delta\phi = \frac{2\pi}{\lambda} \Delta n L$$
Phase change due to refractive index variation in medium.
What is in the formula
ΔφvariablePhase shift — phase shift radian
λvariableWavelength of light — wavelength metre
ΔnvariableChange in refractive index — refractive index change
LvariablePath length through medium — length metre
$$q = Z/X$$
Axis ratio is height divided by length.
What is in the formula
qvariableAxis ratio — axis ratio
ZvariableHeight (vertical extent) — length metre
XvariableLength (horizontal extent) — length metre
$$k(r) = rac{\sigma^2 2^{1-\nu}}{\Gamma(\nu)} \left( \frac{\sqrt{2\nu} r}{l} \right)^\nu K_\nu \left( \frac{\sqrt{2\nu} r}{l} \right)$$
A covariance function for Gaussian processes with smoothness parameter ν.
What is in the formula
rvariabledistance between two points — distance metre
νvariablesmoothness parameter
lvariablelength scale parameter — length metre
σvariablevariance amplitude — variance square metre
ΓoperatorGamma function, generalizes factorial — gamma function
K_νoperatorModified Bessel function of the second kind of order ν — modified bessel function second kind
$$r_{\text{sh}} / r_{\text{H}} \ge \frac{3\sqrt{3}}{2}$$
The shadow radius of a Schwarzschild black hole is at least 3√3/2 times the event horizon radius.
What is in the formula
r_{\text{sh}}variableShadow radius as seen by a distant observer — length metre
r_{\text{H}}variableEvent horizon radius of the black hole — length metre
$$P = 2\pi \sqrt{\frac{a^3}{GM}}$$
Orbital period squared is proportional to semi-major axis cubed.
What is in the formula
Pvariableorbital period — period second
avariablesemi-major axis of the orbit — length metre
Mvariablemass of the central body — mass kilogram
Gconstantconstant of universal gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
sqrtoperatortakes the square root — square root

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