A unit of length equal to the average distance between the Earth and the Sun, used for distances within planetary systems.The astronomical unit (AU) is a unit of length defined as exactly 149,597,870.7 kilometers, which is approximately the average distance between the Earth and the Sun. It serves as a convenient yardstick for measuring distances within our solar system and for expressing the scale of planetary orbits. The AU is fundamental to celestial mechanics, providing a baseline for calculating the distances to other stars via parallax and for communicating the layout of planetary systems.
The concept of the astronomical unit dates back to the ancient Greek astronomer Aristarchus, who first attempted to estimate the Earth-Sun distance. The first reasonably accurate measurement was made in 1672 by Giovanni Cassini and Jean Richer, who used parallax observations of Mars to derive a value close to the modern one.
The AU is not a fixed physical object but a defined constant, based on the average Earth-Sun distance. Historically, it was determined by measuring the transit of Venus across the Sun's disk from different points on Earth, using parallax to triangulate the distance. Today, it is measured with high precision using radar echoes from planets and spacecraft telemetry, and its value is fixed by international definition, independent of the actual Earth orbit, which varies slightly due to gravitational perturbations.
The AU is used to express distances in the solar system, such as the orbital radii of planets, and serves as the basis for the parsec, a unit used for interstellar distances.
Light takes about 8 minutes and 20 seconds to travel one astronomical unit, which is why we see the Sun as it was over 8 minutes ago.


