unit

astronomical unit

A unit of length equal to the average distance between the Earth and the Sun, used for distances within planetary systems.
9 related articles

Description

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.

History

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.

How it works

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.

In practice

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.

Fun fact

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.

Concept graph →

Related articles · 9

High Energy2026-08-051 minarXiv:2608.04658express
Moon Shadows Cast by Giant Cosmic Rays
Cosmic rays aren't rays in the usual sense: they're fast particles bombarding Earth from all directions. Mostly they're protons and atomic nuclei. Their energies vary widely, from modest to fantastically huge. When such a particle heads our way and the Moon or Sun gets in its path, it gets absorbed.
Cosmology2026-08-022 minarXiv:2608.00923express
Neutrinos Reveal the Universe's Expansion Rate
Measuring distances in the universe is no easy task. Almost all methods rely on light, which can be absorbed by dust, scattered, or distorted along the way. It's like trying to spot a distant lighthouse through fog and haze. Neutrinos are a different story. These ghostly particles pass through anything without noticing obstacles.
General Relativity2026-07-082 minarXiv:2607.07741express
Cosmic Mirage: How the Solar Bubble Is Reshaping the Map of the Universe
The cosmological debate is like two craftsmen measuring the same wall but getting different lengths. One uses a tape measure, applying it to nearby landmarks — Cepheids (pulsating beacon stars) and Type Ia supernovae (flashes of dying stars). He finds the wall is stretching at 73.5 arbitrary units.
Exoplanets2026-05-302 minarXiv:2606.00612express
Planet X: The Dance of Twelve Stones
At the edge of the solar system, where the Sun is barely brighter than other stars, icy boulders, trans-Neptunian objects, circle around. Their orbits resemble hoops scattered by someone. But look closer: twelve of these hoops are not just floating in the void.
Exoplanets2026-04-281 minarXiv:2604.25990express
Planet X Loses Its Footing
At the edge of the solar system, far beyond Neptune, hundreds of icy chunks circle the Sun. Some of them move as if an invisible hand had aligned their orbits like compass needles. Ten years ago, this led astronomers to suspect that a massive planet, about ten times heavier than Earth, is hiding there.
Exoplanets2026-04-031 minarXiv:2604.03049express
Seven Planets March in Lockstep
Every 1151 years, seven planets of the Solar System, from Mercury to Neptune, find themselves at almost the same points in their orbits. Their positions scatter by less than a degree, as if the celestial mechanism is wound to the same tune. This rhythm was discovered by comparing planetary positions over 2600 years using precise tables of celestial motion.
Stellar2026-03-241 minarXiv:2603.23291express
The Sun Flickers Like a Candle
The Sun is not a perfectly steady lightbulb. Its brightness quivers slightly: it dims a bit, then brightens. For Earth's climate, even slow variations stretched over thousands and millions of years matter. They could have left their mark in the geological record of the last 540 million years. Astronomer [scientist:A. M.
Stellar2026-01-071 minarXiv:2601.03539express
Dance of the Invisible Giants: Gaia Finds a 'Desert' of Brown Dwarfs
Sun-like stars rarely spin alone. Many of them dance with invisible partners — brown dwarfs: objects bigger than planets but too lightweight for steady stellar burning. In their cores, hydrogen fusion flickers, only to fade fast, never matching the stability of the Sun.
Cosmology2025-10-312 minarXiv:2510.27416express
Earth's Gravitational Lens: Hunting Axions in the Focus of Spacetime
Dark matter is the invisible scaffold of the Universe, revealing itself only through gravity. Vera Rubin, studying the rotation of galaxies, found that stars at the periphery move too fast, as if held by an unseen mass. This became compelling evidence for the existence of dark matter, yet its particles still elude direct detection.