What is the astronomical unit?
The astronomical unit serves primarily for measuring distances within the Solar System or around other stars. It acts as a fundamental component in defining another unit called the parsec.
The astronomical unit serves primarily for measuring distances within the Solar System or around other stars. It acts as a fundamental component in defining another unit called the parsec.
The modern definition of the astronomical unit was established in 2012 when the IAU set its value at exactly 149597870700 meters. Prior to this, the unit depended on the Gaussian gravitational constant k.
Around 280 BC, Aristarchus measured the angle between the Moon and Sun when the Moon was in its first quarter. He estimated this angle at 87 degrees, though the true value is closer to 89.5 degrees.
Observing the transit of Venus across the face of the Sun became the primary method for determining the astronomical unit during the 18th and 19th centuries. Transits occur in pairs less than once every century with the next pair appearing in 1874 and 1882.
In 1976, the International Astronomical Union adopted the symbol A to denote this length while scientific journals commonly used AU instead. The International Bureau of Weights and Measures recommended ua as the symbol in 2006 before au became the standard in 2012.