Astronomical unit

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1 astronomical unit =
SI units
149.60×106 km 149.60×109 m
Astronomical units
4.8481×10−6 pc 15.813×10−6 ly}}
US customary / Imperial units
92.956×106 mi 490.81×109 ft
The semi-major and semi-minor axis of an ellipse

The astronomical unit (AU) is a unit of length got from the Earth's orbit. Its definition is: the length of the semi-major axis of the Earth's elliptical orbit around the Sun. "Semi-major" means half the long axis.

The AU is about 150 million kilometers or 93 million miles. Astronomers usually measure distances within the Solar System in astronomical units. Mars is about 1.4 AU from the Sun, Jupiter lies at roughly 5.2 AU, and Neptune is roughly 30 AU from the Sun.

The Astronomical Unit is much used in solar system studies. Light travels an AU in about 8.317 minutes.

More accuracy[change | change source]

From 1976 to 2012 the AU was defined as “the radius of an unperturbed circular Newtonian orbit about the Sun of a particle having infinitesimal mass, moving with a mean motion of 0.01720209895 radians per day (known as the Gaussian constant)”. [1][2][3] In 2012, the IAU redefined it to be simply 149597870700 m.[4]

In the IERS numerical standards, the speed of light in a vacuum is defined as c0 = 299792458 m/s, in accordance with the SI units. The time to cover an AU is τA = 499.0047838061±0.00000001 s, resulting in the astronomical unit in metres as c0τA = 149597870700±3 m.[5] It is approximately equal to the distance from the earth to the sun.

References[change | change source]

  1. Resolution No. 10 of the XVIth General Assembly of the International Astronomical Union, Grenoble, 1976
  2. H. Hussmann, F. Sohl, J. Oberst (2009), "§4.2.2.1.3: Astronomical units", in Joachim E Trümper, Astronomy, astrophysics, and cosmology. Volume VI/4B Solar System, Springer, p. 4, ISBN 3-540-88054-2, http://books.google.com/?id=wgydrPWl6XkC&pg=RA1-PA4
  3. Gareth V Williams (1997), "Astronomical unit", in James H. Shirley, Rhodes Whitmore Fairbridge, Encyclopedia of planetary sciences, Springer, p. 48, ISBN 0-412-06951-2, http://books.google.com/books?id=dw2GadaPkYcC&pg=PA48
  4. Geoff Brumfiel (14-Sep-2012). "The astronomical unit gets fixed: Earth–Sun distance changes from slippery equation to single number.". http://www.nature.com/news/the-astronomical-unit-gets-fixed-1.11416. Retrieved 14-Sep-2012.
  5. Gérard Petit and Brian Luzum, eds. (2010). "Table 1.1: IERS numerical standards". IERS technical note no. 36: General definitions and numerical standards. International Earth Rotation and Reference Systems Service. ftp://tai.bipm.org/iers/conv2010/chapter1/tn36_c1.pdf. For complete document see Gérard Petit and Brian Luzum, eds. (2010). IERS Conventions (2010): IERS technical note no. 36. International Earth Rotation and Reference Systems Service. ISBN 978-3-89888-989-6. http://www.iers.org/nn_11216/IERS/EN/Publications/TechnicalNotes/tn36.html.