Ecliptic

From Simple English Wikipedia, the free encyclopedia
Jump to navigation Jump to search
As seen from the orbiting Earth, the Sun appears to move with respect to the stars. The ecliptic is the yearly path the Sun follows on the celestial sphere. This process repeats itself in a cycle lasting a little over365 days

The ecliptic is the plane of Earth's orbit around the Sun.[1][2][3]

The Sun appears to move against the background of stars because the Earth orbits the Sun.

The invariable plane is the average plane of the orbits of the planets. Properly, it is defined as the plane passing through its barycenter (center of mass). The present ecliptic plane is inclined to the invariable plane by about 1.5°.

References[change | change source]

  1. United States Naval Observatory Nautical Almanac Office; UK Hydrographic Office, HM Nautical Almanac Office (2008). The Astronomical Almanac for the Year 2010. United States Government Publishing Office. p. M5. ISBN 978-0-7077-4082-9.
  2. "LEVEL 5 Lexicon and Glossary of Terms".
  3. "The Ecliptic: the Sun's annual path on the Celestial Sphere".