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Polar Axis

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Rotational axis

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The polar axis of a planet is its axis of rotation. It is perpendicular to the planet’s equatorial plane. The inclination of the Earth’s polar axis with respect to the plane of its orbit about the Sun is responsible for the phenomenon of seasonal variations. Telescopes with an equatorial mount have one axis, also called the polar axis, which is parallel to the Earth’s rotation axis. The slow (26,000 year period) conical motion of the Earth’s polar axis is responsible for the precession of the equinoxes.

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Correspondence to Daniel Rouan .

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© 2014 Springer-Verlag Berlin Heidelberg

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Rouan, D. (2014). Polar Axis. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1244-2

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1244-2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

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