Axial tilt

Axial tilt of Earth is 23.439278°

In astronomy, axial tilt is the angle between a planet's rotational axis at its north pole and a line perpendicular to the orbital plane of the planet. It is also called axial inclination or obliquity. The axial tilt of Earth is the cause of seasons like summer and winter on Earth.

Axial tilt of bodies in the Solar System

To understand axial tilt, we employ the right-hand rule. When the fingers of the right hand are curled around in the direction of the planet's rotation, the thumb points in the direction of the north pole

Axial tilt of Venus, Uranus, Pluto

The axial tilts of Venus, Uranus and Pluto are greater than 90 degrees for the following reasons:

References

  1. ↑ Musser, George (October 2006). "Double impact may explain why Venus has no moon". Scientific American. Retrieved 2011-12-05.
  2. ↑ Bergstralh, Jay T; Miner, Ellis & Matthews, Mildred (1991). Uranus. pp. 485–486. ISBN 0-8165-1208-6.{{cite book}}: CS1 maint: multiple names: authors list (link)
  3. ↑ "NASA Planetary Fact Sheet". Archived from the original on 2016-11-28. Retrieved 2009-10-18.