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What Is Earth's Axial Tilt or Obliquity?

When an object the size of Mars crashed into the newly formed planet Earth around 4.5 billion years ago, it knocked our planet over and left it tilted at an angle.

Illustration showing Earth's axis drawn as a red line.

Earth's axis is the imaginary red line.

Earth's axis is the imaginary red line that runs through the North and South Poles.


Earth's Axis Is Imaginary

In astronomy, an axis refers to the imaginary line that an object, usually a planet, rotates around.

Earth's rotational axis is an imaginary straight line that runs through the North and South Pole. In our illustrations, Earth's axis is drawn as a straight red line.

Ever since the impact around 4.5 billion years ago, Earth has been orbiting the Sun at a slant. This slant is the axial tilt, also called obliquity.

Earth's obliquity angle is measured from the imaginary line that runs perpendicular to another imaginary line; Earth's ecliptic plane or orbital plane (see illustration).

At the moment, Earth's obliquity is about 23.4 degrees and decreasing. We say 'at the moment' because the obliquity changes over time, although very, very slowly.

Earth's Obliquity Today

Today, on March 28, 2017 at noon, Earth's axial tilt, or true obliquity was 23.43704° or 23°26'13.3".

Earth's true obliquity today is about 0.00001°, or 0.04", less than 30 days ago.

The Arctic circles today are 1.2 m (4 ft) closer to the poles, and the Tropic of Cancer and Tropic of Capricorn are equally closer to the equator than 30 days ago.

The Tilt Changes

Earth's axial tilt actually oscillates between 22.1 and 24.5 degrees. The reason for this changing obliquity angle is that Earth's axis also wobbles around itself. This wobble motion is called axial precession, also known as precession of the equinoxes. It is caused by the gravitational force from the Sun, the Moon, and other planets.

Acts Like Two Spinning Tops

Axial precession can be described as a slow gyration of Earth's axis about another line intersecting it. A complete wobble of Earth's axis takes around 26,000 years. It outlines the shape of a pair of cones or two spinning tops connected at the tips, which would be at the center of Earth.

Ancient Discovery

Greek astronomer Hipparchus of Nicea is historically credited as the man who first proposed that Earths axis gradually shifts, though very slowly. Hipparchus made his discovery around 130 BCE, based on comparisons of astronomical observations more than a century apart.

Illustration showing Earth's position in relation to the Sun at the equinoxes and solstices.
Earth's axial tilt causes seasons.
Earth orbits the Sun at a slant, which is why we have different seasons.

Tilt Causes Seasons

Because Earth orbits the Sun at an angle, the solar energy reaching different parts of our planet is not constant, but varies during the course of a year.

This is the reason we have different seasons and why the seasons are opposite in the Northern and Southern Hemispheres.

Opposite Seasons

From the March equinox to the September equinox, the Northern Hemisphere tilts towards the Sun. During this time, there are more than 12 hours of daylight north of the Equator.

Young girl and boy studying a globe.
Our point of view of Earth may vary.
Our point of view of Earth may vary, but the axis always tilts the same way.

At the same time, the Southern Hemisphere tilts away from the Sun, resulting in shorter days.

From the September equinox to the next March equinox, the days are longer south of the equator and shorter north of the equator.

Illustrator's Point of View

Different illustrators may vary which direction they incline the axis in their images. Some draw it tilted left-to-right, others right-to-left. These illustrations can both be accurate; the only difference is that the artist has chosen the opposite side of the Sun as the point-of-view.

Topics: Astronomy, Seasons, Equinox, Solstice, Earth

Astronomical Season Calculator


The Science of Seasons

  1. What Causes Seasons?
  2. Earth's Axis Is Tilted
  3. Meteorological vs. Astronomical Seasons
  4. What Is a Solar Analemma?

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