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Glossary term: Earth's Axis

Redirected from North Pole

Description: The Earth's axis is an imaginary straight line around which the Earth spins once per day. The two locations where the axis and the Earth's surface intersect define the geographic North Pole at a latitude of 90°N and the geographic South Pole at a latitude of 90°S. In contrast, the equator is an imaginary line where a plane perpendicular to the Earth's axis intersects with the Earth's surface at the greatest distance from the axis. The equator has a latitude of 0°.

The geographic poles are not at the same places as the Earth's magnetic North and South Poles – the magnetic poles are defined as the locations on the surface where Earth's magnetic field points straight down and straight up, respectively.

Earth's orbit has an axis as well: The direction perpendicular to Earth's orbital plane. Earth's axis is inclined by an angle of 23.4° against that orbital axis. This tilt is the cause of Earth's seasons. In particular, over the course of one orbit, there are phases where the northern hemisphere or the southern one are tilted toward the Sun, thus receiving more light.

Relative to the most distant celestial objects, the direction Earth's axis points towards changes slowly over time, in what is called Earth's axial precession. Currently, the Earth's axis intersects the celestial sphere close to Polaris, the North Star. But over roughly 26,000 years, that intersection point describes a small circle in the sky. Celestial coordinate systems that define sky coordinates with reference to Earth need to take the resulting minute coordinate shifts over time into account.

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Term and definition status: This term and its definition have been approved by a research astronomer and a teacher

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

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Related Diagrams


Two views of the Earth with important lines of latitude and longitude marked

Latitude and Longitude

Caption: Two views of the Earth, one viewing the Northern Hemisphere, one viewing the Southern Hemisphere. The Earth rotates around its axis, an imaginary line that runs through the Earth from the North Pole to the South Pole. The Equator is an imaginary line that is the same distant from both the North Pole and the South Pole. The positions of two cities, Rome in the Northern Hemisphere and Sydney in the Southern Hemisphere are marked here with red dots. Arrows indicate the two spherical coordinates latitude and longitude. Latitude marks the position north or south of the equator. Here we can see Rome has the letter N in its latitude as it is in the Northern Hemisphere and Sydney has the letter S in its latitude as it is in the Southern Hemisphere. Latitude can vary from 90° N at the North Pole to 0° at the Equator to 90° S at the South Pole. Longitude measures the position around the equator. While the choice of the zero point for latitude as the equator seems obvious, the choice of the zero point for longitude is more subjective. By convention the zero point in longitude is the prime meridian which passes through the Royal Greenwich Observatory in the UK. This is marked here as a solid line originating at the North Pole. Longitude is measured in degrees east or west of the prime meridian. As both Rome and Sydney lie to the east of Greenwich, they have the letter E as part of their longitude. Moving west to east, longitude varies from 180° W on the other side of the world from the prime meridian to 0° on the prime meridian before reaching 180° E again on the other side of world from the prime meridian. This diagram shows the Earth at the December solstice. Two views are presented, one viewing the Northern Hemisphere and one viewing the Southern Hemisphere about nine hours later. The shaded region shows the night side of the Earth, with the day side being lighter. As it is the December solstice, the Sun appears overhead at the Tropic of Capricorn. This is a line of constant latitude at 23°26′09.3″ S. Six months later, at the June solstice, the Sun will appear to be overhead at the Tropic of Cancer at 23°26′09.3″ N. As the Sun appears over the Tropic of Capricorn more of the Southern Hemisphere is illuminated than the Northern Hemisphere. Indeed below the Antarctic Circle (the Polar Circle around the South Pole) the Sun does not set at this time of year leading to a Polar Day. Conversely, north of the Arctic Circle (the Polar Circle around the North Pole) the Sun does not rise at this time of year, leading to a Polar Night.
Credit: Maria Cristina Fortuna/IAU OAE

License: CC-BY-4.0 Creative Commons Attribution 4.0 International (CC BY 4.0) icons

Related Activities


Why Do We Have Day and Night?

Why Do We Have Day and Night?

astroEDU educational activity (links to astroEDU website)
Description: Explore day and night of Earth.

License: CC-BY-4.0 Creative Commons Attribution 4.0 International (CC BY 4.0) icons
Tags: Tilt
Age Ranges: 6-8 , 8-10 , 10-12
Education Level: Primary , Secondary
Areas of Learning: Modelling , Structured-inquiry learning , Social Research
Costs: Low Cost
Duration: 1 hour 30 mins
Group Size: Group
Skills: Asking questions , Communicating information