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Terme du glossaire : Longitude

Description : La Terre est une sphère. Pour définir les lieux sur la Terre, deux séries de lignes imaginaires sont tracées à la surface de la sphère. Les lignes de longitude sont de grands cercles qui font le tour de la Terre et passent par le pôle Nord et le pôle Sud. Alors que l'équateur fournit un point de référence naturel pour le 0 degré de latitude, la ligne du 0 degré de longitude a dû faire l'objet d'un accord. La ligne reconnue de 0 degré de longitude passe par Greenwich, à Londres, au Royaume-Uni, et est également appelée méridien d'origine ou méridien de Greenwich. L'antiméridien se trouve à l'autre bout du monde, à 180 degrés, et sert de base à la ligne internationale de changement de date. La distance totale angulaire autour de la Terre est de 360 degrés. Il existe également des lignes qui tournent en petits cercles autour de la Terre, et parallèles à l'équateur. Ce sont les lignes de latitude.

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Statut du terme et de sa définition : La définition initiale de ce terme en anglais a été aprouvée par un·e spécialiste de la recherche en astronomie et un·e spécialiste de l’éducation
La traduction de ce terme et de sa définition n'ont pas encore été aprouvées

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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Media associé


Map of the world with different time zones marked by color. The basic pattern is timezones as 15-degree swathes of longitude.

Map of de-facto time zones on Earth

Légende : Due to the Earth's spherical shape and its rotation around its own axis, local noon – the moment in time when, for an observer at a specific geographic location, the Sun reaches its highest position in the sky varies with longitude. That is why a time coordinate, such as Universal Time (UT or UTC), might be of advantage for specifying moments in time in a unified way. But a global time coordinate will be out of synch with the local day-night rhythm in most locations on Earth. A compromise is to divide Earth into zones each comprising 15 degrees of longitude, and in each zone define time as UTC plus or minus an integer number of hours, with the offset chosen so as to make time match as closely with local time at the middle longitude of the time zone. In practice, political considerations have altered the time zone boundaries somewhat. When a country straddles several time zones, it is not uncommon for the country's government to choose one of those time zones to define the country's official time. This map, originally created by the CIA and updated by several Wikimedia Commons users, shows the current definitions of the world's time zones. The IAU OAE is not the original author of this map. The designations employed and the presentation of the material on this maps do not imply the expression of any opinion whatsoever on the part of the IAU or the IAU OAE concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries.
Crédit : Wikimedia Users UnaitxuGV, Heitordp and others based on a map created by the U.S. Central Intelligence Agency (CIA) Lien vers les crédits

License: PD Domaine Public Icônes

Diagrammes associés


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

Latitude and Longitude

Légende : 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.
Crédit : Maria Cristina Fortuna/IAU OAE

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

Activités associées


Let's Map the Earth

Let's Map the Earth

astroEDU educational activity (links to astroEDU website)
Description: Discover how to read and draw maps by observing.

License: CC-BY-4.0 Creative Commons (CC) Attribution 4.0 International (CC BY 4.0) Icônes
Mots clés : Hands-on , Scales , Geography , Maps , GPS , Coordinates
Tranches d'âge : 8-10 , 10-12
Niveau scolaire : Primaire
Domaines d'apprentissage : Modélisation , Apprentissage par enquête
Coûts : Faible
Durée : 1h
Taille du groupe : Par groupe
Compétences : Analyser et interpréter des données


How To Travel on Earth Without Getting Lost

How To Travel on Earth Without Getting Lost

astroEDU educational activity (links to astroEDU website)
Description: Use a globe to describe your position on Earth.

License: CC-BY-4.0 Creative Commons (CC) Attribution 4.0 International (CC BY 4.0) Icônes
Mots clés : Geography , Maps , GPS , Celestial navigation
Tranches d'âge : 8-10 , 10-12 , 12-14
Niveau scolaire : Collège , Primaire
Domaines d'apprentissage : Apprentissage par enquête
Coûts : Faible
Durée : 1h
Taille du groupe : Par groupe
Compétences : Analyser et interpréter des données , Développer et utiliser des modèles , Utiliser les mathématiques et la pensée computationnelle