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Termo do glossário: Círculo Polar

Redirecionado de Dia Polar

Descrição: Os círculos polares são linhas de latitude na Terra. O círculo polar a 66°33′48,8″ N é chamado de Círculo Polar Ártico e o círculo polar a 66°33′48,8″ S é chamado de Círculo Polar Antártico. Devido ao eixo de rotação inclinado da Terra, as regiões ao norte do Círculo Ártico e ao sul do Círculo Antártico experimentam “noites polares” durante o inverno e “dias polares” durante o verão. Durante uma noite polar, o Sol permanece abaixo do horizonte por mais de 24 horas e esse período de escuridão pode durar meses. Durante um dia polar, o Sol permanece acima do horizonte por mais de 24 horas e a luz do dia pode durar meses. Os dias e as noites polares são mais longos quanto mais próximo se está dos pólos. As noites polares ocorrem antes e depois do solstício de inverno de cada região polar, enquanto os dias polares acontecendo antes e depois do solstício de verão.

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O Glossário Multilíngue da OAE é um projeto do Escritório da IAU de Astronomia para a Educação (OAE) em colaboração com o Escritório da IAU para Divulgação da Astronomia (OAO). Os termos e definições foram selecionados, escritos e revisados por meio de um esforço coletivo da OAE, dos Centros e Nós da OAE, dos Coordenadores Nacionais de Educação em Astronomia (NAECs) da OAE e de outros voluntários. Você pode encontrar uma lista completa dos créditos aqui. Todos os termos do glossário e suas definições são disponibilizados sob uma licença Creative Commons CC BY-4.0 e devem ser creditados à "IAU OAE".

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Seven images of the Sun. From the left it sinks, reaching its lowest in the centre image, before rising higher to the right.

When the Sun Bounces

Legenda: First place winner in the 2023 IAU OAE Astrophotography Contest, category of Still images of sunrise and sunset location over the year. This image was taken at Norway's North Cape. Owing to the latitude of this location, the Sun never truly sets during the summer months, from around April to August. This results in the unique spectacle of continuous daylight, known as a polar day. This captivating series of images, taken in 2022, showcases the Sun's relentless journey across the horizon every 30 minutes. At its lowest point in the sky, the Sun does not set, but appears to bounce off the horizon. The globe on the far right in the photo stands as a sentinel, marking the northernmost point of the European continental mainland.
Crédito: Milos Obert/IAU OAE (CC BY 4.0)

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


24 images of the Sun around the edge of a circular image. In the lowest image, a black circle blocks the centre of the Sun.

The Eclipse Clock-Eclipse on a Polar Day

Legenda: First place winner in the 2023 IAU OAE Astrophotography Contest, category of Still images of day arcs of the Sun and Solargraphs. Constructed by combining multiple images over the course of a 24-hour period, the image was captured in Union Glacier, Antarctica, during the total solar eclipse of 4 December 2021, and showcases the day arc of the Sun. It illustrates the unique phenomenon of a polar day, during which the Sun travels around the sky without setting. During polar days, areas within the polar circles experience 24 hours of continuous daylight, and the Sun doesn’t set for an extended period. The image also offers a rare perspective of a solar eclipse, where the Moon passes between the Sun and Earth, and as viewed from Earth. This can be seen in the lower image of the Sun, where the Moon covers the solar disc.
Crédito: Stephanie Ziyi Ye/IAU OAE (CC BY 4.0)

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

Diagramas relacionados


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

Latitude and Longitude

Legenda: 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.
Crédito: Maria Cristina Fortuna/IAU OAE

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

Atividades relacionadas


Discover Earth's climate with a balloon

Discover Earth's climate with a balloon

astroEDU educational activity (links to astroEDU website)
Description: Discover the secrets of Earth's climate zones with a hands-on experience

License: CC-BY-4.0 Creative Commons Attribution 4.0 International (CC BY 4.0) ícones
Faixas etárias: 8-10 , 10-12
Nível de ensino: Ensino fundamental , Básico
Áreas de aprendizagem: Atividade divertida , Aprendizagem por descoberta guiada , Modelagem , Baseado em observação , Aprendizagem baseada em projetos , Aprendizagem por investigação estruturada
Custos: Baixo custo
Duração: 45 mins
Tamanho do grupo: Grupo
Habilidades: Fazer perguntas , Construir explicações , Desenvolver e usar modelos