词条 地轴
描述: 地轴是一条假想的直线,地球每天围绕它旋转一圈。地轴与地球表面相交的两个位置是地理北极(北纬 90°)和地理南极(南纬 90°)。与此相对,赤道也是一条假想线,是垂直于地轴的平面与地球表面相交的大圆,与地轴的距离最远。赤道的纬度为 0°。
地理南北极与地球磁场南北极的位置不同--磁极定义为地球表面上地磁场方向竖直向上和竖直向下的点。
地球公转轨道也有一个轴:方向与地球轨道平面垂直。地轴与轨道轴夹角 23.4°。这一夹角是地球四季变化的原因。特别是,在一个轨道周期中,北半球或南半球会向太阳倾斜,从而接收到更多的光。
相对于最遥远的天体,地轴指向的方向会随着时间的推移而缓慢变化,这就是所谓的岁差(地轴近动)。目前,地轴与天球相交的位置接近北极星。但在大约 2.6 万年的时间里,这个交点会在天空中画出一个小圆圈。以地球为参照定义的天球坐标系需要考虑到由此产生的随时间推移的微小坐标偏移。
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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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其他语言版本
- 阿拉伯语: محور الأرض
- 德语: Erdachse
- 英语: Earth's Axis
- 法语: Axe de la Terre
- 意大利语: Asse terrestre
- 繁体中文: 地軸
相关图表
Latitude and Longitude
图注: 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.
来源: Maria Cristina Fortuna/IAU OAE
相关活动
Why Do We Have Day and Night?
astroEDU educational activity (links to astroEDU website) Description: Explore day and night of Earth.
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