Also known as axial tilt or obliquity.
也被称为转轴倾角(axial tilt)或倾角(obliquity)。
单词 | Axial tilt |
释义 |
Axial tilt
原声例句
听力文摘 Also known as axial tilt or obliquity. 也被称为转轴倾角(axial tilt)或倾角(obliquity)。 双语版 TED-Ed 演讲精选 This is known as the Earth's axial tilt, or obliquity. 这也被称作“轴倾角”。 双语版 TED-Ed 演讲精选 And that axial tilt of the Earth is one of the main reasons for the seasons. 倾斜的地轴是造成四季的主要原因之一。 传说之境 However, perhaps the most catastrophic effect that would happen without a moon would be the extreme change in Earth's axial tilt. 然而,在没有月球的情况下,最具灾难性的影响可能是地球轴心倾角的极端变化。 宇宙奥秘 A full-fledged satellite maintains the stability of the Earth's axial tilt, but a significantly lighter moon would not be able to accomplish this task. 一个饱满的卫星可以保持地球轴向倾斜的稳定性,但一个明显较轻的月球将无法完成这一任务。 iBT新托福突破口 The second movement involved in the hypothesis has to do with axial tilt. 假设中涉及的第二个运动与轴向倾斜有关。 PBS太空科学 Mercury doesn't have much of an axial tilt or much of an atmosphere, so no seasons for you either. 水星没有太多的轴向倾斜或太多的大气层,所以你也没有季节。 2023-39 That represents Earth's axial tilt, which astronomers call its obliquity, relative to the plane of its nearly circular orbit around the sun. 这代表地球相对于其围绕太阳的近圆形轨道平面的轴倾斜,天文学家称之为倾斜角。 宇宙百科学 To figure out which idea is most likely, we have to know more about Venus's early dynamics, specifically its rotation rate and axial tilt. 为了找出最有可能的想法,我们必须更多地了解金星的早期动力学,特别是它的自转速率和轴向倾斜。 TED-Ed(视频版) So the Earth's axial tilt partially explains why the Sun changes positions in the sky and the analemma's length represents the full 46.8 degrees of the sun's declination throughout the year. 所以地球的自转轴的倾斜能够部分解释太阳在天空中位置变化的原因,地球仪的8字曲线的长度也代表了太阳在一整年倾斜的46.8°的角度。
中文百科
转轴倾角![]() ![]() ![]() ![]() 转轴倾角是行星的自转轴相对于轨道平面的倾斜角度,也称为倾角(obliquity)或轴交角(axial inclination),在天文学,是以自转轴与穿过行星的中心点并垂直于轨道平面的直线之间所夹的角度来表示与度量。
英语百科
Axial tilt 转轴倾角![]() ![]() ![]() ![]() In astronomy, axial tilt, also known as obliquity, is the angle between an object's rotational axis and its orbital axis, or, equivalently, the angle between its equatorial plane and orbital plane. It differs from orbital inclination. At an obliquity of zero, the two axes point in the same direction; i.e., the rotational axis is perpendicular to the orbital plane. Over the course of an orbit, the obliquity usually does not change considerably, and the orientation of the axis remains the same relative to the background stars. This causes one pole to be directed more toward the Sun on one side of the orbit, and the other pole on the other side — the cause of the seasons on the Earth. Earth's obliquity oscillates between 22.1 and 24.5 degrees on a 41,000-year cycle. It is currently 23.4 degrees and decreasing. |
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