apparent precession

简明释义

视进动陀螺仪轴由于地球自转的)视进动

英英释义

Apparent precession refers to the observed change in the orientation of the rotational axis of an astronomical body, as seen from a particular point of view, often due to the influence of external gravitational forces.

表观进动是指从特定观察点看,天体的旋转轴方向的观察变化,通常是由于外部引力的影响。

例句

1.The study of celestial mechanics often involves understanding the concept of apparent precession, which refers to the perceived change in the orientation of an astronomical object over time.

天体力学的研究通常涉及理解表观进动的概念,即天文物体随时间变化的方向感知变化。

2.The apparent precession observed in the orbits of planets provides insights into gravitational interactions.

行星轨道中观察到的表观进动提供了对引力相互作用的洞察。

3.The apparent precession of the equinoxes is a critical factor in determining the timing of seasonal changes.

春分的表观进动是确定季节变化时机的重要因素。

4.In physics, the apparent precession of a spinning gyroscope can be explained using classical mechanics.

在物理学中,旋转陀螺的表观进动可以通过经典力学进行解释。

5.Astronomers observed the apparent precession of the Earth's axis, leading to changes in the position of stars in the night sky.

天文学家观察到地球轴线的表观进动,导致夜空中星星位置的变化。

作文

The concept of apparent precession refers to the observed change in the orientation of the rotational axis of a celestial body, such as Earth, due to gravitational forces exerted by other bodies. This phenomenon is particularly significant in understanding the long-term movements and stability of planetary systems. The term 'precession' itself originates from Latin, meaning 'to go before.' In the context of astronomy, it specifically describes how the axis of rotation slowly shifts over time, creating a gradual change in the positions of stars and constellations as seen from Earth.To elaborate further, let us consider the example of Earth’s axial precession. The Earth's axis is tilted at an angle of approximately 23.5 degrees relative to its orbital plane around the Sun. Due to the gravitational pull of the Moon and the Sun, the axis experiences a slow, circular motion that takes about 26,000 years to complete one full cycle. This movement results in the apparent precession of the equinoxes, where the position of the equinoxes shifts westward along the ecliptic plane. As a result, the timing of the seasons gradually changes over millennia, impacting various aspects of life on Earth, including agriculture and climate.The implications of apparent precession extend beyond mere astronomical observation. Ancient civilizations, such as the Egyptians and the Mayans, were keenly aware of the cycles of the stars and their effects on agricultural practices. They developed calendars based on celestial phenomena, which were influenced by the slow changes brought about by precession. For instance, the alignment of the pyramids in Egypt with certain stars can be traced back to specific points in time when those stars would have been in particular positions due to apparent precession.In modern times, the study of apparent precession has led to advancements in navigation and astronomy. Understanding the precessional motion of celestial bodies allows astronomers to create more accurate models of the universe, predict the positions of stars, and even explore the potential for exoplanetary systems. The knowledge gained from this phenomenon is crucial for space exploration, as it helps scientists navigate spacecraft through our solar system and beyond.Moreover, apparent precession is not limited to Earth alone. Other planets in our solar system also exhibit similar precessional behavior. For example, Mars has its own axial tilt and experiences precession, albeit at a different rate than Earth. Studying these differences provides insights into the dynamics of planetary formation and evolution.In conclusion, the phenomenon of apparent precession is a fascinating aspect of celestial mechanics that has profound implications for astronomy, navigation, and our understanding of the universe. By recognizing the significance of this concept, we can appreciate the intricate dance of celestial bodies and their influence on our planet. As we continue to explore the cosmos, the study of apparent precession will undoubtedly remain a vital component in unraveling the mysteries of the universe.

“表观进动”这一概念是指由于其他天体施加的引力作用,观察到的天体(如地球)旋转轴的方向变化。这一现象在理解行星系统的长期运动和稳定性方面尤为重要。“进动”一词源于拉丁语,意为“在前走”。在天文学的背景下,它特指旋转轴如何随时间缓慢移动,从而导致从地球上看星星和星座位置的逐渐变化。进一步阐述,让我们考虑地球轴向进动的例子。地球的轴相对于其围绕太阳的轨道平面倾斜约23.5度。由于月球和太阳的引力作用,地轴经历一种缓慢的圆形运动,完成一个完整周期大约需要26000年。这种运动导致了春分点的表观进动,即春分点沿黄道平面向西移动。因此,季节的时间安排在千年间逐渐变化,影响地球上生活的各个方面,包括农业和气候。“表观进动”的影响不仅限于天文观察。古代文明,如埃及人和玛雅人,敏锐地意识到星星的周期及其对农业实践的影响。他们根据天体现象制定了日历,而这些现象受到了表观进动带来的缓慢变化的影响。例如,埃及金字塔与某些星星的对齐可以追溯到那些星星在特定位置时的特定时间,这些位置是由于表观进动造成的。在现代,研究表观进动促进了导航和天文学的发展。理解天体的进动运动使天文学家能够创建更准确的宇宙模型,预测星星的位置,甚至探索外星行星系统。从这一现象中获得的知识对太空探索至关重要,因为它帮助科学家在我们的太阳系及更远的地方导航航天器。此外,表观进动并不局限于地球。我们太阳系中的其他行星也表现出类似的进动行为。例如,火星具有自己的轴倾斜,并经历进动,尽管其速率与地球不同。研究这些差异提供了关于行星形成和演化动态的见解。总之,表观进动现象是天体力学的一个迷人方面,对天文学、导航以及我们对宇宙的理解具有深远的影响。通过认识到这一概念的重要性,我们可以欣赏天体的复杂舞蹈及其对我们星球的影响。随着我们继续探索宇宙,表观进动的研究无疑将继续成为揭开宇宙奥秘的重要组成部分。

相关单词

precession

precession详解:怎么读、什么意思、用法