https://wikimd.org/index.php?action=history&feed=atom&title=Axial_tiltAxial tilt - Revision history2026-04-25T02:44:31ZRevision history for this page on the wikiMediaWiki 1.44.2https://wikimd.org/index.php?title=Axial_tilt&diff=5603227&oldid=prevPrab: CSV import2024-04-14T21:35:54Z<p>CSV import</p>
<p><b>New page</b></p><div>[[Image:Planet_axis_comparison.png|left|thumb]] [[File:Earth_tilt_animation.gif|left|thumb]] [[File:axial_tilt_vs_tropical_and_polar_circles.svg|left|thumb]] [[File:Obliquity_of_the_ecliptic_laskar.PNG|thumb]] '''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 is a fundamental parameter that influences the [[seasons]] and climate of a planet because it affects the amount of sunlight different parts of the planet receive throughout its year.<br />
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==Overview==<br />
The Earth's axial tilt is currently about 23.44 degrees from the plane of its orbit around the [[Sun]]. This tilt varies between 22.1 and 24.5 degrees over a cycle of approximately 41,000 years due to gravitational interactions with other bodies in the solar system, primarily the [[Moon]] and [[Jupiter]]. The variation in Earth's axial tilt is a significant factor in the complex changes in climate over millennia, including the advance and retreat of ice ages.<br />
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==Effects on Seasons==<br />
The axial tilt of a planet plays a crucial role in the development of seasons. For a planet with a significant tilt, such as Earth, different latitudes receive varying amounts of sunlight at different times of the year. During the planet's orbit, the hemisphere tilted towards the Sun experiences summer, as it receives more direct sunlight, while the opposite hemisphere experiences winter. The equinoxes, when day and night are of approximately equal length, occur when the planet's axis is not tilted towards or away from the Sun.<br />
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==Comparison with Other Planets==<br />
Other planets in the [[Solar System]] have axial tilts that significantly affect their climates and seasons. For example, [[Uranus]] has an axial tilt of about 97.77 degrees, which means it essentially orbits the Sun on its side. This extreme tilt results in extreme seasonal variations, with each pole getting 42 years of continuous sunlight followed by 42 years of darkness.<br />
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[[Mars]] has an axial tilt similar to Earth's, about 25.19 degrees, which gives it seasons somewhat analogous to Earth's, though they are nearly twice as long due to Mars's longer orbital period around the Sun.<br />
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==Cultural and Scientific Significance==<br />
The concept of axial tilt and its effects on seasons has been understood to varying degrees since ancient times. Ancient civilizations built monuments that aligned with the Sun at solstices and equinoxes, indicating an early understanding of the changing seasons and their relationship to the Sun's position in the sky.<br />
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In modern times, the study of axial tilt and its variations is crucial in the fields of [[astronomy]], [[climate science]], and [[planetary science]]. Understanding how axial tilt affects climate and seasons on Earth and other planets provides insights into planetary habitability, climate change, and the dynamics of planetary systems.<br />
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==See Also==<br />
* [[Season]]<br />
* [[Solstice]]<br />
* [[Equinox]]<br />
* [[Climate change]]<br />
* [[Orbital mechanics]]<br />
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[[Category:Astronomy]]<br />
[[Category:Climatology]]<br />
[[Category:Planetary science]]<br />
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