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- Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.The solar rotation period is 25.67 days at the equator and 33.40 days at 75 degrees of latitude.en.wikipedia.org/wiki/Solar_rotationThe Sun rotates on its axis once in about 27 days. This rotation was first detected by observing the motion of sunspots. The Sun’s rotation axis is tilted by about 7.25 degrees from the axis of the Earth’s orbit so we see more of the Sun’s north pole in September of each year and more of its south pole in March.www.nasa.gov/image-article/solar-rotation-varies-b…Moving from the sun's poles to its equator, the time in which this area of plasma rotates shortens. The poles complete a rotation in 35 days, while the area just above the equator completes a rotation in just 25 days. This means that no area of the sun completes an orbit anywhere near as rapidly as our planet does.www.space.com/does-the-sun-rotateAt the equator, the Sun spins around once about every 25 Earth days, but at its poles, the Sun rotates once on its axis every 36 Earth days.science.nasa.gov/sun/facts/On average, the sun rotates on its axis once every 27 days. However, its equator spins the fastest and takes about 24 days to rotate, while the poles take more than 30 days.www.livescience.com/32894-does-the-sun-rotate.ht…
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Solar rotation - Wikipedia
Carrington determined the solar rotation rate from low latitude sunspots in the 1850s and arrived at 25.38 days for the sidereal rotation period. Sidereal rotation is measured relative to the stars, but because the Earth is orbiting the Sun, we see this period as 27.2753 days. See more
Until the advent of helioseismology, the study of wave oscillations in the Sun, very little was known about the internal rotation of the Sun. The differential profile of the surface was thought to extend into the solar interior as rotating cylinders of constant angular … See more
The rotation constants have been measured by measuring the motion of various features ("tracers") on the solar surface. The first and most widely used tracers are See more
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WEBAt its equator, the Sun completes one rotation in 25 Earth days. At its poles, the Sun rotates once on its axis every 36 Earth days. The part of the Sun we see from Earth – the part we call the surface – is the …
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WEBLearn how to use sunspot data to calculate how long it takes for the Sun to spin once. Follow the steps to measure the distance and time of a sunspot group across the Sun's disk and compare your result with the actual value.
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WEBFind out the sidereal rotation period of the Sun, its obliquity, speed, and magnetic field strength. Compare the Sun with the Earth and other planets in various parameters.
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WEBAnd did you know that it takes .xx years for the light to travel from the center of the Sun and 8 minutes to come from the surface of the Sun to Earth. The surface of the Sun has 3 main regions: the photosphere, the …
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WEBMar 13, 2012 · The Sun rotates faster at the equator and slower at the poles, and it has different rotation rates for its interior and surface. Learn how astronomers measure the Sun's rotation period and how it …
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