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  2. 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_rotation
    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…
    The 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…
    The Sun has a north and south pole, just as the Earth does, and rotates on its axis. However, unlike Earth which rotates at all latitudes every 24 hours, the Sun rotates every 25 days at the equator and takes progressively longer to rotate at higher latitudes, up to 35 days at the poles.
    sohowww.nascom.nasa.gov/explore/lessons/diffrot…
     
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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

    Solar rotation varies with latitude. The Sun is not a solid body, but is composed of a gaseous plasma. Different latitudes rotate at different periods. The source of this differential rotation is an area of current research in solar … See more

    At the equator, the solar rotation period is 24.47 days. This is called the sidereal rotation period, and should not be confused with the synodic rotation period of 26.24 days, which is the time for a fixed feature on the Sun to rotate to the same apparent position … 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

    Using sunspots to measure rotation image

    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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  9. Sun Fact Sheet - NSSDCA

    Find 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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    Learn about the Sun's internal structure, surface features, and rotation period through videos and scientific case. Explore the Sun's onion-like layers, thermonuclear reactions, and sunspots with CESAR Space Science Experience.

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