The rotation rate at the equator of the Sun is approximately 25 days, meaning that it takes about 25 days for the Sun to complete one full rotation at its equator.
The rotation rate of the Sun varies with latitude; at the equator, it rotates approximately once every 25 days. In contrast, at the poles, the rotation period can take about 35 days. This differential rotation is due to the Sun's gaseous nature, allowing different latitudinal bands to rotate at different speeds.
The average rotation period of the Sun on its axis is about 25 days at its equator. However, it rotates more quickly at its equator than at its poles.
The starting point of the sun's rotation is typically considered to be the equator of the sun. The sun rotates on its axis, which passes through its equator, completing a full rotation approximately once every 27 days.
No, the Sun's equator rotates faster than its poles. This is known as differential rotation, where different latitudes rotate at different speeds. The equator takes around 25 days to complete one rotation, while the poles take around 35 days.
The Sun rotates faster at the equator. Not only in km/hour, but also in angular speed. From Wikipedia: "The period of this actual rotation is approximately 25.6 days at the equator and 33.5 days at the poles." Note that the Sun is not a rigid body like the Earth. The differential rotation is believed to be caused by a combination of convection currents and Coriolis effects.
The rotation rate of the Sun varies with latitude; at the equator, it rotates approximately once every 25 days. In contrast, at the poles, the rotation period can take about 35 days. This differential rotation is due to the Sun's gaseous nature, allowing different latitudinal bands to rotate at different speeds.
The average rotation period of the Sun on its axis is about 25 days at its equator. However, it rotates more quickly at its equator than at its poles.
The starting point of the sun's rotation is typically considered to be the equator of the sun. The sun rotates on its axis, which passes through its equator, completing a full rotation approximately once every 27 days.
According to the relevant Wiki...Solar rotation is able to vary with latitude because the Sun is composed of a gaseous plasma. The rate of rotation is observed to be fastest at the equator (latitude φ=0 deg), and to decrease as latitude increases.Also according to the Wiki...rotation period(at equator)25.05 days(at 16° latitude)25.38 days25d 9h 7min 12s (at poles)34.4 days Rotation velocity(at equator)7.189×103km/h
No, the Sun's equator rotates faster than its poles. This is known as differential rotation, where different latitudes rotate at different speeds. The equator takes around 25 days to complete one rotation, while the poles take around 35 days.
The Sun rotates faster at the equator. Not only in km/hour, but also in angular speed. From Wikipedia: "The period of this actual rotation is approximately 25.6 days at the equator and 33.5 days at the poles." Note that the Sun is not a rigid body like the Earth. The differential rotation is believed to be caused by a combination of convection currents and Coriolis effects.
The equator of the sun spins faster than its poles. This is known as differential rotation, where the sun's rotation speed varies with latitude. At the equator, the sun completes a full rotation about once every 24 days, while at the poles it takes around 35 days.
rotation is the spiinning of the planet on its axis and revoulution is the orbiting of the planet around the sun
rotation is the spiinning of the planet on its axis and revoulution is the orbiting of the planet around the sun
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The sun has two types of period of rotation, the sidereal rotation period and the synodic rotation period. The sidereal rotation period is 24.47 days. The synodic rotation period is 26.24 days.
The Sun rotates on its axis at varying rates due to its gaseous composition. At the equator, it completes a rotation approximately every 25 days, while at higher latitudes, it takes about 35 days to rotate once. This differential rotation is a result of the Sun's complex magnetic and fluid dynamics.