<P> Solar rotation varies 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 ° ) , and to decrease as latitude increases . The solar rotation period is 24.47 days at the equator and almost 38 days at the poles . The differential rotation rate is usually described by the equation : </P>
<P> Solar rotation varies 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 ° ) , and to decrease as latitude increases . The solar rotation period is 24.47 days at the equator and almost 38 days at the poles . The differential rotation rate is usually described by the equation : </P>
what is the rotation speed of the sun
what is the rotation speed of the sun
24.47 days at the equator and almost 38 days at the poles
24.47 days at the equator and almost 38 days at the poles