The sun rotates counter clock wise, and the sunspots help with the rotation of the sun.
One clue is the movement of sunspots on the surface of the Sun. Observations over several days will show the sunspots moving with the rotation of the Sun. The rotation period of the Sun is between 25 and 34 days (depending on latitude).
No, sunspots are cooler than the photosphere.
What is true about sunspots
Sunspots are the temporary dark spots on the surface of the sun, specifically the photosphere. Sunspots can get as big as 50,000 km long. Sunspots can interrupt terrestrial magnetism.
Galileo looked at the sun and observed dark blemishes on its surface (which are now called sunspots). From the movement of these blemishes, he was able to determine that the sun has a rotation period of about one month.
By the Sun's rotation.
The sun rotates counter clock wise, and the sunspots help with the rotation of the sun.
He looked at the sun and observed dark blemishes on its surface, which are now called sunspots. From the movement of these, he was able to determine that the sun has a rotation period of about one month.
Yes.Yes.Yes.Yes.
Galileo looked at the sun and observed dark blemishes on its surface (which are now called sunspots). From the movement of these blemishes, he was able to determine that the sun has a rotation period of about one month.
this is easy ... i learned it in science class..... OK......they watched the sun and discovered that new sunspots where appearing and they also notices the same ones came back every bit. ;)
One clue is the movement of sunspots on the surface of the Sun. Observations over several days will show the sunspots moving with the rotation of the Sun. The rotation period of the Sun is between 25 and 34 days (depending on latitude).
Suspots don't actually MOVE across the face of the Sun; a sunspot pretty much stays put. So when we see sunspots APPEAR to move, what we're actually seeing is the rotation of the Sun itself.
No, sunspots are cooler than the photosphere.
Taking your question as referring to the Sun, its rotation is inferred by measuring the velocity of sunspots on the Sun's surface. Or of other features such as prominences. The Sun's equator has a velocity of about 7 000km/h. At the equator the rotation period is about 28 days. At 16o latitude, the rotation period is about 25.4 days. At the poles, the rotation period is about 34.4 days.
Yes. This is called sunspot extrapolation. For the past 400 years, scientists have been observing the sunspot populations. They have found a variety of qualitative (non-numerical) and quantitative (numerical) data and have concluded that the number of sunspots peaks and falls at a cycle of approximately 11 years.