The sun is essentially composed of the core and the surface.
he said the sun is stationry
It is day time on the part that the sun is shining on, while night on the other part. Being more precise, it is different stages of the day on the bright areas. Where the division between the light and dark parts are, it is morning or evening, and on other parts it is different stages of the day. It is the same on the dark side, being different stages of the night, from just after sunset to just before sunrise.
The warmest parts. The parts along the equator.
Because it is not really the sun that is moving.It is the earth.While the earth spins on its axis.The sun shines on different parts of the world.When our part of the earth moves away from the sun,it looks like the sun is moving but it is actually the earth spinning on its axis. If you have got any more more questions sent it to: allikerala@yahoo.co.uk
yes full sun.
The sun is essentially composed of the core and the surface.
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Within each shadow . . .The UMBRA is the region from which none of the sun is visible.The PENUMBRA is the region from which part of the sun, but not all, is visible.
the energy of the sun and the divergent parts of the wind cause each and every part of why the sun causes energy which will lead to the wind blowing
"Solar" means "related to the Sun", so any part of the Sun is "solar".
A sunspot is the coolest part of the sun that humans have discovered, but it is still very hot!
core - is the inner most part of the sun. core is also the hottest most part of the sun. corona -is the outer most part of the sun. cromosphere -is pruduces a red light.
The three main parts of the sun are the core, the convective zone, and the radiative zone.
core is the inner part of the sun flare is the darkest part f the sun and also the coldest part that people cannot survive and also sun gives light to us
Your question is unintelligible. There is no "radioactive zone" defined as part of the Sun.
The major part of our Solar System is the Sun.
the season change as the amount of energy each hemisphere receives from the sun changes