It converts into radiant energy
When some amount of the sun's hydrogen is converted to helium in the processof nuclear fusion, the mass winds up being slightly less than when it began. Thatsmall portion of mass has become a quantity of energy, according to E = M c2 ,and has departed from the sun in the form of electromagnetic radiation.
It is, but at twice our suns mass, Sirius A is on the limit, of being an intimidate mass star. Sirius A will have a life cycle similar to that of our own star which is a low mass star, but burns hotter. Sirius B is a companion white dwarf star with a mass of around the same as our sun. Previously, it was thought to have been a star with a mass of around 5 times that of our sun, burning out more quickly than Sirius A.
The Suns mass is 1.9891 × 1030 kg or about 333,000 times that of Earth. The Sun contains about 99% of the total mass of the Solar System.
Pollux is an orange giant star in the constellation of Gemini.It is about 8 times larger than our Sun, so about 512 Suns would fit in Pollux
What happens to Solar Energy is that some of it gets absorbed into air, land and water while the rest gets reflected back to space.
When some amount of the sun's hydrogen is converted to helium in the processof nuclear fusion, the mass winds up being slightly less than when it began. Thatsmall portion of mass has become a quantity of energy, according to E = M c2 ,and has departed from the sun in the form of electromagnetic radiation.
ur mother
The suns mass is 332,950 earths.
It goes back into space.
a big explosion occors
It is, but at twice our suns mass, Sirius A is on the limit, of being an intimidate mass star. Sirius A will have a life cycle similar to that of our own star which is a low mass star, but burns hotter. Sirius B is a companion white dwarf star with a mass of around the same as our sun. Previously, it was thought to have been a star with a mass of around 5 times that of our sun, burning out more quickly than Sirius A.
it s a nuclear process in which smaller nuclei combine to form huge nucleus. in this process some amount of mass convert into energy in the form of light and light
Yes, the sun's mass remains relatively constant over short time scales, such as seconds. The sun's mass is so massive that the amount of matter it gains or loses in a second is negligible. In the long term, the sun does lose mass through the process of nuclear fusion in its core.
cause mercury doesnt trap the suns heat into the surface. It burns in the day time but freezes at the night time. Venus traps the suns heat in its surface.
Hydrogen.
The Suns mass is 1.9891 × 1030 kg or about 333,000 times that of Earth. The Sun contains about 99% of the total mass of the Solar System.
it goes into the inner core.