As the sun burns, it converts some of its mass into energy through nuclear fusion. This process causes a very small amount of the sun's mass to be converted into energy according to Einstein's famous equation, E=mc^2. Overall, the sun's mass is very stable over time.
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 sun's mass is approximately 1.989 x 10^30 kilograms, which is about 333,000 times the mass of Earth. This large mass creates the gravitational force that holds the solar system together.
Approximately 835,000 suns could fit inside the star Pollux, which is about nine times the mass of our sun.
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.
As the sun burns, it converts some of its mass into energy through nuclear fusion. This process causes a very small amount of the sun's mass to be converted into energy according to Einstein's famous equation, E=mc^2. Overall, the sun's mass is very stable over time.
ur mother
The suns mass is 332,950 earths.
a big explosion occors
It goes back into space.
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
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.
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.
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.