Our sun converts 600 million tons of H to He every second, that is 5 million tons of matter into energy through nuclear fission. However, as the core of the sun continues to shrink the outer layers of the sun move closer and experience a stronger gravitational force. This causes more pressure on the core, which is resulted by increases in the rate at which fusion occurs. Hence the rate at which our sun losses its mass is not continuous. I want to know the mass of our sun when the core is depleted of hydrogen about 5 billion years from now. I also want to know its composition, at present 73% of our sun's mass is Hydrogen and 25% is He.

Our sun converts 600 million tons of H to He every second, that is 5 million tons of matter into energy through nuclear fission. However, as the core of the sun continues to shrink the outer layers of the sun move closer and experience a stronger gravitational force. This causes more pressure on the core, which is resulted by increases in the rate at which fusion occurs. Hence the rate at which our sun losses its mass is not continuous. I want to know the mass of our sun when the core is depleted of hydrogen about 5 billion years from now (Mass loss as a result of nuclear fusion only an not due to stellar wind). I also want to know its composition, at present 73% of our sun's mass is Hydrogen and 25% is He.

Our sun converts 600 million tons of H to He every second, that is 5 million tons of matter into energy through nuclear fission. However as the core of the sun continues to shrink the outer layers of the sun move closer and experience a stronger gravitational force. This causess more pressure on the core, which is resulted by increases in the rate at which fusion occurs. Hence the rate at which our sun losses its mass is not continuous. I want to know the mass of our sun when its on the last stage as a red giant before it dies to form a ring nebula. I also want to know its composition, at present 73% our sun mass is Hydrogen and 25% is He.

Our sun converts 600 million tons of H to He every second, that is 5 million tons of matter into energy through nuclear fission. However, as the core of the sun continues to shrink the outer layers of the sun move closer and experience a stronger gravitational force. This causes more pressure on the core, which is resulted by increases in the rate at which fusion occurs. Hence the rate at which our sun losses its mass is not continuous. I want to know the mass of our sun when the core is depleted of hydrogen about 5 billion years from now. I also want to know its composition, at present 73% of our sun's mass is Hydrogen and 25% is He.