The energy from the sun reaches just outside the earth’s atmosphere at a rate of 1400 W m–2. The distance between the sun and the earth is 1.5 × 1011 m.
(a) Calculate the rate at which the sun is losing its mass.
(b) How long will the sun last assuming a constant decay at this rate? The present mass of the sun is 2 × 1030 kg.
a)
The amount of energy radiated by the sun in ![]()
As the energy radiated is dependent on the surface area it covers which is given by ![]()
Energy loosed by the sun till it reaches earth in 1 second is given by ![]()
So, the mass loosed by the sun in 1 second is ![]()
b)
As the rate of decay of the mass is constant it will last up to ![]()
In years ![]()