Solar energy is incident normally on the earth's surface at the rate of about 1.4 kW m-2 . The distance between the earth and the sun is 1.5 × 1011 m. Energy (E) and mass (m) are related by Einstein equation E=mc2 where c (3 × 10 8ms-1) is the speed of light in free space. The decrease in the mass of the sun is
(A) 109kg s-1 (B) 1030kg s-1 (C) 1026 kg s-1 (D) 1011 kg s-1