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 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.
Answers
Given : r = 1.5\times 10^{11}r=1.5×10
11
m I = 1400I=1400 Wm^{-2}Wm
−2
m_o = 2\times 10^{30}m
o
=2×10
30
kg
Power radiated by sun P = I(4\pi r^2) = 1400\times (4\pi \times (1.5\times 10^{11})^2) = 3.96\times 10^{26}P=I(4πr
2
)=1400×(4π×(1.5×10
11
)
2
) =3.96×10
26
WW
Thus rate of losing mass \dfrac{dm}{dt} = \dfrac{P}{c^2} = \dfrac{3.96\times 10^{26}}{(3\times 10^8)^2} =4.4\times 10^9
dt
dm
=
c
2
P
=
(3×10
8
)
2
3.96×10
26
=4.4×10
9
kg/skg/s
Time for which the sun would last t = \dfrac{m_o}{\dfrac{dm}{dt}} =\dfrac{2\times 10^{30}}{4.4\times 10^9} = 4.55 \times 10^{20}t=
dt
dm
m
o
=
4.4×10
9
2×10
30
=4.55×10
20
s
\implies⟹ t = \dfrac{4.55\times 10^{20}}{365\times 86400} = 1.44\times 10^{13}t=
365×86400
4.55×10
20
=1.44×10
13
years
Explanation:
Given:
From the sun, the energy’s intensity,
Distance between Earth and the Sun,
In time t, the emitted energy, E = Pt
Sun has the mass that is used up to form this quantity of energy. So,
the loss in sun’s mass,
=
So, at the rate of , the sun is losing its weight.
(b) In 1 second, there is a loss.
So, in disintegrates