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The average density of the Sun is on the order 103 kg/ m3 . (a) Estimate the diameter of the Sun. (b) Given that the Sun subtends at an angle of about half

1 Answer

3 votes

Answer:

The diameter is
\approx
10^(11)m and
r_(sun) = 10^(9)m

Step-by-step explanation:

Given:


m_(sun) = 10^(30) kg


\\p_(sun)= 10^(3)(kg)/(m^(3))

Required:


r_(sun)=?

d= ?

We know,


{v_(sun) = (m_(sun))/(p_(sun))

=
(10^(30))/(10^(3))

=
10^(27)m^(3)


v_(sun) = (4)/(3)*\pi r^{3_(sun)}


\approx
r^(3)_(sun)


r_(sun) = 10^(9)m

From the figure attached,


sin\theta=(r_(sun))/(d)}


d=(r_(sun))/(sin\theta)}

=
(10^(9))/(sin5)}


\approx
10^(11)m

The diameter is
\approx
10^(11)m and
r_(sun) = 10^(9)m

The average density of the Sun is on the order 103 kg/ m3 . (a) Estimate the diameter-example-1
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