Answer:
Part a)
[tex]M = 7.25 \times 10^{25} kg[/tex]
Part b)
[tex]M = 2\times 10^{30} kg[/tex]
Explanation:
Part a)
As we know that the diameter of the planet is given as
[tex]d = 1.8 \times 10^7 m[/tex]
now the radius of the planet is given as
[tex]r = 9 \times 10^6 m[/tex]
now we know that the acceleration due to gravity of the planet is given by the equation
[tex]g = \frac{GM}{r^2}[/tex]
here we know that
[tex]g = 59.7 m/s^2[/tex]
now from above equation we have
[tex]59.7 = \frac{(6.67 \times 10^{-11})M}{(9\times 10^6)^2}[/tex]
now we have
[tex]M = 7.25 \times 10^{25} kg[/tex]
Part b)
Now by kepler's law we know that
time period of revolution of planet about the star is given as
[tex]T = 2\pi \sqrt{\frac{r^3}{GM}}[/tex]
so we have
[tex]\frac{T_1^2}{T_2^2} = \frac{r_1^3}{r_2^3}[/tex]
now we have
[tex]\frac{1^2}{402^2} = \frac{(1.5 \times 10^11)^3}{r^3}}[/tex]
[tex]rr = 8.17 \times 10^{12} m[/tex]
mula of time period
[tex]402\times (365\times 24 \times 3600) = 2\pi \sqrt{\frac{(8.17\times 10^12)^3}{(6.67\times 10^{-11})M}}[/tex]
Now we have
[tex]M = 2\times 10^{30} kg[/tex]