Answer:
Part a)
[tex]M = 2.31 \times 10^{30} kg[/tex]
Part b)
[tex]M = 1.15 M_s[/tex]
Explanation:
Part a)
As we know that the period of revolution of the planet is given by
[tex]T = 2\pi\sqrt{\frac{r^3}{GM}}[/tex]
now we know that
[tex]r = 10.5 \times 10^6 km = 1.05 \times 10^{10} m[/tex]
T = 6.3 days
[tex]T = 5.44 \times 10^5 s[/tex]
now we have
[tex]5.44 \times 10^5 = 2\pi\sqrt{\frac{(1.05\times 10^{10})^3}{(6.67 \times 10^{-11})M}}[/tex]
[tex]M = 2.31 \times 10^{30} kg[/tex]
Part b)
As we know that mass of sun is given as
[tex]M_s = 2.0 \times 10^{30} kg[/tex]
now we have
[tex]\frac{M}{M_s} = \frac{2.31 \times 10^{30}}{2 \times 10^{30}}[/tex]
[tex]M = 1.15 M_s[/tex]