Step-by-step explanation:
We have,
Semimajor axis is
![4* 10^(12)\ m](https://img.qammunity.org/2021/formulas/physics/high-school/9yl3qqjkbz43wvqrbr5yz9kh44edwjhja4.png)
It is required to find the orbital period of a dwarf planet. Let T is time period. The relation between the time period and the semi major axis is given by Kepler's third law. Its mathematical form is given by :
![T^2=(4\pi ^2)/(GM)a^3](https://img.qammunity.org/2021/formulas/physics/high-school/2u7ouix8qqs1woi3wcbbx5s74rlm746ecd.png)
G is universal gravitational constant
M is solar mass
Plugging all the values,
![T^2=(4\pi ^2)/(6.67* 10^(-11)* 1.98* 10^(30))* (4* 10^(12))^3\\\\T=\sqrt{(4\pi^(2))/(6.67*10^(-11)*1.98*10^(30))*(4*10^(12))^(3)}\\\\T=4.37* 10^9\ s](https://img.qammunity.org/2021/formulas/physics/high-school/6r5yb7nb71l4uodtm47h6pu4ohf7zh2c25.png)
Since,
![1\ s=3.17* 10^(-8)\ \text{years}\\\\4.37* 10^9\ s=4.37\cdot10^(9)\cdot3.17\cdot10^(-8)\\\\4.37* 10^9\ s=138.52\ \text{years}](https://img.qammunity.org/2021/formulas/physics/high-school/emk17c46yp8ni1riiko47lk4djufyxl2mc.png)
So, the orbital period of a dwarf planet is 138.52 years.