Given:
The orbital period of the Ceres, T=4.60 years
To find:
The semimajor axis of the orbit of the Ceres.
Step-by-step explanation:
1 year is 3.154×10⁷ s
Thus the orbital period in seconds is given by,

From Kepler's third law, the orbital period is related to the semi-major axis as,

Where G is the gravitational constant, M is the mass of the sun, and a is the semimajor axis.
On substituting the known values,
![\begin{gathered} (1.451*10^8)^2=(4\pi^2)/(6.67*10^(-11)*2*10^(30))* a^3 \\ \Rightarrow a=\sqrt[3]{((1.451*10^8)^2*6.67*10^(-11)*2*10^(30))/(4\pi^2)} \\ =4.14^(11)\text{ m} \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/s05vef9h6rjl93jbex97v015ngboes8ykw.png)
The semimajor axis of the mars is 2.28×10¹¹ m
The semimajor axis of the Jupiter is 7.78×10¹¹ m
Thus the Ceres is in between the mars and the Jupiter.
Final answer:
The semimajor axis of the Ceres is 4.41×10¹¹ m. Thus it is between Mars and Jupiter.