Answer: 4.6 years
Explanation:
According to Kepler’s Third Law of Planetary motion “The square of the orbital period [tex]T[/tex] of a planet is proportional to the cube of the semi-major axis [tex]a[/tex] (size) of its orbit”:
[tex]T^{2}\propto a^{3}[/tex] (1)
However, if [tex]T[/tex] is measured in Earth years, and [tex]a[/tex] is measured in astronomical units (unit equivalent to the distance between the Sun and the Earth), equation (1) becomes:
[tex]T^{2}=a^{3}[/tex] (2)
Knowing [tex]a=2.768 AU[/tex] and isolating [tex]T[/tex] from (2):
[tex]T=\sqrt{a^{3}}[/tex] (3)
[tex]T=\sqrt{(2.768 AU)^{3}}[/tex] (4)
Finally:
[tex]T=4.6 years[/tex] This is Ceres' orbital period