Answer: 0.107
Step-by-step explanation:
We can solve this problem with Kepler's Third Law of Planetary motion:
(1)
Where:
is the orbital period of Phobos around Mars
is the Gravitational Constant
is the mass of Mars
is the semimajor axis of the orbit Phobos describes around Mars (assuming it is a circular orbit, the semimajor axis is equal to the radius of the orbit)
Well, firstly we have to convert the orbital period to seconds:
Now, we have to find
from (1):
(2)
(3)
(4) This is the mass of Mars
On the other hand, it is known the mass of the Earth is:
(5)
Then, if we want to know the ratio of Mars’s mass to the mass of the earth, we have to divide
by
:
![(M_(MARS))/(M_(EARTH))=(6.436(10)^(23) kg)/(5.972(10)^(24) kg)](https://img.qammunity.org/2021/formulas/physics/high-school/wjib03rlx23iqd1syhrm1x5d0kopse4up3.png)
Finally:
![(M_(MARS))/(M_(EARTH))=0.107](https://img.qammunity.org/2021/formulas/physics/high-school/6f7tqlzqwrxkakkpqyn70284ur2qbwy3t9.png)