Final answer:
To determine the mean distance of Phobos from the center of Mars, we can use Kepler's third law of planetary motion.
Step-by-step explanation:
The mean distance of Phobos from the center of Mars can be determined using Kepler's third law of planetary motion. This law states that the square of a planet's orbital period is proportional to the cube of its mean distance from the center of its orbit.
Given that the period of Phobos is 7 hours and 39 minutes and the period of Deimos is 30 hours and 18 minutes, we can set up the following equation:
(Period of Phobos)^2 / (Mean distance of Phobos)^3 = (Period of Deimos)^2 / (Mean distance of Deimos)^3
Substituting the given values, we have:
(7.65 hours)^2 / (Mean distance of Phobos)^3 = (30.3 hours)^2 / (2.3 x 10^4 km)^3
Simplifying the equation, we can solve for the mean distance of Phobos: