Answer:

Step-by-step explanation:
To calculate the period we need the formula:

Where
is the radius of the moon,
is the universal constant of gravitation and
is the mass of mars.
The period of Phobos:

The period of Deimos:

The ratio of the period of Phobos and Deimos:


Most terms get canceled and we have:

According to the problem

so the ratio will be:
≈

the ratio of the period of revolution of Phobos to that of Deimos is 0.2528