Respuesta :
Answer:
c) Less than 27.3 days.
Explanation:
According to Kepler's laws of planetary motion, a celestial body in a smaller orbit will have a shorter orbital period.
Answer:
c) Less than 27.3 days.
Explanation:
The orbital period of a celestial body is determined by its distance from the object it is orbiting. According to Kepler's laws of planetary motion, the orbital period (T) is directly proportional to the semi-major axis (a) raised to the 3/2 power.
The formula for Kepler's third law is:
[tex]\sf  T^2 \propto a^3 [/tex]
If the moon is brought into a new circular orbit with a smaller radius (a smaller semi-major axis), its orbital period (T) will decrease. Therefore, the correct answer is:
c) Less than 27.3 days.