Here are the essential concepts you must grasp in order to answer the question correctly.
Acceleration due to Gravity
Acceleration due to gravity is the rate at which an object accelerates towards a celestial body due to gravitational force. On Earth, this value is approximately 9.81 m/s². It varies on different celestial bodies depending on their mass and radius, affecting how quickly objects fall.
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Kinematic Equations
Kinematic equations describe the motion of objects under constant acceleration. They relate displacement, initial velocity, final velocity, acceleration, and time. In this scenario, the equation s = ut + 0.5at² can be used, where 's' is displacement, 'u' is initial velocity, 'a' is acceleration, and 't' is time.
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Free Fall
Free fall refers to the motion of an object falling solely under the influence of gravity, with no other forces acting on it, such as air resistance. In free fall, all objects accelerate at the same rate regardless of their mass, which is crucial for understanding the different fall times on Earth and Enceladus.
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