Here are the essential concepts you must grasp in order to answer the question correctly.
Escape Velocity
Escape velocity is the minimum speed an object must reach to break free from a celestial body's gravitational pull without any additional propulsion. It depends on the mass of the body and the distance from its center, calculated using the formula v = √(2GM/r), where G is the gravitational constant, M is the mass of the celestial body, and r is the radius from the center of the body.
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Gravitational Force
Gravitational force is the attractive force between two masses, described by Newton's law of universal gravitation. It states that the force is directly proportional to the product of the two masses and inversely proportional to the square of the distance between their centers. This force is what determines the escape velocity, as a stronger gravitational pull requires a higher speed to escape.
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Gravitational Forces in 2D
Independence from Mass
The escape speed is independent of the mass of the spacecraft because it is derived from the gravitational potential energy and kinetic energy principles. When calculating escape velocity, the mass of the object cancels out, meaning that all objects, regardless of their mass, require the same speed to escape a gravitational field, assuming no air resistance or other forces act on them.
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