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 and radius of the body, calculated using the formula v = √(2GM/R), where G is the gravitational constant, M is the mass of the body, and R is its radius.
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Gravitational Constant
The gravitational constant (G) is a fundamental physical constant that quantifies the strength of gravitational attraction between two masses. Its value is approximately 6.674 × 10^-11 N(m/kg)^2. This constant is crucial in calculating escape velocity, as it directly influences the gravitational force exerted by a planet like Jupiter.
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Jupiter's Mass and Radius
Jupiter is the largest planet in our solar system, with a mass about 318 times that of Earth and a radius approximately 11 times greater. These characteristics significantly affect its gravitational pull, resulting in a higher escape velocity compared to smaller planets. Understanding Jupiter's mass and radius is essential for accurately calculating the escape speed from its surface.
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