How Does Planet X's Gravity Affect Rocket Escape Velocity?

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SUMMARY

The escape velocity on Planet X, which has half the radius of Earth and where an astronaut weighs twice as much, is equal to the escape velocity on Earth, denoted as v. This conclusion is derived from the relationship between gravitational potential energy and kinetic energy, specifically using the formula for escape velocity, which is influenced by the planet's radius and mass. The mathematical reasoning confirms that the escape velocity remains unchanged despite the differences in gravity and radius.

PREREQUISITES
  • Understanding of gravitational potential energy and kinetic energy concepts
  • Familiarity with the formula for escape velocity: \( v_{esc} = \sqrt{\frac{2GM}{R}} \)
  • Basic knowledge of planetary physics, including mass and radius relationships
  • Concept of gravitational acceleration and its calculation
NEXT STEPS
  • Research the derivation of escape velocity formulas for different celestial bodies
  • Explore the implications of varying gravitational forces on astronaut weight
  • Study the effects of radius and mass on gravitational potential energy
  • Examine case studies of escape velocities on other planets and moons
USEFUL FOR

Astronauts, aerospace engineers, physicists, and students studying planetary science and gravitational mechanics will benefit from this discussion.

15ongm
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1. Problem
A rocket has landed on Planet X, which has half the radius of Earth. An astronaut onboard the rocket weighs twice as much on Planet X as on Earth. If the escape velocity for the rocket taking off from Earth is v , then its escape velocity on Planet X is

a) 2 v
b) (√2)v
c) v
d) v/2
e) v/4

The answer is C.

I reasoned out this problem mathematically, but what is the conceptual reasoning behind this?
 
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15ongm said:
1. Problem
A rocket has landed on Planet X, which has half the radius of Earth. An astronaut onboard the rocket weighs twice as much on Planet X as on Earth. If the escape velocity for the rocket taking off from Earth is v , then its escape velocity on Planet X is

a) 2 v
b) (√2)v
c) v
d) v/2
e) v/4

The answer is C.

I reasoned out this problem mathematically, but what is the conceptual reasoning behind this?

I would say this is a mathematical question. To see it more clearly, you could try to derive a formula for escape velocity in terms of the radius ##R## and the surface gravity ##g## of a planet.
 
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Conceptually you are supposed to quickly approach this from the other end: ##{\tfrac 1 2}mv_{esc}^2## is the kinetic energy needed to overcome the gravitational potential energy. I expect you know how to write the latter as ##GM_{planet}\over R_{planet}##. To see how this ratio relates to idem Earth you need Mplanet/Mearth. That follows from the factor 2 in g and the expression for g PeroK is asking for
 
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