+5 votes
in Velocity physics by
edited by

Your answer

Your name to display (optional):
Privacy: Your email address will only be used for sending these notifications.
+1 vote
by

The critical velocity is the minimum velocity required for an object to escape the gravitational pull of a celestial body. It is given by the formula:

vc=2GMrv_c = sqrt{frac{2GM}{r}}

Where:

  • vcv_c is the critical velocity
  • GG is the gravitational constant
  • MM is the mass of the celestial body
  • rr is the distance from the center of the celestial body to the object

If the radius of the Earth is doubled, the new radius would be 2r2r. Substituting this value into the formula, we have:

vc′=2GM2rv_c' = sqrt{frac{2GM}{2r}}

Simplifying the expression, we get:

vc′=GMr=2GMrv_c' = sqrt{frac{GM}{r}} = sqrt{2} sqrt{frac{GM}{r}}

Welcome to Physicsgurus Q&A, where you can ask questions and receive answers from other members of the community.
...