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}}vc=r2GM
Where:
- vcv_cvc is the critical velocity
- GGG is the gravitational constant
- MMM is the mass of the celestial body
- rrr 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 2r2r2r. Substituting this value into the formula, we have:
vc′=2GM2rv_c' = sqrt{frac{2GM}{2r}}vc′=2r2GM
Simplifying the expression, we get:
vc′=GMr=2GMrv_c' = sqrt{frac{GM}{r}} = sqrt{2} sqrt{frac{GM}{r}}v<span class="vlist-t