Velocity of escape is equal to
A. r × √(2g); where r: radius of Earth or any other planet for that matter, g:
gravitational field strength
B. g × √(2r); where r: radius of Earth or any other planet for that matter, g:
gravitational field strength
C. √(2g) ⁄ r; where r: radius of Earth or any other planet for that matter, g:
gravitational field strength
D. √(2gr); where r: radius of Earth or any other planet for that matter, g:
gravitational field strength