The program must accept three floating point values as G (gravitational constant), M (mass) and R (radius) of a planet. The program must calculate and print the escape speed of the object with precision up to 3 decimal places.
Formula: Escape speed = squareroot(2GM/R)
Example Input/Output 1:
Input: 1.567 2.4783 3.4671
Output: 1.497
Example Input/Output 2:
Input: 1.9038 2.7920 4.3937
Output: 1.555
#include<stdio.h>
#include<stdlib.h>
int main()
{
float g, m, r;
scanf("%f %f %f", &g, &m, &r);
printf("%.3f", (sqrt((2*g*m)/r)));
}
#Adopted from GitHub-Anbu0646
