Law of Universal Gravitation
Author: shiroeExecutions: 1450
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Enter the gravitational constant G.
Enter the mass M (in m).
Enter the distance r.
Enter the exponent n for r^2.
Enter a non-zero positive real number for r.
Enter a non-negative real number for n.
The program outputs the magnitude of the force f.
The result is multiplied by -1 to indicate that it is a gravitational force.
Enter the mass M (in m).
Enter the distance r.
Enter the exponent n for r^2.
Enter a non-zero positive real number for r.
Enter a non-negative real number for n.
The program outputs the magnitude of the force f.
The result is multiplied by -1 to indicate that it is a gravitational force.
| f | N (Multiplied by -1) |
Considering the inverse of 2.03 rather than the inverse of the square involves handling deviations from elliptical orbits when dealing with perihelion shifts and perturbations.
In such cases, celestial-scale masses are involved.
Display setting: 50 digits. Digit count can be changed. Complex number calculation mode.
In such cases, celestial-scale masses are involved.
Display setting: 50 digits. Digit count can be changed. Complex number calculation mode.
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Calculates the magnitude of the force f
based on the gravitational constant G, mass M, mass m, and distance r.
Note that -1 is multiplied here to indicate that this is a gravitational force.