Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
183_notes:examples:calcgravforce [2014/07/18 15:20] – [Example: Calculating the gravitational force exerted by the Earth on the Moon.] caballero | 183_notes:examples:calcgravforce [2018/02/09 18:33] (current) – [Solution] hallstein | ||
---|---|---|---|
Line 30: | Line 30: | ||
==== Solution ==== | ==== Solution ==== | ||
- | | + | In order to find the gravitational force we must first calculate the center to center |
| | ||
Line 39: | Line 39: | ||
- | | + | We also must find the direction of this force. The direction of the force will be in the same direction as the radius vector. We can find the direction of a vector by computing |
ˆrM−E=→rM−E|→rM−E| | ˆrM−E=→rM−E|→rM−E| | ||
Line 47: | Line 47: | ||
| | ||
- | | + | Adding both the direction of the radius and the length of the radius to the mass of the Earth and the mass of the Moon and the gravitational constant we now have all of the variables |
- | →FM−E=→FgravonMbyE | + | →FM−E=→FgravonMbyE |
- | | + | |
- | | + | |
- | | + | Results in the magnitude of the force by unit vector (direction). |
- | | + | |
+ | |||
+ | Results in the vector force, with the x,y,z components interpretable. | ||
+ | |||
+ | |