You will need to use your scientific calculator to check the math in the following examples. You may find, like so many students of introductory astronomy, that the hardest thing about exponents is figuring out which buttons to push on your calculator. For the calculator provided with Microsoft Windows, there is an "Exp" key. First, put in the base number (for example, in the number 6.67 ×1011, the "6.67" is the base number). Then click on the "Exp" key and enter the exponent, clicking on "+/" to make the exponent negative if needed.
The equation that we use for determining the force between the Earth and you is:
force =
where M1 is the mass of Earth in kilograms; M2, your mass in kilograms; and R, the radius of the Earth in meters. The G is the gravitational constant: 6.67 ×1011 N m2/kg2. Let's not worry too much about the units of measure, however.


If you guess "more" or "less," then predict how much more or less.
The new radius of the Earth, after shrinking, is 3.19 × 106 meters, so the new force becomes:
force == 2744 N
Let's see: 2744 divided by 686 = 4. If the Earth were to shrink to 1/2 of its current radius, you would weigh four times as much!
You may have wondered during the above examples why we always measured from the center of the Earth to the surface, in other words, used the radius of the Earth. That is because solid, spherical objects act as if all of the mass were contained right in the very center (this is not strictly true, but a good enough approximation for our use).
Let's
take look at other examples, now involving two spherical worlds. This time let's
use some values for the masses that makes our arithmetic a bit more manageable,
and get rid of those pesky exponents. Because we want to look at relative
changes, we are also going to ignore "Big G." The equation we use
here is similar to the one above, but this time we substitute D,
meaning the distance between the centers of the two worlds. The equation
is
force =
where this time the two masses, M1 and M2 represent the masses of the two worlds. The worlds are shown here all at approximately the same size, but the radii do not matter, just the distances between the centers.
Calculate the force between each of the worlds, substituting the values shown in the figure into the equation above. Do not bother with units of measure here, it's the concept we want to understand. Make sure you try each example before looking at the answers.