A geodesic, or the shortest or longest path between
two nearby points, was first suggested by Einstein in his Theory of
General Relativity. Einstein proposed that gravity was not a separate
force by itself, but the result of the warping of space-time by the
mass and energy of a body. This complicated explanation can be seen
in this simple example: Put a heavy ball in the center of a trampoline.
Notice the curvatures that are created by the ball. Now, a planet
orbits the sun because it follows the curvatures that are created
by the star. So now send a smaller ball into the curvatures of the
trampoline. Notice how the ball begins to rotate around the larger
ball. On Earth the smaller ball will eventually stop because of frictions
and because it is attracted toward the center by the Earth's Gravity.
Yet, in space, these conditions are not present, so the planets in
our solar system will always orbit the sun, following its curvatures.
Yet this theory of gravity was not always present. Before Einstein's
theory of General Relativity, scientists and physicists were following
Newton's theories and Newton's form of gravity. What his theory basically
stated was that each object exerts some sort of a pull. This object
can be as large as the earth or the sun or anything else, or as small
as an apple and even smaller. This ability of any object to exert
a pull is shown in this example:
When an apple falls off of a tree, it is influenced by the pull of
the earth, which is very strong. But the apple itself exerts a pull
that attracts the Earth to it. The reason Newton said the Earth did
not jump up to the apple was because the apple exerted such a small
pull on the earth that it was hardly measurable.
Einstein's theory basically states that objects just
follow a natural course, but orbit, for example like planets, because
they naturally follow the curvatures their respective star creates.
This theory has been proven by the comparison of the positions of
stars at night, and during a solar eclipse. If the curving of space-time
really existed, then the position of the star measured during the
solar eclipse should be different than the position at night because
the light would follow the natural curves and bend towards a certain
direction. This assumption proved to be true and the geodesic theory
of gravity began to be seriously accepted by most physicists.
There are two aspects that should be pointed out in the Theory of
Relativity. The first is that there are, in actuality, two theories,
the general theory and the special theory of relativity. The second
aspect is the explanation of both of them. Another main idea in the
General Theory of Relativity, other than gravity, is that as a person
accelerates and begins to approach the speed of light, a significant
slowing down of the aging process will occur. This means that say
an astronaut leaves the earth in a rocket ship traveling at close
to the speed of light, he will age more slowly than the people on
Earth will. So for example in ten years for the humans on Earth, the
astronaut may return only one year older. The Special Theory explains
that this aspect may change depending on the observer. In other words,
while the astronaut is leaving Earth at close to the speed of light,
the Earth and its people are heading away from him at close to the
speed of light as well. So in his view, the humans may get older more
slowly than he does because he is the observer. For the humans on
Earth, this is vice versa. However, for now there is no way to accurately
verify this theory and it still provides as many perplexing questions
as it has solved.