Gravity
History of gravity
Gravitational force
Sir Isaac Newton(source: Wikipedia) |
The gravitational force refers to the force of attraction between two planets or astronomical bodies. The scientists were before Newton observed that planets were moving faster when they came close to the Sun and were moving slower when they were far from the Sun. But, they couldn’t explain the reason behind it. What type of force was acting on that phenomenon. Newton explained that the force acting between them is a gravitational force. It depends on the distance between them. He gave the following formula to calculate
that force.
Where F = Gravitational force,
G =
Gravitational Constant,
m1 =
Mass of the first object,
m2 =
Mass of the second Object
r =
Distance between them.
The Gravitational Force |
This solve the unanswered question that
how the force acting between object in the universe. Also, why planet moves
around the sun in elliptical locus.
Acceleration due to gravity (g)
Newton’s first law states that an
object will continue its state of motion until some external force applied on
it. It means that the velocity of any object will change if we apply external
force to it. From this, we can say that the gravitational force also causes a
change in the velocity of an object. In physics, the change in velocity
indicates acceleration. Thus, the acceleration related to gravitational force
is known as acceleration due to gravity or simply g. The value of g depends on
two factors mass of the planet or body and the radius of the planet or body.
Where G = Gravitational constant
M = Mass of the planet
R = Radius
of the planet
Value of acceleration due to gravity at different height form earth(source: Wikipedia) |
Einstein's general relativity
Newton illustrates that gravity works as a pulling force towards the center. After that, for a long time, gravity was assumed only as a force. Later Einstein found that gravity does not only work as a force. A new concept of curve space come into focus after Einstein proposed the general theory of relativity in 1915. Einstein reveals that matter curves the space around it due to the effect of its gravity. The evidence of the general theory of relativity had observed by a team led by an English Astronomer Eddington in 1919.
Solar eclipse in 1919(source: Wikipedia) |
They studied the sky during the total solar eclipse. They observed that the star near the sun had appeared at a different position than expected to be in that position calculated by studying those stars at night. This experiment indicates that the sun bends the light coming from those stars due to its gravity. But, light always moves in the shortest distance between two points. If space is flat, the light will move in a straight line. In this case, light moves in a curve line that is only possible when space has curved. This experiment concludes that gravity curves space. In the solar system, mercury moves in a different type of orbit than other planets. Its orbit continuously changes its position that is it had precession of the perihelion. This type of motion of mercury wasn't able to describe by Newton's gravitational formula.
Motion of the Mercury around the Sun |
Good Work dude.
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