what is gravitation tell about its types?
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Gravitation:
Every object in the universe attracts every other object with a force which is called the force of gravitation.
Gravitation is one of the four classes of interactions found in nature.
These are
(i) the gravitational force
(ii) the electromagnetic force
(iii) the strong nuclear force (also called the hadronic force).
(iv) the weak nuclear forces.
Although, of negligible importance in the interactions of elementary particles, gravity is of primary importance in the interactions of objects. It is gravity that holds the universe together.
Newton’s Law of Gravitation
Gravitational force is a attractive force between two masses m1and m2 separated by a distance r.
The gravitational force acting between two point objects is proportional to the product of their masses and inversely proportional to the square of the distance between them.
Gravitational force.
where G is universal gravitational constant.
The value of G is 6.67 X 10-11Nm2 kg-2 and is same throughout the universe.
The value of G is independent of the nature and size of the bodies well as the nature of the medium between them.
Dimensional formula of G is [M-1L3T-2].
Important Points about Gravitation Force
(i) Gravitational force is a central as well as conservative force.
(ii) It is the weakest force in nature.
(iii) It is 1036 times smaller than electrostatic force and 10’l8 times smaller than nuclear force.
(iv) The law of gravitational is applicable for all bodies, irrespective of their size, shape and position.
(v) Gravitational force acting between sun and planet provide it centripetal force for orbital motion.
(vi) Gravitational pull of the earth is called gravity.
(vii) Newton’s third law of motion holds good for the force of gravitation. It means the gravitation forces between two bodies are action-reaction pairs.
Following three points are important regarding the gravitational force
(i) Unlike the electrostatic force, it is independent of the medium between the particles.
(ii) It is conservative in nature.
(iii) It expresses the force between two point masses (of negligible volume). However, for external points of spherical bodies the whole mass can be assumed to be concentrated at its centre of mass.
Note Newton’s law of gravitation holds goods for object lying at very large distances and also at very short distances. It fails when the distance between the objects is less than 10-9 m i.e., of the order of intermolecular distances.
Acceleration Due to Gravity
The uniform acceleration produced in a freely falling object due to the gravitational pull of the earth is known as acceleration due to gravity.
It is denoted by g and its unit is m/s2. It is a vector quantity and its direction is towards the centre of the earth.
The value of g is independent of the mass of the object which is falling freely under gravity.
The value of g changes slightly from place to place. The value of g is taken to be 9.8 m/s2 for all practical purposes.
The value of acceleration due to gravity on the moon is about. one sixth of that On the earth and on the sun is about 27 times of that on the earth.
Among the planets, the acceleration due to gravity is minimum on the mercury.
Relation between g and a is given by
g = Gm / R2
where M = mass of the earth = 6.0 * 1024 kg and R = radius of the earth = 6.38 * 106 m.
Acceleration due to gravity at a height h above the surface of the earth is given by
gh = Gm / (R+h)2 = g (1 – 2h / R)
Factors Affecting Acceleration Due to Gravity
(i) Shape of Earth Acceleration due to gravity g &infi; 1 / R2 Earth is elliptical in shape. Its diameter at poles is approximately 42 km less than its diameter at equator.
Therefore, g is minimum at equator and maximum at poles.
(ii) Rotation of Earth about Its Own Axis If ω is the angular velocity of rotation of earth about its own axis, then acceleration due to gravity at a place having latitude λ is given by
g’ = g – Rω2 cos2 λ
At poles λ = 90° and g’ = g
Therefore, there is no effect of rotation of earth about its own axis at poles.
At equator λ = 0° and g’ = g – Rω2
The value of g is minimum at equator
If earth stapes its rotation about its own axis, then g will remain unchanged at poles but increases by Rω2 at equator.
(iii) Effect of Altitude The value of g at height h from earth’s surface
g’ = g / (1 + h / R)2
Therefore g decreases with altitude.
(iv) Effect of Depth The value of gat depth h A from earth’s surface
g’ = g * (1 – h / R)
Therefore g decreases with depth from earth’s surface.
The value of g becomes zero at earth’s centre.
Every object in the universe attracts every other object with a force which is called the force of gravitation.
Gravitation is one of the four classes of interactions found in nature.
These are
(i) the gravitational force
(ii) the electromagnetic force
(iii) the strong nuclear force (also called the hadronic force).
(iv) the weak nuclear forces.
Although, of negligible importance in the interactions of elementary particles, gravity is of primary importance in the interactions of objects. It is gravity that holds the universe together.
Newton’s Law of Gravitation
Gravitational force is a attractive force between two masses m1and m2 separated by a distance r.
The gravitational force acting between two point objects is proportional to the product of their masses and inversely proportional to the square of the distance between them.
Gravitational force.
where G is universal gravitational constant.
The value of G is 6.67 X 10-11Nm2 kg-2 and is same throughout the universe.
The value of G is independent of the nature and size of the bodies well as the nature of the medium between them.
Dimensional formula of G is [M-1L3T-2].
Important Points about Gravitation Force
(i) Gravitational force is a central as well as conservative force.
(ii) It is the weakest force in nature.
(iii) It is 1036 times smaller than electrostatic force and 10’l8 times smaller than nuclear force.
(iv) The law of gravitational is applicable for all bodies, irrespective of their size, shape and position.
(v) Gravitational force acting between sun and planet provide it centripetal force for orbital motion.
(vi) Gravitational pull of the earth is called gravity.
(vii) Newton’s third law of motion holds good for the force of gravitation. It means the gravitation forces between two bodies are action-reaction pairs.
Following three points are important regarding the gravitational force
(i) Unlike the electrostatic force, it is independent of the medium between the particles.
(ii) It is conservative in nature.
(iii) It expresses the force between two point masses (of negligible volume). However, for external points of spherical bodies the whole mass can be assumed to be concentrated at its centre of mass.
Note Newton’s law of gravitation holds goods for object lying at very large distances and also at very short distances. It fails when the distance between the objects is less than 10-9 m i.e., of the order of intermolecular distances.
Acceleration Due to Gravity
The uniform acceleration produced in a freely falling object due to the gravitational pull of the earth is known as acceleration due to gravity.
It is denoted by g and its unit is m/s2. It is a vector quantity and its direction is towards the centre of the earth.
The value of g is independent of the mass of the object which is falling freely under gravity.
The value of g changes slightly from place to place. The value of g is taken to be 9.8 m/s2 for all practical purposes.
The value of acceleration due to gravity on the moon is about. one sixth of that On the earth and on the sun is about 27 times of that on the earth.
Among the planets, the acceleration due to gravity is minimum on the mercury.
Relation between g and a is given by
g = Gm / R2
where M = mass of the earth = 6.0 * 1024 kg and R = radius of the earth = 6.38 * 106 m.
Acceleration due to gravity at a height h above the surface of the earth is given by
gh = Gm / (R+h)2 = g (1 – 2h / R)
Factors Affecting Acceleration Due to Gravity
(i) Shape of Earth Acceleration due to gravity g &infi; 1 / R2 Earth is elliptical in shape. Its diameter at poles is approximately 42 km less than its diameter at equator.
Therefore, g is minimum at equator and maximum at poles.
(ii) Rotation of Earth about Its Own Axis If ω is the angular velocity of rotation of earth about its own axis, then acceleration due to gravity at a place having latitude λ is given by
g’ = g – Rω2 cos2 λ
At poles λ = 90° and g’ = g
Therefore, there is no effect of rotation of earth about its own axis at poles.
At equator λ = 0° and g’ = g – Rω2
The value of g is minimum at equator
If earth stapes its rotation about its own axis, then g will remain unchanged at poles but increases by Rω2 at equator.
(iii) Effect of Altitude The value of g at height h from earth’s surface
g’ = g / (1 + h / R)2
Therefore g decreases with altitude.
(iv) Effect of Depth The value of gat depth h A from earth’s surface
g’ = g * (1 – h / R)
Therefore g decreases with depth from earth’s surface.
The value of g becomes zero at earth’s centre.
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