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Plan 0f talk
• Gravitation
• Isaac Newton
• The universal law of gravitation
• Newton’s First law
• Newton’s second law
• Newton’s third law
• Weight and Gravitational Potential Energy
• Escape velocity
• Motion of planets
• Kepler’s Laws of Planetary Motion
• Uses of Gravitation
Gravitation
The force of attraction by
the earth on bodies is
called gravitation.
Isaac Newton
• Sir Isaac Newton
(1643- 1726) was an
English mathematician,
physicist and scientist.
He is widely regarded as
one of the most influential
scientists of all time, developing new laws of
mechanics, gravity and laws of motion.
Newton?
THE UNIVERSAL LAW OF
GRAVITATION
• Every particle of matter in the universe attracts every
other particle with a force that is directly proportional
to the product of the masses of the particles and
inversely proportional to the square of the distance
between them.
• Any two point particles with masses m1 and m2
attract each other by a force whose magnitude is
directly proportional to the product of the two
masses, that is m1m2 and inversely proportional to
the square of the distance R between them. The
direction of the force is along the line joining the two
masses.
In the mathematical form the law can be represented
as…
Newton’s First law
• A body cannot change its state of rest or that
of uniform motion along a straight line ,
unless an external force acts on it.
• According to this law ,the net external force
on a body is zero, its acceleration is zero. A
body will have acceleration only if there is a
net external force on it.
Newton’s second law
• The rate of change of momentum of a body is
directly proportional to the force acting on it
and takes place in the direction of the force.
• Newton’s second law written in the form
F=ma
Newton’s third law
• For every action, there is an equal and
opposite reaction.
• According to this law ,if a body A exerts a
certain force (action)on another body B , then
B would exert on A an equal force(reaction)
in the opposite direction.
Weight and Gravitational Potential
Energy
• The force exerted by the earth on a particle of mass
m by its weight
w=mg
where , g the gravitational acceleration due to the earth.
• we can now easily evaluate this quantity by equating the
weight with the gravitational force exerted by the earth at its
surface. That is,
• More generally for any two masses m1 and
m2 separated by centre-to-centre distance r :
Escape velocity
• The minimum speed with which a body must be projected
from the earth’s surface so that it completely overcomes the
gravitational pull of the earth and does not return to earth’s
surface is known as escape velocity.
Motion of planets
Planets are the non-luminous celestial
bodies revolving around the sun. The planets
in the increasing order of the distance from
the sun. The planets vary in
size,mass,temperature,atmospere
etc…….The observed motion of the planets
are described using the Kepler’s laws.
Kepler’s Laws of Planetary Motion
• Kepler’s First Law
All planets move around the sun in
elliptical paths with the sun at one
focus of the ellipse.
F1 F2
Sun
Planet
P
Kepler’s Second
Law
An imaginary line drawn from the sun to
the planet sweep out equal areas in equal
intervals of time.
Sun C
D
A
B
Kepler’s Third Law
The square of the period of
revolution of the planet around the
sun is proportional to the cube of
its mean distance from the sun.
Uses of Gravitation
1)It is the gravitational
force that keep
everything at its
place. Otherwise
we would have
been floating in the air.
Weightlessness in space vehicle
It is due to gravitation that we are walking on the Earth.
2)It also keeps the
earth, sun and
other celestial
bodies at their
right places
3)It is responsible for many natural
phenomenon on the earths like tides and
orbiting of moon around the earth.
 gravitation ppt srinivasa

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gravitation ppt srinivasa

  • 1.
  • 2. Plan 0f talk • Gravitation • Isaac Newton • The universal law of gravitation • Newton’s First law • Newton’s second law • Newton’s third law • Weight and Gravitational Potential Energy • Escape velocity • Motion of planets • Kepler’s Laws of Planetary Motion • Uses of Gravitation
  • 3. Gravitation The force of attraction by the earth on bodies is called gravitation.
  • 4. Isaac Newton • Sir Isaac Newton (1643- 1726) was an English mathematician, physicist and scientist. He is widely regarded as one of the most influential scientists of all time, developing new laws of mechanics, gravity and laws of motion.
  • 6. THE UNIVERSAL LAW OF GRAVITATION • Every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of the masses of the particles and inversely proportional to the square of the distance between them. • Any two point particles with masses m1 and m2 attract each other by a force whose magnitude is directly proportional to the product of the two masses, that is m1m2 and inversely proportional to the square of the distance R between them. The direction of the force is along the line joining the two masses.
  • 7. In the mathematical form the law can be represented as…
  • 8. Newton’s First law • A body cannot change its state of rest or that of uniform motion along a straight line , unless an external force acts on it. • According to this law ,the net external force on a body is zero, its acceleration is zero. A body will have acceleration only if there is a net external force on it.
  • 9. Newton’s second law • The rate of change of momentum of a body is directly proportional to the force acting on it and takes place in the direction of the force. • Newton’s second law written in the form F=ma
  • 10. Newton’s third law • For every action, there is an equal and opposite reaction. • According to this law ,if a body A exerts a certain force (action)on another body B , then B would exert on A an equal force(reaction) in the opposite direction.
  • 11. Weight and Gravitational Potential Energy • The force exerted by the earth on a particle of mass m by its weight w=mg where , g the gravitational acceleration due to the earth. • we can now easily evaluate this quantity by equating the weight with the gravitational force exerted by the earth at its surface. That is,
  • 12. • More generally for any two masses m1 and m2 separated by centre-to-centre distance r :
  • 13. Escape velocity • The minimum speed with which a body must be projected from the earth’s surface so that it completely overcomes the gravitational pull of the earth and does not return to earth’s surface is known as escape velocity.
  • 14. Motion of planets Planets are the non-luminous celestial bodies revolving around the sun. The planets in the increasing order of the distance from the sun. The planets vary in size,mass,temperature,atmospere etc…….The observed motion of the planets are described using the Kepler’s laws.
  • 15. Kepler’s Laws of Planetary Motion • Kepler’s First Law All planets move around the sun in elliptical paths with the sun at one focus of the ellipse. F1 F2 Sun Planet P
  • 16. Kepler’s Second Law An imaginary line drawn from the sun to the planet sweep out equal areas in equal intervals of time. Sun C D A B
  • 17. Kepler’s Third Law The square of the period of revolution of the planet around the sun is proportional to the cube of its mean distance from the sun.
  • 18. Uses of Gravitation 1)It is the gravitational force that keep everything at its place. Otherwise we would have been floating in the air. Weightlessness in space vehicle It is due to gravitation that we are walking on the Earth.
  • 19. 2)It also keeps the earth, sun and other celestial bodies at their right places
  • 20. 3)It is responsible for many natural phenomenon on the earths like tides and orbiting of moon around the earth.