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UNIVERSAL GRAVITATION
Submitted To :
Mrs. Linimol.k.s Faculty in physical science department
Sreenarayana training college poochakkal
Submitted By :
Renju.R Option : Physical Science
Register Number : 18214383018 Submitted On : 7.9.2015
Isaac Newton
1643 - 1727
Newton & Physics
Newton’s Law of Universal Gravitation states that gravity is an attractive force acting between all pairs of massive objects.
Gravity depends on: Masses of the two objects Distance between the objects
Universal Gravitation
Universal Gravitation - Apple
Bottom LineGravity’s Inverse Square Law
Bottom Line
• Gravity is reduced as the inverse square of its distance from its source increased
• Fg ~ 1/r2•
Gravity’s Inverse Square Law
r 2r 3r 4r 5r 6r 60r
Fg Fg Fg Fg Fg Fg Fg
1 4 9 16 25 36 3600
Bottom LineGravity’s Inverse Square Law
Gravity decreases with altitude, since greater altitude means greater distance from the Earth's centre
If all other things being equal, on the top of Mount Everest (8,850 metres), weight decreases about 0.28%
Bottom LineGravity’s Inverse Square Law
Astronauts in orbit are NOT weightless
At an altitude of 400 km, a typical orbit of the Space Shuttle, gravity is still nearly 90% as strong as at the Earth's surface
Bottom LineLaw of Universal Gravitation
Newton’s discovery
Newton didn’t discover gravity. In stead, he discovered that the gravity is universal
Everything pulls everything in a beautifully simple way that involves only mass and distance
Bottom LineLaw of Universal Gravitation
Universal gravitation formula
Fg = G m1 m2 / d2
Fg: gravitational force between objectsG: universal gravitational constantm1: mass of one objectm2: mass of the other objectd: distance between their centers of
mass
Bottom LineLaw of Universal Gravitation
p.83
m1m2
d
Fg Fg
Fg Gm1m2
d 2
Bottom LineLaw of Universal Gravitation
Fg = G m1 m2 / d2
Gravity is always there
Though the gravity decreases rapidly with the distance, it never drop to zero
The gravitational influence of every object, however small or far, is exerted through all space
Bottom LineLaw of Universal Gravitation Example
Mass 1 Mass 2 Distance Relative Force
m1 m2 d F
2m1 m2 d
m1 3m2 d
2m1 3m2 d
m1 m2 2d
m1 m2 3d
2m1 2m2 2d
Law of Universal Gravitation Example
Mass 1 Mass 2 Distance Relative Force
m1 m2 D F
2m1 m2 d 2F
m1 3m2 d 3F
2m1 3m2 d 6F
m1 m2 2d F/4
m1 m2 3d F/9
2m1 2m2 2d F
Universal Gravitational Constant
The Universal Gravitational Constant (G) was first measured by Henry Cavendish 150 years after Newton’s discovery of universal gravitation
Henry Cavendish
1731 - 1810
Universal Gravitational Constant
Cavendish’s experiment
Use Torsion balance (Metal thread, 6-foot wooden rod and 2” diameter lead sphere) Two 12”, 350 lb lead spheres The reason why Cavendish measuring the G is to “Weight the Earth” The measurement is accurate to 1% and his data was lasting for a century
Cavendish’s Experiment
Universal Gravitational Constant
Universal Gravitational Force
Isaac Newton’s Influence
People could uncover the workings of the physical universe
Moons, planets, stars, and galaxies have such a beautifully simple rule to govern them
Phenomena of the world might also be described by equally simple and universal laws