law of gravitation

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    Newtons Law of Gravitation

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    Gravity is More Than a Name

    Gravity is the name associated with the

    reason for what goes up, must come

    down

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    We all know of the word gravity- it is

    the thing which causes objects to fall to

    Earth.

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    ROLE of PHYSICS

    To do more than to associate words with

    phenomenon.

    To explain phenomenon in terms of underlying

    principles

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    A students conception of gravity must grow in

    sophistication to the point that it becomes more

    than a mere name associated with falling

    phenomenon

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    Gravity must be understood in terms of its

    cause, its source, and its far-reaching

    implications on the structure and the motion of

    the objects in the universe.

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    Fgrav ,GRAVITY, is a force which exists

    between the Earth and the objects which are near

    it.

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    As we rise upwards after our jump, the force of

    gravity slows us down; and as we fall back to

    Earth after reaching our peak, the force of

    gravity speeds us up.

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    In this sense, the force gravity causes an

    acceleration of our bodies during this brief trip

    away from the earths surface and back.

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    The acceleration of gravity (g) is the acceleration

    experienced by an object when the only force

    acting upon it is the force of gravity.

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    The value of g varies slightly from place to place

    on the earths surface.

    It is 9.83 m/s2 at the North or South Pole and is

    9.87 m/s2 at the equator.

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    No matter what their mass, all objects fall

    freely at the same acceleration, 9.8 m/s2

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    History

    Kelplers Three Laws of Planetary System

    1. Each planet moves in an elliptical orbit aboutthe sun with the sun at one forces.

    (Law of Elliptical Orbit)

    2. The line joining the sun and the planet sweepsequal area in equal time ( Law of Area)

    3. The ratio of the cube of the mean distance of theplanet from the sun to the square of its period isa constant. (Law of Period)

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    Question

    If planets do move in the way described byKepler, what keeps them continuously moving in

    their orbits.

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    The gravitational force exerted by a mass m1 on another

    mass m2 is proportional to the products of their masses

    and inversely proportional to the square of their

    separation r:

    F = G m1m2/ r2,

    Where G is a constant called the universal gravitation

    constant and has a value

    G = 6.67 x 10-11 N.m2/kg2

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    This means that there are gravitational force

    between the sun and the planets, between

    the earth and the moon, between the earthand an object near its surface, or between

    any two objects.

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    Example

    The gravitational force between two identical

    objects, each with a mass of 10 kg, is 1 N.

    What is the distance between their centers?

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    WEIGHT

    The pull of gravity

    Is the gravitational force acting on it by the earth.

    Measured in Newtons. If the object falls freely, its weight gives it na

    acceleration of g.

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    Applying F = ma, the weightW of an object of

    mass m is

    W= mg

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    Objects of greater mass have a greater resistance

    to acceleration, but a larger gravitational force

    acts on them.

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    Another important force that causes centripetal

    acceleration is the force of gravity. The quantitative

    description of this force was discovered by Isaac Newton.

    As he put together the ideas for his three laws of motion,

    he also wondered about the circular motion of the planets

    about the sun. What prevented these bodies from leaving

    their paths?

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    According to one of his biographers, Newton was

    sitting under an apple tree one day when an applefell.

    Newton was struck by the idea that the force

    causing the apple to fall might also cause themoon to fall toward the earth.

    However, since the moon moved forward as it

    fell, the moon followed a circular path ratherthan falling into the earth as the apple had done.

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    According to Newton, he began to think of

    gravity extending to the orbit of the moon

    Using observations about planetary motion byKepler, Newton deducedthat the force that kept

    planets in orbit could also account for the earthsgravitational force on an apple.

    Newton had developed a logical and basic

    understanding of an important aspect of thestructure of our universe.

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    1. One pan of the laboratory balance has a mass

    of 150 g. The distance between the pans is

    250 cm and the force acting on the pans in 12N.What is the mass of the second pan in

    grams?

    2. Two kids are playing see saw. The masses ofthe kids are 45 kg and 51 kg respectively and

    the force acting upon them is 35 N.What is

    the distance of separation between the kids?

    3. A man is carrying two loads in his hands. Oneof the loads is 4.5 kg while the other is 350 g.

    If the distance between his hands is 180 cm,

    how much force is he exerting on the loads?