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•Gravitation •Planetary Motion •Laws of Gravitation

May 30, 2018

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    Gravitation PlanetaryMotion Laws of Gravitation

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    GravitationGravitationGravitation is the namegiven to the force ofattraction between any twobodies of the universe, wasdiscovered by Newton in1665.

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    The constant of proportionality G isknown as the universalgravitational constant.It is termed a "universalconstant" because it isthought to be the sameat all places and all

    times, and thusuniversallycharacterizes theintrinsic strength of thegravitational force.

    Laboratoryexperiments haveyielded a value for G of G = 6.67 10 11 Newton. (m 2/kg 2)

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    Law Of UniversalGravitation

    The law of universalgravitation accounts forplanets not falling into the Sunnor the Moon crashing into the

    Earth.

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    = 2 21r

    mmG Force

    v

    m 2Now suppose Earthprovides pull insteadof string and arm

    m1

    =r

    vm Force

    2

    2

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    = 2 21r

    mmG Force

    =r

    vm Force

    2

    2

    = 2

    21

    2

    2

    r

    mmG

    r

    vm

    r

    Gmv 12 =

    (Force needed to keep it in orbit)(Force that can be provided)

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    r

    Gm 12v =

    G = 6.7 x 10 -11 N .m 2/kg 2

    m 1 = 2 x 10 30 kg

    Mars Orbital velocity = 24 km/s Distance from Sun = 228 x 10 9 km

    Earth Orbital velocity = 30 km/s Distance from Sun = 150 x 10 9 km

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    o ge some ng n or , weneed a special horizontal

    velocity The law of universalgravitation accounts for planets not falling into theSun nor the Moon crashinginto the Earth

    Paths A, B, and C do nothave enough horizontalvelocity to escape Earthssurface whereas Paths D,E, and F do.

    Path E is where thehorizontal velocity is exactlywhat is needed so its orbitmatches the circular curveof the Earth

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    Keplers Laws of PlanetaryMotion

    Using precise measurements of thepositions of the planets in the skycollected by Tycho Brahe, JohannesKepler deduced three laws of planetarymotion:

    1. The orbits are ellipses.

    2. Planets move faster when closer to the Sun andslower when farther away.3. Planets farther from the Sun take longer to

    orbit.

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    Orbits are ellipses

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    Planets move faster whencloser to the Sun

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    Planets farther from the Suntake longer to orbit