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The speed at which any planet moves through space is constantly changing. In a perfectly circular orbit, the orbital radius of the planet would be constant and therefore so would be its observed angular velocity. In elliptical orbits, the velocity varies. In elliptical orbits, the orbital radius of the satellite will vary and therefore so will its velocity. The planet travels "faster" when closer to the Sun, then "slower" at a more distant radius. According to Newton's 2nd Law, what is the underlying force behind this change in velocity?
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According to Kepler's 3rd law, the square of the time it takes for an object to orbit, T, is directly related to the cube of the distance, r, between the object and what it is orbiting.
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Diagram shows a planet orbiting around the sun. Based on Kepler's Second Law, Which of the following regarding the speeds of the planet at positions P(vp), Q(vQ) and R(vR)P\left(v_p\right),\ Q\left(v_Q\right)\ and\ R\left(v_R\right)P(vp), Q(vQ) and R(vR) is correct
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Kepler's third law is represented by the following equation:Hukum Kepler ketiga ditunjukkan oleh persamaan:
What did Kepler discover about planets and their orbital speed?
A kine drawn from a planet to the Sun always sweeps over equal areas in equal intervals of time When the planet moves further from the sun, the planet will move
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Which statement best describes Kepler’s 3rd Law of Planetary Motion?
What is Kepler's 3rd Law?
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What unit to we usually use to to measure a planet's orbital period?
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