Question:

The motion of planets in the solar system is an example of conservation of

Updated On: Jul 5, 2022
  • mass
  • momentum
  • angular momentum
  • kinetic energy
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The Correct Option is C

Solution and Explanation

Areal speed of planet is constant. From Kepler's second law of motion, a line joining any planet to the sun sweeps out equal areas in equal intervals of time. Let any instant $t$, the planet is in position $A$. Then area swept out be $SA$ is
$dA =$ area of the curved triangle $SAB$ $ =\frac{1}{2}(AB\times SA) $ $ =\frac{1}{2}(rd\theta \times r)=\frac{1}{2}{{r}^{2}}d\theta $ The instantaneous areal speed is $ \frac{dA}{dt}=\frac{1}{2}{{r}^{2}}\left( \frac{d\theta }{dt} \right)=\frac{1}{2}{{r}^{2}}\omega $ Let $J$ be angular momentum $I$ the moment of inertia and $m$ the mass, then $ J=I\omega =m{{r}^{2}}\omega $ $ \therefore $ $ \frac{dA}{dt}=\frac{J}{2m}=$ constant Hence, angular momentum of the planet is conserved.
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Concepts Used:

Gravitation

In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.

Newton’s Law of Gravitation

According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,

  • F ∝ (M1M2) . . . . (1)
  • (F ∝ 1/r2) . . . . (2)

On combining equations (1) and (2) we get,

F ∝ M1M2/r2

F = G × [M1M2]/r2 . . . . (7)

Or, f(r) = GM1M2/r2

The dimension formula of G is [M-1L3T-2].