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Tamil Nadu Board of Secondary EducationSSLC (English Medium) Class 9

State Kepler’s laws. - Science

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Question

State Kepler’s laws.

Answer in Brief

Solution

In the early 1600s, Johannes Kepler proposed three laws of planetary motion.

  • First Law – The Law of Ellipses
    The path of the planets about the Sun is elliptical in shape, with the center of the Sun being located at one of the foci.
  • Second Law – The Law of Equal Areas
    An imaginary line drawn from the center of the Sun to the center of the planet will sweep out equal areas in equal intervals of time.
  • Third Law – The Law of Harmonies
    The ratio of the squares of the periods of any two planets is equal to the ratio of the cubes of their semi major axis from the Sun.
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Chapter 9: Universe - Exercise [Page 111]

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Samacheer Kalvi Science [English] Class 9 TN Board
Chapter 9 Universe
Exercise | Q IV. 7. | Page 111

RELATED QUESTIONS

Answer the following question.

State Kepler’s law of equal areas.


Answer the following question in detail.

State Kepler’s three laws of planetary motion.


If the distance between the sun and the earth is made three times, then attraction between the two will ______


The earth moves around the sun in an elliptical orbit as shown in the figure. The ratio, `"OA"/"OB"` = x. The ratio of the speed of the earth at Band at A is ______.


Supposing Newton’s law of gravitation for gravitation forces F1 and F2 between two masses m1 and m2 at positions r1 and r2 read F1 = – F2 = `- r_12/r_12^3 GM_0^2 ((m_1m_2)/M_0^2)^n` where M0 is a constant of dimension of mass r12 = r1 – r2 and n is a number. in such a case.

  1. the acceleration due to gravity on earth will be different for different objects.
  2. none of the three laws of Kepler will be valid.
  3. only the third law will become invalid.
  4. for n negative, an object lighter than water will sink in water.

A star like the sun has several bodies moving around it at different distances. Consider that all of them are moving in circular orbits. Let r be the distance of the body from the centre of the star and let its linear velocity be v, angular velocity ω, kinetic energy K, gravitational potential energy U, total energy E and angular momentum l. As the radius r of the orbit increases, determine which of the above quantities increase and which ones decrease.


A satellite is in an elliptic orbit around the earth with aphelion of 6R and perihelion of 2 R where R= 6400 km is the radius of the earth. Find eccentricity of the orbit. Find the velocity of the satellite at apogee and perigee. What should be done if this satellite has to be transferred to a circular orbit of radius 6R ?

[G = 6.67 × 10–11 SI units and M = 6 × 1024 kg]


A planet revolving in an elliptical orbit has:

  1. a constant velocity of revolution.
  2. has the least velocity when it is nearest to the sun.
  3. its areal velocity is directly proportional to its velocity.
  4. areal velocity is inversely proportional to its velocity.
  5. to follow a trajectory such that the areal velocity is constant.

Choose the correct answer from the options given below:


lf the angular momentum of a planet of mass m, moving around the Sun in a circular orbit is L, about the center of the Sun, and its areal velocity is ______.


Halley's Comet revolves around the sun for a time period of 76 years. The aphelion distance if perihelion is given by 8.9 × 1010 m, will be ______.

(Take, the mass of sun = 2 × 1030 kg and G = 6.67 × 10-11 Nm3/kg2)


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