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Kepler's third law states that the square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance of r between sun and planet i.e. T^(2) prop k r^(3) where k is constant. If the mass of sun and planet are M, m respectively than as per Newtons law of gravitation force of ttracion, F = (GMm)/(r^(2)). The relation between G & K s describe as |
Answer» <html><body><p>`<a href="https://interviewquestions.tuteehub.com/tag/gk-468580" style="font-weight:bold;" target="_blank" title="Click to know more about GK">GK</a> = 4 PI^(2)`<br/>`<a href="https://interviewquestions.tuteehub.com/tag/gmk-3648666" style="font-weight:bold;" target="_blank" title="Click to know more about GMK">GMK</a> = 4PI^(2)`<br/>K = G<br/>`K = (<a href="https://interviewquestions.tuteehub.com/tag/1-256655" style="font-weight:bold;" target="_blank" title="Click to know more about 1">1</a>)/(G)`</p>Answer :<a href="https://interviewquestions.tuteehub.com/tag/b-387190" style="font-weight:bold;" target="_blank" title="Click to know more about B">B</a></body></html> | |