Exercises
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1. The average distance of the Sun from the Earth is
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152.02 million km...................
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According to Kepler's third law,
According to Kepler's third law,T
According to Kepler's third law,T 2
According to Kepler's third law,T 2 ∝r
According to Kepler's third law,T 2 ∝r 3
According to Kepler's third law,T 2 ∝r 3 orT∝r
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ D
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =(
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 )
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D(
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2 )
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2 ) 3/2
According to Kepler's third law,T 2 ∝r 3 orT∝r 3/2 ∴ DD ′ =( L 1 L 2 ) 3/2 or D ′ =D( L 1 L 2 ) 3/2 days
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