Two stars of masses 3 x 1031 kg each and at distance 2 x 1011 m rotate in a plane about their common centre of mass O. A meteorite passes through O moving perpendicular to the star's rotation plane. In order to escape from the gravitational field of this double star, the minimum speed that meteorite should have at O is (Take, gravitational constant, G = 6.67 × 1011 N-m2 kg2)

Principles of Physics: A Calculus-Based Text
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ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
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Chapter11: Gravity, Planetary Orbits, And The Hydrogen Atom
Section: Chapter Questions
Problem 50P: Two stars of masses M and m, separated by a distance d, revolve in circular orbits about their...
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Two stars of masses 3 x 1031 kg each and at
distance 2 x 10' m rotate in a plane about
their common centre of mass O. A meteorite
passes through O moving perpendicular to the
star's rotation plane. In order to escape from
the gravitational field of this double star, the
minimum speed that meteorite should have at
O is
(Take, gravitational constant, G = 6.67 x 1011
N-m² kg2)
Transcribed Image Text:Two stars of masses 3 x 1031 kg each and at distance 2 x 10' m rotate in a plane about their common centre of mass O. A meteorite passes through O moving perpendicular to the star's rotation plane. In order to escape from the gravitational field of this double star, the minimum speed that meteorite should have at O is (Take, gravitational constant, G = 6.67 x 1011 N-m² kg2)
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