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Gravitation

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Question : 5 of 25
Marks: +1, -0
Let us assume that our galaxy consists of 2.5×10112.5 \times 10^{11} stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution? Take the diameter of the Milky Way to be 10510^{5} ly.
Solution:  
Using, M=4π2R3GT2M = \frac{4 \pi^{2} R^{3}}{G T^{2}} or T=(4π2R3GM)1/2T = \left( \frac{4 \pi^{2} R^{3}}{G M} \right)^{1/2}
Given, M=2.5×1011M = 2.5 \times 10^{11}
Solar mass =2.5×1011×(2×1030)kg= 2.5 \times 10^{11} \times (2 \times 10^{30}) \text{kg}
=5.0×1041kg= 5.0 \times 10^{41} \text{kg}
and R=50,0001yR = 50,0001 y
=50,000×9.4×1015m= 50,000 \times 9.4 \times 10^{15} \text{m}
=4.73×1020m= 4.73 \times 10^{20} \text{m}
T=[4×(3.14)2×(4.73×1020)3(6.67×1011)×(5.0×1041)]1/2\therefore T = \left[ \frac{4 \times (3.14)^{2} \times (4.73 \times 10^{20})^{3}}{(6.67 \times 10^{-11}) \times (5.0 \times 10^{41})} \right]^{1/2}
T=1.12×1016sT = 1.12 \times 10^{16} \text{s}
=3.54×108years= 3.54 \times 10^{8} \text{years}
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