A) 4.2 T
B) 2.8 T
C) 5.6 T
D) 8.4 T
Correct Answer: B
Solution :
Applying Kepler s third law \[{{T}^{2}}\propto {{R}^{3}}\] Hence,\[{{\left( \frac{{{T}_{1}}}{{{T}_{2}}} \right)}^{2}}={{\left( \frac{{{R}_{1}}}{{{R}_{2}}} \right)}^{3}}={{\left( \frac{R}{2\,\,R} \right)}^{3}}\] \[\frac{T}{{{T}_{2}}}={{\left( \frac{1}{2} \right)}^{3/2}}\] So, \[{{T}_{2}}=2.8\,\,T\]
You need to login to perform this action.
You will be redirected in
3 sec
