A) \[\frac{{{\varepsilon }^{2}}R}{\sqrt{{{R}^{2}}+{{\left( L\omega -\frac{1}{C\omega } \right)}^{2}}}}\]
B) \[V=-{{x}^{2}}y-x{{z}^{3}}+4\]
C) \[\overrightarrow{E}\]
D) \[\overrightarrow{E}=\hat{i}(2xy+{{z}^{3}})+\hat{j}{{x}^{2}}+\hat{k}3x{{z}^{2}}\]
Correct Answer: C
Solution :
Key Idea Apply Kepler's law of area of planetary motion. The line joining the sun to the planet sweeps out equal areas in equal time interval ie, areal velocity is constant. \[{{Z}_{2}}\]constant or\[{{M}_{2,}}\] \[{{r}_{0.}}\]\[{{M}_{1}}\times {{M}_{2}}\] Given \[{{Z}_{1}}{{Z}_{2}}\] \[{{Z}_{1}}\]\[{{M}_{1}}\]You need to login to perform this action.
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