Step 1: The magnetic force on a moving charge is given by: \[ \vec{F} = q (\vec{v} \times \vec{B}) \]
Step 2: Given: \[ q = 3 \times 10^{-6} C, \quad \vec{v} = (10^5 \hat{i} + 10^5 \hat{j}) { m/s}, \quad \vec{B} = 5 \hat{j} { T} \]
Step 3: Compute the cross product:

Step 4: Expanding the determinant: \[ \vec{v} \times \vec{B} = (10^5 \times 0 - 10^5 \times 0) \hat{i} - (10^5 \times 0 - 5 \times 10^5) \hat{j} + (10^5 \times 5 - 10^5 \times 0) \hat{k} \] \[ = 0 \hat{i} + 5 \times 10^5 \hat{j} + 5 \times 10^5 \hat{k} \] \[ = 5 \times 10^5 \hat{k} \]
Step 5: Compute force: \[ \vec{F} = (3 \times 10^{-6}) (5 \times 10^5 \hat{k}) \] \[ = 1.5 \hat{k} { N} \]
Step 6: Since $\hat{k}$ represents the $+z$ direction, the force is $1.5$ N in the $+z$ direction.
Step 7: Therefore, the correct answer is (E).
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of