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Two particles move in a uniform gravitat...

Two particles move in a uniform gravitational field with an acceleration g. At the initial moment the particles were located over a tower at one point and moved with velocities `v_1 = 3m//s and v_2= 4m//s` horizontally in opposite directions. Find the distance between the particles at the moment when their velocity vectors become mutually perpendicular.

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To solve the problem of finding the distance between two particles moving in a uniform gravitational field when their velocity vectors become mutually perpendicular, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding Initial Conditions:** - Two particles are thrown horizontally from the same height with initial velocities: - Particle 1: \( v_1 = 3 \, \text{m/s} \) (to the right) - Particle 2: \( v_2 = 4 \, \text{m/s} \) (to the left) 2. **Velocity Components:** - The horizontal component of the velocities remains constant since there is no horizontal acceleration: - Particle 1: \( \vec{V_1} = 3 \hat{i} - gt \hat{j} \) - Particle 2: \( \vec{V_2} = -4 \hat{i} - gt \hat{j} \) 3. **Condition for Perpendicular Vectors:** - The velocity vectors are perpendicular when their dot product is zero: \[ \vec{V_1} \cdot \vec{V_2} = 0 \] - This gives: \[ (3 \hat{i} - gt \hat{j}) \cdot (-4 \hat{i} - gt \hat{j}) = 0 \] - Expanding the dot product: \[ 3 \cdot (-4) + (-gt) \cdot (-gt) = 0 \] \[ -12 + g^2 t^2 = 0 \] - Rearranging gives: \[ g^2 t^2 = 12 \] \[ t^2 = \frac{12}{g^2} \] \[ t = \frac{\sqrt{12}}{g} \] 4. **Substituting the Value of g:** - Given \( g = 10 \, \text{m/s}^2 \): \[ t = \frac{\sqrt{12}}{10} = \frac{2\sqrt{3}}{10} = \frac{\sqrt{3}}{5} \, \text{s} \] 5. **Calculating Horizontal Displacements:** - Horizontal displacement of Particle 1: \[ x_1 = v_1 \cdot t = 3 \cdot \frac{\sqrt{3}}{5} = \frac{3\sqrt{3}}{5} \, \text{m} \] - Horizontal displacement of Particle 2: \[ x_2 = v_2 \cdot t = 4 \cdot \frac{\sqrt{3}}{5} = \frac{4\sqrt{3}}{5} \, \text{m} \] 6. **Finding the Distance Between the Particles:** - The total distance between the two particles when they are perpendicular: \[ \text{Distance} = x_1 + x_2 = \frac{3\sqrt{3}}{5} + \frac{4\sqrt{3}}{5} = \frac{7\sqrt{3}}{5} \, \text{m} \] ### Final Answer: The distance between the two particles when their velocity vectors become mutually perpendicular is: \[ \frac{7\sqrt{3}}{5} \, \text{m} \]

To solve the problem of finding the distance between two particles moving in a uniform gravitational field when their velocity vectors become mutually perpendicular, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding Initial Conditions:** - Two particles are thrown horizontally from the same height with initial velocities: - Particle 1: \( v_1 = 3 \, \text{m/s} \) (to the right) - Particle 2: \( v_2 = 4 \, \text{m/s} \) (to the left) ...
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