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Question: Two students simultaneously start from the same place on a circular track and run for 2 min. In this...

Two students simultaneously start from the same place on a circular track and run for 2 min. In this time, one of them completes three and the other four revolutions. Due to thick vegetation in a circular area as shown in the figure, either of the boys can see only one third of the track at a time. How long during their run do they remain visible to each other?

A

20 s

B

40 s

C

80 s

D

160 s

Answer

40 s

Explanation

Solution

To solve this problem, we need to determine the relative motion of the two students and the conditions under which they are visible to each other.

1. Calculate the angular speeds of the students: Let the total duration of the run be T=2 min=120 sT = 2 \text{ min} = 120 \text{ s}.

For student 1: Number of revolutions = 3 Angular displacement = 3×2π=6π3 \times 2\pi = 6\pi radians Angular speed of student 1, ω1=Angular displacementTime=6π120=π20 rad/s\omega_1 = \frac{\text{Angular displacement}}{\text{Time}} = \frac{6\pi}{120} = \frac{\pi}{20} \text{ rad/s}.

For student 2: Number of revolutions = 4 Angular displacement = 4×2π=8π4 \times 2\pi = 8\pi radians Angular speed of student 2, ω2=Angular displacementTime=8π120=π15 rad/s\omega_2 = \frac{\text{Angular displacement}}{\text{Time}} = \frac{8\pi}{120} = \frac{\pi}{15} \text{ rad/s}.

2. Calculate the relative angular speed: Since both students start from the same place and move on a circular track, their relative angular speed is the difference between their individual angular speeds (assuming they move in the same direction, as implied by the problem statement). ωrel=ω2ω1=π15π20\omega_{rel} = \omega_2 - \omega_1 = \frac{\pi}{15} - \frac{\pi}{20} To subtract, find a common denominator (60): ωrel=4π603π60=π60 rad/s\omega_{rel} = \frac{4\pi}{60} - \frac{3\pi}{60} = \frac{\pi}{60} \text{ rad/s}. This is the rate at which student 2 gains on student 1.

3. Determine the visibility range: Each student can see one-third of the track at a time. A full circular track corresponds to an angle of 2π2\pi radians. So, the angular range of visibility for each student is 13×2π=2π3\frac{1}{3} \times 2\pi = \frac{2\pi}{3} radians. For two students to be visible to each other, their angular separation must be within this range. If one student is at an angle θ\theta, they can see another student if the other student is within the angular interval [θπ3,θ+π3][\theta - \frac{\pi}{3}, \theta + \frac{\pi}{3}] (considering the visibility range centered around their position). This means the absolute difference in their angular positions, Δθ|\Delta\theta|, must be less than or equal to π3\frac{\pi}{3}. So, they are visible when π3Δθπ3-\frac{\pi}{3} \le \Delta\theta \le \frac{\pi}{3} (modulo 2π2\pi).

4. Calculate the time for one relative revolution: The time it takes for student 2 to gain one full revolution (2π2\pi radians) on student 1 is: Trel=2πωrel=2ππ/60=2×60=120 sT_{rel} = \frac{2\pi}{\omega_{rel}} = \frac{2\pi}{\pi/60} = 2 \times 60 = 120 \text{ s}.

5. Calculate the total visibility time: The total duration of the run is 120 seconds. This is exactly equal to the time for one relative revolution (TrelT_{rel}). During one relative revolution, the relative angular position Δθ\Delta\theta changes from 00 to 2π2\pi. They are visible when Δθ\Delta\theta is in the range [π3,π3][-\frac{\pi}{3}, \frac{\pi}{3}] (modulo 2π2\pi). This corresponds to an angular interval of 2π3\frac{2\pi}{3}. The fraction of time they are visible during one relative revolution is: Fraction visible = Visible angular rangeTotal angular range in one relative revolution=2π/32π=13\frac{\text{Visible angular range}}{\text{Total angular range in one relative revolution}} = \frac{2\pi/3}{2\pi} = \frac{1}{3}.

Since the total run time is exactly one relative revolution (120 s), the total time they remain visible to each other is: Total visible time = Fraction visible ×\times Total run time Total visible time = 13×120 s=40 s\frac{1}{3} \times 120 \text{ s} = 40 \text{ s}.

Alternatively, we can calculate the time intervals: At t=0t=0, Δθ=0\Delta\theta = 0, they are visible. They remain visible until Δθ=π3\Delta\theta = \frac{\pi}{3}. Time taken: t1=π/3π/60=20 st_1 = \frac{\pi/3}{\pi/60} = 20 \text{ s}. So, they are visible from t=0t=0 to t=20t=20 s. The relative angle continues to increase. They become visible again when Δθ\Delta\theta (modulo 2π2\pi) enters the range [π3,π3][-\frac{\pi}{3}, \frac{\pi}{3}] from the other side. This happens when Δθ\Delta\theta reaches 2ππ3=5π32\pi - \frac{\pi}{3} = \frac{5\pi}{3} (which is equivalent to π3-\frac{\pi}{3}). Time taken to reach 5π3\frac{5\pi}{3}: t2=5π/3π/60=100 st_2 = \frac{5\pi/3}{\pi/60} = 100 \text{ s}. So, from t=100t=100 s, they become visible again. They remain visible until Δθ=2π\Delta\theta = 2\pi (which is 00, the starting point), which occurs at t=120 st = 120 \text{ s}. The duration of this second interval is 120 s100 s=20 s120 \text{ s} - 100 \text{ s} = 20 \text{ s}. Total visible time = 20 s+20 s=40 s20 \text{ s} + 20 \text{ s} = 40 \text{ s}.

The final answer is 40 s\boxed{\text{40 s}}.