The Symphony of Relative Motion
Imagine standing on a quiet street when an ambulance races past you with its sirens blaring. You've likely noticed how the pitch of the siren sounds higher as it approaches and suddenly drops as it speeds away. This everyday phenomenon is the Doppler Effect, a beautiful interplay between the relative motion of a source and an observer.
In this problem, we are given a source emitting a sound of frequency f0​=240 Hz. We have two distinct scenarios: first, the source and observer are rushing towards each other, and second, they are retreating from one another. Our goal is to find the apparent frequency heard during their retreat.
The Master Equation of Doppler Effect
To solve any Doppler effect problem, we rely on one master equation. The apparent frequency f′ heard by the observer is given by:
f′=f0​(c∓vs​c±vo​​)
Here, c is the speed of sound in the medium, vo​ is the speed of the observer, and vs​ is the speed of the source. The true challenge lies not in the formula itself, but in the sign convention.
The rule of thumb is simple: any motion that tends to bring the source and observer closer together will increase the apparent frequency. Therefore, an approaching observer gets a positive sign in the numerator, and an approaching source gets a negative sign in the denominator.
Case 1
The Approach
Let's analyze the first case. Both the source and the observer are moving towards each other with a speed v. Applying our sign convention, the observer's motion increases the frequency (so we use +v in the numerator), and the source's motion also increases the frequency (so we use −v in the denominator).
This gives us our first working equation:
We are given that during this approach, the observer hears a frequency of 288 Hz. Substituting the known values:
Unlocking the Speed Ratio
This equation is a treasure map that leads us to the relationship between the speed of sound c and the speed of the objects v. Let's simplify the fraction:
c−vc+v​=240288​=56​
Now, we cross-multiply to solve for c in terms of v:
Bringing the terms together, we find a remarkably clean relationship:
This tells us that the speed of sound is exactly 11 times the speed of the source and observer. We don't need the absolute values of these speeds; their ratio is all the power we need.
Case 2
The Retreat
Now, the scene shifts. The source and observer have crossed paths and are now moving away from each other at the same speed v.
Because they are separating, the apparent frequency must drop. The observer moving away gets a negative sign in the numerator, and the source moving away gets a positive sign in the denominator. Our new equation is:
The Final Crescendo
We are ready for the final calculation. We substitute our golden ratio, c=11v, into the new equation:
f2​=240(11v+v11v−v​)
The variable v elegantly cancels out, leaving us with a simple arithmetic step:
Thus, when the source and observer are receding, the measured frequency drops to 200 Hz. The value of n is exactly 200. By carefully managing our sign conventions and leveraging the ratio of speeds, a seemingly complex relative motion problem unravels into a beautiful, logical conclusion.