Imagine you are standing in a grand physics laboratory. The simple pendulum swinging before you is not just a bob on a string; it is a timekeeping marvel that connects the length of a string directly to the gravitational pull of the Earth. But here is the catch: no measurement is perfect. Every instrument has its limits, and this is where the beautiful mathematics of error propagation comes into play.
The Master Equation
Isolating g
The time period of a simple pendulum is governed by the classic equation:
Our goal is to find the percentage error in the determination of the acceleration due to gravity, g. To do this, we first need to make g the subject of our formula. By squaring both sides, we strip away the square root:
Rearranging this to isolate g, we get our master equation:
The Art of Error Propagation
Now, we apply the rules of error propagation. This is a favorite concept for JEE examiners! When physical quantities are multiplied or divided, their relative errors add up. Furthermore, if a quantity is raised to a power, that power becomes a multiplier for its relative error.
The term 4π2 is a pure mathematical constant. It has infinite precision, meaning its error contribution is exactly zero. Therefore, the relative error in g is solely determined by the measurements of L and T:
Notice how the T2 in the denominator translates to a factor of 2 in the error equation. Errors always compound; they never cancel each other out.
Crunching the Numbers
Precision Matters
Let's carefully extract the values from the problem. The measured length L is 1.0 m. The absolute error ΔL is the least count of the metre scale, which is 1 mm or 10−3 m.
The measured time T for one oscillation is 1.95 s. The absolute error ΔT is the resolution of the stopwatch, which is 0.01 s.
Substituting these into our error equation:
gΔg=1.010−3+2(1.950.01)
Let's break down the calculation. The length error term is simply 0.001. The time error term requires a bit more care:
2×1.950.01=1.950.02≈0.010256
Adding these together gives us the total relative error:
gΔg≈0.001+0.010256=0.011256
The Final Verdict
To find the percentage error, we simply multiply the relative error by 100:
% error=0.011256×100=1.1256%
Looking at our options, we round this off to two decimal places, giving us a final answer of 1.13%.
The Way Forward
Chasing Perfection
Did you get the feel of it? Think about how we could improve this experiment. If we measured the time for 100 oscillations instead of just 1, the total time T would be much larger. However, the least count ΔT of the stopwatch would remain the same 0.01 s. This would make the fraction TΔT significantly smaller, drastically reducing the overall error in g. In experimental physics, more observations always lead to higher accuracy!