Q.The length of a second's pendulum on the surface of the Earth is 0.9 m. The length of the same pendulum on surface of planet X such that the acceleration of the planet X is n times greater than the Earth is a) 0.9n m b) 0.9/n m c) 0.9n2 m d) 0.9/n2 m
Imagine tying a small weight to a string, holding the other end fixed, and giving it a gentle push. It swings back and forth — that’s a simple pendulum. The question is: what determines how fast it swings? Does a heavier bob swing faster? Does a longer string make it slower?
Let’s start with what you already feel. If you hold a short string (say 20 cm) and swing it, the bob zips back and forth quickly. If you use a long string (say 1 m), the swing is noticeably slower. So length matters — longer means slower.
What about the weight? Try a light plastic bob and a heavy metal one of the same size, on the same string. You’ll find they swing at the same speed. That’s surprising — heavier things don’t fall faster, and here they don’t swing faster either. So mass does not affect the period (the time for one complete back-and-forth swing).
What about how hard you push? If you give a big push, the bob swings wider, but does it take more time? For small swings (small angles, say less than about 15°), the period is almost the same regardless of amplitude. That’s the key: for small oscillations, the pendulum is isochronous — its period is independent of amplitude.
Note
This is only true for small angles. If you pull the bob to 60° and let go, the period becomes noticeably longer. In most exam problems, you assume “small oscillations” (usually < 10°).
The Precise Statement
For a simple pendulum of length L (measured from pivot to centre of bob), swinging with small amplitude in a uniform gravitational field g, the time periodT (time for one complete oscillation) is:
T=2πgL
That’s it. No mass term. No amplitude term (for small angles).
T=2πgL
Why does this formula make sense?
L in numerator: longer string → larger T (slower swing). Doubling L multiplies T by 2≈1.4.
g in denominator: stronger gravity (larger g) → smaller T (faster swing). On the Moon (g≈1.6 m/s²), the same pendulum swings much slower.
2π: comes from the mathematics of simple harmonic motion — the pendulum’s motion is approximately sinusoidal for small angles.
Tip
To remember: the formula is identical to that of a mass on a spring (T=2πm/k), but here the “restoring force per unit displacement” is mg/L, so the effective “k” is mg/L, giving T=2πL/g.
Common exam pitfalls
Don’t confuse L with amplitude.L is the string length, not how far you pull it.
Don’t include mass. The period does not depend on the bob’s mass — a common trick question.
Small-angle assumption. If the problem says “small oscillations” or gives an angle < 10°, use this formula. If the angle is large, the formula changes (and is rarely asked in basic exams).
Quick check
A pendulum of length 1 m on Earth (g=9.8 m/s²) has period:
T=2π9.81≈2π×0.319≈2.0 seconds
That’s why a “seconds pendulum” (period exactly 2 s) has length about 1 m — a classic exam fact.
Final answer: For a simple pendulum with small amplitude, the period is T=2πL/g, independent of mass and amplitude.
Many students find this page while searching "Simple Pendulum Period formula physics" or "Simple Pendulum Period important questions and answers"; the concept sits firmly within the Class 11 Physics NCERT/CBSE syllabus. It's also a frequent building block for numericals in JEE Main, NEET and state engineering/medical entrance exams, so treating it as a one-time memorisation task rather than an understood idea tends to backfire later.
A seconds pendulum always has T=2 s, so l/g must be the same constant on both planets: l∝g.
✓Final answer
(a) 0.9n m
Step 1. A 'seconds pendulum' is, by definition, one whose time period is exactly T=2 s, on Earth or on planet X alike, since T is fixed at 2 s in both cases.
Step 2. From T=2πl/g, squaring gives l/g=(T/2π)2, a constant, the same on Earth and on planet X since T=2 s on both.
Step 3. So gEarthlEarth=gXlX, giving lX=lEarth×gEarthgX.
Step 4. Given gX=ngEarth and lEarth=0.9 m, lX=0.9×n=0.9n m.
✓Final answer
(a) 0.9n m
Use T = 2 pi sqrt(l/g) with T fixed at 2 s on both planets, so l is directly proportional to g.
Assuming the length stays fixed at 0.9 m and trying to solve for a changed time period, when the question actually fixes T = 2 s and asks for the new length.
Inverting the proportionality and writing l_X = 0.9/n instead of 0.9n.