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7.2 - Frequency and Period of SHM

Period and Frequency

Period (TT) and frequency (ff) in SHM are inverse relationships:
T=1for equivalentlyf=1TT = \frac{1}{f} \qquad \text{or equivalently} \qquad f = \frac{1}{T}
where TT is period, measured in seconds per cycle, and ff is frequency, measured in cycles per second, or Hertz (Hz). Period is the time to complete one full oscillation, and frequency is the number of complete oscillations per unit time.
Because TT and ff are reciprocals, they always change in opposite directions: double the frequency and the period is cut in half. In the lab, it’s more accurate to time many oscillations and divide than to time just one. Your reaction time on the stopwatch adds about the same error either way, but dividing by the number of oscillations spreads that error out.

Angular Frequency

Angular frequency (ω\omega) relates to period and frequency:
ω=2πTor equivalentlyω=2πf\omega = \frac{2\pi}{T} \qquad \text{or equivalently} \qquad \omega = 2\pi f
with units of rad/s. In the context of oscillations, ω\omega represents angular frequency, not angular speed, even though it’s the same symbol used in rotational motion.

Period of a Mass-Spring Oscillator

For an ideal spring-mass system in SHM:
T=2πmkT = 2\pi\sqrt{\frac{m}{k}}
where mm is the mass in kg and kk is the spring constant in N/m. Larger mass gives a longer period (heavier objects oscillate more slowly), a larger kk (stiffer spring) gives a shorter period (stiffer springs oscillate faster), and notably, the period doesn’t depend on amplitude at all, how far you pull the mass back doesn’t matter. This equation is provided on the AP Physics 1 formula sheet.
Why mass and stiffness matter: a larger mass has more inertia, so the same spring force gives it a smaller acceleration and each cycle takes longer. A stiffer spring pulls harder at the same displacement, so the acceleration is larger and each cycle is quicker. Gravity doesn’t appear in the equation at all, so a spring-object system has the same period whether it hangs vertically, lies on a table, or is taken to the Moon.
Functional dependence: Ts∝mT_s \propto \sqrt{m} and Ts∝1kT_s \propto \frac{1}{\sqrt{k}}. Multiply the mass by 4 and the period doubles. Multiply kk by 4 and the period is cut in half. The AP equation sheet writes this equation as Ts=2πmkT_s = 2\pi\sqrt{\frac{m}{k}}, with the subscript ss for spring.
The frequency follows as f=1T=12πkmf = \frac{1}{T} = \frac{1}{2\pi}\sqrt{\frac{k}{m}}.

Period of a Simple Pendulum

For a simple pendulum undergoing small-angle oscillations:
T=2πLgT = 2\pi\sqrt{\frac{L}{g}}
where LL is the pendulum’s length in meters and gg is gravitational acceleration in m/s². A longer pendulum gives a longer period, stronger gravity gives a shorter period, and notably, the bob’s mass doesn’t affect the period at all, nor does amplitude, for small angles. This equation is also on the AP Physics 1 formula sheet.
Why mass doesn’t matter for a pendulum: for a small angle, the restoring force is about mgθmg\theta, and the bob’s distance from equilibrium along the arc is x=Lθx = L\theta. So the restoring force is about mgLx\frac{mg}{L}x, which has the same form as a spring force, kxkx, with an effective spring constant of mgL\frac{mg}{L}. Put that into the spring formula:
T=2πmmg/L=2πLgT = 2\pi\sqrt{\frac{m}{mg/L}} = 2\pi\sqrt{\frac{L}{g}}
The mass cancels. A heavier bob feels a bigger restoring force, but it also has more inertia, by exactly the same factor, so its acceleration at each point of the swing (and its period) stays the same. The AP equation sheet writes this equation as Tp=2πℓgT_p = 2\pi\sqrt{\frac{\ell}{g}}, using ℓ\ell for the length.
This formula only holds for small angles. Up to about 15°, the true period is within 0.5% of 2πLg2\pi\sqrt{\frac{L}{g}}. At 20° it’s about 0.8% longer, and at 30° about 1.7% longer. The reason is the restoring force: it’s really mgsin⁡θmg\sin\theta, and at larger angles sin⁡θ\sin\theta is noticeably smaller than θ\theta, so the restoring force is no longer proportional to the displacement. The pendulum still swings back and forth (it’s still periodic), but it isn’t SHM anymore, and its period grows a little as the amplitude grows.
7.2 - Frequency and Period of SHM

Application: Determining Gravitational Acceleration

The pendulum equation lets you experimentally measure gravitational acceleration. Starting from T=2πLgT = 2\pi\sqrt{\frac{L}{g}}: dividing by 2π2\pi gives T2π=Lg\frac{T}{2\pi} = \sqrt{\frac{L}{g}}, squaring both sides gives T24π2=Lg\frac{T^2}{4\pi^2} = \frac{L}{g}, cross multiplying gives gT2=4π2LgT^2 = 4\pi^2 L, and solving for gg:
g=4π2LT2g = \frac{4\pi^2 L}{T^2}
This method could, in principle, be used on other planets (Mars, the Moon, and so on) to find their gravitational acceleration, just by timing a pendulum of known length.

Linearizing Data for Lab Analysis

Both mass-spring and pendulum systems can be analyzed by linearizing their equations into straight-line graphs.
Mass-spring linearization: starting from T=2πmkT = 2\pi\sqrt{\frac{m}{k}}. Plotting TT vs. m\sqrt{m} gives a straight line with slope 2πk\frac{2\pi}{\sqrt{k}}, letting you solve for kk. Alternatively, squaring gives T2=4π2mkT^2 = 4\pi^2\frac{m}{k}, and plotting T2T^2 vs. mm gives a straight line with slope 4π2k\frac{4\pi^2}{k}, so k=4π2slopek = \frac{4\pi^2}{\text{slope}}. This method involves varying the mass and measuring how the period responds to determine the spring constant.
Pendulum linearization: starting from T=2πLgT = 2\pi\sqrt{\frac{L}{g}}. Plotting TT vs. L\sqrt{L} gives a straight line with slope 2πg\frac{2\pi}{\sqrt{g}}, letting you solve for gg. Alternatively, T2=4π2LgT^2 = 4\pi^2\frac{L}{g}, and plotting T2T^2 vs. LL gives a straight line with slope 4π2g\frac{4\pi^2}{g}, so g=4π2slopeg = \frac{4\pi^2}{\text{slope}}. This involves varying the pendulum length and measuring the resulting periods to find gravitational acceleration.

Worked Example: Finding g from Pendulum Data

A simple pendulum has length L=95L = 95 cm and period T=1.957T = 1.957 s. Find the local acceleration due to gravity.
Using g=4π2LT2g = \frac{4\pi^2L}{T^2}, with L=0.95L = 0.95 m:
g=4π2(0.95)(1.957)2=4(9.8696)(0.95)3.830=37.503.830≈9.79 m/s2g = \frac{4\pi^2(0.95)}{(1.957)^2} = \frac{4(9.8696)(0.95)}{3.830} = \frac{37.50}{3.830} \approx 9.79 \text{ m/s}^2
That’s very close to the standard value of 9.8 m/s².

Worked Example: Period of a Mass-Spring System

A mass m=0.80m = 0.80 kg is attached to a spring with k=125k = 125 N/m and set oscillating. Find the period and frequency.
Period:
T=2π0.80125=2π0.0064=2π(0.08)≈0.503 sT = 2\pi\sqrt{\frac{0.80}{125}} = 2\pi\sqrt{0.0064} = 2\pi(0.08) \approx 0.503 \text{ s}
Frequency:
f=1T=10.503≈1.99 Hzf = \frac{1}{T} = \frac{1}{0.503} \approx 1.99 \text{ Hz}
About 2.0 Hz, roughly 2 oscillations per second.

Worked Example: Comparing Two Pendulums

Pendulum A has length LA=1.5L_A = 1.5 m, Pendulum B has length LB=0.60L_B = 0.60 m, both on Earth. Find the ratio TATB\frac{T_A}{T_B}.
TATB=2πLAg2πLBg=LALB=1.50.60=2.5≈1.58\frac{T_A}{T_B} = \frac{2\pi\sqrt{\frac{L_A}{g}}}{2\pi\sqrt{\frac{L_B}{g}}} = \sqrt{\frac{L_A}{L_B}} = \sqrt{\frac{1.5}{0.60}} = \sqrt{2.5} \approx 1.58
Pendulum A’s period is about 1.58 times longer than Pendulum B’s.

Worked Example: Period and Frequency from a Count

A toy hanging from a spring completes 24 full oscillations in 15.0 s. Find its period and frequency.
T=15.0 s24=0.625 sf=1T=10.625 s=1.60 HzT = \frac{15.0\text{ s}}{24} = 0.625\text{ s} \qquad f = \frac{1}{T} = \frac{1}{0.625\text{ s}} = 1.60\text{ Hz}
Check: f=2415.0 s=1.60f = \frac{24}{15.0\text{ s}} = 1.60 Hz, the same answer. The 24 is an exact count, so the answers keep the three significant figures of 15.0 s. If your stopwatch reaction time is off by 0.2 s, that’s an error of less than 0.01 s in each period, since it’s spread over 24 oscillations.

Worked Example: Factors of Change

A 0.50 kg block on a spring oscillates with a period of 1.2 s. Find the new period if (a) the block is replaced with a 2.0 kg block, (b) the 0.50 kg block is hung from a spring that is twice as stiff, or (c) the original system is taken to the Moon, where g=1.6g = 1.6 m/s².
(a) The mass is multiplied by 4, and Ts∝mT_s \propto \sqrt{m}, so the period is multiplied by 4=2\sqrt{4} = 2: T=2(1.2 s)=2.4T = 2(1.2\text{ s}) = 2.4 s.
(b) kk is multiplied by 2, and Ts∝1kT_s \propto \frac{1}{\sqrt{k}}, so the period is divided by 2\sqrt{2}: T=1.2 s2≈0.85T = \frac{1.2\text{ s}}{\sqrt{2}} \approx 0.85 s.
(c) Ts=2πmkT_s = 2\pi\sqrt{\frac{m}{k}} has no gg in it, so the period is still 1.2 s. The spring stretches less when the block hangs at rest on the Moon, but that only moves the equilibrium position.

Worked Example: A Pendulum on the Moon

A pendulum has a period of 2.0 s on Earth. Find its period on the Moon, where g=1.6g = 1.6 m/s² (use g=10g = 10 m/s² for Earth). Set up a ratio so the length cancels:
TMoonTEarth=2πL/gMoon2πL/gEarth=gEarthgMoon=101.6=2.5\frac{T_{\text{Moon}}}{T_{\text{Earth}}} = \frac{2\pi\sqrt{L/g_{\text{Moon}}}}{2\pi\sqrt{L/g_{\text{Earth}}}} = \sqrt{\frac{g_{\text{Earth}}}{g_{\text{Moon}}}} = \sqrt{\frac{10}{1.6}} = 2.5TMoon=2.5(2.0 s)=5.0 sT_{\text{Moon}} = 2.5(2.0\text{ s}) = 5.0\text{ s}
Weaker gravity means a weaker restoring force on the same mass, so the bob speeds up more slowly and each swing takes longer. Compare this with part (c) of the last example: the spring’s period didn’t change on the Moon, but the pendulum’s more than doubled.

Worked Example: Finding the Spring Constant from a Graph

A student hangs different masses from the same spring, pulls each one down a few centimeters, and times 10 full oscillations. Sample data are below. Find the spring constant using a graph.
Mass mm (kg)
Time for 10 oscillations (s)
Period TT (s)
T2T^2 (s²)
0.20
9.0
0.90
0.81
0.40
12.5
1.25
1.56
0.60
15.5
1.55
2.40
0.80
17.7
1.77
3.13
1.00
19.9
1.99
3.96
Choosing what to graph: TT vs. mm would curve, because T∝mT \propto \sqrt{m}. Squaring Ts=2πmkT_s = 2\pi\sqrt{\frac{m}{k}} gives a straight-line form:
T2=(4π2k)m(y=slope×x)T^2 = \left(\frac{4\pi^2}{k}\right)m \qquad (y = \text{slope} \times x)
So plot T2T^2 on the vertical axis and mm on the horizontal axis. The points should fall on a line through the origin with a slope of 4π2k\frac{4\pi^2}{k}.
7.2 - Frequency and Period of SHM
Slope: draw one best-fit line through the data (not a line connecting the first and last points), then pick two points on the line that are far apart. Here, (0.10 kg, 0.40 s²) and (0.90 kg, 3.55 s²):
slope=3.55 s2−0.40 s20.90 kg−0.10 kg=3.15 s20.80 kg≈3.94 s2/kg\text{slope} = \frac{3.55\text{ s}^2 - 0.40\text{ s}^2}{0.90\text{ kg} - 0.10\text{ kg}} = \frac{3.15\text{ s}^2}{0.80\text{ kg}} \approx 3.94\text{ s}^2/\text{kg}k=4π2slope=39.483.94 s2/kg≈10.0 N/mk = \frac{4\pi^2}{\text{slope}} = \frac{39.48}{3.94\text{ s}^2/\text{kg}} \approx 10.0\text{ N/m}
The units work out because kgs2=kg⋅m/s2m=N/m\frac{\text{kg}}{\text{s}^2} = \frac{\text{kg}\cdot\text{m/s}^2}{\text{m}} = \text{N/m}. Using the slope of a best-fit line instead of a single trial averages out the random timing errors. The line also passes very close to the origin, as the equation predicts, which is a good sign the model fits.
Procedure tips: keep the amplitude small (it doesn’t change the period, but big bounces can make the spring swing sideways), start and stop timing as the mass passes through equilibrium, where it moves fastest and the moment is easiest to judge, and repeat each trial a few times and average.

Common Mistakes

Thinking amplitude affects period: for ideal SHM, period never depends on amplitude, pulling a spring 5 cm or 10 cm doesn’t change the period, and neither does displacing a pendulum 10° or 15° (within the small angle approximation).
Confusing the mass-spring and pendulum formulas: mass-spring is T=2πmkT = 2\pi\sqrt{\frac{m}{k}} (mass in the numerator), while the pendulum is T=2πLgT = 2\pi\sqrt{\frac{L}{g}} (no mass dependence at all), don’t mix these up.
Using the pendulum formula for large angles: it only holds for small angles, under about 15° (where the error in the period is under about 0.5%), larger angles need more complex analysis.
Forgetting unit conversions: length has to be in meters, period in seconds, always convert before plugging into the equations.
Confusing angular frequency with angular velocity: in oscillations, ω=2πf\omega = 2\pi f is angular frequency, in rotation, ω\omega is angular velocity, same symbol, different context.
Algebra errors solving for gg or kk: squaring T=2πLgT = 2\pi\sqrt{\frac{L}{g}} properly gives g=4π2LT2g = \frac{4\pi^2 L}{T^2}, not 2πLT\frac{2\pi L}{T}, the 2π2\pi becomes 4π24\pi^2 once squared.
Using diameter instead of length for a pendulum: LL is the distance from the pivot to the bob’s center of mass, not the bob’s diameter, and not the total length of string plus bob.
Thinking stiffer springs have longer periods: it’s the opposite, stiffer springs (larger kk) have shorter periods, since kk sits in the denominator of T=2πmkT = 2\pi\sqrt{\frac{m}{k}}.
Plotting the wrong variables when linearizing: TT vs. mm isn’t linear, you need TT vs. m\sqrt{m} or T2T^2 vs. mm to get a straight line, check that your chosen variables actually give a y=mx+by = mx + b form.
Forgetting multiple trials in lab design: always collect multiple data points, vary the independent variable (mass for springs, length for pendulums), and measure the period more than once for each setup to reduce error.

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