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Exercises · 2.7

Q.Calculate the wavelength, frequency and wavenumber of a light wave whose period is 2.0×10−10 s2.0 \times 10^{-10}\ s.

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The key idea is that wavelength, frequency, and wavenumber are all linked through the speed of light and the period. Given the period T=2.0×10−10 sT = 2.0 \times 10^{-10}\ \text{s}, the frequency is f=5.0×109 Hzf = 5.0 \times 10^{9}\ \text{Hz}, the wavelength is λ=0.06 m\lambda = 0.06\ \text{m} (or 6.0 cm6.0\ \text{cm}), and the wavenumber is νˉ≈16.7 m−1\bar{\nu} \approx 16.7\ \text{m}^{-1}.


Concept and Intuition

When we talk about a light wave, its period TT is the time it takes for one complete oscillation at a fixed point. The frequency ff is simply how many such oscillations happen per second — they are reciprocals: f=1/Tf = 1/T.

Once we know the frequency, the wavelength λ\lambda tells us the spatial distance between successive crests. For any electromagnetic wave in vacuum, the product of wavelength and frequency equals the speed of light cc: λf=c\lambda f = c.

The wavenumber νˉ\bar{\nu} (often denoted by ν~\tilde{\nu} or kk in different contexts) is the number of wavelengths per unit distance. In spectroscopy, it's usually defined as νˉ=1/λ\bar{\nu} = 1/\lambda, giving units of m−1\text{m}^{-1} (or cm−1\text{cm}^{-1}).

So the path is: period → frequency → wavelength → wavenumber. Each step uses a simple relation, but the key is to keep track of units and not confuse angular wavenumber (k=2π/λk = 2\pi/\lambda) with the spectroscopic wavenumber (1/λ1/\lambda). The problem asks for "wavenumber" in the simplest sense — so we'll use 1/λ1/\lambda.


Step-by-Step Solution

1. Find the frequency from the period.

The period TT is given as 2.0×10−10 s2.0 \times 10^{-10}\ \text{s}. Frequency is the reciprocal:

f=1T=12.0×10−10=5.0×109 s−1f = \frac{1}{T} = \frac{1}{2.0 \times 10^{-10}} = 5.0 \times 10^{9}\ \text{s}^{-1}

Since 1 s−1=1 Hz1\ \text{s}^{-1} = 1\ \text{Hz}, we have f=5.0×109 Hzf = 5.0 \times 10^{9}\ \text{Hz}.

Tip

A quick check: 10−1010^{-10} s is 0.1 nanosecond. The reciprocal gives 101010^{10} Hz, but here it's 2.0×10−102.0 \times 10^{-10}, so half that — 5×1095 \times 10^{9} Hz. That's in the microwave region of the EM spectrum.

2. Calculate the wavelength using c=λfc = \lambda f.

The speed of light in vacuum is c=3.0×108 m/sc = 3.0 \times 10^{8}\ \text{m/s}. Rearranging:

λ=cf=3.0×1085.0×109=0.06 m\lambda = \frac{c}{f} = \frac{3.0 \times 10^{8}}{5.0 \times 10^{9}} = 0.06\ \text{m}

That's 6.0×10−2 m6.0 \times 10^{-2}\ \text{m}, or 6.0 cm6.0\ \text{cm}. …

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