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ScienceQuest
Waves & Optics Practice School

Waves Practice Problems

Waves and optics practice problems on wave speed, refraction, lenses, photon energy and decibels, marked to within 1.5 percent with the working shown.

Practice

Question 1 of 40

Wavelength and Frequency Calculator

Frequency
f = 1700 THz
Wave speed
v = 2.998 × 10⁸ m/s
nm

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Worked answers

The first ten questions from the set above, each with its answer and the working that gets there. The working is carried out in the units each equation takes, so its last line can show the answer before it is converted.

  1. Frequency
    f = 1700 THz
    Wave speed
    v = 2.998 × 10⁸ m/s

    Find the wavelength (λ).

    Show the answer and working

    Answer λ = 176.3 nm

    Rearranged λ = v ÷ f

    1. lambda = v / f
    2. = 2.99792 × 10⁸ m/s / 1700 THz
    3. = 2.99792 × 10⁸ / (1.7 × 10¹⁵)
    4. = 1.763 × 10⁻⁷ m = 176.35 nm

    Check it with the Wavelength and Frequency Calculator.

  2. Photon energy
    E = 8.5 eV

    Find the wavelength (λ).

    Show the answer and working

    Answer λ = 145.9 nm

    Rearranged λ = hc ÷ E

    1. lambda = h c / E
    2. h c = 1.9864 × 10⁻²⁵ J m
    3. = 1.9864 × 10⁻²⁵ / (1.362 × 10⁻¹⁸ J)
    4. = 1.459 × 10⁻⁷ m = 145.86 nm

    Check it with the Photon Energy Calculator.

  3. Refractive index, medium 1
    n₁ = 2.2
    Angle of incidence
    θ₁ = 32°
    Refractive index, medium 2
    n₂ = 1.3

    Find the angle of refraction (θ₂).

    Show the answer and working

    Answer θ₂ = 63.74°

    Rearranged θ₂ = arcsin(n₁ sin θ₁ / n₂)

    1. n1 sin(t1) = n2 sin(t2)
    2. sin(t2) = 2.2 x sin(32 deg) / 1.3
    3. sin(t2) = 0.89679
    4. t2 = 63.74 deg

    Check it with the Snell’s Law Calculator.

  4. Focal length
    f = 16 cm
    Image distance
    dᵢ = 37 cm

    Find the object distance (dₒ).

    Show the answer and working

    Answer dₒ = 28.19 cm

    Rearranged 1/dₒ = 1/f − 1/dᵢ

    1. 1/f = 1/do + 1/di
    2. 1/0.16 = 1/0.2819 + 1/0.37

    Check it with the Thin Lens Calculator.

  5. Sound level
    L = 22 dB
    Reference intensity
    I₀ = 1 pW/m²

    Find the intensity (I).

    Show the answer and working

    Answer I = 0.0001585 µW/m²

    Rearranged I = I₀ × 10^(L ÷ 10)

    1. I = I0 x 10^(L / 10)
    2. = 1 × 10⁻¹² x 10^(22 / 10)
    3. = 1 × 10⁻¹² x 10^2.2
    4. = 1.585 × 10⁻¹⁰ W/m2 = 0.00015849 uW/m2

    Check it with the Decibel Calculator.

  6. Wavelength
    λ = 2100 nm
    Wave speed
    v = 2.998 × 10⁸ m/s

    Find the frequency (f).

    Show the answer and working

    Answer f = 142.8 THz

    Rearranged f = v ÷ λ

    1. f = v / lambda
    2. = 2.99792 × 10⁸ m/s / 2.1 um
    3. = 2.99792 × 10⁸ / (2.1 × 10⁻⁶ m)
    4. = 1.4276 × 10¹⁴ Hz = 142.76 THz

    Check it with the Wavelength and Frequency Calculator.

  7. Wavelength
    λ = 1100 nm

    Find the photon energy (E).

    Show the answer and working

    Answer E = 1.127 eV

    Rearranged E = hc ÷ λ

    1. E = h c / lambda
    2. h c = 6.62607 × 10⁻³⁴ x 2.99792 × 10⁸ = 1.9864 × 10⁻²⁵ J m
    3. = 1.9864 × 10⁻²⁵ / (1.1 × 10⁻⁶ m)
    4. = 1.806 × 10⁻¹⁹ J = 1.1271 eV

    Check it with the Photon Energy Calculator.

  8. Refractive index, medium 1
    n₁ = 2
    Refractive index, medium 2
    n₂ = 1.5
    Angle of refraction
    θ₂ = 81°

    Find the angle of incidence (θ₁).

    Show the answer and working

    Answer θ₁ = 47.8°

    Rearranged θ₁ = arcsin(n₂ sin θ₂ / n₁)

    1. n1 sin(t1) = n2 sin(t2)
    2. 2 x sin(47.8) = 1.5 x sin(81)

    Check it with the Snell’s Law Calculator.

  9. Wavelength
    λ = 230 nm
    Wave speed
    v = 2.998 × 10⁸ m/s

    Find the frequency (f).

    Show the answer and working

    Answer f = 1303 THz

    Rearranged f = v ÷ λ

    1. f = v / lambda
    2. = 2.99792 × 10⁸ m/s / 230 nm
    3. = 2.99792 × 10⁸ / (2.3 × 10⁻⁷ m)
    4. = 1.3034 × 10¹⁵ Hz = 1303.4 THz

    Check it with the Wavelength and Frequency Calculator.

  10. Photon energy
    E = 3.9 eV

    Find the wavelength (λ).

    Show the answer and working

    Answer λ = 317.9 nm

    Rearranged λ = hc ÷ E

    1. lambda = h c / E
    2. h c = 1.9864 × 10⁻²⁵ J m
    3. = 1.9864 × 10⁻²⁵ / (6.248 × 10⁻¹⁹ J)
    4. = 3.179 × 10⁻⁷ m = 317.91 nm

    Check it with the Photon Energy Calculator.

Fix the geometry before the algebra

Optics problems are geometry with a formula attached, so draw the surface and the normal before writing anything down. Every angle in refraction is measured from the normal, the line perpendicular to the surface, so a ray striking glass at 20 degrees to the surface has an angle of incidence of 70 degrees. Note which medium is the denser one, because that decides which way the ray bends.

Then convert. Wavelengths are quoted in nanometres and the formulas want metres, so 550 nm is 5.5 × 10⁻⁷ m, and a terahertz is 10¹² hertz. For lenses, settle the sign convention first: a converging lens has a positive focal length and a positive image distance means a real image.

The conventions that cost marks

  • Angles taken from the surface. The single most common error in refraction, and it produces an answer that still looks like an angle.
  • The ratio of angles instead of the ratio of sines. Light entering water at 30 degrees refracts to 22.03 degrees, from 1 × sin 30 = 1.333 × sin θ₂. Dividing 30 by 1.333 gives 22.5, close enough to pass unnoticed.
  • Decibels added. Two 60 dB sources together make 63 dB, not 120, because doubling the intensity adds 3.01 dB. Intensities are what add.
  • Nanometres left in place. A wavelength entered as 550 rather than 5.5 × 10⁻⁷ puts the frequency out by 10⁹, which lands a green photon in the radio band.
  • A negative image distance read as an error. It is the answer: the image is virtual, on the same side as the object, which is what happens when the object sits inside the focal length.

Two checks that catch most slips

For photons, E = 1239.84 / λ gives the energy in electronvolts from a wavelength in nanometres. A 550 nm green photon is 2.25 eV, and the visible range spans about 1.59 eV at 780 nm to 3.26 eV at 380 nm. The wave equation pairs with it: 550 nm in vacuum is 545 THz.

For refraction, direction is the check: light entering a denser medium always bends toward the normal, so the refracted angle is the smaller one. A critical angle exists only going the other way, at 48.6 degrees for water into air, 41.1 degrees for crown glass at 1.52 and 24.4 degrees for diamond. Sound levels scale in tens: a factor of ten in intensity is 10 dB, and doubling the distance from a point source costs 6.02 dB.

What changes at a boundary and what does not

When light crosses into a denser medium its speed and wavelength both drop by the factor n, while its frequency does not change, because frequency is set by the source. Light at 550 nm in vacuum is 413 nm inside water, still 545 THz, and still green.

A decibel level is a ratio rather than a quantity, referenced for airborne sound to the threshold of hearing at 1 × 10⁻¹² W/m², so 60 dB means a million times that intensity. And the speed of sound depends on the medium and its temperature, about 343 m/s in air at 20 °C, which makes a 440 Hz tone 0.78 m long.

Common questions

Do I have to match the number of significant figures?

No. An answer counts as correct within 1.5 percent of the computed value, so three significant figures carried through the working is always enough, and rounding an intermediate step will not fail you. The tolerance is relative rather than absolute because answers on this topic run from picowatts per square metre to hundreds of terahertz.

Are the angles measured from the normal or from the surface?

From the normal, the line perpendicular to the surface, which is the standard convention and the one the calculators use. So an angle of incidence of 70 degrees describes a ray at 20 degrees to the surface itself, close to grazing. Answers are marked against the same convention, which means an angle measured from the surface will be marked wrong even when the arithmetic behind it was sound.