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When monochromatic light is incident on a slit \(22.0 \mu \mathrm{m}\) wide, the first diffraction minimum lies at \(1.80^{\circ}\) from the direction of the incident light. What is the wavelength?

Short Answer

Expert verified
The wavelength is approximately 691 nm.

Step by step solution

01

Understanding the Formula for Diffraction Minimum

For a single slit diffraction pattern, the formula for the angle of the diffraction minimum is given by \( a \sin \theta = m \lambda \), where \(a\) is the slit width, \(\theta\) is the angle of the diffraction minimum, \(m\) is the order of the minimum (\(m = 1\) for the first minimum), and \(\lambda\) is the wavelength of the light. In this problem, we know \(a = 22.0 \times 10^{-6} \text{ m}\), \(\theta = 1.80\degree \), and \(m = 1\). We need to solve for \(\lambda\).
02

Convert Angle to Radians

To use the formula \( a \sin \theta = m \lambda \), the angle must be in radians. We convert the angle \(1.80\degree \) to radians using the conversion \(1 \, \text{degree} = \frac{\pi}{180} \, \text{radians}\): \(1.80\degree \times \frac{\pi}{180} = 0.03142 \, \text{radians}\).
03

Substitute Values into the Formula

With all known values, substitute into the formula: \(22.0 \times 10^{-6} \times \sin(0.03142) = 1 \times \lambda\). Solve for \(\lambda\): \(\lambda = 22.0 \times 10^{-6} \times \sin(0.03142)\).
04

Calculate the Wavelength

Calculate the sine: \(\sin(0.03142) \approx 0.03139\). Then calculate \(\lambda: \lambda = 22.0 \times 10^{-6} \times 0.03139 = 0.00069058 \times 10^{-6} \text{ m}\). Adjusting the scientific notation: \(\lambda \approx 6.91 \times 10^{-7} \text{ m} \) or \(691 \, \text{nm}\) after converting meters to nanometers by multiplying by \(10^9\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Wavelength Calculation
When studying diffraction, an important concept to grasp is how to calculate the wavelength of light involved. The wavelength is a key property of light, reflecting how long one complete cycle of the wave is. In the context of diffraction, we use the equation \[ a \sin \theta = m \lambda \] where \( \lambda \) is the wavelength and is what we're solving for.
  • \( a \) represents the slit width.
  • \( \theta \) is the angle of diffraction (calculated in radians).
  • \( m \) is the order of the minimum, for the first minimum \( m = 1 \).
By rearranging the equation, \[ \lambda = \frac{a \sin \theta}{m} \] you can easily substitute known values to find the wavelength. Remember to ensure the angle \( \theta \) is converted from degrees to radians before calculating! This conversion is crucial since the trigonometric functions use radians.
Slit Width
The slit width, denoted as \( a \), plays a critical role in the diffraction process. It is defined as the distance between two edges of the slit through which light travels. In our exercise, the slit width is given as \( 22.0 \, \mu \text{m} \) or \( 22.0 \times 10^{-6} \text{ m} \).
  • A smaller slit width results in more spreading or wider diffraction patterns due to the way light waves bend around the edges.
  • Larger slit widths result in sharper, more narrow diffraction patterns.
Adjusting the slit width can help focus or spread the light accordingly, which is why precision in measuring this value is crucial in experiments involving diffraction.
Angle of Diffraction
The angle of diffraction, represented as \( \theta \), is the angle between the direction of the incident light and the direction of the minimum in the diffraction pattern. In this exercise, we have an angle of \( 1.80^{\circ} \).
Before using it in calculations, always convert this angle into radians because: \[ 1 \text{ degree} = \frac{\pi}{180} \text{ radians} \] By converting \( 1.80^{\circ} \) we find it equals approximately \( 0.03142 \text{ radians} \).
  • This conversion allows the calculation of sine values accurately which is then applied in the diffraction formula.
  • Different angles result in different diffraction patterns as they dictate the position of minima and maxima.
Monochromatic Light
Monochromatic light refers to light that has a single wavelength or color. It consists of electromagnetic waves all having the same frequency. In diffraction experiments, using monochromatic light simplifies calculations and observations, as the patterns formed are more predictable due to the uniformity of the light wave properties.
  • Common sources of monochromatic light include lasers or specific discharge lamps.
  • The consistency in wavelength allows for precise investigations of diffraction patterns and aids in the measurement of physical properties like slit width or wavelength itself.
In practical applications, monochromatic light allows scientists and engineers to explore wave properties without the complexity introduced by variables that come with white or polychromatic light sources. This setup ensures high accuracy in diffraction experiments.

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Most popular questions from this chapter

Millimeter-wave radar generates a narrower beam than conventional microwave radar, making it less vulnerable to antiradar missiles than conventional radar. (a) Calculate the angular width \(2 \theta\) of the central maximum, from first minimum to first minimum, produced by a 220 GHz radar beam emitted by a \(55.0-\) cm-diameter circular antenna. (The frequency is chosen to coincide with a low-absorption atmospheric "window.") (b) What is \(2 \theta\) for a more conventional circular antenna that has a diameter of \(2.3\) \(\mathrm{m}\) and emits at wavelength \(1.6 \mathrm{~cm} ?\)

The \(D\) line in the spectrum of sodium is a doublet with wavelengths \(589.0\) and \(589.6 \mathrm{~nm}\). Calculate the minimum number of lines needed in a grating that will resolve this doublet in the secondorder spectrum.

What is the smallest Bragg angle for \(x\) rays of wavelength 30 \(\mathrm{pm}\) to reflect from reflecting planes spaced \(0.30 \mathrm{~nm}\) apart in a calcite crystal?

The telescopes on some commercial surveillance satellites can resolve objects on the ground as small as \(85 \mathrm{~cm}\) across (see Google Earth), and the telescopes on military surveillance satellites reportedly can resolve objects as small as \(10 \mathrm{~cm}\) across. Assume first that object resolution is determined entirely by Rayleigh's criterion and is not degraded by turbulence in the atmosphere. Also assume that the satellites are at a typical altitude of \(400 \mathrm{~km}\) and that the wavelength of visible light is \(550 \mathrm{~nm}\). What would be the required diameter of the telescope aperture for (a) \(85 \mathrm{~cm}\) resolution and (b) \(10 \mathrm{~cm}\) resolution? (c) Now, considering that turbulence is certain to degrade resolution and that the aperture diameter of the Hubble Space Telescope is \(2.4 \mathrm{~m}\), what can you say about the answer to (b) and about how the military surveillance resolutions are accomplished?

The wings of tiger beetles (Fig. \(36-41\) ) are colored by interference due to thin cuticle-like layers. In addition, these layers are arranged in patches that are \(60 \mu \mathrm{m}\) across and produce different colors. The color you see is a pointillistic mixture of thin-film interference colors that varies with perspective. Approximately what viewing distance from a wing puts you at the limit of resolving the different colored patches according to Rayleigh's criterion? Use \(550 \mathrm{~nm}\) as the wavelength of light and 3,00 mm as the diameter of your pupil.

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