Lab Manual: Resolving Power of Plane Diffraction Grating

To Determine the Resolving Power of a Plane Diffraction Grating

1 Aim

To determine the Resolving Power of a plane diffraction grating using sodium light and to verify the theoretical relationship between resolving power and the order of diffraction.

2 Apparatus Used

Spectrometer: For measuring angles of diffraction accurately
Plane Diffraction Grating: With known grating element (e.g., 15000 lines/inch)
Sodium Lamp: Source of sodium doublet (λ₁ = 5890 Å, λ₂ = 5896 Å)
Convex Lens: For collimating light from the source
Reading Lens: For precise observation of spectral lines
Spirit Level: For leveling the spectrometer

3 Diagram

Diagram of Diffraction Grating Setup
(Insert experimental setup diagram here showing spectrometer, grating, and light source arrangement)

Figure: Experimental setup for determining resolving power of plane diffraction grating

4 Theory

A diffraction grating is an optical component with a periodic structure that splits and diffracts light into several beams traveling in different directions. The resolving power of a grating is its ability to separate two spectral lines of nearly equal wavelengths.

When monochromatic light falls normally on a plane diffraction grating, it gets diffracted according to the grating equation. For sodium light, which consists of a doublet with wavelengths λ₁ = 5890 Å and λ₂ = 5896 Å, the resolving power can be determined by observing the separation of these two lines in different orders of diffraction.

The theoretical resolving power of a grating is given by the product of the order of diffraction (m) and the total number of lines (N) illuminated on the grating. Higher orders of diffraction provide better resolution, allowing us to distinguish between closely spaced spectral lines.

The angular dispersion of the grating increases with the order of diffraction, making it easier to resolve the sodium doublet in higher orders. This experiment demonstrates the fundamental relationship between the physical parameters of the grating and its optical resolving capability.

5 Formula

Grating Equation:
$$d \sin \theta = m\lambda$$

where d = grating element, θ = angle of diffraction, m = order, λ = wavelength

Theoretical Resolving Power:
$$R_t = mN$$

where m = order of diffraction, N = total number of lines illuminated

Practical Resolving Power:
$$R_p = \frac{\bar{\lambda}}{\Delta\lambda}$$

where $\bar{\lambda}$ = mean wavelength, Δλ = difference in wavelengths

For Sodium Doublet:
$$\bar{\lambda} = \frac{\lambda_1 + \lambda_2}{2} = \frac{5890 + 5896}{2} = 5893 \text{ Å}$$ $$\Delta\lambda = \lambda_2 - \lambda_1 = 5896 - 5890 = 6 \text{ Å}$$ $$R_p = \frac{5893}{6} = 982.17$$
Number of Lines Illuminated:
$$N = \frac{W}{d}$$

where W = width of grating illuminated, d = grating element

6 Procedure

Adjust the spectrometer for parallel rays by setting the collimator and telescope for parallel light. Use the spirit level to ensure the instrument is properly leveled.
Mount the plane diffraction grating on the prism table with its surface perpendicular to the collimator axis. The grating lines should be vertical.
Illuminate the collimator slit with sodium light. Adjust the slit width to obtain clear, sharp spectral lines while maintaining sufficient intensity.
Observe the direct beam (zero order) through the telescope and set the vernier readings to zero or note the initial reading.
Rotate the telescope to observe the first-order spectrum on one side. Carefully examine the sodium doublet and determine if the two lines are resolved (clearly separated).
Measure the angle of diffraction for the first-order spectrum. Record whether the sodium doublet is resolved or not.
Repeat the observations for the first-order spectrum on the other side of the direct beam to minimize systematic errors.
Similarly, observe and measure the angles for second-order and third-order spectra on both sides, noting the resolution of the doublet in each case.
For each order where the doublet is resolved, calculate the practical resolving power and compare with the theoretical value.
Record all observations systematically and calculate the grating element using the grating equation for verification.

7 Observation Table

Given Data:

  • Grating specification: _______ lines per inch
  • Grating element (d): _______ cm
  • Width of grating illuminated (W): _______ cm
  • Sodium wavelengths: λ₁ = 5890 Å, λ₂ = 5896 Å
Order of Diffraction (m) Left Side Right Side Mean Angle θ Doublet Resolved? Calculated λ (Å)
Position 1 Position 2 Position 1 Position 2
1
2
3

8 Calculations

Sample Calculation for Order m = 2:

Step 1: Calculate grating element if not given:

$$d = \frac{2.54}{N_{lines/inch}} \text{ cm}$$

Step 2: Verify grating equation:

$$\lambda = \frac{d \sin \theta}{m}$$

Step 3: Calculate theoretical resolving power:

$$R_t = mN = m \times \frac{W}{d}$$

Step 4: Calculate practical resolving power:

$$R_p = \frac{\bar{\lambda}}{\Delta\lambda} = \frac{5893}{6} = 982.17$$

Step 5: Compare theoretical and practical values:

$$\text{Percentage difference} = \frac{|R_t - R_p|}{R_t} \times 100\%$$

Calculation Space:

Show detailed calculations for each order of diffraction here...





9 Result

Experimental Results:

1. Minimum order at which sodium doublet is resolved: _____ order


2. Resolving power values:

  • Theoretical resolving power (Rt): _____
  • Practical resolving power (Rp): 982.17
  • Percentage difference: _____%

3. Verification of grating equation:

Calculated wavelength: _____ Å (Expected: ~5893 Å)


4. Conclusion:

The resolving power of the plane diffraction grating increases linearly with the order of diffraction, confirming the theoretical relationship R = mN. The sodium doublet becomes clearly resolved from the _____ order onwards.

10 Precautions

  • Ensure the spectrometer is properly leveled using the spirit level before starting measurements.
  • The grating surface should be clean and free from dust. Handle it carefully to avoid scratches.
  • Mount the grating perpendicular to the collimator axis with grating lines vertical.
  • Use minimum slit width that still provides clear visibility of spectral lines to improve resolution.
  • Allow the sodium lamp to warm up completely before taking measurements for stable light output.
  • Take readings from both sides of the direct beam to minimize systematic errors.
  • Avoid parallax error while reading the vernier scale. Keep the eye in line with the scale.
  • Do not force the telescope or prism table movements. Use gentle, smooth motions.
  • Record observations immediately to avoid confusion and ensure accuracy.
  • Check the alignment frequently, especially after handling the instrument.

11 Viva Voice Questions

What is meant by resolving power of a diffraction grating?
Why does resolving power increase with the order of diffraction?
What is the difference between theoretical and practical resolving power?
Why is sodium light preferred for this experiment?
What is the significance of the grating element in diffraction?
How does the width of the illuminated grating affect resolving power?
What happens to the intensity of spectral lines with increasing order?
Explain the condition for just resolving two spectral lines.
What is the difference between transmission and reflection gratings?
How is angular dispersion related to resolving power?
What are the advantages of diffraction grating over prism for spectroscopy?
Explain the formation of secondary maxima in diffraction pattern.

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