contestada

The central star of a planetary nebula emits ultraviolet light with wavelength 104nm. This light passes through a diffraction grating with 5000 slits per mm. What is the first-order diffraction angle?

Respuesta :

Answer: 31.33 degrees

Explanation:

The diffraction angles [tex]\theta_{n}[/tex] when we have a slit divided into [tex]n[/tex] parts are obtained by  the following equation:

[tex]dsin\theta_{n}=n\lambda[/tex]   (1)

Where:

[tex]d[/tex] is the width of the slit

[tex]\lambda[/tex]  is the wavelength of the light

[tex]n[/tex] is an integer different from zero.

Now, the first-order diffraction angle is given when [tex]n=1[/tex], hence equation (1) becomes:

[tex]dsin\theta_{1}=\lambda[/tex]   (2)

Now we have to find the value of [tex]\theta_{1}[/tex]:

[tex]sin\theta_{1}=\frac{\lambda}{d}[/tex]  

[tex]\theta_{1}=arcsin(\frac{\lambda}{d})[/tex]   (3)

We know:

[tex]\lambda=104nm=104(10)^{-9}m[/tex]

In addition we are told the diffraction grating has 5000 slits per mm, this means:

[tex]d=\frac{1mm}{5000}=\frac{1(10)^{-3}m}{5000}[/tex]

Substituting the known values in (3):

[tex]\theta_{1}=arcsin(\frac{104(10)^{-9}m}{\frac{1(10)^{-3}m}{5000}})[/tex]

[tex]\theta_{1}=arcsin(0.52)[/tex]

Finally:

[tex]\theta_{1}=31.33\º[/tex] >>>This is the first-order diffraction angle