Spectral lines in the emission spectrum for an electron at n= 3

In summary, the conversation discusses the possible paths of an excited electron in a simplified model of hydrogen and the number of lines that can be produced in an emission spectrum. It is noted that the assumption is that there is only one energy value for each value of n and that three lines can be produced corresponding to the initial state n = 3.
  • #1
Pushoam
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Homework Statement
Find the spectral lines of in the emission spectrum for an electron excited to 3rd Orbit.
Relevant Equations
One line belonging to n=3 to n =1or two lines belonging to n=3 to n =2 and then n=2 to =1.
Since there is only one excited electron, it could come from n=3 to n =1directly or n=3 to n =2 and then n=2 to =1.

Hence, there could be one or two lines depending upon the path taken by electron.
Is this right?
 
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  • #2
Yes. This assumes you're considering a simplified model of hydrogen, say, where effects due to electron spin are ignored. In particular, the assumption here is that there is only one energy value corresponding to a particular value of n.

Instead of saying there could be one or two lines depending upon the path taken by the electron, I think most people would say there are three lines that can be produced corresponding to the initial state n = 3. This is because emission spectra are usually generated by repeated transitions from many atoms. Some of these transitions are directly from ##3 \rightarrow 1## and some are the indirect ##3 \rightarrow 2 \rightarrow 1##. So, all three lines would occur in the spectrum. But you are thinking about it correctly.
 
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  • #3
Thank you.
 
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FAQ: Spectral lines in the emission spectrum for an electron at n= 3

What are spectral lines in the emission spectrum?

Spectral lines in the emission spectrum are distinct wavelengths of light emitted by electrons when they transition from a higher energy level to a lower one. Each element has a unique set of spectral lines, acting like a fingerprint for that element.

What transitions produce spectral lines for an electron at n=3?

For an electron at n=3, spectral lines are produced when the electron transitions to lower energy levels, such as n=2 or n=1. These transitions release energy in the form of photons, which correspond to specific wavelengths of light.

What is the Balmer series in relation to n=3?

The Balmer series refers to the set of spectral lines emitted when an electron transitions from a higher energy level (n ≥ 3) to n=2. For an electron at n=3, the transition to n=2 produces a spectral line in the visible region of the electromagnetic spectrum.

Why are spectral lines important in spectroscopy?

Spectral lines are crucial in spectroscopy because they allow scientists to identify the elements present in a sample. By analyzing the wavelengths of emitted light, researchers can determine the composition and properties of distant stars, gases, and other substances.

How do energy level transitions determine the wavelength of spectral lines?

The energy difference between the initial and final energy levels of an electron determines the wavelength of the emitted photon. Larger energy differences result in shorter wavelengths (higher energy photons), while smaller energy differences produce longer wavelengths (lower energy photons).

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