Balmer Series & Lyman Series

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In summary: You may want to try substituting 1 for R in the equation to see if that provides a more accurate answer.
  • #1
ussrasu
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Q: What are the widths of the wavelength intervals over which (a) the Lyman series and (b) the Balmer series extend? (Each width begins at the longest wavelength and ends at the series limit.) (c) What are the widths of the corresponding frequency intervals? Express the frequency intervals in tetrahertz (1THz = 10^12 Hz).

Dont understand what to do - and don't really understand Balmer and Lyman Series either - Any help with this question would be appreciated - thankyou!
 
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  • #2
ussrasu said:
Q: What are the widths of the wavelength intervals over which (a) the Lyman series and (b) the Balmer series extend? (Each width begins at the longest wavelength and ends at the series limit.) (c) What are the widths of the corresponding frequency intervals? Express the frequency intervals in tetrahertz (1THz = 10^12 Hz).
Dont understand what to do - and don't really understand Balmer and Lyman Series either - Any help with this question would be appreciated - thankyou!

Does your text not explain what these are, especially in the context of the Rydberg or hydrogen atom?

http://hyperphysics.phy-astr.gsu.edu/hbase/hyde.html#c2

Zz.
 
  • #3
Yeh but what i don't understand is how many different energy levels there are for each of the series? Like does it go on forever or does it stop at a certain number? Ie they start at n = 2 or n = 3, but where do they stop? Do they go up to infinity? Is it as simple as plugging the number in for each energy level into the formula and determining the wavelength?

Thanks
 
  • #4
ussrasu said:
Yeh but what i don't understand is how many different energy levels there are for each of the series? Like does it go on forever or does it stop at a certain number?

In theory, they go to [itex]n=\infty[/itex]. In practice, this isn't the case, but you need not worry about such technicalities for this problem. Consider them to go to infinity.


Is it as simple as plugging the number in for each energy level into the formula and determining the wavelength?

Yup, though perhaps you should type out the formula you're using and tell us how you plan to use it to solve the problem.
 
  • #5
The formula is 1/lamba = R (1/2^2 - 1/n^2)

sorry if that doesn't make sense

But i will put in the number 2 in n for one wavelength and infinity for the other wavelength - and then subtract the 2 answers to get the wavelength range?

Is this along the right lines?
 
  • #6
ussrasu said:
The formula is 1/lamba = R (1/2^2 - 1/n^2)
sorry if that doesn't make sense
But i will put in the number 2 in n for one wavelength and infinity for the other wavelength - and then subtract the 2 answers to get the wavelength range?
Is this along the right lines?

Looks right to me, at least for the Balmer series width.
 

1. What are the Balmer Series and Lyman Series?

The Balmer Series and Lyman Series are two series of spectral lines that are observed in the emission spectrum of hydrogen atoms. They represent the transitions of electrons between different energy levels within the atom.

2. What is the difference between the Balmer Series and Lyman Series?

The main difference between the Balmer Series and Lyman Series is the energy levels involved in the transitions. The Balmer Series involves transitions from higher energy levels to the second energy level, while the Lyman Series involves transitions from higher energy levels to the first energy level.

3. How are the spectral lines in the Balmer Series and Lyman Series produced?

The spectral lines in the Balmer Series and Lyman Series are produced when an electron in a hydrogen atom transitions from a higher energy level to a lower energy level, emitting a photon of light with a specific energy. Each transition corresponds to a specific spectral line in the series.

4. What is the significance of the Balmer Series and Lyman Series in astronomy?

The Balmer Series and Lyman Series are important in astronomy because they provide information about the composition and temperature of celestial objects. By analyzing the spectral lines in these series, scientists can determine the elements present and the temperature of stars and other objects in the universe.

5. Can the Balmer Series and Lyman Series be observed in other elements besides hydrogen?

No, the Balmer Series and Lyman Series are unique to hydrogen because they are based on the energy levels of the hydrogen atom. Other elements have different energy levels for their electrons, resulting in different spectral lines and series in their emission spectra.

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