How Is the Rydberg Constant Calculated from Photon Absorption Wavelengths?

AI Thread Summary
The discussion focuses on calculating the effective Rydberg constant and nuclear charge from observed photon absorption wavelengths. Participants analyze the energy transitions of an ionized atomic gas, converting wavelengths into photon energies. They identify energy levels and ratios, concluding that the emissions correspond to transitions from higher energy states to the ground state. The calculations suggest that the nuclear charge is 3, indicating the presence of lithium, and the Rydberg constant is determined to be approximately 1.09 x 10^7. The conversation emphasizes the importance of understanding photon energies in relation to energy states.
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Homework Statement



The following photon wavelengths are observed in absorption at room temperature from an ionized atomic gas with a single electron orbiting the nucleus: λ=
13:5 nm, 11:4 nm, 10:8 nm. Use this data to determine the effective Rydberg constant
and the nuclear charge.

Homework Equations





The Attempt at a Solution



I know that energy is emitted/absorbed when electron transits between different energy levels.
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Thing is, I don't even know what the n=1 energy is, to find the rydberg constant. I can't tell what the energy levels are just from the photons absorbed, as they could be between any two levels.
 
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Don't give up before you even started.
Did you convert the wavelength values to photon energies?
Which patterns do you expect in the energy spectrum?
 
mfb said:
Don't give up before you even started.
Did you convert the wavelength values to photon energies?
Which patterns do you expect in the energy spectrum?

I expect, the gaps between energy levels to become smaller as you go higher up..
 
mfb said:
Don't give up before you even started.
Did you convert the wavelength values to photon energies?
Which patterns do you expect in the energy spectrum?

13.5nm -> 92.1 eV
11.4nm -> 109.0 eV
10.8nm -> 115.1 eV

So

n=1 is 92.1 eV
n=2 is 109.0 eV
n=3 is 115.5 eV

Then what is the point of giving us the other 2 absorption wavelengths?
 
unscientific said:
So

n=1 is 92.1 eV
n=2 is 109.0 eV
n=3 is 115.5 eV

Then what is the point of giving us the other 2 absorption wavelengths?
Photon energies are not the energies of states!

Which photon energies (not electron energy states) do you get for a hydrogen atom? Which ratios do you have between those values? Do you see a similarity to your problem?
 
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For Hydrogen:

E1 = -13.6 eV
E2 = -3.4 eV
E3 = -1.51 eV
E4 = -0.850 eV

Based on the wavelengths given, 92.1eV, 109eV, 115.5eV are differences in energy between En and E1.

The ratio of first energy level between the gas and hydrogen = Z2, where Z is the proton number of the gas.
 
mfb said:
Photon energies are not the energies of states!

Which photon energies (not electron energy states) do you get for a hydrogen atom? Which ratios do you have between those values? Do you see a similarity to your problem?

Ok using the relation ΔE = (1- 1/n2)

First emission:
92.1 = E1(3/4)

Second emission:
109 = E1(8/9)

Third Emission:

115.5 = E1(15/16)

These ratios match, so somehow these are the emissions from the second, third and fourth energy levels.

E1 = (13.6)Z2

Solving, Z = 3 (Lithium) and E1 = 122.4eV, R = (13.6eV)/hc = 1.09*107
 
Last edited:
That is correct.

R = (13.6eV)/hc = 1.09*107
I think the factor of 9 is missing here, and the last value should have units.
 
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