Help with the Bohr Model Problem

In summary, the conversation revolves around calculating the wavelength and energy levels for a given emission of energy. The initial energy level is n = 7 and the change in energy is 1.977x10^-19 J. The equation E = E(1/ni^2) is used to calculate the initial energy level, and the final energy level is determined by solving E*(1/nfinal^2) = 2.016947*10^-19. The final energy level is found to be n = 1. The conversation also includes discussions about finding initial energy levels, using the Bohr model for hydrogen atoms, and the difficulty of understanding question 9.
  • #1
RJLiberator
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Okay, I am in need of some guidance:

7)Calculate the wavelength that corresponds to an emission of energy of 1.977x10^-19 J.

Okay, well here is my thought process initially: Change in Energy = hc/wavelength.

First question: Is 1.977*10^-19 THE change in energy? OR is that the Energy FINAL and the Energy initial is some constant that I SHOULD know already?

If it is the CHANGE in energy then using the equation I can get the wavelength rather easy by simply plugging in Planck's constant and the speed of light. My answer was 1005 nm doing this process.

My question to YOU is is this correct? OR am I missing the initial energy, and if so, where can I find this 'initial energy?'

Next,
8)If the initial energy level for the energy change in problem seven is n = 7, what is the final energy level?

Uhhh.. how do I find this? Any leads on this? I feel like I am missing some chart of numbers that corresponds the energy changes to certain "n" levels.

And finally,
prooooof_zpsd6b6643c.jpg


Any leads, websites, directions I can check out to get me started here?

Thanks all for your help.
 
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  • #2
7) By the way the question is worded, the energy given should be the energy of the emitted photon (light) and so with your terminology, specifically for the Bohr atom, would be the change in energy.

8) If your initial energy is X and your change in energy is Y, then what's your final energy? What energy level does this correspond to?
 
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  • #3
Well, sure, for 7: "an emission of energy", sure that means the energy taken away by the photon.
Why would you need to know more: you have a photon and its energy.
Forget about these states, that doesn't make sense.

For 8: Ei-Ef = DE, and Ei=E(n=7) . The problem is: there is no indication about which atom is involved.
For hydrogen, have a look at wikipedia (http://en.wikipedia.org/wiki/Hydrogen_atom).
You should know the level of hydrogen: En = -Rydberg/n² where Rydberg = 13.6 eV

For 9: So trivial that the difficulty is to understand why they ask.
 
  • #4
Thanks guys for the posts.

So it seems on Question 7) My assumption was correct with the wording that the change in energy was what was giving. This is excellent, that problem is solved and I feel great about it.

For question 8) I'm not quite sure how to find the initial energy. Is the initial energy = to 13.6 eV ?

As far as Question 9 goes... Trivial... maybe, but I'd like to understand it =).
 
  • #5
9. Express the Ei and Ef using equation for energy that they supplied (the middle one).
 
  • #7
I'm sorry guys, I'm having a hard time with number 8.

I keep reading the wikipedia article and my notes, but keep coming up with loose theories on what to do and I'm not too confident in it.

So, let me think about this situation here.

We have a energy change of 1.977 * 10^-19 J.
We have the initial Energy level of n = 7.
From question 7, I've found the wavelength to be 1005 nm.

So what piece of information tells me whether the emission of energy in it's initial state was lower then n=7 or higher than n=7?

Is it this equation that I keep looking at:
(1/initial n^2 - 1/final n^2)

Under this scenario, initial n^2 would be 7^2 or 49.
But where the hell do you find initial n from :O. There's got to be some equation that I am simply missing or some constant that I do not have.

I will continue to read my book now, but if anyone can lead me further I would be greatful :D
 
  • #8
Oh, and can anyone confirm my answer to 7 is correct ?

What I did was the following:

Wavelength = hc/Change in energy.

wavelength = ((6.626068*10^-34)(2.998*10^8))/(1.977*10^-19)
Which gave me 1005 nm.
 
  • #9
I think I may have made a breakthrough.

So we know that the energy is 1.997*10^-19 J we will call this "E" for simplicity.

If I throw that piece of information in an equation : E = E(1/ni^2) where n initial = 7. Then we have E*(1/49) Which will be the n=7 level.

Great.

Now I need E*(1/nfinal^2) But how do I find this n'final number that I am looking for.

From these equations I can find out if the change in level caused an electron to be absorbed or emitted!
 
  • #10
Solve 9 first. Once you will know the equation is correct, just plug everything into it and solve for nf. Pure (and quite simple) algebra.
 
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  • #11
okay, here is what I am doing:

Ephoton = Change in Energy = Efinal-Einitial=plancks constant * frequency.

So what I did was, I used the wavelength I got in Question 7 which was 1005 and plugged that into find the frequency. The frequency was 2.9831*10^14.

I multiplied that frequency with Plancks constant to receive Ephoton which was 1.9766*10^-19.

I then used my earlier understanding of 1.977*10^-19* (1/49) to find Einitial.

I added Einitial to the Energy final to receive the total of Efinal which came out to be 2.016947*10^-19.

These answers make sense to me. I guess I have to find out the final energy level now by:
1.977*10^-19(1/n^2)=2.016947*10^-19

Based on this, the final N level is 1.
So the energy change went from n=7 to n=1. Does this sound proper?
 
  • #12
Can anyone confirm that I am on the correct path?
 

Related to Help with the Bohr Model Problem

1. What is the Bohr Model and why is it important in science?

The Bohr Model is a simplified representation of the structure of an atom proposed by Niels Bohr in 1913. It is important because it helped scientists better understand the behavior of atoms and paved the way for further advancements in atomic theory.

2. How is the Bohr Model different from the earlier atomic models?

The Bohr Model introduced the concept of energy levels or shells, where electrons orbit the nucleus in fixed, discrete energy levels. This was different from earlier models, such as the Thomson and Rutherford models, which proposed that electrons moved freely around the nucleus.

3. How do I draw a Bohr Model for a specific element?

To draw a Bohr Model, you will need to know the atomic number of the element, which tells you the number of protons in the nucleus. The number of electrons in the Bohr Model will be equal to the number of protons. You will then need to distribute the electrons into energy levels according to the 2-8-8 rule, where the first energy level can hold up to 2 electrons and the second and third energy levels can hold up to 8 electrons each.

4. Can the Bohr Model be used for all elements?

No, the Bohr Model is only applicable for elements with a small number of electrons, typically up to 20. For elements with more electrons, a more complex model, such as the quantum mechanical model, is needed to accurately represent the electron configuration.

5. How does the Bohr Model explain the properties of elements?

The Bohr Model explains the properties of elements by showing how the number of electrons in the outermost energy level, also known as the valence electrons, determines an element's chemical behavior. Elements with the same number of valence electrons have similar chemical properties, while elements with different numbers of valence electrons have different properties.

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