Question #03297

1 Answer
Nov 21, 2017

n_f = 3nf=3

Explanation:

Your tool of choice here will be the Rydberg equation, which allows you to calculate the wavelength of the photon emitted when an electron in a hydrogen atom makes an n_i -> n_fninf transition.

1/(lamda) = R * (1/n_f^2 - 1/n_i^2)1λ=R(1n2f1n2i)

Here

  • RR is the Rydberg constant, equal to 1.097 * 10^(7)1.097107 "m"^(-1)m1
  • n_ini is the energy level from which the electron falls
  • n_fnf is the energy level to which the electron falls

In your case, you know that the electron falls from the seventh energy level, so

n_i = 7ni=7

Your goal here is to find the value of the final energy level, n_fnf. Rearrange the Rydberg equation to solve for n_fnf.

1/lamda = R * (n_i^2 - n_f^2)/(n_i^2 * n_f^2)1λ=Rn2in2fn2in2f

n_i^2 * n_f^2 = lamda * R * (n_i^2 - n_f^2)n2in2f=λR(n2in2f)

n_i^2 * n_f^2 + lamda * R * n_f^2 = lamda * R * n_i^2n2in2f+λRn2f=λRn2i

This is equivalent to

n_f^2 * (n_i^2 + lamda * R) = lamda * R * n_i^2n2f(n2i+λR)=λRn2i

which gets you

n_f = sqrt( (n_i^2 * lamda * R)/(n_i^2 + lamda * R))nf= n2iλRn2i+λR

Now all you have to do is to plug in the values that you have--do not forget that the wavelength of the photon must be expressed in meters!

n_f = sqrt( (7^2 * 1005 * 10^(-9)color(red)(cancel(color(black)("m"))) * 1.097 * 10^7 color(red)(cancel(color(black)("m"^(-1)))))/(7^2 + 1005 * 10^(-9)color(red)(cancel(color(black)("m"))) * 10.97 * 10^7 color(red)(cancel(color(black)("m"^(-1))))))

n_f = 2.99983 ~~ 3

Therefore, you can say that a photon of wavelength "1005 nM" is emitted when an electron in a hydrogen atom falls from n_i = 7 to n_f = 3, a transition that is part of the Paschen series.

![https://thecuriousastronomer.wordpress.com/2013/08/20/emission-line-spectra/](useruploads.socratic.org)