Calculating Hydrogen Bohr Orbit Transition and Series using Wavelength 410.7 nm

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SUMMARY

The discussion focuses on calculating the hydrogen Bohr orbit transition responsible for the emission of light at a wavelength of 410.7 nm. The transition belongs to the Balmer series, with the initial state identified as m = 6 and the final state as n = 2. The calculations utilize the Rydberg formula, specifically 1/λ = Z² * R(1/n² - 1/m²), where R is the Rydberg constant for hydrogen, valued at 1.096776 × 107 m-1. The conclusion confirms the transition from the sixth orbit to the second orbit in the hydrogen atom.

PREREQUISITES
  • Understanding of the Bohr model of the hydrogen atom
  • Familiarity with the Rydberg formula for spectral lines
  • Knowledge of the electromagnetic spectrum, particularly the visible range
  • Basic algebra and manipulation of equations
NEXT STEPS
  • Study the derivation and applications of the Rydberg formula
  • Explore the Balmer series and its significance in atomic physics
  • Learn about the electromagnetic spectrum and its various regions
  • Investigate the quantum mechanics underlying atomic transitions
USEFUL FOR

Students of physics, particularly those studying atomic structure and spectroscopy, as well as educators looking for practical examples of quantum transitions in hydrogen.

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Homework Statement


Light of wavelength 410.7 nm is observed in emission from a hydrogen source. a) what transition between hydrogen bohr orbits is responsible for this radiation? b) to what series does this transition belong to?

Homework Equations

1/lambda=Z^2 *R(1/n^2-m^2) ,

n being the final transition and m being the initial transition state. R is the Rydberg constant and the Rydberg constant for hydrogen is 1.096776*10^7 m^-1 and Z being the atomic number.

The Attempt at a Solution



Since the the wavelength is light , I know that its going to be in the visible spectrum of the E-M spectrum and the Balmer series is always part o the visible spectrum. the initial transition energy state in the balmer series is always m=2. Therefore since I know the initial transition state , R , Z and the wavelength , I thought I could find the n, the final transition state. here are my calculations below:

1/lambda)*1/(R)= (1/n^2-1/m^2) =>(1/(4.10e-7 m))*(1/(1.096776e7 m^-1))= (1/(2^2)-1/(m^2)) => .2224=(1/4-1/(m^2))=> -1/m^2 = -(.222-.25) => m^2= 1/.028 = 5.97 m = 6
 
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Looks right. But the final state, n = 2... and you're finding m which is the initial state... so the initial state is m = 6.
 

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