a. Calculate the energy of photon in singly ionized helium if the electron makes a transition from the n= 3 orbital (shown) down to the n= 1 orbital
a. Calculate the energy of photon in singly ionized helium if the electron makes a transition from the n= 3 orbital (shown) down to the n= 1 orbital
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Transcribed Image Text:2. The value of 13.6 eV used in the Bohr model is better known to physicists as the Rydberg
constant RH
те4
RH =
8h³ce?
= 13.6 eV
Thus, the Bohr energy equation for hydrogen can equally be written as
1
13.6 eV
En = -RH
n2
n2
The Bohr formula can be applied to other elements having only a single electron, like singly
ionized helium (shown below), simply by replacing RH with R as defined below
m(Ze?)?
R =
8h³ce?
Note that if the atomic number Z is equal to 1 this reduces to Bohr's formula.
13
Figure 1 Singly ionized helium has only one electron, thus is hydrogen-like. The electron is in then= 3 orbital.

Transcribed Image Text:a. Calculate the energy of photon in singly ionized helium if the electron makes a
transition from the n= 3 orbital (shown) down to the n = 1 orbital
b. Calculate the wavelength of this transition in nanometers. To make life easier, you
may take the product of h*c to be 1239.8 eV*nm
c. Based on your answer to part b) and on the figure below, what part of the
electromagnetic spectrum does this photon belong to?
Wavelength (jum)
106 105 10 103 102 10 10° 101 102 103 10 105 106 107
Gamma Ray
XRay
Infrared
Radio Waves
Ultraviolet
Microwaves
The Visible Spectrum
ultraviolet violet
blue
green
yellow
red
infrared
400
480
540
580
700
Wavelength (nm)
Figure 2 The electromagnetic spectrum in units of nm
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