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Integrated Concepts

A galaxy moving away from the earth has a speed of 0.0100c. What wavelength do we observe for an ni = 7 to nf = 2 transition for hydrogen in that galaxy?

Short Answer

Expert verified

The observed wavelength is 401 nm.

Step by step solution

01

Determine the formulas:

Consider the formula for the charge to mass ratio in the electron and the proton as follows:

\[\begin{array}{c}\frac{{{q_e}}}{{{m_e}}} = - 1.76 \times {10^{11}}\;\frac{{\rm{C}}}{{{\rm{kg}}}}\\\frac{{{q_p}}}{{{m_p}}} = 9.57 \times {10^7}\;\frac{{\rm{C}}}{{{\rm{kg}}}}\end{array}\]

Here,\[{m_e} = 9.11 \times {10^{ - 31}}\;{\rm{kg}}\]is the mass of the electron and\[{m_p} = 1.67 \times {10^{ - 27}}\;{\rm{kg}}\]is the mass of the proton.

Consider the formula for the Bohr's theory of hydrogen atom.

\[\frac{{\bf{1}}}{{\bf{\lambda }}}{\bf{ = R}}\left( {\frac{{\bf{1}}}{{{\bf{n}}_{\bf{f}}^{\bf{2}}}}{\bf{ - }}\frac{{\bf{1}}}{{{\bf{n}}_{\bf{i}}^{\bf{2}}}}} \right)\]

Here, wavelength of the emitted electromagnetic radiation is λ, and the Rydberg constant is R = 1.097 x 107 m-1.

02

Find the observed wavelength

Substitute the values and determine the wavelength as:

\[\begin{array}{l}\frac{1}{\lambda } = \left( {1.097 \times {{10}^7}\;{{\rm{m}}^{ - 1}}} \right)\left( {\frac{1}{{{2^2}}} - \frac{1}{{{7^2}}}} \right)\\\frac{1}{\lambda } = \left( {1.097 \times {{10}^7}\;{{\rm{m}}^{ - 1}}} \right)\left( {\frac{1}{4} - \frac{1}{{49}}} \right)\\\frac{1}{\lambda } = 2518622.449\;{{\rm{m}}^{ - 1}}\\\lambda = \frac{1}{{2518622.449\;\;{{\rm{m}}^{ - 1}}}}\\\lambda = 397 \times {10^{ - 9}}\;{{\rm{m}}^{ - 1}}\end{array}\]

The wavelength observed is calculated as

\[{\lambda _{observed{\rm{ }}}} = \lambda \sqrt {\frac{{1 + \frac{u}{c}}}{{1 - \frac{u}{c}}}} \]

By changing the values in the formula above:

\[\begin{array}{l}{\lambda _{Observed{\rm{ }}}} = 397 \times {10^{ - 9}}\;{\rm{m}}\sqrt {\frac{{1 + \frac{{0.01c}}{c}}}{{1 - \frac{{0.01}}{c}}}} \\{\lambda _{Observed{\rm{ }}}} = 397 \times {10^{ - 9}}\;{\rm{m}}\sqrt {\frac{{1 + 0.01}}{{1 - 0.01}}} \\{\lambda _{Observed{\rm{ }}}} = 401 \times {10^{ - 9}}\;{\rm{m}}\\{\lambda _{Observed{\rm{ }}}} = 401\;\;{\rm{nm}}\end{array}\]

Therefore,therequired observed wavelength is 401 nm.

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Most popular questions from this chapter

A student in a physics laboratory observes a hydrogen spectrum with a diffraction grating for the purpose of measuring the wavelengths of the emitted radiation. In the spectrum, she observes a yellow line and finds its wavelength to be 589 nm. (a) Assuming this is part of the Balmer series, determine ni , the principal quantum number of the initial state. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?

An x ray tube has an applied voltage of 100 kV.

(a) What is the most energetic x-ray photon it can produce? Express your answer in electron volts and joules.

(b) Find the wavelength of such an X–ray.

In a laboratory experiment designed to duplicate Thomson’s determination of\({{\rm{q}}_{\rm{e}}}{\rm{/}}{{\rm{m}}_{\rm{e}}}\), a beam of electrons having a velocity of\({\rm{6}}{\rm{.00}}\)×\({\rm{10}}_{}^7\)m/s enters a\({\rm{5}}{\rm{.00}}\)×\({\rm{10}}_{}^{ - 3}\)T magnetic field. The beam moves perpendicular to the field in a path having a 6.80-cm radius of curvature. Determine\({{\rm{q}}_{\rm{e}}}{\rm{/}}{{\rm{m}}_{\rm{e}}}\)from these observations, and compare the result with the known value.

The maximum characteristic x-ray photon energy comes from the capture of a free electron into a K shell vacancy. What is this photon energy in keV for tungsten, assuming the free electron has no initial kinetic energy?

(a) How many electrons can be in the\(n{\rm{ }} = {\rm{ }}4\)shell? (b) What are its subshells, and how many electrons can be in each?

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