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A hypothetical NH molecule makes a rotational-level transition from l = 3 to l = 1 and gives off a photon of wavelength 1.780 nm in doing so. What is the separation between the two atoms in this molecule if we model them as point masses? The mass of hydrogen is 1.67 × 10$$2$$7 kg, and the mass of nitrogen is 2.33 × 10$$2$$6 kg.

Short Answer

Expert verified
The separation is approximately 91.0 pm.

Step by step solution

01

Calculating Reduced Mass

The reduced mass μ of the diatomic molecule is calculated using the formula:μ=m1m2m1+m2where m1=1.67×1027 kg is the mass of hydrogen and m2=2.33×1026 kg is the mass of nitrogen.μ=1.67×10272.33×10261.67×1027+2.33×1026=3.89×10532.50×1026=1.56×1027 kg.
02

Rotational Energy Change

The change in rotational energy when the molecule transitions from l=3 to l=1 is calculated using the formula:ΔE=E3E1=h28π2I(l(l+1))h28π2I(l(l+1))where l=3 and l=1, and I=μr2 is the moment of inertia.
03

Photon Energy Calculation

The energy of the emitted photon can also be calculated from its wavelength:Eγ=hcλ Substituting for h=6.626×1034 Js and c=3×108 m/s and λ=1.780×109 m:Eγ=6.626×1034×3×1081.780×109=1.12×1017 J.
04

Equating Energy and Solving for r

Set the change in rotational energy equal to the photon's energy:ΔE=Eγh28π2μr2(l(l+1)l(l+1))=1.12×1017Substituting μ from Step 1 and solving for r:r=h2(122)8π2μ1.12×10179.10×1011 m.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Reduced Mass Calculation
In molecular physics, the reduced mass is a crucial concept often used to simplify the analysis of two-body systems like diatomic molecules. It allows us to treat the motion of two interacting bodies as if it were one single body. The reduced mass μ is defined by the formula:μ=m1m2m1+m2Where m1 and m2 are the masses of the two atoms. This method focuses on the center of mass of the system, permitting us to eliminate the individual motions of the atoms. In simpler terms, the reduced mass helps us to express the system's behavior by combining both masses into a single effective mass. This makes the mathematics behind calculating physical properties such as rotational energy or vibrational frequency much easier to deal with. In this specific exercise, we calculated the reduced mass for the NH diatomic molecule as 1.56×1027 kg.
Rotational Energy Change
All molecules exhibit rotational energy due to their rotational motion around a bond. The quantized levels of this energy are given by:El=h28π2Il(l+1)where l is the rotational quantum number, h is Planck’s constant, and I is the moment of inertia. When a molecule transitions between different rotational levels, there is a change in rotational energy ΔE. In our problem, the transition occurs from l=3 to l=1, and the change in rotational energy can be computed by subtracting the energies of these levels. By calculating the difference (E3E1), we get the energy emitted or absorbed during the transition. Understanding these energy changes aids in interpreting spectral lines we observe in spectroscopy, providing insights into molecular structure and behavior.
Photon Energy Calculation
Photon energy is directly related to the wavelength of light, via the equation:Eγ=hcλHere, h is Planck's constant, c is the speed of light, and λ is the wavelength of the photon. This equation underpins why instruments like spectrometers can measure light energy by evaluating its wavelength. In the given problem, the NH molecule emits a photon with a wavelength of 1.780 nm during its rotational transition. Plugging in the values for h(6.626×1034Js), c(3×108 m/s), and the wavelength, we obtain that the emitted photon's energy is 1.12×1017 J. Understanding this concept helps connect the dots between quantum mechanical phenomena and observable quantities in laboratories.
Moment of Inertia
The moment of inertia I is a pivotal concept in rotational dynamics for molecular systems, much like mass is for linear dynamics. In diatomic molecules, it reflects how the mass is distributed around the rotational axis and is given by:I=μr2Where μ is the reduced mass, and r is the distance between the two atoms. This "rotational equivalent of mass" helps determine the resistance of the molecule to changes in its rotation. A larger moment of inertia implies a molecule is harder to spin. In rotational transitions, I directly influences the energy levels, as seen in the formula for rotational energy. In the original problem, we used the moment of inertia to help link the change in rotational energy to the observed photon energy. Solving for r, we deduced the separation between the nitrogen and hydrogen atoms, giving insights into their molecular structure.

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Most popular questions from this chapter

To determine the equilibrium separation of the atoms in the HCl molecule, you measure the rotational spectrum of HCl. You find that the spectrum contains these wavelengths (among others): 60.4μm, 69.0μm, 80.4μm, 96.4μm, and 120.4μm. (a) Use your measured wavelengths to find the moment of inertia of the HCl molecule about an axis through the center of mass and perpendicular to the line joining the two nuclei. (b) The value of l changes by ±1 in rotational transitions. What value of l for the upper level of the transition gives rise to each of these wavelengths? (c) Use your result of part (a) to calculate the equilibrium separation of the atoms in the HCl molecule. The mass of a chlorine atom is 5.81×1026 kg, and the mass of a hydrogen atom is 1.67×1027 kg. (d) What is the longest-wavelength line in the rotational spectrum of HCl?

Consider a system of N free electrons within a volume V. Even at absolute zero, such a system exerts a pressure p on its surroundings due to the motion of the electrons. To calculate this pressure, imagine that the volume increases by a small amount dV. The electrons will do an amount of work p dV on their surroundings, which means that the total energy Etot of the electrons will change by an amount dEtot=pdV. Hence p=dEtot/dV. (a) Show that the pressure of the electrons at absolute zero is p=32/3π4/325mNV 5/3 (b) Evaluate this pressure for copper, which has a freeelectron concentration of 8.45×1028m3. Express your result in pascals and in atmospheres. (c) The pressure you found in part (b) is extremely high. Why, then, don't the electrons in a piece of copper simply explode out of the metal?

Germanium has a band gap of 0.67 eV. Doping with arsenic adds donor levels in the gap 0.01 eV below the bottom of the conduction band. At a temperature of 300 K, the probability is 4.4 × 10$$4 that an electron state is occupied at the bottom of the conduction band. Where is the Fermi level relative to the conduction band in this case?

Our galaxy contains numerous molecular clouds, regions many lightyears in extent in which the density is high enough and the temperature low enough for atoms to form into molecules. Most of the molecules are H2, but a small fraction of the molecules are carbon monoxide (CO). Such a molecular cloud in the constellation Orion is shown in Fig. P42.42. The upper image was made with an ordinary visiblelight telescope; the lower image shows the molecular cloud in Orion as imaged with a radio telescope tuned to a wavelength emitted by CO in a rotational transition. The different colors in the radio image indicate regions of the cloud that are moving either toward us (blue) or away from us (red) relative to the motion of the cloud as a whole, as determined by the Doppler shift of the radiation. (Since a molecular cloud has about 10,000 hydrogen molecules for each CO molecule, it might seem more reasonable to tune a radio telescope to emissions from H2 than to emissions from CO. Unfortunately, it turns out that the H2 molecules in molecular clouds do not radiate in either the radio or visible portions of the electromagnetic spectrum.) (a) Using the data in Example 42.2 (Section 42.2), calculate the energy and wavelength of the photon emitted by a CO molecule in an l = 1 l = 0 rotational transition. (b) As a rule, molecules in a gas at temperature T will be found in a certain excited rotational energy level, provided the energy of that level is no higher than kT (see Problem 42.39). Use this rule to explain why astronomers can detect radiation from CO in molecular clouds even though the typical temperature of a molecular cloud is a very low 20 K.

The water molecule has an l = 1 rotational level 1.01 × 10$$5 eV above the l = 0 ground level. Calculate the wavelength and frequency of the photon absorbed by water when it undergoes a rotational-level transition from l = 0 to l = 1. The magnetron oscillator in a microwave oven generates microwaves with a frequency of 2450 MHz. Does this make sense, in view of the frequency you calculated in this problem? Explain.

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