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exercise_3_chem_soultion.docx

General Chemistry I - CHEM 181

Critical Thinking Exercise #3

Due Thursday, Oct. 24

Name_________________________

Section _______

Why do excited hydrogen atoms emit only specific wavelengths of light?

Introduction

In the 1800’s scientists discovered that a glass cylinder containing a low pressure of a gas will emit light when high voltage electricity is applied to metal electrodes inserted at opposite ends of the cylinder. This principal is used in fluorescent lighting today. When the light emitted by a particular gas, for instance hydrogen, was analyzed by passing it through a prism, scientists were surprised to find that only a few specific wavelengths of visible light were emitted, rather than a continuous range of wavelengths. This mystery took over 70 years to fully solve.

wavelength, (nm)

Infrared

Ultraviolet (uv)

Over time, scientists discovered that the wavelengths of radiation emitted by hydrogen extended from the ultraviolet through the visible into the infrared, microwave, and radio wave portions of the electromagnetic (EM) spectrum. There appeared to be a pattern in the wavelengths that consisted of a series of series of lines. The first 4 series starting from the shortest wavelength line are named for the people that discovered them.

In 1885 J.J. Balmer discovered a mathematical pattern in the wavelengths emitted by hydrogen in the visible and near ultraviolet regions of the electromagnetic spectrum:

Each allowed value for n plugged into this equation produces one of the wavelengths of light emitted by hydrogen in the region of the spectrum that Balmer studied.

Five years later another scientist, Johannes Rydberg, extended this equation so that it could predict all of the wavelengths emitted by hydrogen in all regions of the electromagnetic spectrum:

(eq. 1)

This equation contains two integers that must be greater than zero and the value of n must be greater than the value of m . The way it works is that the value of m specifies the series, e.g. m = 3 is necessary to generate the wavelengths observed in the Paschen series and n = 4,5,6… will generate the wavelengths emitted within that series. The constant R is known as the Rydberg constant.

Though the equations from Balmer and Rydberg demonstrated mathematical skill, they did not answer the big question on the minds of many scientists: Why do the atoms of hydrogen in the gas phase emit only certain wavelengths of radiation and why do the wavelengths have the pattern described by these clever equations. As it turned out, the solution to this riddle completely altered civilization on this planet.

Part I – Putting together pieces of the puzzle

Part of the reason that it took so long to solve hydrogen line spectrum puzzle was that scientists at the time had an incomplete understanding of light. Specifically, they were not aware of any relationship between the energy of light and the wavelength. It was assumed that the energy of light depended entirely on the intensity, which was the square of the amplitude of the light waves according to accepted theory.

This understanding was changed drastically by 1905 due to experiments that revealed that light had a particle nature in addition to its wave nature and that particles of light, which we now call photons, have an energy that is directly proportional to frequency and inversely proportional to the wavelength of the light.

Ephoton = where h is a constant called Plank’s constant

Since , we can also write Eph = (we’ll abbreviate photon as ph)

Step 1: Notice that the left hand side of the Rydberg equation (eq. 1) can easily be converted from into photon energy, Eph, just by multiplying by hc . Naturally, the right hand side of the equation will also need to be multiplied by hc to keeps things equal. Rewrite the Rydberg equation (eq. 1) below in terms of photon energy. The left side of the equation should look like; Eph =

From the equation Ephoton = hc/λ, re-arrange it to get the expression 1/λ.

Step 2: The right side of your revised Rydberg equation above is really a difference between two terms (in parentheses). To make this more apparent, multiply both terms by to remove the parentheses and rewrite the equation below.

Just distribute the term hcR∞ in the two terms in the parenthesis. The equation will be:

Step 3: What is the unit for each of these two terms on the right side of the equation. The values (with units) for h and c are 6.626 X 10-34 Js and 2.998 X 108 m/s, respectively. The unit for the Rydberg constant is given with eq. 1 on page 2. Use unit cancellation to obtain the final unit for each term and write that below.

The values of m and n are unitless, so it will not be included. The units will be like:

=J So that unit of Eph is in Joules.

It should be clear from the unit you obtained above, that the right side of the equation is simply the difference between two energies. So right now the equation is telling us that the energy of the photon of light emitted by a hydrogen atom for some allowed combination of the integers m and n is equal to the difference between the two energies given by the terms on the right hand side. What do the energies on the right refer to? The Law of Conservation of Energy can help us here. “During any process, energy can be neither created nor destroyed.” Energy may be converted from one form into another, however. So if a hydrogen atom emits a specific amount of energy in the form of a photon of light, Eph, then what must happen to the energy of the atom? It must decrease by an amount that is exactly equal the energy of the photon. We can represent this relationship with a simple equation:

Eph = ∆Eatom = Einitial - Efinal (eq. 2)

If you compare this equation with your equation obtained in step 2, you might be tempted to conclude that

and

However we run into a little problem here that becomes evident if we ask ourselves what kind of energy would an atom of hydrogen have?

Step 4: Work through the following questions to determine the form(s) of energy existing within an atom of hydrogen.

a) What does an atom of the common isotope of hydrogen consist of, i.e. what subatomic particles are present? For hydrogen (H1), it consists of 1 electron and 1 proton. For deuterium (H2), 1 electron, 1 proton and 1 neutron. For tritium (H3), 2 neutrons, 1 electron and 1 proton.

b) What type of force, if any, would exist between these particles? There’s this attractive electrostatic force of interaction that exist between electrons and protons. Between protons and neutrons, there’s what they call strong nuclear force.

c) Should an atom of hydrogen have potential energy? (Note: Whenever a force is acting on an object, the object must contain potential energy.) Yes.

d) Are there other forms of energy that would likely exist within a hydrogen atom? Yes. There should be kinetic energy.

Taking potential energy to be the primary form of energy existing in an atom of hydrogen due to the attractive force acting between the electron and the proton, we can consult a physics source to find the equation for this form of energy, which is known as Coulomb’s Law:

This tells us that the potential energy is proportional to the product of the two charges and inversely proportional to the distance between the charged objects. Note that k is simply a proportionality constant.

The thing we need to notice here is that when the charges are opposite and force is attractive, the value of the potential energy must be a negative number. The equations that we inferred earlier (restated below) from the comparison of the Conservation of Energy equation with your revised Rydberg equation from step 2 give positive values for the energy of the atom, because all the constants are positive as well as the integers m and n.

and

(eqs. 3)

Energies that are negative, rather than positive, can be obtained by first switching the order of the two terms in the revised Rydberg equation (step 2), as follows:

Then replacing the “+” with “-(-)” as follows:

(eq. 4)

Now each of the energy terms on the right must always have a negative value, as it should to represent the energy of a hydrogen atom. Note that since the integer n must always be larger than the integer m , as defined in the original Rydberg equation, the first term must have a smaller negative value than the second term and thus represents a larger energy value. (If this is confusing, just consider that the number -2 is greater than -4.)

Step 5: Now with the exchange of the terms on the right, compare eq. 4 with the Conservation of Energy equation, eq. 2, and write two new equations for Einitial and Efinal similar to eqs. 3 above, such that the initial and final energies generated by the equations will necessarily have negative values.

Equation 4 is . Equation 2 is Eph = ∆Eatom = Einitial – Efinal. Therefore, Einitial is -hcR∞/n2 and Efinal is -hcR∞/m2.

Compare the two equations just written. How are they different? The numerators on the right hand side are exactly the same, and the denominators must each be some positive integer squared. The only difference between the two equations is that the value of the integer for the initial energy of the atom must be larger than the value of the integer for the final energy. There would be nothing wrong with using the same integer variable n for both equations if we subscript the variable to distinguish initial and final values of n as ni and nf .

We can consider these two equations as special cases of a more general equation that gives us all the possible energies that a hydrogen atom can contain

where n =1,2,3,… (eq. 5)

Step 6: At this point you have derived an equation for the energy of a hydrogen atom that must be satisfied in order to account for the observed emission wavelengths in hydrogen’s atomic emission spectrum. How does this equation limit the energy that a hydrogen atom can contain due to the interaction between the electron and the proton? Is any energy possible for the atom over a broad range of values, as is the case for golf balls, bicycles, and objects orbiting the planet (everyday life in general)? Describe two ways in which this equation limits the energy of a hydrogen atom. {Hint: The answer to this question may be clearer after you complete Part II of this exercise.}

Limitation 1: The value of En approaches a certain number as the value of n approaches infinity. That means that is the minimum energy the H atom can have.

Limitation 2: The value of n should not be equal to zero. So the lowest energy level that is allowed to H is n=1.

Part II – Testing the equation derived in part I for the allowed energy levels for an atom of hydrogen.

Please show your work on all calculations.

1) Use the final equation from step 7 along with values for h and c given in step 3, and the value of R given in eq. 1 to calculate values for the first 10 allowed energies, n = 1,2,3,…10. List these values below (or include a copy of the relevant cells if you used Excel to perform the calculations). Be sure to include the appropriate unit for your values.

Using equation 5, the following data were obtained using Excel.

h

6.63E-34

J-s

n

En, Joules

c

3.00E+08

m/s

1

-2.17916E-18

R

1.10E+07

1/m

2

-5.44791E-19

3

-2.42129E-19

4

-1.36198E-19

5

-8.71665E-20

6

-6.05323E-20

7

-4.44727E-20

8

-3.40494E-20

9

-2.69032E-20

10

-2.17916E-20

infinity

1E+40

-2.17916E-98

2) Next, use your energy values to create an energy level diagram akin to Figure 3.22 in the textbook (but without the vertical arrows) on a full size sheet of paper that you can attach to this exercise. Try to make the diagram accurate to scale using either graph paper or Excel. Be sure to label and scale your energy axis appropriately.

Plotting the values of n versus wavelength, the graph is shown below.

3) Recall that the Balmer series in the hydrogen spectrum extends from the visible region into the uv portion of the electromagnetic spectrum.

a. What do the electron transitions giving rise to the Balmer series wavelengths have in common? {Hint: A transition is specified by giving the integer values of the initial and final energy levels, e.g. ni = 4 nf = 3. You may want to look up the Balmer series in your textbook.}

The electron transitions that give rise to the Balmer series are from the energy that is released from the atom instead of having supplied to it. This is indicated by the negative Eph values.

b. Refer to the figure on the 1st page of this exercise to notice that there are only 4 emission wavelengths from the Balmer series that are in the visible portion of the EM spectrum. Use the allowed energies that you calculated above in (1) to predict the wavelengths (in nm) for the two longest wavelength emission lines in the series. (Be sure to show your calculations.) {Hint: The longest wavelength corresponds to the smallest photon energy, which in turn corresponds to the smallest energy difference between the initial level and final level of the electron jump.}

The longest wavelength emission lines are 656 and 486 nm. The wavelengths that are calculated for n=1 to 10 is summarized below. 121 is not part of the UV-Vis spectrum.

En, J

delE, J

lambda, m

lambda, nm

-2.17916E-18

-5.44791E-19

1.63437E-18

1.21544E-07

121.5436038

-2.42129E-19

3.02662E-19

6.56335E-07

656.3354603

-1.36198E-19

4.08593E-19

4.86174E-07

486.1744151

-8.71665E-20

4.57624E-19

4.34084E-07

434.0842992

-6.05323E-20

4.84258E-19

4.1021E-07

410.2096627

-4.44727E-20

5.00318E-19

3.97042E-07

397.042439

-3.40494E-20

5.10741E-19

3.8894E-07

388.9395321

-2.69032E-20

5.17887E-19

3.83573E-07

383.5726716

-2.17916E-20

5.22999E-19

3.79824E-07

379.8237618

-2.17916E-98

5.44791E-19

3.64631E-07

364.6308113

The solution below is how to calculate wavelengths.

En is calculated using equation 5. Example of calculation:

N= 3 En = [(6.626x10-34 J-s)(3.0x108m/s)(1.10x107/m)]/3 = -2.42129E-19 Joules

∆E(32) = -2.42129E-19 – (-5.44791E-19) = 3.02662E-19 Joules

λ = hc/∆En = [(6.626x10-34 J-s)(3.0x108m/s)/ 3.02662E-19 Joules] = 6.56335E-07m

in nm 6.56335E-07m (1nm/1.0x10-9m) = 656.3354603nm.

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