Orbitals and the 4th Quantum Number, (M7Q6) – UW-Madison Chemistry 103/104 Resource Book (2024)

Introduction

Atomic orbitals are mathematical solutions to the Schrödinger equation so how can we visualize orbitals to enhance our understanding of them? Orbitals have no fixed boundaries and electrons are wave particles that cannot be precisely located, which presents quite the challenge when attempting to draw them. There is no one perfect way of drawing an atomic orbital. This section explores the different ways we represent orbitals using 3-dimensional drawings and 2-dimensional graphing, the choice depending on what property of the orbital we are emphasizing.
This section also introduces the fourth quantum number, an outcome of electrons possessing the property of spin. This section includes worked examples, sample problems, and a glossary.

Learning Objectives for 4th Quantum Number, Orbitals

  • Describe orbital shapes and relative energy levels.
    | Orbital Shapes | Orbital Energies |
  • Ascribe and evaluate sets of four quantum numbers.
    | Spin Quantum Number | Pauli Exclusion Principle | Summary Table of Quantum Numbers and Significance |

| Key Concepts and Summary |Glossary | End of Section Exercises |

Orbital Shapes

An orbital is the quantum mechanical generalization of Bohr’s orbit. In contrast to his concept of a simple circular orbit with a fixed radius, orbitals are mathematically derived regions of space with differentprobabilitiesof having an electron in them.

s-Orbitals

One way of representing electron probability distributions is illustrated in Figure 1 for the 1s orbital of hydrogen. Recall that orbitals are described by wavefunctions, which are represented with ψ. Recall from the M7Q6, that Max Born proposed an interpretation of the wavefunction,ψ, that is still accepted today: the probability density of finding an electron at a given point in space is [ψ(r)]2. In Figure 1a, a dot density diagram is represented. This dot density diagram displays black dots where there is a probability of finding an electron—the higher density of dots, the higher the probability of finding the electron in that region. Taking the information from the dot density diagram, a plot of [ψ(r)]2versus distance from the nucleus (r) can be constructed. This type of plot (shown in Figure 1b) is a plot of the probability density. This plot shows the probability of finding the electron near a particular point in space that lies a distance r from the nucleus. The 1sorbital is spherically symmetrical, so the probability of finding a 1selectron at any given point dependsonlyon its distance from the nucleus. The probability density is greatest atr= 0 (at the nucleus) and decreases steadily with increasing distance. At very large values ofr, the electron probability density is tiny butnotexactly zero.

In contrast to the probability density, we can calculate theradial probability(the probability of finding a 1selectron at a distancerfrom the nucleus) by adding together the probabilities of an electron being at all points on a series ofxspherical shells of radiusr1,r2,r3,…,rx− 1,rx. In effect, we are dividing the atom into very thin concentric shells, much like the layers of an onion (Figure 1a), and calculating the probability of finding an electron on each spherical shell. Recall that the electron probability density is greatest atr = 0 (Figure 1b), so the density of dots is greatest for the smallest spherical shells in Figure 1a.

The surface area of each spherical shell is equal to 4πr2, which increases rapidly with increasingr (Figure 1c). Because the surface area of the spherical shells increases at first more rapidly with increasingr than the electron probability density decreases, the plot of radial probability has a maximum at a particular distance (Figure 1d). Importantly, when ris very small, the surface area of a spherical shell is so small that thetotal probability of finding an electron close to the nucleus is very low; at the nucleus, the electron probability vanishes because the surface area of the shell is zero (Figure 1d).

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Another representation of the 1sorbital is given in Figure 2. Again, this dot density diagram illustrates the regions where an electron is likely to be found in the “electron cloud”.

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A second characteristic evident from Figure 2 is the shapeof the electron cloud. In this two-dimensional diagram it appears to be approximatelycircular; in three dimensions it would bespherical(Figure 3). The following image is a three-dimensional dot-density diagram for the orbital of the hydrogen atom shown in Figure 2. These boundary surface diagrams are constructed by drawing a circle (or sphere) around a large percentage (say 75 or 90%) of the dots, as has been done in Figure 2 (red line). Since such a sphere or circle encloses most of (but not all) the electron density, it is about as close as one can come to drawing a boundary which describes the shape of the orbital. Boundary surface plots in two and three dimensions are easier to draw quickly than dot-density diagrams, so chemists use them a great deal. Remember that these boundary surface plots are not a specific orbit on which to find an electron (i.e., electrons are not racing around it like a racetrack), but rather a construct to help us visualize where an electron is likely to reside. Therefore, based on Figure 2 and Figure 3, we can say thats orbitals generally have a spherical shape.
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Not all s orbitals are the same, however. While the 1sorbital looks like that shown in Figure 2, recall that there are alsosorbitals inn= 2, 3, etc. (called 2s, 3s, and ns orbitals). Figure 4 compares the electron probability densities for the hydrogen 1s, 2s, and 3sorbitals. Note that all three are spherically symmetrical. For the 2sand 3sorbitals, however (and for all othersorbitals as well), the electron probability density does not fall off smoothly with increasingr. Instead, a series of minima and maxima are observed in the radial probability plots (Figure 4c). The minima correspond to radial nodes (regions of zero electron probability), which alternate with spherical regions of nonzero electron probability. The orbitals depicted in Figure 4 are of the s type, thus l = 0 for all of them.

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Three things happen tosorbitals asn increases (Figure 4):

  1. They become larger, extending farther from the nucleus.
  2. They contain more nodes. This is similar to a standing wave that has regions of significant amplitude separated by nodes (points with zero amplitude). The number of radial nodes in an orbital is nl – 1.
  3. For a given atom, thesorbitals also become higher in energy asn increases because of the increased distance from the nucleus.

Orbitals are generally drawn as three-dimensional surfaces that enclose 90% of theelectron density.Although such drawings show the relative sizes of the orbitals, they do not normally show the spherical nodes in the 2sand 3sorbitals because the spherical nodes lie inside the 90% surface. Fortunately, the positions of the spherical nodes are not important for chemical bonding. This makes sense because bonding is an interaction of electrons from two atoms which will be most sensitive to forces at the edges of the orbitals.

p-Orbitals

Onlysorbitals are spherically symmetrical. As the value oflincreases, the number of orbitals in a given subshell increases, and the shapes of the orbitals become more complex. Because the 2psubshell hasl= 1, with three values ofml(−1, 0, and +1), there are three 2p orbitals.

The dot density diagram for one of the hydrogen 2porbitals is shown inFigure 5. This orbital has two lobes of electron density arranged along the z axis with an electron density of zero in thexy plane. This type of node is called a nodal plane (instead of a radial node which was seen in thes orbitals). Since the xy plane is the nodal plane in Figure 5, it is a 2pz orbital (the orbital is oriented along thez axis).

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As shown in Figure 6, the other two 2porbitals have identical shapes, but they lie along thexaxis (2px) andyaxis (2py), respectively. Note that each 2p orbital has just one nodal plane.

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Just as with thesorbitals, the size and complexity of theporbitals for any atom increase as the principal quantum numbernincreases. The shapes of the 90% probability surfaces of the 3p, 4p, and higher-energyp orbitals are, however, essentially the same as those shown in Figure 6.The shapes of porbitals for n > 2 look like strings of beads oriented along the x, y, and z axis with two additional nodes per unit increases in n.

d-Orbitals

Subshells withl= 2 have fived orbitals; the first shell to have adsubshell corresponds ton = 3. The five dorbitals havemlvalues of −2, −1, 0, +1, and +2.

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The hydrogen 3d orbitals, shown in Figure 7, have more complex shapes than the 2porbitals. All five 3d orbitals contain two nodal planes, as compared to one for each p orbital and zero for eachsorbital. In three of thedorbitals, the lobes of electron density are oriented between thexandy,xandz, andyandzplanes; these orbitals are referred to as the 3dxy, 3dxz, and 3dyzorbitals, respectively. A fourthdorbital has lobes lying along thexandy axes; this is the 3dx2-y2orbital. The fifth 3d orbital, called the 3dz2orbital, has a unique shape: it looks like a 2pzorbital combined with an additional doughnut of electron probability lying in thexy plane. Despite its peculiar shape, the 3dz2 orbital is mathematically equivalent to the other four and has the same energy. Like thesandporbitals, asnincreases, the size of thed orbitals increases, but the overall shapes remain similar to those depicted in Figure 7.

f-Orbitals

Principal shells with n = 4 can have subshells with l = 3 and ml values of −3, −2, −1, 0, +1, +2, and +3. These subshells consist of seven f orbitals. Although these orbitals play an important role in the heavier elements, their shapes are complicated and we will not consider these shapes in this course

Orbital Energies

Although we have discussed the shapes of orbitals, we have said little about their comparative energies. We begin our discussion oforbital energies by considering atoms or ions with only a single electron (such as H or He+). This is the simplest case.

The relative energies of the atomic orbitals withn ≤ 4 for a hydrogen atom are plotted in Figure 8. Note that the orbital energies depend ononlythe principal quantum numbern, not on l. Consequently, the energies of the 2sand 2porbitals of hydrogen are the same; the energies of the 3s, 3p, and 3dorbitals are the same; and so forth. The orbital energies obtained for hydrogen using quantum mechanics are exactly the same as the allowed energies calculated by Bohr. In contrast to Bohr’s model, however, which allowed only one orbit for each energy level, quantum mechanics predicts that there are4orbitals with different electron density distributions in then= 2 principal shell (one 2sand three 2p orbitals),9in then= 3 principal shell, and16in then = 4 principal shell. As we have just seen, quantum mechanics predicts that in the hydrogen atom, all orbitals with the same value of n(e.g., the three 2porbitals) aredegenerate, meaning that they have the same energy. Figure 8 shows that the energy levels become closer and closer together as the value ofnincreases, as expected because of the 1/n2dependence of orbital energies.

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Spin Quantum Number

It was demonstrated in the 1920s that when hydrogen line spectra (which we saw previously) are examined at extremely high resolution, some lines are actually not single peaks but rather pairs of closely spaced lines. This is the so-called fine structure of the spectrum, and it implies that there are additional small differences in energies of electrons even when they are located in the same orbital. These observations led Samuel Goudsmit and George Uhlenbeck to propose that electrons have a fourth quantum number. They called this the spin quantum number, or ms.

The other three quantum numbers—n, l, and mlare properties of specific atomic orbitals that define the most likely location in space of an electron. These orbitals are a result of solving the Schrödinger equation for electrons in atoms. The electron spin is a different kind of property. It is a completely quantum phenomenon with no analogues in the classical realm. In addition, it cannot be derived from solving the Schrödinger equation and is not related to the normal spatial coordinates (such as the Cartesian x, y, and z). Electron spin describes an intrinsic electron “rotation” or “spinning.” Each electron acts as a tiny magnet, just as if it were a tiny rotating object charged with an angular momentum, even though this rotation cannot be observed in terms of the spatial coordinates.

The magnitude of the overall electron spin can only have one value, and an electron can only “spin” in one of two quantized states. One is termed the α state, with the z component of the spin being in the positive direction of the z axis. This corresponds to the spin quantum number ms = +½. The other is called the β state, with the z component of the spin being negative and ms = -½. Any electron, regardless of the atomic orbital it is located in, can only have one of those two values of the spin quantum number. The energies of electrons having ms = -½ and ms = ½ are different if an external magnetic field is applied.

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Figure 9illustrates this phenomenon. An electron acts like a tiny magnet. Its moment is directed up (in the positive direction of the z axis) for the +½ spin quantum number and down (in the negative z direction) for the -½ spin quantum number. A magnet has a lower energy if its magnetic moment is aligned with the external magnetic field (the left electron in Figure 19) and a higher energy for the magnetic moment being opposite to the applied field. This is why an electron withms = +½ has a slightly lower energy in an external field in the positive z direction, and an electron with ms = -½ has a slightly higher energy in the same field. This is true even for an electron occupying the same orbital in an atom. A spectral line corresponding to a transition for electrons between the same orbitals but with different spin quantum numbers has two possible values of energy; thus, the line in the spectrum will show a fine structure splitting.

The Pauli Exclusion Principle

An electron in an atom is completely described by four quantum numbers: n, l, ml, and ms. The first three quantum numbers define the orbital and the fourth quantum number describes the intrinsic electron property called spin. An Austrian physicist Wolfgang Pauli formulated a general principle that gives the last piece of information that we need to understand the general behavior of electrons in atoms. The Pauli exclusion principle can be formulated as follows: No two electrons in the same atom can have exactly the same set of all four quantum numbers. What this means is that electrons can share the same orbital (the same set of the quantum numbers n, l, and ml), but only if their spin quantum numbers, ms, have different values. Since the spin quantum number can only have two values (± ½), no more than two electrons can occupy the same orbital (and if two electrons are located in the same orbital, they must have opposite spins). Therefore, any atomic orbital can be populated by only zero, one, or two electrons.

The properties and meaning of the quantum numbers of electrons in atoms are briefly summarized in Table 1.

NameSymbolAllowed valuesPhysical meaning
principal quantum numbern1, 2, 3, 4, ….shell, the general region of an electron in the orbital (distance away from the nucleus)
azimuthal (or angular momentum) quantum numberl0 ≤ ln – 1subshell, the shape of the orbital
magnetic quantum numbermllmllorientation of the orbital
spin quantum numberms+½, −½direction of the intrinsic quantum “spinning” of the electron
Table 1. Quantum numbers, their properties, and significance

Example 1

Maximum Number of Electrons
Calculate the maximum number of electrons that can occupy a shell with (a) n = 2, (b) n = 5, and (c) n as a variable. Note you are only looking at the orbitals with the specified n value, not those at lower energies.

Solution
(a) When n = 2, there are four orbitals (a single orbital with l = 0, and three orbitals labeled l = 1). These four orbitals can contain eight electrons.

(b) When n = 5, there are five subshells of orbitals that we need to sum:

1 orbital withl = 0

3 orbitals withl = 1

5 orbitals withl = 2

7 orbitals withl = 3

+ 9 orbitals withl = 4

———————————————

25 orbitals total

Again, each orbital holds two electrons, so 50 electrons can fit in this shell.

(c) The number of orbitals in any shell n will equal n2. There can be up to two electrons in each orbital, so the maximum number of electrons will be 2 × n2

Check Your Learning
If a shell contains a maximum of 32 electrons, what is the principal quantum number, n?

Answer:

n = 4

Key Concepts and Summary

The azimuthal quantum number determines the general shape of the orbital. For l = 0 (an s orbital), the orbital is spherical. Forl = 1 (p orbitals), there are three different p orbitals, but they all have a dumbbell shape. Different ml values are used to differentiate between the three orbitals. The d orbitals, with l = 2, generally have a four-lobed shape.As the n value increases, so does the complexity of the orbitals in each subshell. The first three quantum numbers describe these orbitals. The fourth quantum number is the spin quantum number. Each electron has a spin quantum number, ms, that can be equal to ±½. No two electrons in the same atom can have the same set of values for all the four quantum numbers, known as the Pauli exclusion principle. A consequence of the Pauli exclusion principle is that each orbital can hold at most two electrons.

Glossary

degenerate orbitals
orbitals with the same energy level

d orbital
region of space with high electron density that is either four lobed or contains a dumbbell and torus shape; describes orbitals with l = 2. An electron in this orbital is called a d electron

f orbital
multilobed region of space with high electron density, describes orbitals with l = 3. An electron in this orbital is called an f electron
p orbital
dumbbell-shaped region of space with high electron density, describes orbitals with l = 1. An electron in this orbital is called a p electron
Pauli exclusion principle
specifies that no two electrons in an atom can have the same value for all four quantum numbers
s orbital
spherical region of space with high electron density, describes orbitals with l = 0. An electron in this orbital is called an s electron

spin quantum number (ms)
number specifying the electron spin direction, either +½ or -½

Chemistry End of Section Exercises

  1. Consider the orbitals shown here in outline.
    Orbitals and the 4th Quantum Number, (M7Q6) – UW-Madison Chemistry 103/104 Resource Book (10)
    1. What is the maximum number of electrons contained in an orbital of type (x)? Of type (y)? Of type (z)?
    2. How many orbitals of type (x) are found in a shell with n = 2? How many of type (y)? How many of type (z)?
    3. Write a set of quantum numbers for an electron in an orbital of type (x) in a shell with n = 4. Of an orbital of type (y) in a shell with n = 2. Of an orbital of type (z) in a shell with n = 3.
    4. What is the smallest possible n value for an orbital of type (x)? Of type (y)? Of type (z)?
    5. What are the possible l and ml values for an orbital of type (x)? Of type (y)? Of type (z)?
  2. What are the allowed values for each of the four quantum numbers: n, l, ml, and ms?
  3. How many electrons could be held in the second shell of an atom if the spin quantum number ms could have three values instead of just two? (Hint: Consider the Pauli exclusion principle.)
  4. Write a set of quantum numbers for each of the electrons with an n of 4 in a Se atom.
  5. Identify the subshell in which electrons with the following quantum numbers are found:
    1. n = 2, l = 1
    2. n = 4, l = 2
    3. n = 6, l = 0
  6. Identify the subshell in which electrons with the following quantum numbers are found:
    1. n = 3, l = 2
    2. n = 1, l = 0
    3. n = 4, l = 3

Answers to Chemistry End of Section Exercises

  1. (a) x. 2, y. 2, z. 2; (b) x. 1, y. 3, z. 0; (c) x. 4 0 0, y. 2 1 0, z. 3 2 0; (d) x. 1, y. 2, z. 3; (e) x. l = 0, ml = 0, y. l = 1, ml = –1, 0, or +1, z. l = 2, ml = –2, –1, 0, +1, +2
  2. n = 1, 2, 3…, l = 0, … n-1, ml = –l, … l, ms = -½, +½
  3. 12
  4. nlmlms
    400
    400
    41−1
    410
    41+1
    41−1
    Table 4.
  5. (a) 2p; (b) 4d; (c) 6s
  6. (a) 3d; (b) 1s; (c) 4f
Orbitals and the 4th Quantum Number, (M7Q6) – UW-Madison Chemistry 103/104 Resource Book (2024)
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