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← General Chemistry I

2. Quantum Theory and Electronic Structure

Why does hydrogen glow in only a few colours?

Connect light to energy, read atomic spectra, use the Bohr model, and describe orbitals with quantum numbers.

TheoryFirst, the vocabulary of lightWavelength, frequency and the energy of a photon. You need these for everything that follows.
Theory 1 · the vocabulary

Light as a wave, and its energy

How are a light wave's wavelength, frequency and energy connected?

schematic: the real range is 24 powers of ten, squeezed into a few crestsgamma raysX-raysultravioletvisibleinfraredmicrowavesradio waves1 pm1 nm1 µm1 mm1 m1 kmwavelength (each mark is 1000 times longer) → longer waves, lower frequency, less energy per photon
Wavelength λ550 nm
Frequency ν5.45 × 10¹⁴ Hz
Photon energy2.25 eV
Per mole of photons218 kJ/mol
Regionvisible
Step 1 of 3 · Explore the spectrumDrag the marker along the spectrum, or click the examples. Visit at least five different regions. Watch what happens to the wave, the frequency and the energy of one photon.Regions visited: 1 of 5 needed.
The maths
Every electromagnetic wave travels at the speed of light: c = λ ν = 2.998 × 10⁸ m/s
Frequency: ν = c / λ = 2.998 × 10⁸ m/s ÷ 5.50 × 10⁻⁷ m = 5.45 × 10¹⁴ Hz
Energy of one photon: E = hν = (6.626 × 10⁻³⁴ J·s)(5.45 × 10¹⁴ Hz) = 3.61 × 10⁻¹⁹ J = 2.254 eV
One mole of photons: E × N_A = (3.61 × 10⁻¹⁹ J)(6.022 × 10²³/mol) = 217.5 kJ/mol
Shortcut: E (eV) = 1239.8 eV·nm ÷ λ (nm). Shorter wave, higher frequency, more energy per photon.
Questions you might have (4)
Why can a microwave oven heat food if its photons have so little energy?

Brightness is the number of photons. An oven sends an enormous number of them, and food's water molecules absorb them by rotating faster, which is heat. One microwave photon cannot break a bond, but a trillion trillion of them can warm a cup of tea. A single ultraviolet photon can break a bond.

What is the difference between wavelength, frequency and speed?

Wavelength is the distance from one crest to the next. Frequency is how many crests pass a point each second. Speed is how fast the crests move: speed = wavelength × frequency. All light moves at c in a vacuum, so a shorter wavelength can only mean a higher frequency.

Why does the scale go up in steps of 1000?

The wavelengths of light run from smaller than an atomic nucleus to longer than a football field. A scale that jumps by a factor of 1000 at each mark is the only way to fit them all on one line. Each mark on it is 1000 times the one before.

How do I convert between eV, J and kJ/mol?

1 eV = 1.602 × 10⁻¹⁹ J. To go from the energy of one photon to the energy of a mole of them, multiply by Avogadro's number (6.022 × 10²³). 1 eV per photon is 96.485 kJ/mol. Chemists quote bond energies in kJ/mol and physicists quote photon energies in eV.

Work through it to see what it shows.
ExperimentsHow light and matter turned out to come in packetsEach result breaks the old picture, and forces the next idea.
Experiment 1 · 1900

The furnace

A hot object glows, and the colour changes with the heat. Why does the classical theory fail, and what fixes it?

Berlin, 1900
↑ drag
450 K
ultravioletinfrared5001000150020002500wavelength, nm

Hot things glow, and the color changes with the heat. Nobody can say why.

Drag the furnace up to heat it.

What it showed

The old theory of light gets the red end of the glow right and then climbs without limit toward the ultraviolet. Planck fixed it with one assumption: a hot object gives off light only in packets of energy E = hf, where f is the frequency and h is a new constant of nature.

Chemistry takes one thing from this: energy is not smooth. It comes in steps. Hold on to h, because the next experiment measures it again.

Experiment 2 · 1887–1916

The photoelectric effect

When light hits a metal, electrons can come out. Does a brighter light knock them out harder, as a wave should?

Kcollectorammeter: 0.0 µA
Brightness
brighter (more photons)
dimmer
50%
Collector voltage
against the electrons
none
0.00 V
fine
Colour of the light: drag along the strip. 700 nm, red, 1.77 eV per photon
200300400500600700800900UVIR
Metal:
Step 1 of 7 · PredictLight is a wave, and a brighter wave carries more energy. Predict: will very bright red light free electrons from this metal?
Current against collector voltage012345voltage against the electrons (V)no current at any voltage
Energy of the fastest electrons against frequency05101501234frequency (× 10¹⁴ Hz)kinetic energy (eV)
0 recorded
Photon energy hf1.77 eV
Work function φ2.29 eV
Fastest electronsnone
Current0.0 µA
The maths
A photon of this light: E = hf = hc/λ = 1239.8 eV·nm ÷ 700 nm = 1.77 eV (f = 4.28 × 10¹⁴ Hz)
The metal holds its electrons with a work function φ = 2.29 eV. Threshold: λ ≤ hc/φ = 541 nm
hf = 1.77 eV is less than φ = 2.29 eV, so one photon cannot free an electron. More photons do not help: each electron takes one photon, not a share of many.
Questions you might have (4)
Why should a wave not behave like this?

A wave spreads its energy over its whole front, and a brighter wave has more energy in every spot. Give an electron time and it should soak up enough to escape, whatever the colour. And a brighter wave should send electrons out faster. The measurements show neither: no electrons below a threshold frequency, at once above it, and speed set by colour alone.

What is a work function?

The least energy that frees an electron from the metal's surface. The electrons are held in by the attraction of the positive ions, and each metal holds them with a different strength. Caesium holds them loosely (1.95 eV) and lead tightly (4.25 eV). Real values depend on how clean the surface is.

Why does the current fall to zero at the stopping voltage?

Raising the collector's voltage against the electrons makes each one climb a potential hill of height eV. An electron with kinetic energy less than eV turns back. At V_s, even the fastest, with KE_max, just fails to arrive, so eV_s = KE_max.

Is a photon a particle? And is this the same h as Planck's?

In this experiment, light is absorbed in lumps of energy hf, one lump per electron. It is the same constant, h, that Planck needed to fit the furnace in 1900. Two quite different experiments give the same value. That agreement convinced physicists the packets are real. (Light also shows wave behaviour in other experiments: later in this unit.)

Run the experiment to see what it showed.
Experiment 3 · 1885–1913

The spectrum of hydrogen

A hot solid glows in every colour. What does a glowing gas give?

A hot solid glows with a smooth rainbow. But a glowing gas gives off only a few sharp colours, and hydrogen gives the simplest set. Why those colours and no others? Each colour is a clue about how the electron sits in the atom. First you will measure them. Then you will look for the rule that ties them together. That rule is the clue that points to Bohr's model, in the next section.
Light source:
400450500550600650700750wavelength (nm)
Marker at550.0 nm
Colour heregreen
SourceWhite-hot filament
Tube glowswhite
Step 1 of 4 · Compare the lightClick the white-hot filament, then at least two of the gases. Look at how the light is spread out. What is different about a hot solid and a gas?Looked at so far: 1 of the sources.
The maths
Nothing to calculate yet. Compare how the light from each source is spread out.
Questions you might have (4)
How is the light made?

The gas sits at low pressure in a glass tube. A high voltage drives electrons through it, and they collide with the atoms. A collision gives an atom energy, and the atom gives it back as light. In a hot solid the atoms are packed together and disturb each other, which smears the light into a smooth rainbow.

How does the instrument split the light into colours?

A prism, or better a diffraction grating, bends each wavelength by a different amount, so the colours spread out along a line. The scale under the picture is the wavelength of each position.

Are the lines really a fingerprint?

Yes. No two elements have the same set of lines, so a spectrum names the elements in a flame, a lamp or a star. Helium was found in the Sun's spectrum in 1868, a quarter of a century before anyone found it on Earth.

Where do the other lines' wavelengths come from?

Helium, mercury and sodium are from the NIST Handbook of Basic Atomic Spectroscopic Data (wavelengths in air). Hydrogen's are computed from the Rydberg formula, which agrees with the measured values.

Run the experiment to see what it showed.
TheoryFrom one electron to the periodic tableBohr's ladder, then the wave nature of the electron, orbitals, and the rules that build the table.
Theory 2 · 1913

Bohr's ladder of energy levels

Why does hydrogen give off exactly those colours? Drag the electron down the ladder and see which colours come out.

Your taskMake hydrogen give off the four visible colours you measured (falls to level 2 from levels 3, 4, 5 and 6). Then find a colour you cannot see: one fall that gives ultraviolet and one that gives infrared.Visible lines made: 0 of 4 · ultraviolet found: not yet · infrared found: not yet
energy (eV)0 (free)-13.60-3.40-1.51true spacing: levels crowd together near 0n = 1n = 2n = 3n = 4n = 5n = 6n = 7
orbit radius grows as n² (not to exact scale)
The electron is on n = 6. Click or drag a rung to move it there (or press a number key, 1 to 7). A fall makes light come out.
The spectrum you have made (visible light). Faint white marks are the four lines you measured in Experiment 3.
400450500550600650700750
The maths
Allowed energies: E_n = −13.6 eV / n² (at n = ∞ the electron is free: 13.6 eV is the energy to ionize hydrogen)
Now n = 6: E = −13.6 / 6² = -0.38 eV, orbit radius r = 0.0529 n² nm = 1.91 nm
Questions you might have (5)
Why are only certain levels allowed?

Bohr did not know. He assumed it, because it fit the spectrum. The reason comes from the electron behaving like a wave, which only fits around the atom for certain energies. That is the next experiment, and it leads to orbitals.

Why is the energy negative?

Zero is chosen as the energy of an electron that has just escaped the atom. An electron still bound to the nucleus has less energy than that, so its energy is negative. Level 1 is the most negative (−13.6 eV) and is the most tightly bound. It takes 13.6 eV to pull the electron free from there: the ionization energy of hydrogen.

Can the electron sit between two levels?

No. It is on one level or another. When it changes level it does so in one jump, and the energy goes into (or comes out as) a single photon of exactly the energy difference. That is why only certain colours come out.

Is the electron really going round in a circle?

No. The circles are a picture. The energy levels are real, and Bohr's formula for them is right for hydrogen. The idea of a circular track was replaced by orbitals, regions where the electron is likely to be found. Orbitals are coming up.

What about atoms with more than one electron?

Bohr's model gets hydrogen right, and one-electron ions like He⁺, but fails for atoms with two or more electrons, because the electrons repel each other. For those we need orbitals, subshells and the rules for filling them: that is electron configuration, and it is what the periodic table is built on.

Work through it to see what it shows.
ExperimentsThe electron is a waveBohr left a question open: why those levels? The answer starts with an experiment.
Experiment 4 · 1924–1927

Electrons behave like waves

Light acts like particles. Do particles, like electrons, act like waves?

Photons are packets of light, but they also behave as waves. Is the reverse true? Can a particle, such as an electron, behave as a wave? A wave would be diffracted by the regular rows of atoms in a crystal, and a bullet would not. Look for the difference.
0°15°30°45°60°75°90°electron gunnickel crystal: rows of atoms 0.215 nm apartdetector
Electron voltage
faster electrons
slower
54 V
fine
Electrons counted at each angle (54 V)0°30°60°90°detector angle from the normalrelative count
Step 1 of 3 · Sweep the detectorAt 54 volts, drag the detector round the arc (or use the sweep button) and watch the count. If electrons are only tiny bullets, it should follow the dashed curve. Does it?
Detector at10.0°
Count here0.38
Electron wavelength λ = h/p0.1669 nm
Peaks marked0
The maths
De Broglie (1924): a particle of momentum p has a wavelength λ = h / p. Electrons accelerated through V volts: p = √(2 m e V), so λ = 1.226 / √V nm
At 54 V: p = √(2 m e V) = 3.97 × 10⁻²⁴ kg·m/s λ = h / p = 0.1669 nm
Questions you might have (4)
How could Davisson and Germer tell it was a wave?

A bullet bounces off in a smooth spread of directions. A wave scattered by many regularly spaced atoms goes in only where the waves from neighbouring rows arrive in step, and cancels everywhere else. That gives sharp peaks at angles set by the wavelength and the spacing: n λ = D sin θ. They found a peak at the angle the formula gave for the wavelength h/p. (They found it by accident in 1925, when a nickel target they were studying was heated and became a crystal. G. P. Thomson, J. J. Thomson's son, found the same effect with thin films in 1927. They shared the 1937 Nobel Prize in Physics.)

Is the electron a wave or a particle?

Both descriptions are needed. Each electron arrives at the detector as a single point, like a particle. But where the electrons arrive follows the wave pattern. The wave tells you the probability of finding the electron at each place. This idea is the heart of quantum mechanics, and it is how orbitals are described later in this unit.

Why do I not diffract when I walk through a door?

Wavelength = h / (mass × speed). For a 0.145 kg baseball at 40 m/s that is 1.1 × 10⁻³⁴ m, about 10¹⁹ times smaller than a nucleus, so there is nothing for it to diffract around. An electron is about 10²⁹ times lighter than a baseball, so its wavelength is large enough to fit between the atoms of a crystal.

What is D, and why 0.215 nm?

D is the spacing between the rows of atoms on the surface of the nickel crystal, which acts as the diffraction grating. For the crystal face Davisson and Germer used it is 0.215 nm. The wave needs a wavelength about as large as D to be diffracted noticeably, which is why electrons of a few tens of volts work.

Run the experiment to see what it showed.
TheoryWhy the levels existPut the electron's wave round the atom, and the ladder falls out.
Theory 3 · 1924

Why only certain levels? Standing waves

Bohr assumed the electron can only have certain energies. De Broglie's waves explain why.

Your taskDrag the electron outward from the nucleus. At each radius the electron has a wavelength, and that wave has to be drawn around the circle. Find every radius where the wave joins up with itself. Find at least four.Closed waves found: none yet
1234567the wave does not meet itselfdrag the electron in or out (number keys 1 to 7 jump to a ring)
Jump to a radius:
Orbit radius2.40 a₀
Wavelength0.515 nm
Waves round the orbit1.55
Closes up?no
The maths
Classical physics allows any radius. At r = 2.40 a₀ = 0.127 nm the electron moves at v = 1.41 × 10⁶ m/s
De Broglie: λ = h / (m v) = 0.5151 nm
Wavelengths that fit around the circle: N = 2πr / λ = 1.549 (it turns out N = √(r / a₀))
N is not a whole number: after one trip the wave is out of step with its start. The next trip cancels it. No standing wave, so this orbit is not allowed.
Questions you might have (4)
Why must the wave join up with itself?

The electron goes round and round. If one trip ends out of step with where it began, the second trip overlaps the first with a shift, the third with another shift, and so on. Crests meet troughs and the wave cancels itself out. Only if the wave repeats exactly after one trip can the pattern survive, and that needs a whole number of wavelengths round the circle. A guitar string works the same way: it must fit a whole number of half-wavelengths between its ends.

Is this really a derivation of Bohr's levels?

Yes, for hydrogen. Combine the classical balance of forces (which gives the speed on a circular orbit), de Broglie's wavelength λ = h/mv, and the condition that a whole number of wavelengths fit. The radius comes out as r = n² × 0.0529 nm and the energy as −13.6 eV / n². The model was a stepping stone: the real picture, quantum mechanics, treats the electron as a wave spread through three-dimensional space, not a ring.

Where does the Bohr radius 0.0529 nm come from?

It is a combination of constants: a₀ = 4πε₀ħ² / (m e²), where m is the electron's mass, e its charge, ħ = h / 2π and ε₀ the permittivity of free space. It is the radius of the smallest standing-wave orbit.

What changes when there is more than one electron, or three dimensions?

The wave can fit round the nucleus in more patterns than a ring: with nodes, lobes and different shapes. Each allowed pattern is an orbital, labelled by a set of whole numbers, the quantum numbers. Electrons also repel each other, which splits levels of the same n into subshells. All of that is next.

Work through it to see what it shows.
Theory 4 · 1927

The uncertainty principle

If the electron is a wave, can we know exactly where it is and how fast it is going?

The pointIn Bohr's picture the electron goes round the nucleus on a track, with an exact position and speed at every moment. The wave picture says that cannot be true. See why, and see how big the effect is for an electron, a proton and a baseball.
Particle:
schematic: a narrow packet is built from many different wavelengths
How precisely is the position known? Drag the marker (each tick is 1000 times bigger). Smaller means more precisely.
1 fm1 pm1 nm1 µm1 mmnucleusatombacteriumgrain of sand
The smallest possible uncertainty in the electron's speed (m/s, log scale):
10⁻³⁰10⁻²⁰10⁻¹⁰10⁰10¹⁰walkingelectron in Hlight
Try:
Step 1 of 3 · An electron in an atomWith the electron chosen, drag the marker until the uncertainty in its speed equals its speed in hydrogen, 2.19 × 10⁶ m/s. How big is the region?
Position known to Δx100 pm
Momentum uncertain by Δp ≥5.3 × 10⁻²⁵ kg·m/s
Speed uncertain by Δv ≥5.8 × 10⁵ m/s
Compared with light1.9e-3 × c
The maths
Heisenberg: Δx · Δp ≥ ħ/2 (ħ = h/2π = 1.05 × 10⁻³⁴ J·s; some books write Δx·Δp ≥ h/4π, the same thing)
Position known to Δx = 100 pm = 1.0 × 10⁻¹⁰ m → Δp ≥ ħ / (2Δx) = 5.27 × 10⁻²⁵ kg·m/s
For a electron (m = 9.11 × 10⁻³¹ kg): Δv = Δp / m ≥ 5.79 × 10⁵ m/s
Questions you might have (4)
Is this because our instruments disturb the particle?

No. That was Heisenberg's first way of describing it, but the deeper reason is that a particle is a wave. A wave that is spread out can have one wavelength, so one momentum, but no precise position. A wave squeezed into a small space needs many wavelengths added together, so it has no precise momentum. It is a property of the waves, however good the measurement.

How does this affect Bohr's orbits?

It means the electron cannot have a definite path, because a path needs an exact position and speed at every moment. What we can know is where the electron is likely to be found, and that is what an orbital shows. Bohr's energy levels are right, but his circular orbits are only a picture.

Why can an electron not be inside the nucleus?

Hold it in a region the size of a nucleus (5 × 10⁻¹⁵ m) and its speed would be uncertain by more than the speed of light, which is impossible. In other words it would need a huge amount of energy to stay confined. That is why electrons form a cloud around the nucleus, and not in it.

Why does a baseball not seem uncertain?

Because the uncertainty Δv = ħ / (2mΔx) is divided by the mass. For a 145 g baseball located to a millimetre it is about 4 × 10⁻³¹ m/s, which is far smaller than anything that can be measured, or that matters. The principle is always true, but it only shows up for the very small, such as electrons.

Work through it to see what it shows.
TheoryFrom a ring to orbitalsIn three dimensions the electron's wave has more patterns. Each one is an orbital, named by quantum numbers.
Theory 5 · 1926

Orbitals and quantum numbers

A ring is the simplest wave round a nucleus. What does the electron's wave look like in three dimensions?

Your taskLook at the orbitals of the first three shells: 1s, 2s, 2p, 3s, 3p and 3d. Count the nodes and the orientations, and see how the quantum numbers set the shape.Orbitals visited: 1 of 6
Click an orbital (l can only go up to n − 1):
l = 0 (s)l = 1 (p)l = 2 (d)l = 3 (f)
n = 1
n = 2
n = 3
n = 4
The 3 p orbitals (one for each ml from −1 to +1):
zx
wave positivewave negativebrighter = more likelyslice in the xz plane
Chance of finding the 2p electron at distance r from the nucleus4.0 a₀r (a₀ = 0.0529 nm). Gold: likeliest r. Red: nodes.
Orbital2p pz
Radial nodes0
Angular nodes1
Orbitals in subshell3
Electrons it holds6
Step 1 of 3 · Look at six orbitalsClick the six orbitals in the table, 1s up to 3d. Notice how the shape changes with l and how the number of rings grows with n.Not yet visited: 1s, 2s, 3s, 3p, 3d
The maths
Quantum numbers of this orbital: n = 2, l = 1 (p), m_l = −1 … +1 (3 orientations), m_s = ±½
Energy in hydrogen: E = −13.6 eV / n² = -3.40 eV (it depends only on n, so all the 2 subshells of this shell have the same energy in hydrogen)
Nodes (places where the electron is never found): radial = n − l − 1 = 0, angular = l = 1, total = n − 1 = 1
Room for electrons: 2p holds 2(2l + 1) = 6; the whole shell n = 2 holds 2n² = 8
Questions you might have (5)
What does the picture show?

A slice through the orbital, with the nucleus in the middle. The brightness is ψ², the chance of finding the electron at each point. It is a cloud, not a path: the electron is not going round on a track. The colour is the sign (positive or negative) of the wave. For one orbital on its own the sign has no effect, but it matters when orbitals overlap to form bonds, which you will meet in the unit on bonding.

Is the graph the same thing as the picture?

No. They are two views of the same wave. The picture shows the chance of finding the electron at each point in space (ψ² at that point), so it has the orbital's shape. The graph adds up all the directions and asks a simpler question: how likely is the electron to be at a given distance from the nucleus, anywhere on the sphere of that radius? It is P(r) = r²R(r)², and it has no shape in space.

The two can disagree. The 1s picture is brightest right at the nucleus, but the graph peaks at one Bohr radius (0.0529 nm). That is because there is a lot more room, a much bigger sphere, at a larger radius, even though the chance per point is lower. So the dip to zero at the nucleus in the graph is not an empty centre: it is just a tiny sphere.

What is a node?

A place where the wave is zero, so the electron is never found there. A radial node is a spherical shell. An angular node is a flat plane or a cone through the nucleus, which is why a p orbital has two lobes with a plane of zero between them. Each extra node costs energy, like the extra crest in a standing wave.

Why do 2s and 2p have the same energy here?

In hydrogen the energy depends only on n, so 2s and 2p have exactly the same energy: −3.40 eV. In an atom with more than one electron, the other electrons shield the nucleus and the subshells split: s is lower than p, and p lower than d. That splitting decides the order in which orbitals fill, which is electron configuration, the next unit.

Where does the electron's spin come from?

Spin does not come from the wave pattern. It is a property of the electron itself, found in 1922 when a beam of silver atoms was split in two by a magnetic field (the Stern–Gerlach experiment). An electron has just two spin states, ms = +½ or −½. That is why each orbital holds two electrons, and it leads to the Pauli exclusion principle, also in the next unit.

Work through it to see what it shows.
Theory 6 · 1930

A whole atom: all the shells together

One orbital at a time is not an atom. What does an atom with many electrons look like, with every shell at once?

Your taskCompare atoms. Look at lithium, sodium and potassium (down a group). Then sodium and chlorine (across a period). Finish on bromine, with its 35 electrons in four shells. Notice where the outer shell sits each time.Looked at: ○ Li ○ Na ○ K ○ Cl ✓ Br
n = 1: 2 e⁻n = 2: 8 e⁻n = 3: 18 e⁻n = 4: 7 e⁻
Picture is 312 pm across the radius. Brightness is on a log scale (about 7 powers of ten).
Where the electrons are, by distance from the nucleus1 pm10 pm100 pmdistance from the nucleus (log scale: each tick is 10 times further out)electrons per log steptabulated radius 115 pm
The picture is round on purpose: see the outer electrons
A full subshell is perfectly round: add up every orientation of its p or d orbitals and the lobes fill in a ball. A half-full one is round too. The picture above averages over direction, so every atom looks like a ball. But the outer, partly filled subshell, the valence electrons, is not round. Here it is, orbital by orbital, with the electrons placed one to an orbital first (Hund's rule), which you will meet properly in the next unit.
Bromine: outer subshell 4p⁵
pz: 2 e⁻ ↑↓px: 2 e⁻ ↑↓py: 1 e⁻ ↑
The orbitals hold different numbers of electrons, so the cloud is lopsided: more electron density in the more filled orbitals, and a dent where an orbital is short of electrons. Switch the plane to look from different sides. These lobes point in particular directions, and they are what bonds form along.
ElementBromine (35)
Electrons per shell2, 8, 18, 7
Valence electrons7
Effective charge felt, Zeff7.60
The maths
Bromine (Z = 35): 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d¹⁰ 4p⁵ electrons per shell: 2, 8, 18, 7
Valence electrons (outermost s and p): 7. Core electrons: 28.
Shielding felt by an outer 4p electron (Slater): the 6 others in its group count 0.35, the 18 in shell 3 count 0.85, the 10 deeper ones count 1.00: S = 27.40
Effective nuclear charge: Zeff = Z − S = 35 − 27.40 = 7.60. The outer electrons feel 7.6+ of the nucleus's 35+ charge.
Where the outer shell sits in this model: 164 pm (tabulated radius 115 pm: the model peak is not the same thing as the measured radius, but the trends agree)
Questions you might have (5)
Is this what a real atom looks like?

It is a model. Each filled subshell is drawn as a hydrogen-like orbital, with the nuclear charge replaced by the effective charge from Slater's rules, and averaged over direction. That is good enough to show the shells, how close the inner ones are, and the trends. It is not exact: a real atom needs a numerical calculation, and the exact sizes differ. Notice that the peak of the outer shell sits further out than the tabulated radius. Radii are defined in several ways, and none of them is the position of the peak.

What is effective nuclear charge?

The part of the nucleus's pull that an electron actually feels. The other electrons, mostly the inner ones, sit between it and the nucleus and cancel part of the charge. This is shielding. Zeff = Z − S, where S counts the shielding. Slater's rules give S: electrons in the same shell count a little (0.35), the shell below counts a lot (0.85), deeper ones count fully (1.00). Zeff for the outer electron rises steadily across a period, which is why atoms shrink from left to right.

Why is a full subshell round, and a half-full one too?

Each p orbital has a lobe along one axis. In the maths, px depends on x/r, py on y/r and pz on z/r. The density of each is the square of that, so add the three orbitals up with the same number of electrons in each: (x² + y² + z²)/r² = 1. The answer is the same in every direction, so the cloud is a perfect ball. The same happens with the five d orbitals.

That only works when every orbital in the subshell has the same number of electrons: all empty, all single (half-full, such as p³ or d⁵), or all paired (full, such as p⁶ or d¹⁰). With p⁵, one orbital has only one electron while the others have two. The sum no longer cancels, and the cloud has a dent. Rotate the 3D cloud above to see it, and try nitrogen (p³, round) against oxygen (p⁴, lopsided).

Why do all the atoms look round?

Because the big picture averages over direction, and a full subshell really is round: the lobes of all the p orbitals (or all the d orbitals) add up to a sphere. A half-full subshell is round too. Only a partly filled subshell, usually the outer valence electrons, is lopsided, and the second picture shows it. Those lobes point in particular directions, and that is what chemical bonds form along.

Why is the centre so bright, and why is the 1s shell so tiny?

The two 1s electrons feel nearly the full nuclear charge. For bromine that is about +34, so they are squeezed to about 1/35 of the size they have in hydrogen. The picture uses a log scale so that the faint outer shells show up next to this tight, dense core.

Work through it to see what it shows.
PracticeProblemsNumbers from this unit, in the style of a college problem set.
Practice

Practice

Numbers from the experiments, in the style of a college problem set. Every problem has a hint and a worked solution.

Photon energy0 right of 0 · streak 0

What is the energy of a photon of light with a wavelength of 670 nm, in electron-volts?

eV
← Previous unit1. Atoms and the Periodic TableNext unit →3. Periodic Trends of the Elements