ARMCQs DIGITAL STUDY NOTES
Chapter 2: Atomic Structure
Atomic Structure: The Essential Idea
Definition
Atomic structure describes how the nucleus and electrons are arranged in an atom. Protons and usually neutrons are inside the nucleus. Electrons are found outside it.
Understand it simply
Picture a tiny central nucleus with electrons outside it. Most of the mass is in that centre.
From an indivisible atom to subatomic particles
The Greek word atomos means “cannot be divided”. Democritus suggested that matter is made of tiny particles. Later, Dalton used atoms to explain how substances combine. Experiments then showed that atoms contain smaller particles.
Particle | Symbol | Relative charge | Mass in u (approx.) | Location |
|---|---|---|---|---|
Electron | e⁻ | −1 | 0.0005486 | Outside nucleus |
Proton | p⁺ | +1 | 1.0073 | Nucleus |
Neutron | n | 0 | 1.0087 | Nucleus |
The unit u is based on carbon-12: 1 u is one-twelfth of the mass of one carbon-12 atom. A proton is about 1836 times heavier than an electron.
A neutron is slightly heavier than a proton. Almost all the mass of an atom is in its nucleus.
A neutral atom has the same number of protons and electrons. Their charges balance. Ordinary hydrogen, ¹H, has one proton but no neutron.
Discovery of the Electron
Cathode-ray experiment
J. J. Thomson identified the electron in 1897. He studied beams called cathode rays. Crookes had studied discharge tubes earlier. Faraday’s work also helped scientists understand electricity and matter.
Apparatus and production
A discharge tube is a glass tube with a small amount of gas inside. A vacuum pump removes most of the gas. Two metal terminals connect to a high-voltage supply. The negative terminal is the cathode. The positive terminal is the anode.
High voltage produces a beam of electrons. It travels from the cathode towards the anode. The beam can make the glass or a screen glow. This glow is fluorescence: the material takes in energy and gives out light.
Cathode rays: test the electron beam
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Field off. At low gas pressure and high voltage, electrons travel from the negative cathode towards the anode. With no deflecting field, the beam travels straight.
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Properties and evidence
Observation / property | Meaning |
|---|---|
Travel straight when no deflecting field acts | Can cast a sharp shadow behind an opaque object |
Deflect towards a positive electric plate | Carry negative charge |
Are deflected by magnetic fields | Are moving charged particles; direction depends on field orientation |
Cause fluorescence; carry kinetic energy and momentum | The electron beam transports energy and momentum |
Same charge-to-mass ratio for different gases and electrode materials | Electrons are present in atoms of all elements |
An opaque object blocks the beam. Kinetic energy means energy of motion. The charge-to-mass ratio tells us how much charge a particle has for its mass.
Magnitude of electron charge-to-mass ratio: |e|/me ≈ 1.759 × 10¹¹ C kg⁻¹ = 1.759 × 10⁸ C g⁻¹. The electron’s charge is negative; C denotes coulomb, the charge unit.
Canal Rays and the Proton
Canal-ray experiment
In 1886, Goldstein used a cathode with holes in it. Positive gas ions moved towards the negative cathode. Some passed through the holes. These streams were called canal rays.
Canal rays come from gas particles that lose electrons. They do not come out of the anode. One fast electron can knock an electron out of a gas particle:
M + e⁻ → M⁺ + 2e⁻.
One electron enters. Two electrons leave, along with a positive ion.
Canal rays: positive gas ions
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Ionize the gas. Fast electrons remove electrons from gas particles: M + e⁻ → M⁺ + 2e⁻. Positive ions form in the gas; they are not emitted by the anode.
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Essential properties
Without a deflecting field, the rays travel roughly straight.
Positive ions bend towards a negative electric plate.
Their charge-to-mass ratio depends on the gas and the ion.
The ions are much heavier than electrons.
Identifying the proton
The lightest positive ion is H⁺. It is the nucleus of hydrogen: one proton. Canal rays made from other gases contain other positive ions. Rutherford later identified hydrogen nuclei produced in nuclear reactions. He reported this work in 1919.
Example: ¹⁴₇N + ⁴₂He → ¹⁷₈O + ¹₁H.
Mass numbers: 14 + 4 = 17 + 1.
Atomic numbers: 7 + 2 = 8 + 1.
The emitted ¹₁H nucleus is a proton.
Discovery of the Neutron
Chadwick’s experiment, 1932
In 1932, James Chadwick directed alpha particles at beryllium. Beryllium gave out radiation that knocked protons out of paraffin wax. The results showed that the radiation contained particles with no charge. Their mass was close to that of a proton. Chadwick had found neutrons.
An alpha particle is a helium nucleus: 2 protons and 2 neutrons. Bombardment means sending fast particles towards a target.
⁹₄Be + ⁴₂He → ¹²₆C + ¹₀n.
Mass numbers: 9 + 4 = 12 + 1.
Atomic numbers: 4 + 2 = 6 + 0.
Chadwick: follow the neutron evidence
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Alpha particles hit Be. Alpha particles from a radioactive source strike a beryllium target. Each alpha particle contains 2 protons and 2 neutrons.
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Properties
A neutron has no charge. Its mass is about 1 u. Neutrons are found in most atomic nuclei. An electric field does not directly bend their paths. Their ability to pass through matter depends on their energy and the material.
Atomic Number, Mass Number and Particle Counts
Definitions
Atomic number, Z = number of protons. It identifies the element. Mass number, A = protons + neutrons. Neutron number = A − Z. For a neutral atom, electron number = Z.
Understand it simply
Z counts protons. A counts protons plus neutrons. For a neutral atom, electrons equal protons.
A and Z count particles, so they are whole numbers with no units. Write A at the upper left of the element symbol. Write Z at the lower left. This is nuclide notation. A nuclide is identified by its numbers of protons and neutrons.
Reading carbon-12 notation
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Choose a heavier isotope of the same element. What must change?
Choose what you expect, then test it below. You can explore without answering first.
Start with the selected neutral atom. Compare its proton, neutron and electron counts.
Choose the isotope with the next higher mass number. Read A, Z and the three particle counts.Changing the isotope changes neutrons and mass number. Proton number and the neutral atom’s electron count stay fixed. Shell rings are a model, not literal paths.
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Worked counts
Species | Protons = Z | Neutrons = A − Z | Electrons |
|---|---|---|---|
²³₁₁Na | 11 | 23 − 11 = 12 | 11 |
²³₁₁Na⁺ | 11 | 12 | 11 − 1 = 10 |
³⁵₁₇Cl⁻ | 17 | 35 − 17 = 18 | 17 + 1 = 18 |
An atom becomes an ion by losing or gaining electrons. Its proton number and mass number stay the same. Mass number counts protons and neutrons. Atomic mass is a mass, usually measured in u.
Rutherford’s Atomic Model
Gold-foil experiment
Geiger and Marsden carried out the experiment under Rutherford’s direction. Rutherford used their results to suggest the nuclear model in 1911.
Positive alpha particles passed through a narrow opening in a lead block. This made a narrow beam. The beam hit thin gold foil. A zinc sulfide screen gave a tiny flash wherever a particle arrived. A change in a particle’s direction is called scattering.
Rutherford: three scattering outcomes
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Most pass straight. Most alpha particles pass almost straight through thin gold foil. Most atomic volume is outside the very small nucleus.
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Observation → conclusion
Observation | Conclusion |
|---|---|
Most alpha particles passed almost straight through | Most atomic volume is outside the tiny nucleus |
Some were deflected | Positive charge is concentrated in a small region |
Very few were strongly deflected or backscattered | The nucleus is extremely small, dense and massive |
Nuclear model
The nucleus is small and positively charged.
It contains almost all the mass of the atom.
Electrons are outside the nucleus. Rutherford pictured them moving around it.
In a neutral atom, positive and negative charges balance.
The nucleus is much smaller than the whole atom.
The experiment showed that positive charge is concentrated in a small nucleus. Neutrons were discovered later. They were not part of Rutherford’s original 1911 model.
Limitations
1. The model could not explain why an atom stays stable. Classical physics says that an electron in a circular path should lose energy. It would then spiral into the nucleus.
2. The model could not explain why atoms give out only certain colours of light.
A spectrum shows radiation arranged by wavelength or frequency. A line spectrum has separate lines with gaps between them. A continuous spectrum has a full range without gaps. Atoms give line spectra.
Bohr’s Atomic Model
Core idea, 1913
In 1913, Niels Bohr suggested that electrons can have only certain energies. This helped explain hydrogen’s line spectrum. Quantized means “only certain values are allowed”.
Postulates
1. In the Bohr model, electrons occupy allowed circular orbits of definite energy.
2. An electron in an allowed stationary state does not radiate energy. Stationary means its energy stays constant, not that it stops moving.
3. An electron moves to a higher level when it absorbs energy. A drop to a lower level emits a photon—a packet of electromagnetic radiation.
4. The energy change equals the photon energy: |ΔE| = hν.
5. Allowed angular momentum: mvr = nh/(2π), where n = 1, 2, 3, … .
The number n labels the main energy level. Levels 1, 2, 3 and 4 are called K, L, M and N. The lowest allowed state is the ground state. An atom with extra energy is in an excited state.
h is the Planck constant: about 6.626 × 10⁻³⁴ J s. The symbol ν is frequency: the number of cycles each second. In mvr, m is electron mass, v is speed and r is orbit radius. Angular momentum describes motion around a centre.
Bohr transitions: absorb or emit
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An electron moves from n = 1 to n = 3. Does it take in or give out energy?
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The electron starts at n = 1. The level spacings in this picture are schematic.
Choose n = 3, then return to n = 1. Read the message after each change.Choose a higher level to absorb energy. Photon energy equals the difference between the two allowed levels.
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Why a line spectrum?
Only certain energy levels are allowed. An electron can therefore give out only certain photon energies.
E(high) − E(low) = hν.
A bigger energy gap gives a photon with a higher frequency.
Success and limitations
Bohr’s model works well for species with one electron: H, He⁺, Li²⁺ and Be³⁺. It does not fully explain atoms with several electrons. It also misses some fine details of spectra and the effects of electric and magnetic fields.
A magnetic field can split spectral lines: the Zeeman effect. An electric field can also split them: the Stark effect. The uncertainty principle says we cannot know an electron’s exact position and exact momentum together. A fixed classical path does not fit this idea.
H⁺ has no electron, so it is not a one-electron species. Bohr’s circular orbits belong to a historical model. Modern theory does not give electrons fixed circular paths.
Quantum Ideas and de Broglie’s Hypothesis
Planck and Einstein
In 1900, Planck suggested that energy is taken in or given out in small packets. In 1905, Einstein used packets of light, called photons, to explain the photoelectric effect. In this effect, suitable light knocks electrons out of a material.
Photon energy: E = hν.
Wave relation for light in vacuum: c = νλ.
Hence E = hc/λ.
λ (lambda) = wavelength; c = speed of light. A shorter wavelength means higher photon energy.
de Broglie’s hypothesis
Matter can show both particle and wave behaviour. The de Broglie wavelength is λ = h/p, where p is momentum. At speeds much lower than light speed, p = mv. So λ = h/(mv).
Connection with photon relations
For a photon, E = pc and E = hc/λ.
Therefore pc = hc/λ.
Cancel c: p = h/λ, giving λ = h/p.
de Broglie extended this wavelength–momentum relationship to matter. He proposed that matter also follows this relation. An electron is not a photon.
E = mc² gives rest energy: energy linked to mass even when an object is at rest. It does not give an electron’s energy of motion. For the electron’s wavelength, use λ = h/p. At low speeds, p ≈ mv.
Electron momentum and wavelength
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p. De Broglie wavelength λ = h/p. The wave shown represents matter-wave behaviour, not a wavy path traced by an electron.
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Key consequences
Electron diffraction is evidence of wave behaviour. Waves spread and form patterns when they meet obstacles or openings.
Greater momentum means a shorter wavelength.
Everyday objects have wavelengths too small to notice in daily life.
Schrödinger’s Model: Orbitals, Not Orbits
Quantum mechanical model
In 1926, Schrödinger developed a wave equation for electrons. It helps predict where an electron is likely to be. It does not give a fixed circular path. Probability means the chance of finding something.
Understand it simply
Instead of drawing one exact electron path, modern theory predicts where we are likely to find the electron.
Orbital
An atomic orbital describes an allowed electron state and where the electron is likely to be found. It is described mathematically by a wavefunction. In an electron-cloud picture, a denser region means a greater chance of finding the electron there.
Bohr orbit | Atomic orbital |
|---|---|
A definite path in the historical model | An electron state showing where the electron is likely to be found |
Described by a circular radius and energy | Described by quantum numbers (labels for the state) and a wavefunction (a mathematical description) |
Electron drawn on a fixed track | No fixed electron trajectory assigned |
Orbital probability-region shapes
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s orbital. An s orbital has a spherical probability distribution. The drawing is not a solid ball or an electron path.
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Subshells are labelled s, p, d and f. Each contains one or more orbitals. An s orbital is spherical. A p orbital has two main lobes. The d and f shapes are more complex.
Shells, Subshells and Their Capacities
Shell
A shell contains electron states with the same principal quantum number, n. This number labels the main energy level. K, L, M, N, O and P correspond to n = 1–6. A shell is an energy-level group, not a physical ring.
Understand it simply
Think of a shell as a main energy group. It contains smaller groups called subshells. Subshells contain orbitals.
n | Shell | Subshells available | Maximum electrons, 2n² |
|---|---|---|---|
1 | K | 1s | 2 |
2 | L | 2s, 2p | 8 |
3 | M | 3s, 3p, 3d | 18 |
4 | N | 4s, 4p, 4d, 4f | 32 |
5 | O | 5 subshells | 50 |
6 | P | 6 subshells | 72 |
Shell n contains n subshells. Its maximum electron capacity is 2n². This is a limit, not the number of electrons it must contain.
Subshell and orbital
A subshell is a division of a shell containing orbitals of the same type. Each orbital holds at most two electrons.
Subshell | Number of orbitals | Maximum electrons |
|---|---|---|
s | 1 | 2 |
p | 3 | 6 |
d | 5 | 10 |
f | 7 | 14 |
Shell → subshell → orbital
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Shell. The L shell has principal quantum number n = 2. It contains the 2s and 2p subshells.
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In hydrogen, a higher n means higher energy. In atoms with several electrons, subshell type also matters. For example, 4s starts filling before 3d. An inner shell does not always fill to its full capacity before the next shell starts.
Electronic Configuration: First 18 Elements
Definition
Electronic configuration is the distribution of electrons among shells, subshells and orbitals. A ground-state configuration is the lowest-energy arrangement.
Understand it simply
Electronic configuration tells us where to place the electrons. Fill the lower-energy places first.
How to write it
1. Find the number of electrons. For a neutral atom, it equals Z.
2. Fill lower-energy orbitals first.
3. Keep within each orbital’s and subshell’s capacity.
4. Add the superscripts. Their total must equal the number of electrons.
For the first 18 elements: 1s → 2s → 2p → 3s → 3p. In 2p⁴, 2 labels the shell, p the subshell and 4 the electrons in it.
Ground-state filling order
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1s then 2s. For the first elements, electrons fill 1s before 2s. Each s subshell can hold 2 electrons.
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Worked example: oxygen, Z = 8
Electron count = 8.
1s receives 2 → 6 remain.
2s receives 2 → 4 remain.
2p receives the remaining 4.
Configuration = 1s² 2s² 2p⁴.
Shell distribution = 2, 6. Check: 2 + 2 + 4 = 8.
Oxygen: electron distribution 2, 6
Change the model · explore the parts
Choose a heavier isotope of the same element. What must change?
Choose what you expect, then test it below. You can explore without answering first.
Start with the selected neutral atom. Compare its proton, neutron and electron counts.
Choose the isotope with the next higher mass number. Read A, Z and the three particle counts.Changing the isotope changes neutrons and mass number. Proton number and the neutral atom’s electron count stay fixed. Shell rings are a model, not literal paths.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
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Configuration table
Z | Element | Shell distribution | Subshell configuration |
|---|---|---|---|
1 | Hydrogen (H) | 1 | 1s¹ |
2 | Helium (He) | 2 | 1s² |
3 | Lithium (Li) | 2, 1 | 1s² 2s¹ |
4 | Beryllium (Be) | 2, 2 | 1s² 2s² |
5 | Boron (B) | 2, 3 | 1s² 2s² 2p¹ |
6 | Carbon (C) | 2, 4 | 1s² 2s² 2p² |
7 | Nitrogen (N) | 2, 5 | 1s² 2s² 2p³ |
8 | Oxygen (O) | 2, 6 | 1s² 2s² 2p⁴ |
9 | Fluorine (F) | 2, 7 | 1s² 2s² 2p⁵ |
10 | Neon (Ne) | 2, 8 | 1s² 2s² 2p⁶ |
11 | Sodium (Na) | 2, 8, 1 | 1s² 2s² 2p⁶ 3s¹ |
12 | Magnesium (Mg) | 2, 8, 2 | 1s² 2s² 2p⁶ 3s² |
13 | Aluminium (Al) | 2, 8, 3 | 1s² 2s² 2p⁶ 3s² 3p¹ |
14 | Silicon (Si) | 2, 8, 4 | 1s² 2s² 2p⁶ 3s² 3p² |
15 | Phosphorus (P) | 2, 8, 5 | 1s² 2s² 2p⁶ 3s² 3p³ |
16 | Sulfur (S) | 2, 8, 6 | 1s² 2s² 2p⁶ 3s² 3p⁴ |
17 | Chlorine (Cl) | 2, 8, 7 | 1s² 2s² 2p⁶ 3s² 3p⁵ |
18 | Argon (Ar) | 2, 8, 8 | 1s² 2s² 2p⁶ 3s² 3p⁶ |
The M shell can hold up to 18 electrons. In the first 18 elements, only its 3s and 3p subshells fill. Argon is therefore 2,8,8. This does not mean that the M shell can hold only 8 electrons.
Isotopes and Their Structures
Definition
Isotopes are atoms of the same element with the same atomic number but different mass numbers. They have equal proton counts and different neutron counts.
Understand it simply
Keep the protons the same and change the neutrons. The element stays the same, but its mass number changes.
Neutral isotopes have the same electron arrangement. Their chemical behaviour is therefore very similar. Their masses differ, so some physical properties differ. Some isotopes are radioactive.
Hydrogen isotopes
Isotope | Notation | Protons | Neutrons | Electrons if neutral |
|---|---|---|---|---|
Protium | ¹₁H | 1 | 0 | 1 |
Deuterium | ²₁H (D) | 1 | 1 | 1 |
Tritium | ³₁H (T) | 1 | 2 | 1 |
Hydrogen: same Z, different neutrons
Change the model · explore the parts
Choose a heavier isotope of the same element. What must change?
Choose what you expect, then test it below. You can explore without answering first.
Start with the selected neutral atom. Compare its proton, neutron and electron counts.
Choose the isotope with the next higher mass number. Read A, Z and the three particle counts.Changing the isotope changes neutrons and mass number. Proton number and the neutral atom’s electron count stay fixed. Shell rings are a model, not literal paths.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Other textbook examples
Element / Z | Isotopes | Neutrons, A − Z | Key point |
|---|---|---|---|
Carbon / 6 | ¹²C, ¹³C, ¹⁴C | 6, 7, 8 | ¹²C and ¹³C stable; ¹⁴C radioactive |
Chlorine / 17 | ³⁵Cl, ³⁷Cl | 18, 20 | About 75% and 25%, using textbook rounding |
Uranium / 92 | ²³⁴U, ²³⁵U, ²³⁸U | 142, 143, 146 | All radioactive; ²³⁸U makes up about 99.27% of natural uranium |
Chlorine isotopes: compare counts
Change the model · explore the parts
Choose a heavier isotope of the same element. What must change?
Choose what you expect, then test it below. You can explore without answering first.
Start with the selected neutral atom. Compare its proton, neutron and electron counts.
Choose the isotope with the next higher mass number. Read A, Z and the three particle counts.Changing the isotope changes neutrons and mass number. Proton number and the neutral atom’s electron count stay fixed. Shell rings are a model, not literal paths.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
Abundance tells us how common an isotope is in a sample. Carbon-12 is the most common natural carbon isotope: about 98.9% with the textbook’s rounding.
Applications of Isotopes
Why useful?
Some isotopes have unstable nuclei. Their nuclei change on their own and give out radiation. We can use a detectable isotope as a tracer to follow a substance. Radiation is also used for treatment, sterilizing equipment and producing power.
Isotope | Application | Essential distinction |
|---|---|---|
Phosphorus-32; strontium-90 | Specialist beta-radiation treatments, including selected superficial applications | Not a general treatment for every skin cancer |
Cobalt-60 | Radiotherapy and sterilization of medical materials | Gamma radiation treats tissue or destroys microorganisms |
Iodine-123 / iodine-131 | Thyroid imaging / treatment of selected thyroid conditions | Diagnosis finds disease; therapy treats it |
Technetium-99m | Diagnostic imaging, including bone scans | A tracer for scans; not routine radiotherapy |
Americium-241 | Ionization smoke detectors; some industrial gauges | Smoke alters an ionization current |
Gold-198 / technetium-labelled tracers | Specialist tracer studies of flows, sediments and pollutants | Trace movement rather than remove pollution |
Uranium-235 | Fuel in nuclear fission reactors | Splitting nuclei releases heat; steam drives a turbine |
Plutonium-238 | Heat source for power systems; historically some pacemaker batteries | Supplies energy, not direct regulation of each heartbeat |
Carbon-14 | Dating once-living material in archaeology | Not suitable for all fossils or all geological ages |
Radiotherapy uses radiation to treat disease. Sterilization destroys living microorganisms. Fission splits a heavy nucleus. Technetium-99m has extra nuclear energy and changes after a short time. The m stands for metastable.
Choose an isotope to suit the task. Its radiation and lifetime both matter. Radioactive decay changes the nucleus. An ordinary chemical reaction does not.
The thyroid is a gland in the neck. It helps control metabolism: the body’s chemical reactions.
Textbook Exercise: Short Questions
1. Show isotopes using chlorine structures.
³⁵₁₇Cl: 17 p, 18 n, 17 e; shells 2, 8, 7.
³⁷₁₇Cl: 17 p, 20 n, 17 e; shells 2, 8, 7.
Same Z = 17, different A = 35 and 37: they are isotopes.
Chlorine isotopes: compare counts
Change the model · explore the parts
Choose a heavier isotope of the same element. What must change?
Choose what you expect, then test it below. You can explore without answering first.
Start with the selected neutral atom. Compare its proton, neutron and electron counts.
Choose the isotope with the next higher mass number. Read A, Z and the three particle counts.Changing the isotope changes neutrons and mass number. Proton number and the neutral atom’s electron count stay fixed. Shell rings are a model, not literal paths.
Change the controls to see the result. Choose Explore diagram parts for a guided explanation.
View complete static diagram
2. An atom has 5 electrons in its M shell.
For the first-18-element ground-state arrangement:
(a) K = 2, L = 8, M = 5. Total = 15 electrons; a neutral atom has Z = 15.
(b) Shells: 2, 8, 5; subshells: 1s² 2s² 2p⁶ 3s² 3p³.
(c) Element: phosphorus, P.
This answer assumes a neutral atom in its lowest-energy, or ground, state. The M-shell count alone is not enough if the particle is an ion or is in an excited state.
3. Why does Rutherford’s model have defects?
Classical orbiting electrons should radiate energy and spiral into the nucleus, so the model cannot explain stability. It also does not explain discrete line spectra.
4. Explain de Broglie’s wave–particle duality.
Electrons and other matter exhibit particle and wave behaviour. Their wavelength is λ = h/p, or approximately h/(mv) at low speeds. Electron diffraction provides evidence of wave behaviour.
5. State Bohr-model limitations.
It works mainly for one-electron species. It does not adequately explain multi-electron spectra, fine details or field-induced splitting. A fixed electron path conflicts with the uncertainty principle.
6. Differentiate shell and subshell.
Shell | Subshell |
|---|---|
Main group with principal number n | Division within a shell |
K, L, M, N; n = 1, 2, 3, 4 | s, p, d, f types |
Maximum 2n² electrons | Maximum s², p⁶, d¹⁰, f¹⁴ |
L shell: up to 8 electrons | L contains 2s and 2p |
7. Compare oxygen-17 and oxygen-16.
Both have Z = 8: 8 protons and, if neutral, 8 electrons, with configuration 1s² 2s² 2p⁴. Oxygen-17 has 17 − 8 = 9 neutrons; oxygen-16 has 16 − 8 = 8. They are isotopes with very similar chemical behaviour but different masses.
9. Give subatomic-particle masses and charges.
Particle | Approximate mass in u | Relative charge |
|---|---|---|
Electron | 0.0005486 | −1 |
Proton | 1.0073 | +1 |
Neutron | 1.0087 | 0 |
Textbook Exercise: Detailed Questions
1. Explain the gold-foil experiment and atomic structure.
A narrow alpha beam struck thin gold foil. A zinc sulfide screen detected particles as flashes. Most passed almost straight through; a few deflected; very few returned.
Hence the atom has a tiny dense positive nucleus and a much larger surrounding region occupied by electrons. Nearly all mass is nuclear. The experiment did not establish neutrons or fixed energy shells.
2. Give isotope applications in daily life.
Cobalt-60: selected radiotherapy and medical-material sterilization.
Iodine-123: thyroid imaging; iodine-131: selected thyroid treatments.
Technetium-99m: diagnostic imaging, including bone scans.
Americium-241: ionization smoke detectors.
Uranium-235: nuclear-reactor fuel.
Carbon-14: dating once-living material.
Gold-198 and technetium-labelled tracers: specialist flow and environmental studies.
Phosphorus-32 and strontium-90: selected specialist beta-radiation treatments.
Plutonium-238: heat-based power, historically including some pacemaker batteries.
3. Compare Bohr’s and Rutherford’s models.
Point | Rutherford | Bohr |
|---|---|---|
Common feature | Tiny positive nucleus with external electrons | Retains the nuclear atom |
Electron motion | Classical orbital picture | Only certain allowed orbits |
Energy | No successful quantization rule | Definite allowed electron energies |
Stability | Not explained classically | Proposed allowed states in which electrons do not give out energy |
Hydrogen lines | Not explained | Transitions give |ΔE| = hν |
4. Relate de Broglie’s idea to Planck and Einstein.
Planck–Einstein photon relation: E = hν.
Since c = νλ, E = hc/λ.
For a photon, E = pc.
Equate: pc = hc/λ.
Cancel c: p = h/λ, so λ = h/p.
de Broglie proposed this relation for matter too. For a slow electron, p ≈ mv, giving λ ≈ h/(mv). Do not substitute the rest-energy expression mc² for the kinetic energy of a slow electron.
5. Explain production and properties of cathode rays.
A discharge tube contains low-pressure gas, electrodes and a high-voltage supply. Cathode rays are streams of electrons moving from the negative cathode towards the anode.
They travel straight without deflecting fields, cast shadows, cause fluorescence, carry energy and momentum, and bend towards a positive electric plate. Magnetic fields also deflect them.
Their charge-to-mass ratio stays the same when the gas or electrode material is changed. This shows that atoms of all elements contain electrons.
6. Describe Schrödinger’s model.
Schrödinger’s wave equation describes allowed electron states. A wavefunction is the mathematical description used to find where an electron is likely to be. An orbital is an electron state, not a fixed path.
A denser electron cloud means a greater chance of finding the electron there. Orbitals form subshells, and subshells form shells. s orbitals are spherical; p orbitals have two lobes.
The model includes the wave nature of electrons.
7. Outline evidence for electron, proton and neutron.
Electron: Thomson’s cathode rays had negative charge and a common charge-to-mass ratio.
Proton: positive hydrogen ions are hydrogen nuclei; Rutherford identified hydrogen nuclei ejected in nuclear reactions. Goldstein’s canal rays established positive gas ions, not protons in every gas.
Neutron: Chadwick’s beryllium radiation ejected protons from wax, demonstrating neutral particles with masses close to a proton.
8. Calculate protons, neutrons and electrons.
For each neutral atom: protons = Z; electrons = Z; neutrons = A − Z.
Atom | A | Z | Protons | Neutrons = A − Z | Electrons |
|---|---|---|---|---|---|
⁵⁶₂₆Fe | 56 | 26 | 26 | 56 − 26 = 30 | 26 |
¹⁷₈O | 17 | 8 | 8 | 17 − 8 = 9 | 8 |
³⁷₁₇Cl | 37 | 17 | 17 | 37 − 17 = 20 | 17 |
²³⁵₉₂U | 235 | 92 | 92 | 235 − 92 = 143 | 92 |
¹⁴₆C | 14 | 6 | 6 | 14 − 6 = 8 | 6 |
Test Yourself: Answers
Atomic and mass numbers
(a) Oxygen with 8 protons has Z = 8.
(b) Chlorine with 17 protons and 18 neutrons has A = 17 + 18 = 35.
(c) ⁵⁹₂₇Co: 27 protons, 59 − 27 = 32 neutrons, 27 electrons if neutral.
(d) Ordinary hydrogen, ¹H, has no neutron.
Models and atomic mass
Protons and neutrons account for nearly all atomic mass. Rutherford used classical electron motion, which predicts continuous energy loss; Bohr introduced quantized stationary states and discrete transitions. Living processes such as digestion and respiration involve chemical reactions.
Shell filling
(a) s subshell: maximum 2 electrons.
(b) Neutral Z = 11: shells 2, 8, 1; L contains 8 electrons.
(c) K fills first in ground-state atoms because 1s has the lowest energy.
(d) Full K + full L = 2 + 8 = 10 electrons.
Isotopes
Tritium has the most neutrons among hydrogen isotopes: 2. Isotopes have very similar chemical behaviour because neutral atoms share the same electron configuration; masses differ because neutron counts differ.
Carbon isotopes all have 6 protons; hydrogen isotopes all have 1 proton. Their neutron numbers vary within each element.
Formula Sheet
Quantity / relation | Expression |
|---|---|
Proton count | Z |
Neutron count | A − Z |
Neutral electron count | Z |
Photon energy | E = hν = hc/λ |
Transition energy | |ΔE| = hν |
Matter wavelength | λ = h/p; approximately h/(mv) at low speed |
Bohr angular momentum | mvr = nh/(2π) |
Shell capacity | 2n² |
Subshell capacities | s: 2; p: 6; d: 10; f: 14 |