NCERT Solutions for Class 11 Chemistry Chapter 2: Structure of Atom
Complete NCERT solutions for Class 11 Chemistry Chapter 2 Structure of Atom — all 67 exercise questions with step-by-step numerical working, every NCERT figure (2.1–2.18) redrawn as an original diagram with PDF page links, worked Problems 2.1–2.18, Tables 2.1–2.6 (including the electronic configurations of the elements), comparison tables, exam tips and full chapter-at-a-glance revision notes.
Chapter at a glance — complete revision notes
The existence of atoms was proposed by early Indian and Greek philosophers (about 400 B.C.); the word atom comes from the Greek a-tomio — “uncut-able”. John Dalton (1808) placed the atomic theory on a scientific basis and explained the laws of conservation of mass, constant composition and multiple proportions, but could not explain why glass or ebonite becomes charged on rubbing with silk or fur. Experiments at the end of the nineteenth century showed that the atom is divisible and made of electrons, protons and neutrons.
2.1 Discovery of sub-atomic particles
Basic rule: like charges repel and unlike charges attract. Insight into atomic structure came from electrical discharge through gases at very low pressure and very high voltage. (Faraday’s electrolysis in 1830 had already suggested the particulate nature of electricity.)
2.1.1 Discovery of the electron — cathode rays
- A cathode ray tube is a glass tube containing two metal electrodes (cathode, anode) at very low pressure. At high voltage a stream of particles flows from the cathode to the anode — cathode rays. A hole in the anode and a ZnS coating behind it gives a bright spot where the rays strike.
Properties of cathode rays:
- They start from the cathode and move towards the anode.
- They are invisible but their path is seen through fluorescent or phosphorescent materials that glow when hit (television tubes work this way).
- In the absence of electric or magnetic fields they travel in straight lines.
- In electric and magnetic fields they behave like negatively charged particles — called electrons.
- Their characteristics do not depend on the material of the electrodes or on the gas in the tube — so electrons are a basic constituent of all atoms.
2.1.2 Charge-to-mass ratio of the electron (J. J. Thomson, 1897)
Thomson applied electric and magnetic fields perpendicular to each other and to the path of the electrons. With only the electric field the beam strikes point A; with only the magnetic field it strikes C; by balancing the two fields the beam returns to the undeflected position B. The deflection depends on (i) the magnitude of the charge (larger charge → larger deflection), (ii) the mass (lighter particle → larger deflection) and (iii) the strength of the field.
e / me = 1.758820 × 1011 C kg−1
2.1.3 Charge on the electron (R. A. Millikan oil-drop experiment, 1906–14)
Oil droplets from an atomiser fall through a hole in the upper plate of a condenser; the air is ionised by X-rays, so the drops acquire charge by collision with gaseous ions. The fall of a charged drop can be retarded, accelerated or made stationary by the applied voltage. Millikan concluded that the charge on a drop is always an integral multiple of e — q = n e (n = 1, 2, 3 …).
e = −1.602176 × 10−19 C; me = 9.1094 × 10−31 kg (from e and e/me)
2.1.4 Discovery of protons and neutrons
- A modified discharge tube produced canal rays of positively charged gaseous ions. Their mass and e/m depend on the gas; some carry multiples of the fundamental charge; they deflect opposite to cathode rays.
- The smallest, lightest positive ion (from hydrogen) is the proton (characterised in 1919).
- Chadwick (1932) bombarded a thin sheet of beryllium with α-particles and obtained neutral particles slightly heavier than the proton — the neutrons.
Table 2.1 — Properties of fundamental particles
| Name | Symbol | Absolute charge / C | Relative charge | Mass / kg | Mass / u | Approx. mass / u |
|---|---|---|---|---|---|---|
| Electron | e | −1.602176 × 10−19 | −1 | 9.109382 × 10−31 | 0.00054 | 0 |
| Proton | p | +1.602176 × 10−19 | +1 | 1.6726216 × 10−27 | 1.00727 | 1 |
| Neutron | n | 0 | 0 | 1.674927 × 10−27 | 1.00867 | 1 |
2.2 Atomic models
After the discovery of sub-atomic particles the problems were to explain the stability of the atom, the physical and chemical behaviour of elements, the formation of molecules, and the origin of the electromagnetic radiation absorbed or emitted by atoms.
Other rays: X-rays (Röntgen, 1895) are produced when electrons strike a dense metal anode; they are not deflected by electric or magnetic fields, have very high penetrating power and very short wavelength (≈ 0.1 nm). Radioactivity (Becquerel; Curie; Rutherford; Soddy): α-rays are helium nuclei (2 units positive charge, 4 units of mass), β-rays are electrons, γ-rays are neutral high-energy radiation like X-rays. Penetrating power: α < β (about 100 times α) < γ (about 1000 times α).
2.2.1 Thomson model (1898) — “plum pudding”
The atom is a sphere (radius ≈ 10−10 m) in which positive charge is uniformly distributed and electrons are embedded to give the most stable electrostatic arrangement (plum pudding / raisin pudding / watermelon model). Mass is assumed uniformly distributed. It explained overall neutrality but was inconsistent with later experiments (Rutherford).
2.2.2 Rutherford’s nuclear model (α-particle scattering experiment)
Rutherford, Geiger and Marsden bombarded a very thin gold foil (thickness ≈ 100 nm) with α-particles from a radioactive source; a circular ZnS screen gave a flash wherever an α-particle struck it. According to Thomson’s model the α-particles should have passed through with only small deflections.
| Observation | Conclusion |
|---|---|
| Most α-particles passed undeflected | Most of the space in the atom is empty |
| A small fraction was deflected by small angles | Positive charge is concentrated in a tiny volume (huge repulsion), not spread over the atom |
| Very few (~1 in 20,000) bounced back by nearly 180° | The tiny positive centre (nucleus) is also very massive; radius of atom ≈ 10−10 m, nucleus ≈ 10−15 m (if a cricket ball were the nucleus, the atom would have a radius ≈ 5 km) |
Rutherford’s nuclear model: (i) positive charge and most of the mass are concentrated in an extremely small nucleus; (ii) electrons revolve around it at very high speed in circular orbits (solar-system model); (iii) electrons and nucleus are held by electrostatic attraction.
2.2.3 Atomic number and mass number
Atomic number (Z) = number of protons = number of electrons in a neutral atom
Mass number (A) = number of protons (Z) + number of neutrons (n)
Protons and neutrons are collectively called nucleons. The composition of an atom is written as AZX (mass number as left superscript, atomic number as left subscript).
2.2.4 Isobars and isotopes
- Isobars — same mass number, different atomic number (e.g. 146C and 147N).
- Isotopes — same atomic number, different mass number (different number of neutrons). Hydrogen: protium 11H (99.985%), deuterium 21D (0.015%), tritium 31T (traces). Carbon: 6, 7 or 8 neutrons with 6 protons; chlorine: 35Cl and 37Cl (18 and 20 neutrons, 17 protons).
- Chemical properties are controlled by the number of electrons (= number of protons), so all isotopes of an element show the same chemical behaviour.
Problem 2.1 — 8035Br (neutral): protons = electrons = 35; neutrons = 80 − 35 = 45.
Problem 2.2 — 18 electrons, 16 protons, 16 neutrons: Z = 16 (sulphur), A = 16 + 16 = 32; excess electrons = 18 − 16 = 2 so the species is an anion: 3216S2−. Always decide first whether the species is a neutral atom, cation or anion; neutrons = A − Z in every case.
2.2.5 Drawbacks of the Rutherford model
- An electron moving in a circular orbit is accelerated; by Maxwell’s theory an accelerated charge must emit radiation, lose energy and spiral into the nucleus (in ≈ 10−8 s). The model cannot explain the stability of the atom. (Stationary electrons would simply fall into the nucleus.)
- It says nothing about the distribution and the energies of electrons around the nucleus.
2.3 Developments leading to Bohr’s model of the atom
Two developments led to Bohr’s model: (i) the dual character of electromagnetic radiation (wave-like and particle-like) and (ii) experimental results on atomic spectra.
2.3.1 Wave nature of electromagnetic radiation
Maxwell (1870) showed that an accelerated charged particle produces alternating electric and magnetic fields that are transmitted as electromagnetic waves (confirmed by Hertz). Properties:
- The oscillating electric and magnetic fields are perpendicular to each other and both are perpendicular to the direction of propagation.
- Unlike sound or water waves, electromagnetic waves need no medium — they travel in vacuum.
- Different types of radiation differ in wavelength/frequency and form the electromagnetic spectrum; all travel at the same speed c = 3.0 × 108 m s−1 in vacuum.
- Characterised by frequency ν (SI unit hertz, Hz = s−1), wavelength λ (m) and wavenumber ν̄ (number of wavelengths per unit length, m−1; commonly cm−1).
c = ν λ ν̄ = 1/λ = ν/c
| Region | Approx. frequency | Use / note |
|---|---|---|
| Radio | 106 Hz | broadcasting |
| Microwave | 1010 Hz | radar |
| Infrared | 1013 Hz | heating |
| Visible | ~1015 Hz (4.0–7.5 × 1014 Hz) | the only part the eye detects |
| Ultraviolet | 1016 Hz | component of sunlight |
| X-rays | λ ≈ 0.1 nm | penetrating, electromagnetic |
Problem 2.3 (Vividh Bharati, 1368 kHz): λ = c/ν = (3.00 × 108 m s−1)/(1368 × 103 s−1) = 219.3 m — a radio wave. Problem 2.4 (visible range): violet 400 nm → ν = 3.0 × 108/400 × 10−9 = 7.50 × 1014 Hz; red 750 nm → 4.00 × 1014 Hz. Problem 2.5 (5800 Å): ν̄ = 1/λ = 1/(5800 × 10−10 m) = 1.724 × 106 m−1 (1.724 × 104 cm−1); ν = cν̄ = 5.17 × 1014 s−1.
2.3.2 Particle nature of electromagnetic radiation — Planck’s quantum theory
Wave nature explains diffraction (bending around an obstacle) and interference (combination of waves), but classical physics could not explain: (i) black-body radiation, (ii) the photoelectric effect, (iii) the variation of the heat capacity of solids with temperature, and (iv) line spectra of atoms (especially hydrogen). These show that a system can take up or radiate energy only in discrete amounts.
Black-body radiation
Hot objects emit radiation of many wavelengths; as the temperature rises, more short-wavelength light is produced (an iron rod glows dull red → red → white → blue-white). An ideal body that emits and absorbs all frequencies uniformly is a black body (carbon black is a close approximation; a cavity with a tiny hole is a good one — a ray entering the hole is eventually absorbed by the walls). The intensity and its spectral distribution depend only on temperature. At a given temperature the intensity rises with wavelength to a maximum and then falls; the maximum shifts to shorter wavelength as the temperature increases.
Planck (1900) assumed that atoms (oscillators) in the walls can emit or absorb energy only in discrete packets called quanta; the energy of a quantum is proportional to its frequency:
E = hν (h = 6.626 × 10−34 J s) allowed energies: 0, hν, 2hν, 3hν, … n hν
Quantisation is like a staircase: one can stand on any step but not in between.
Photoelectric effect
Hertz (1887): electrons are ejected when light falls on certain metals (K, Rb, Cs …).
- Electrons are ejected instantly (no time lag).
- The number of electrons is proportional to the intensity of the light.
- For each metal there is a minimum threshold frequency ν0; below it no electrons are emitted whatever the intensity (red light for hours on potassium: nothing; even weak yellow light: effect; ν0 for K = 5.0 × 1014 Hz). Above ν0 the kinetic energy rises with frequency (not with intensity).
Einstein (1905): light is a stream of photons of energy hν. A photon transfers its energy to an electron instantaneously; if the minimum energy needed is hν0 (the work function W0), the rest appears as kinetic energy. A more intense beam has more photons, hence more electrons.
hν = hν0 + ½ mev2 ⇒ K.E. = ½ mev2 = h(ν − ν0)
Table 2.2 — Work function W0 of a few metals
| Metal | Li | Na | K | Mg | Cu | Ag |
|---|---|---|---|---|---|---|
| W0 / eV | 2.42 | 2.3 | 2.25 | 3.7 | 4.8 | 4.3 |
Dual behaviour of electromagnetic radiation
Light behaves as a wave when it propagates (interference, diffraction) and as a stream of particles (photons) when it interacts with matter (black body, photoelectric effect). Some microscopic particles like electrons also show this duality.
Problem 2.6 (one mole of photons, ν = 5 × 1014 Hz): E = hν = 3.313 × 10−19 J; per mole = 3.313 × 10−19 × 6.022 × 1023 = 199.5 kJ mol−1. Problem 2.7 (100 W bulb, 400 nm): E = hc/λ = 4.969 × 10−19 J; photons per second = 100/4.969 × 10−19 = 2.012 × 1020 s−1. Problem 2.8 (300 nm on Na, K.E. = 1.68 × 105 J mol−1): photon energy = 6.626 × 10−19 J = 3.99 × 105 J mol−1; W0 = (3.99 − 1.68) × 105 = 2.31 × 105 J mol−1 = 3.84 × 10−19 J per electron; λmax = hc/W0 = 517 nm (green). Problem 2.9 (ν0 = 7.0 × 1014, ν = 1.0 × 1015 s−1): K.E. = h(ν − ν0) = 6.626 × 10−34 × 3.0 × 1014 = 1.988 × 10−19 J.
2.3.3 Evidence for quantised electronic energy levels — atomic spectra
A prism bends short wavelengths more than long ones, so white light gives a continuous spectrum (violet 7.50 × 1014 Hz to red 4 × 1014 Hz; a rainbow is similar). When atoms absorb energy they become excited and return to lower energy by emitting radiation.
- Emission spectrum — spectrum of radiation emitted by a substance that has absorbed energy (heating or irradiation).
- Absorption spectrum — a continuum is passed through the sample; the absorbed wavelengths appear as dark gaps; it is like the photographic negative of the emission spectrum.
- The study of these is spectroscopy. Gas-phase atoms give line spectra (atomic spectra): bright lines at specific wavelengths with dark spaces between. Each element has a unique line spectrum (a “fingerprint”) used in chemical analysis. Rb, Cs, Tl, In, Ga and Sc were discovered by spectroscopy; helium was discovered in the sun by spectroscopy (Bunsen was a pioneer).
Line spectrum of hydrogen
When an electric discharge is passed through gaseous hydrogen, H2 molecules dissociate and the excited H atoms emit radiation of discrete frequencies. Balmer (1885) showed that the visible lines obey
ν̄ = 109,677 (1/22 − 1/n2) cm−1, n = 3, 4, 5 … (Balmer series, the only series in the visible region).
Rydberg generalised this for all series:
ν̄ = 109,677 (1/n12 − 1/n22) cm−1 (n1 = 1, 2 …; n2 = n1 + 1, n1 + 2 …)
The value 109,677 cm−1 is the Rydberg constant for hydrogen.
Table 2.3 — Spectral lines of atomic hydrogen
| Series | n1 | n2 | Spectral region |
|---|---|---|---|
| Lyman | 1 | 2, 3 … | Ultraviolet |
| Balmer | 2 | 3, 4 … | Visible |
| Paschen | 3 | 4, 5 … | Infrared |
| Brackett | 4 | 5, 6 … | Infrared |
| Pfund | 5 | 6, 7 … | Infrared |
All line spectra share two features: (i) the line spectrum of an element is unique, and (ii) there is regularity in the lines of each element — clues to electronic structure.
2.4 Bohr’s model for the hydrogen atom
Niels Bohr (1913) used Planck’s idea of quantised energy to explain the structure and spectrum of hydrogen. Postulates:
- The electron moves around the nucleus in circular paths of fixed radius and energy called orbits, stationary states or allowed energy states, arranged concentrically.
- The energy of an electron in an orbit does not change with time. It moves to a higher state only on absorbing the required energy and to a lower state by emitting energy; the change is not continuous.
- The frequency of radiation absorbed or emitted in a transition between two states of energy difference ΔE is ν = ΔE/h = (E2 − E1)/h (Bohr’s frequency rule; E2 higher, E1 lower).
- The angular momentum is quantised: mevr = n h/2π (n = 1, 2, 3 …). (Angular momentum = I ω = mer2 · v/r = mevr.)
Hence Maxwell’s theory is not applicable to these orbits — radiation is emitted or absorbed only when the electron changes from one quantised angular momentum to another.
Results of Bohr’s theory for hydrogen:
- The stationary states are numbered n = 1, 2, 3 … (principal quantum numbers).
- Radius: rn = n2a0, where a0 = 52.9 pm; the first Bohr orbit has radius 52.9 pm. Radius increases as n2.
- Energy: En = −RH(1/n2) with RH = 2.18 × 10−18 J. Ground state (n = 1): E1 = −2.18 × 10−18 J; E2 = −0.545 × 10−18 J. For n = ∞ (free electron) E = 0 — the ionised atom.
- The negative sign means the electron in the atom has lower energy than a free electron at rest (E∞ = 0); the most negative value (n = 1) is the most stable (ground) state.
Hydrogen-like species (one electron: He+, Li2+, Be3+ …):
En = −2.18 × 10−18 (Z2/n2) J atom−1 rn = 52.9 (n2/Z) pm
As Z increases the energy becomes more negative and the radius smaller — the electron is more tightly bound. The speed of the electron increases with Z and decreases with n.
2.4.1 Explanation of the line spectrum of hydrogen
Radiation is absorbed when the electron moves from a lower to a higher n and emitted when it drops from higher to lower n:
ΔE = Ef − Ei = −2.18 × 10−18 J (1/nf2 − 1/ni2) = 2.18 × 10−18 J (1/ni2 − 1/nf2)
ν = ΔE/h = 3.29 × 1015 (1/ni2 − 1/nf2) Hz ν̄ = 1.09677 × 107 (1/ni2 − 1/nf2) m−1
This is the same as Rydberg’s empirical expression; each spectral line corresponds to a particular transition. For absorption nf > ni (positive bracket, energy absorbed); for emission ni > nf (ΔE negative, energy released). The brightness of a line depends on the number of photons of that frequency.
Problem 2.10 (n = 5 → 2): ΔE = 2.18 × 10−18(1/25 − 1/4) = −4.58 × 10−19 J (emission, Balmer, visible); ν = 4.58 × 10−19/6.626 × 10−34 = 6.91 × 1014 Hz, λ = c/ν ≈ 434 nm. Problem 2.11 (first orbit of He+): E1 = −2.18 × 10−18 × 22/12 = −8.72 × 10−18 J atom−1; r1 = 0.0529 nm × 12/2 = 0.02645 nm.
2.4.2 Limitations of Bohr’s model
- It cannot account for the finer details (doublets) of the hydrogen spectrum, the spectrum of atoms other than hydrogen (e.g. helium with two electrons), or the splitting of lines in a magnetic field (Zeeman effect) and an electric field (Stark effect).
- It cannot explain the ability of atoms to form molecules by chemical bonds.
2.5 Towards the quantum mechanical model of the atom
Because of the shortcomings of Bohr’s model, a more general model was developed using two ideas: (1) dual behaviour of matter and (2) Heisenberg’s uncertainty principle.
2.5.1 Dual behaviour of matter (de Broglie, 1924)
Just as a photon has momentum and wavelength, every material particle has a wavelength associated with it:
λ = h/(m v) = h/p
- The prediction was confirmed when an electron beam showed diffraction; this is the basis of the electron microscope (magnification about 15 million times).
- Every moving object has a wave character, but for ordinary (heavy) objects the wavelength is so small that it cannot be detected; for electrons and other subatomic particles it can.
Problem 2.12 (ball 0.1 kg at 10 m s−1): λ = 6.626 × 10−34/(0.1 × 10) = 6.626 × 10−34 m (undetectable). Problem 2.13 (electron, K.E. = 3.0 × 10−25 J): v = √(2K.E./m) = 812 m s−1; λ = h/mv = 8.967 × 10−7 m = 896.7 nm. Problem 2.14 (photon of λ = 3.6 Å): m = h/(λc) = 6.626 × 10−34/(3.6 × 10−10 × 3 × 108) = 6.135 × 10−33 kg (the printed solution gives the exponent as −29; our arithmetic gives −33).
2.5.2 Heisenberg’s uncertainty principle (1927)
It is impossible to determine simultaneously the exact position and exact momentum (or velocity) of an electron:
Δx · Δpx ≥ h/4π or Δx · Δvx ≥ h/(4π m)
If the position is known accurately (small Δx) the velocity is very uncertain, and vice versa (measuring paper thickness with an unmarked metre stick is an analogy). To “see” an electron we need light of wavelength smaller than the electron; the high-momentum photons (p = h/λ) change the electron’s energy on collision, so we know its position but not its velocity afterwards.
Significance: it rules out definite paths (trajectories) for electrons. The effect is significant only for microscopic objects. For a milligram-sized object Δv·Δx ≥ h/4πm ≈ 5 × 10−29 m2 s−1 (insignificant); for an electron Δv·Δx ≥ 5.8 × 10−5 (≈ 10−4) m2 s−1, so locating it within 10−8 m gives Δv of the order of 104 m s−1, and the picture of electrons in fixed Bohr orbits cannot hold. Statements about position and momentum must be replaced by probabilities.
Problem 2.15 (locating an electron within 0.1 Å = 10−11 m): Δv = h/(4π m Δx) = 5.79 × 106 m s−1. Problem 2.16 (golf ball 40 g, 45 m s−1, speed known to 2%): Δv = 0.9 m s−1; Δx = h/(4π m Δv) = 1.46 × 10−33 m — of no practical consequence.
Why Bohr’s model fails: it treats the electron as a particle in a well-defined circular orbit (path needs exact position and velocity — forbidden by Heisenberg) and ignores the wave character of the electron. It was therefore not extended to other atoms; quantum mechanics was needed.
2.6 Quantum mechanical model of the atom
Quantum mechanics is the theory of motion of microscopic objects that takes into account their dual (wave and particle) behaviour; for macroscopic objects it gives the same results as classical (Newtonian) mechanics. It was developed independently in 1926 by Heisenberg and Schrödinger. Schrödinger’s equation (Nobel Prize 1933) for a system whose energy does not change with time is written Ĥψ = Eψ (Ĥ = Hamiltonian operator built from kinetic energies of electrons and nuclei, attraction between electrons and nuclei, repulsion among electrons and among nuclei). Its solutions give the energy E and the wave function ψ.
For hydrogen the solutions give quantised energy states and wave functions characterised by three quantum numbers n, l, ml (the restrictions on their values arise naturally). The wave function ψ has no physical meaning by itself; the probability of finding the electron at a point is proportional to |ψ|2 (probability density, always positive). Wave functions of one-electron species are called atomic orbitals. For multi-electron atoms the equation cannot be solved exactly (approximate methods are used); the orbitals are similar to hydrogen’s but contracted by the increased nuclear charge, and their energies depend on both n and l (in hydrogen only on n).
Important features of the quantum mechanical model:
- The energy of electrons in atoms is quantised.
- Quantised levels are a direct result of the wave-like properties of electrons (allowed solutions of the Schrödinger equation).
- Exact position and velocity cannot both be known (uncertainty principle) — the path of an electron can never be determined; only the probability of finding it is discussed.
- An atomic orbital is the wave function ψ of an electron in an atom; an orbital cannot contain more than two electrons; in a multi-electron atom electrons fill orbitals in order of increasing energy; all information about the electron is stored in ψ.
- The probability of finding an electron at a point is proportional to |ψ|2; from |ψ|2 the region where the electron is most probably found can be predicted.
2.6.1 Orbitals and quantum numbers
Orbitals differ in size, shape and orientation; they are labelled by the quantum numbers n, l and ml; a fourth number ms describes the electron spin.
| Quantum number | Symbol | Allowed values | Determines |
|---|---|---|---|
| Principal | n | 1, 2, 3 … | shell (K, L, M, N …), size and (to a large extent) energy; n2 orbitals in a shell |
| Azimuthal (orbital angular momentum / subsidiary) | l | 0 to (n − 1) | subshell (n subshells in the nth shell), shape of the orbital; also energy in multi-electron atoms |
| Magnetic orbital | ml | −l, …, 0, …, +l (2l + 1 values) | orientation of the orbital; 2l + 1 orbitals per subshell |
| Spin (Uhlenbeck and Goudsmit, 1925) | ms | +½ or −½ | orientation of electron spin (↑ ↓); explains doublets and triplets in spectra |
Table 2.4 — Subshell notation
| n | l | Subshell notation |
|---|---|---|
| 1 | 0 | 1s |
| 2 | 0, 1 | 2s, 2p |
| 3 | 0, 1, 2 | 3s, 3p, 3d |
| 4 | 0, 1, 2, 3 | 4s, 4p, 4d, 4f |
| Value of l | 0 | 1 | 2 | 3 | 4 | 5 |
|---|---|---|---|---|---|---|
| Subshell notation | s | p | d | f | g | h |
| Number of orbitals (2l + 1) | 1 | 3 | 5 | 7 | 9 | 11 |
The shells are K (n = 1), L (2), M (3), N (4). An orbital with n = 2, l = 1, ml = 0 is a 2p orbital. Two electrons with different ms (+½, −½) have opposite spins; an orbital holds at most two electrons and they must have opposite spins.
Orbit and orbital are not synonymous. An orbit (Bohr) is a circular path around the nucleus; a precise path is impossible by the uncertainty principle and Bohr orbits have no real meaning. An atomic orbital is the one-electron wave function ψ characterised by n, l, ml; |ψ|2 at a point is the probability density (probability per unit volume); |ψ|2 × (small volume element) gives the probability of finding the electron in that volume.
Problem 2.17: for n = 3, l = 0, 1, 2 → one 3s, three 3p, five 3d orbitals = 1 + 3 + 5 = 9 = n2. Problem 2.18: (a) n = 2, l = 1 → 2p; (b) n = 4, l = 0 → 4s; (c) n = 5, l = 3 → 5f; (d) n = 3, l = 2 → 3d.
2.6.2 Shapes of atomic orbitals
Plots of ψ(r) and ψ2(r) against the distance r from the nucleus differ for different orbitals. For 1s the probability density is maximum at the nucleus and decreases sharply; for 2s it first falls to zero (a node), rises to a small maximum and then falls again. Regions where the probability density is zero are nodes (nodal surfaces); an ns orbital has (n − 1) nodes (one for 2s, two for 3s).
Charge-cloud (dot) diagrams show probability density by the density of dots. Boundary surface diagrams enclose a region of constant probability density in which the probability of finding the electron is high (about 90%). A 100% surface cannot be drawn because |ψ|2 is never exactly zero at any finite distance. The boundary surface of an s orbital is a sphere centred on the nucleus (a circle in two dimensions); all s orbitals are spherically symmetric and their size increases with n (4s > 3s > 2s > 1s).
p orbitals (l = 1): each consists of two lobes on either side of a plane through the nucleus where the probability density is zero (nodal plane). The three 2p orbitals have the same size, shape and energy and differ only in orientation along the x, y or z axis (2px, 2py, 2pz); the three axes are mutually perpendicular (there is no simple relation between ml = −1, 0, +1 and x, y, z). Size and energy increase 2p < 3p < 4p; the number of radial nodes is (n − 2) (one for 3p, two for 4p).
d orbitals (l = 2): the minimum n is 3; there are five (ml = −2, −1, 0, +1, +2): dxy, dyz, dxz, dx²−y² and dz². The first four have similar (four-lobed) shapes; dz² is different; all five 3d orbitals are equivalent in energy (4d, 5d … have similar shapes but differ in size and energy).
Nodes: besides radial nodes, np and nd orbitals have angular nodes (nodal planes) through the nucleus; the number of angular nodes = l (one for p, two for d). The total number of nodes is (n − 1) = l angular nodes + (n − l − 1) radial nodes.
| Orbital | Angular nodes (l) | Radial nodes (n − l − 1) | Total nodes (n − 1) |
|---|---|---|---|
| 1s | 0 | 0 | 0 |
| 2s | 0 | 1 | 1 |
| 2p | 1 | 0 | 1 |
| 3s | 0 | 2 | 2 |
| 3p | 1 | 1 | 2 |
| 3d | 2 | 0 | 2 |
| 4f | 3 | 0 | 3 |
2.6.3 Energies of orbitals
- Hydrogen (and hydrogen-like species): energy depends only on n: 1s < 2s = 2p < 3s = 3p = 3d < 4s = 4p = 4d = 4f < … Orbitals of the same energy are degenerate. 1s is the ground state; an electron in 2s, 2p or higher is in an excited state.
- Multi-electron atoms: energy depends on both n and l; for a given n it increases s < p < d < f; for higher shells the subshell energies may overlap (4s < 3d, 6s < 5d, 4f < 6p). The reason is the mutual repulsion among electrons (in hydrogen there is only electron–nucleus attraction).
Shielding and effective nuclear charge: inner-shell electrons partly screen the nuclear charge from outer electrons (shielding); the net positive charge felt is the effective nuclear charge Zeffe. The attraction increases with nuclear charge Ze, so orbital energy becomes more negative as Z increases: E2s(H) > E2s(Li) > E2s(Na) > E2s(K). Within a shell, s electrons spend more time near the nucleus (more penetration) than p, which spend more than d; so s electrons shield better and Zeff decreases with increasing l (s > p > d > f) — an s electron is held more tightly (lower energy) than p, then d.
(n + l) rule: the lower the value of (n + l), the lower the energy of the orbital; if two orbitals have the same (n + l), the one with lower n has lower energy.
Table 2.5 — Orbitals in increasing energy by the (n + l) rule
| Orbital (in increasing energy) | n | l | n + l |
|---|---|---|---|
| 1s | 1 | 0 | 1 |
| 2s | 2 | 0 | 2 |
| 2p | 2 | 1 | 3 |
| 3s | 3 | 0 | 3 |
| 3p | 3 | 1 | 4 |
| 4s | 4 | 0 | 4 |
| 3d | 3 | 2 | 5 |
| 4p | 4 | 1 | 5 |
| 5s | 5 | 0 | 5 |
| 4d | 4 | 2 | 6 |
| 5p | 5 | 1 | 6 |
| 6s | 6 | 0 | 6 |
| 4f | 4 | 3 | 7 |
| 5d | 5 | 2 | 7 |
| 6p | 6 | 1 | 7 |
| 7s | 7 | 0 | 7 |
2.6.4 Filling of orbitals in an atom
Filling follows the aufbau principle (German aufbau = building up), which is based on the relative energies of orbitals, Pauli’s exclusion principle and Hund’s rule of maximum multiplicity.
Aufbau principle: in the ground state, orbitals are filled in the order of increasing energy — electrons occupy the lowest-energy orbital available first. There is no single universal order of energies for all atoms, but the following sequence is extremely useful (and remarkably accurate for valence electrons; exceptions exist):
Pauli exclusion principle (1926): no two electrons in an atom can have the same set of four quantum numbers. Equivalently, only two electrons can occupy an orbital and they must have opposite spins (same n, l, ml but different ms). Maximum electrons: s = 2, p = 6, d = 10, f = 14; the maximum in the shell with principal quantum number n is 2n2.
Hund’s rule of maximum multiplicity: in a subshell (degenerate orbitals), pairing of electrons does not start until each orbital has one electron (singly occupied, parallel spins). Pairing therefore begins with the 4th electron in p, the 6th in d and the 8th in f. Half-filled and fully filled sets of degenerate orbitals have extra stability.
2.6.5 Electronic configuration of atoms
The distribution of electrons among orbitals is the electronic configuration. Two notations: (i) sapbdc notation (e.g. 1s22s22p1) and (ii) orbital (box) diagram in which each orbital is a box and each electron an arrow (↑ spin up, ↓ spin down) — the box diagram shows all four quantum numbers.
- H: 1s1; He: 1s2 (the two electrons have opposite spins).
- Li: 1s22s1 (third electron cannot enter 1s by Pauli); Be: 1s22s2.
- B (1s22s22p1), C (2p2), N (2p3), O (2p4), F (2p5), Ne (2p6): the 2p orbitals fill progressively.
- Na to Ar follow the same pattern with 3s and 3p: Na [Ne]3s1 … Ar [Ne]3s23p6. Electrons of completely filled shells are core electrons; those added to the shell of highest principal quantum number are valence electrons.
- K and Ca: 4s (lower than 3d) fills first (4s1, 4s2). From Sc to Zn the 3d orbitals fill (Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn); Cr and Cu adopt 3d54s1 and 3d104s1 instead of 3d44s2 and 3d94s2 because half-filled and fully filled subshells are extra stable (exceptions do exist).
- 4p fills from Ga to Kr; Rb to Xe repeat the pattern with 5s, 4d, 5p; Cs and Ba fill 6s; La to Hg fill 4f and 5d; then 6p, 7s, and finally 5f and 6d. Elements after uranium are short-lived and artificial.
The electronic configuration explains why atoms combine, why some elements are metals and others non-metals, and why helium and argon are unreactive while halogens are reactive — questions that Dalton’s model could not answer.
2.6.6 Stability of completely filled and half-filled subshells
The ground-state configuration is the one of lowest total electronic energy. In elements such as Cu and Cr, where 4s and 3d differ slightly in energy, an electron shifts from the lower (4s) to the higher (3d) subshell if that makes the 3d subshell half filled or completely filled. Hence the valence configurations are Cr: 3d54s1 and Cu: 3d104s1 (not 3d44s2 and 3d94s2). Stable (half-filled or filled) sets: p3, p6, d5, d10, f7, f14.
Causes of the extra stability:
- Symmetrical distribution of electrons — symmetry gives stability. Electrons in the same subshell have equal energy but different spatial distribution, so they shield one another relatively little and are attracted more strongly by the nucleus.
- Exchange energy — whenever two or more electrons of the same spin occupy degenerate orbitals of a subshell they can exchange positions, and the energy released is the exchange energy. The number of possible exchanges is maximum when the subshell is half filled or completely filled (Fig. 2.18), so the exchange energy and the stability are maximum. Exchange energy is the basis of Hund’s rule.
In short, the extra stability of half-filled and filled subshells is due to (i) relatively small shielding, (ii) smaller coulombic repulsion energy and (iii) larger exchange energy.
Table 2.6 — Electronic configurations of the elements (Z = 1–111), written in the noble-gas core notation. * marks elements with exceptional electronic configurations (as in the NCERT table). The NCERT table lists the f-block entries as printed here; some other reference tables give slightly different ground-state configurations for a few f-block elements (for example Ce and Bk).
| Z | El. | Configuration | Z | El. | Configuration |
|---|---|---|---|---|---|
| 1 | H | 1s1 | 57 | La* | [Xe] 5d1 6s2 |
| 2 | He | 1s2 | 58 | Ce* | [Xe] 4f2 6s2 |
| 3 | Li | [He] 2s1 | 59 | Pr | [Xe] 4f3 6s2 |
| 4 | Be | [He] 2s2 | 60 | Nd | [Xe] 4f4 6s2 |
| 5 | B | [He] 2s2 2p1 | 61 | Pm | [Xe] 4f5 6s2 |
| 6 | C | [He] 2s2 2p2 | 62 | Sm | [Xe] 4f6 6s2 |
| 7 | N | [He] 2s2 2p3 | 63 | Eu | [Xe] 4f7 6s2 |
| 8 | O | [He] 2s2 2p4 | 64 | Gd* | [Xe] 4f7 5d1 6s2 |
| 9 | F | [He] 2s2 2p5 | 65 | Tb | [Xe] 4f9 6s2 |
| 10 | Ne | [He] 2s2 2p6 | 66 | Dy | [Xe] 4f10 6s2 |
| 11 | Na | [Ne] 3s1 | 67 | Ho | [Xe] 4f11 6s2 |
| 12 | Mg | [Ne] 3s2 | 68 | Er | [Xe] 4f12 6s2 |
| 13 | Al | [Ne] 3s2 3p1 | 69 | Tm | [Xe] 4f13 6s2 |
| 14 | Si | [Ne] 3s2 3p2 | 70 | Yb | [Xe] 4f14 6s2 |
| 15 | P | [Ne] 3s2 3p3 | 71 | Lu | [Xe] 4f14 5d1 6s2 |
| 16 | S | [Ne] 3s2 3p4 | 72 | Hf | [Xe] 4f14 5d2 6s2 |
| 17 | Cl | [Ne] 3s2 3p5 | 73 | Ta | [Xe] 4f14 5d3 6s2 |
| 18 | Ar | [Ne] 3s2 3p6 | 74 | W | [Xe] 4f14 5d4 6s2 |
| 19 | K | [Ar] 4s1 | 75 | Re | [Xe] 4f14 5d5 6s2 |
| 20 | Ca | [Ar] 4s2 | 76 | Os | [Xe] 4f14 5d6 6s2 |
| 21 | Sc | [Ar] 3d1 4s2 | 77 | Ir | [Xe] 4f14 5d7 6s2 |
| 22 | Ti | [Ar] 3d2 4s2 | 78 | Pt* | [Xe] 4f14 5d9 6s1 |
| 23 | V | [Ar] 3d3 4s2 | 79 | Au* | [Xe] 4f14 5d10 6s1 |
| 24 | Cr* | [Ar] 3d5 4s1 | 80 | Hg | [Xe] 4f14 5d10 6s2 |
| 25 | Mn | [Ar] 3d5 4s2 | 81 | Tl | [Xe] 4f14 5d10 6s2 6p1 |
| 26 | Fe | [Ar] 3d6 4s2 | 82 | Pb | [Xe] 4f14 5d10 6s2 6p2 |
| 27 | Co | [Ar] 3d7 4s2 | 83 | Bi | [Xe] 4f14 5d10 6s2 6p3 |
| 28 | Ni | [Ar] 3d8 4s2 | 84 | Po | [Xe] 4f14 5d10 6s2 6p4 |
| 29 | Cu* | [Ar] 3d10 4s1 | 85 | At | [Xe] 4f14 5d10 6s2 6p5 |
| 30 | Zn | [Ar] 3d10 4s2 | 86 | Rn | [Xe] 4f14 5d10 6s2 6p6 |
| 31 | Ga | [Ar] 3d10 4s2 4p1 | 87 | Fr | [Rn] 7s1 |
| 32 | Ge | [Ar] 3d10 4s2 4p2 | 88 | Ra | [Rn] 7s2 |
| 33 | As | [Ar] 3d10 4s2 4p3 | 89 | Ac | [Rn] 6d1 7s2 |
| 34 | Se | [Ar] 3d10 4s2 4p4 | 90 | Th | [Rn] 6d2 7s2 |
| 35 | Br | [Ar] 3d10 4s2 4p5 | 91 | Pa | [Rn] 5f2 6d1 7s2 |
| 36 | Kr | [Ar] 3d10 4s2 4p6 | 92 | U | [Rn] 5f3 6d1 7s2 |
| 37 | Rb | [Kr] 5s1 | 93 | Np | [Rn] 5f4 6d1 7s2 |
| 38 | Sr | [Kr] 5s2 | 94 | Pu | [Rn] 5f6 7s2 |
| 39 | Y | [Kr] 4d1 5s2 | 95 | Am | [Rn] 5f7 7s2 |
| 40 | Zr | [Kr] 4d2 5s2 | 96 | Cm | [Rn] 5f7 6d1 7s2 |
| 41 | Nb* | [Kr] 4d4 5s1 | 97 | Bk | [Rn] 5f8 6d1 7s2 |
| 42 | Mo* | [Kr] 4d5 5s1 | 98 | Cf | [Rn] 5f10 7s2 |
| 43 | Tc | [Kr] 4d5 5s2 | 99 | Es | [Rn] 5f11 7s2 |
| 44 | Ru* | [Kr] 4d7 5s1 | 100 | Fm | [Rn] 5f12 7s2 |
| 45 | Rh* | [Kr] 4d8 5s1 | 101 | Md | [Rn] 5f13 7s2 |
| 46 | Pd* | [Kr] 4d10 | 102 | No | [Rn] 5f14 7s2 |
| 47 | Ag* | [Kr] 4d10 5s1 | 103 | Lr | [Rn] 5f14 6d1 7s2 |
| 48 | Cd | [Kr] 4d10 5s2 | 104 | Rf | [Rn] 5f14 6d2 7s2 |
| 49 | In | [Kr] 4d10 5s2 5p1 | 105 | Db | [Rn] 5f14 6d3 7s2 |
| 50 | Sn | [Kr] 4d10 5s2 5p2 | 106 | Sg | [Rn] 5f14 6d4 7s2 |
| 51 | Sb | [Kr] 4d10 5s2 5p3 | 107 | Bh | [Rn] 5f14 6d5 7s2 |
| 52 | Te | [Kr] 4d10 5s2 5p4 | 108 | Hs | [Rn] 5f14 6d6 7s2 |
| 53 | I | [Kr] 4d10 5s2 5p5 | 109 | Mt | [Rn] 5f14 6d7 7s2 |
| 54 | Xe | [Kr] 4d10 5s2 5p6 | 110 | Ds | [Rn] 5f14 6d8 7s2 |
| 55 | Cs | [Xe] 6s1 | 111 | Rg | [Rn] 5f14 6d10 7s1 |
| 56 | Ba | [Xe] 6s2 |
Quick summary of the quantum numbers
| Subshell | l | ml values | Orbitals | Max. electrons | Angular nodes |
|---|---|---|---|---|---|
| s | 0 | 0 | 1 | 2 | 0 |
| p | 1 | −1, 0, +1 | 3 | 6 | 1 |
| d | 2 | −2 … +2 | 5 | 10 | 2 |
| f | 3 | −3 … +3 | 7 | 14 | 3 |
| Shell (n) | Subshells | Orbitals (n2) | Max. electrons (2n2) |
|---|---|---|---|
| K (1) | 1s | 1 | 2 |
| L (2) | 2s, 2p | 4 | 8 |
| M (3) | 3s, 3p, 3d | 9 | 18 |
| N (4) | 4s, 4p, 4d, 4f | 16 | 32 |
Summary of the chapter
- Atoms consist of electrons, protons and neutrons; Thomson’s uniform-sphere model was disproved by Rutherford’s α-scattering (1909) which gave the nuclear model; it could not explain atomic stability or the arrangement of electrons.
- Bohr (1913): electron in quantised circular orbits of fixed energy — explains hydrogen (and one-electron ions) but ignores the wave nature of the electron and contradicts the uncertainty principle.
- Schrödinger (1926): wave-mechanical model consistent with de Broglie duality and Heisenberg uncertainty; energy states and wave functions are characterised by n, l, ml.
- In hydrogen-like species the orbital energy depends only on n; in multi-electron atoms on n and l (lower n + l = lower energy; equal n + l → lower n).
- Electrons fill orbitals by the aufbau principle, Pauli exclusion principle and Hund’s rule — the basis of electronic configurations.
Ex 2.1 — (i) Calculate the number of electrons which will together weigh one gram. (ii) Calculate the mass and charge of one mole of electrons.
Concept. The mass of a single electron is me = 9.109 × 10−31 kg (= 9.109 × 10−28 g) and its charge is e = 1.602 × 10−19 C. The number of electrons in a given mass is (total mass)/(mass of one electron); one mole contains Avogadro’s number NA = 6.022 × 1023 particles, so the mass and charge of a mole of electrons are NA times those of one electron.
Number = (1 g)/(9.109 × 10−28 g) Mass of 1 mol = NA me Charge of 1 mol = NA e
- (i) Number of electrons in 1 g: 1 g = 10−3 kg, so N = 10−3 kg / 9.109 × 10−31 kg = 1.098 × 1027 electrons.
- (ii) Mass of one mole of electrons: 6.022 × 1023 × 9.109 × 10−31 kg = 5.485 × 10−7 kg (= 5.485 × 10−4 g).
- Charge of one mole of electrons: 6.022 × 1023 × 1.602 × 10−19 C = 9.647 × 104 C (negative; with e = 1.602176 × 10−19 C it is 96,485 C).
| Quantity | One electron | One mole of electrons |
|---|---|---|
| Mass | 9.109 × 10−31 kg | 5.485 × 10−7 kg |
| Charge | −1.602 × 10−19 C | −9.647 × 104 C |
Extra depth. The charge of one mole of electrons, about 96,485 C, is called one faraday (F) and is the key quantity of electrolysis you will meet in Class XII. The mass of a mole of electrons, 5.485 × 10−4 g, is only about 1/1836 of the mass of a mole of hydrogen atoms (1.008 g), which is why the mass of an atom is practically the mass of its nucleus.
Conclusion: One gram contains 1.098 × 1027 electrons; one mole of electrons has a mass of 5.485 × 10−7 kg and a charge of 9.647 × 104 C.
Ex 2.2 — (i) Calculate the total number of electrons present in one mole of methane. (ii) Find (a) the total number and (b) the total mass of neutrons in 7 mg of 14C (mass of a neutron = 1.675 × 10−27 kg). (iii) Find (a) the total number and (b) the total mass of protons in 34 mg of NH3 at STP. Will the answer change if the temperature and pressure are changed?
Concept. The number of sub-atomic particles in a sample = (number of moles) × NA × (particles per atom or molecule). Per atom the number of protons is Z, electrons Z (neutral) and neutrons A − Z. Mass of particles = number × mass of one particle.
(i) One mole of methane, CH4. Electrons per molecule = 6 (C) + 4 × 1 (H) = 10. Electrons in one mole = 10 × 6.022 × 1023 = 6.022 × 1024.
(ii) 7 mg of 14C (Z = 6, A = 14, so 8 neutrons per atom; molar mass 14 g mol−1).
- Moles = 7 × 10−3 g / 14 g mol−1 = 5.0 × 10−4 mol.
- Atoms = 5.0 × 10−4 × 6.022 × 1023 = 3.011 × 1020.
- (a) Neutrons = 8 × 3.011 × 1020 = 2.409 × 1021.
- (b) Mass of neutrons = 2.409 × 1021 × 1.675 × 10−27 kg = 4.03 × 10−6 kg.
(iii) 34 mg of NH3 (molar mass 17 g mol−1; protons per molecule = 7 + 3 = 10).
- Moles = 34 × 10−3 / 17 = 2.0 × 10−3 mol; molecules = 2.0 × 10−3 × 6.022 × 1023 = 1.2044 × 1021.
- (a) Protons = 10 × 1.2044 × 1021 = 1.2044 × 1022.
- (b) Mass of protons = 1.2044 × 1022 × 1.6726 × 10−27 kg = 2.01 × 10−5 kg (proton mass from Table 2.1).
| Part | Species | Per atom / molecule | Amount in sample | Result |
|---|---|---|---|---|
| (i) | 1 mol CH4 | 10 e− | 1 mol | 6.022 × 1024 electrons |
| (ii) | 7 mg 14C | 8 neutrons | 5.0 × 10−4 mol | 2.409 × 1021 neutrons; 4.03 × 10−6 kg |
| (iii) | 34 mg NH3 | 10 protons | 2.0 × 10−3 mol | 1.2044 × 1022 protons; 2.01 × 10−5 kg |
Will the answer change with temperature and pressure? No. The number of particles and their mass depend only on the amount of substance (number of moles), not on temperature or pressure. T and P change only the volume of the gas (22.4 L per mole at STP), not the number of protons, neutrons or electrons in a given mass.
Extra depth. Notice that the neutron/proton mass is used only in the final step; the counting uses the mole concept. The same logic gives, e.g., the number of electrons in 1.8 g of water: 1.8/18 = 0.1 mol × 10 e− × NA = 6.022 × 1023.
Conclusion: (i) 6.022 × 1024 electrons; (ii) 2.409 × 1021 neutrons of mass 4.03 × 10−6 kg; (iii) 1.2044 × 1022 protons of mass 2.01 × 10−5 kg; no change with temperature or pressure.
Ex 2.3 — How many neutrons and protons are there in the following nuclei? 136C, 168O, 2412Mg, 5626Fe, 8838Sr
Concept. In the symbol AZX, the atomic number Z (lower left) equals the number of protons and the mass number A (upper left) equals protons + neutrons. Hence neutrons = A − Z (equations 2.3 and 2.4 of the chapter).
Protons = Z Neutrons = A − Z
| Nucleus | Z (protons) | A | Neutrons = A − Z |
|---|---|---|---|
| 136C | 6 | 13 | 13 − 6 = 7 |
| 168O | 8 | 16 | 16 − 8 = 8 |
| 2412Mg | 12 | 24 | 24 − 12 = 12 |
| 5626Fe | 26 | 56 | 56 − 26 = 30 |
| 8838Sr | 38 | 88 | 88 − 38 = 50 |
Extra depth. Light stable nuclei such as 16O and 24Mg have equal numbers of neutrons and protons; heavier nuclei need a progressively larger neutron excess (Fe: 30 n for 26 p; Sr: 50 n for 38 p) to offset the proton–proton repulsion. 13C is an isotope of carbon (7 neutrons) used in NMR; 88Sr has the magic number of 50 neutrons.
Conclusion: 13C: 6 p, 7 n; 16O: 8 p, 8 n; 24Mg: 12 p, 12 n; 56Fe: 26 p, 30 n; 88Sr: 38 p, 50 n.
Ex 2.4 — Write the complete symbol for the atom with the given atomic number (Z) and atomic mass (A): (i) Z = 17, A = 35. (ii) Z = 92, A = 233. (iii) Z = 4, A = 9.
Concept. The complete symbol of an atom is AZX: the symbol X of the element (identified from Z using the periodic table) with the mass number A as left superscript and the atomic number Z as left subscript. The element is fixed by Z alone (number of protons).
- Z = 17 is chlorine (Cl); A = 35 → 3517Cl (neutrons = 35 − 17 = 18).
- Z = 92 is uranium (U); A = 233 → 23392U (neutrons = 141).
- Z = 4 is beryllium (Be); A = 9 → 94Be (neutrons = 5).
| Z | Element | A | Complete symbol | Neutrons |
|---|---|---|---|---|
| 17 | Chlorine | 35 | 3517Cl | 18 |
| 92 | Uranium | 233 | 23392U | 141 |
| 4 | Beryllium | 9 | 94Be | 5 |
Extra depth. 35Cl is the more abundant isotope of chlorine (the other being 37Cl, Chapter 1 and Section 2.2.4); 233U is a fissile isotope made by neutron capture in thorium reactors; 9Be is the only stable isotope of beryllium and is the target in Chadwick’s neutron discovery (Section 2.1.4).
Conclusion: (i) 3517Cl; (ii) 23392U; (iii) 94Be.
Ex 2.5 — Yellow light emitted from a sodium lamp has a wavelength (λ) of 580 nm. Calculate the frequency (ν) and wavenumber (ν̄) of the yellow light.
Concept. For an electromagnetic wave in vacuum, the speed of light c, frequency ν and wavelength λ are related by c = νλ (equation 2.5). The wavenumber is the number of wavelengths per unit length, ν̄ = 1/λ. Always convert the wavelength to metres first.
ν = c/λ ν̄ = 1/λ
- λ = 580 nm = 580 × 10−9 m = 5.80 × 10−7 m.
- Frequency: ν = (3.0 × 108 m s−1)/(5.80 × 10−7 m) = 5.17 × 1014 s−1 (Hz).
- Wavenumber: ν̄ = 1/(5.80 × 10−7 m) = 1.724 × 106 m−1 = 1.724 × 104 cm−1.
| Quantity | Formula | Value |
|---|---|---|
| Wavelength λ | given | 580 nm = 5.80 × 10−7 m |
| Frequency ν | c/λ | 5.17 × 1014 Hz |
| Wavenumber ν̄ | 1/λ | 1.724 × 106 m−1 (1.724 × 104 cm−1) |
Extra depth. The value lies inside the visible range (4.0–7.5 × 1014 Hz) — it is the sodium D line (589 nm in Ex 2.50). It is also the same as Problem 2.5 of the chapter (5800 Å), which is the same wavelength.
Conclusion: ν = 5.17 × 1014 Hz and ν̄ = 1.724 × 106 m−1 (= 1.724 × 104 cm−1).
Ex 2.6 — Find the energy of each of the photons which (i) correspond to light of frequency 3 × 1015 Hz. (ii) have wavelength of 0.50 Å.
Concept. By Planck’s quantum theory the energy of one photon is E = hν where h = 6.626 × 10−34 J s. Since ν = c/λ, a photon of wavelength λ has E = hc/λ.
E = hν = hc/λ
- (i) ν = 3 × 1015 Hz: E = (6.626 × 10−34 J s)(3 × 1015 s−1) = 1.988 × 10−18 J.
- (ii) λ = 0.50 Å = 0.50 × 10−10 m = 5.0 × 10−11 m: E = (6.626 × 10−34)(3.0 × 108)/(5.0 × 10−11) = 3.976 × 10−15 J.
| Case | Given | Formula | Energy per photon |
|---|---|---|---|
| (i) | ν = 3 × 1015 Hz | hν | 1.988 × 10−18 J (≈ 12.4 eV, ultraviolet) |
| (ii) | λ = 0.50 Å | hc/λ | 3.976 × 10−15 J (≈ 24.8 keV, X-ray) |
Extra depth. The wavelength in (ii) corresponds to ν = c/λ = 6 × 1018 Hz, so the photon is an X-ray photon with about 2000 times the energy of the ultraviolet photon in (i) — energy increases with frequency and decreases with wavelength. (1 eV = 1.602 × 10−19 J was used only for the comparison.)
Conclusion: (i) E = 1.988 × 10−18 J; (ii) E = 3.976 × 10−15 J.
Ex 2.7 — Calculate the wavelength, frequency and wavenumber of a light wave whose period is 2.0 × 10−10 s.
Concept. The period T of a wave is the time for one complete oscillation; it is the reciprocal of the frequency, ν = 1/T. The wavelength then follows from c = νλ and the wavenumber from ν̄ = 1/λ = ν/c.
ν = 1/T λ = c/ν = cT ν̄ = 1/λ
- Frequency: ν = 1/(2.0 × 10−10 s) = 5.0 × 109 s−1 (Hz).
- Wavelength: λ = c/ν = (3.0 × 108 m s−1)/(5.0 × 109 s−1) = 6.0 × 10−2 m (6 cm).
- Wavenumber: ν̄ = 1/λ = 1/(6.0 × 10−2 m) = 16.67 m−1 (= 0.1667 cm−1).
| Quantity | Relation | Value |
|---|---|---|
| Period T | given | 2.0 × 10−10 s |
| Frequency ν | 1/T | 5.0 × 109 Hz |
| Wavelength λ | c/ν | 6.0 × 10−2 m |
| Wavenumber ν̄ | 1/λ | 16.67 m−1 |
Extra depth. A frequency of 5 × 109 Hz and a wavelength of 6 cm place the wave in the microwave region (radar, about 1010 Hz in Section 2.3.1). Period, frequency and wavelength are three descriptions of the same wave: T = 1/ν = λ/c.
Conclusion: ν = 5.0 × 109 Hz, λ = 6.0 × 10−2 m, ν̄ = 16.67 m−1.
Ex 2.8 — What is the number of photons of light with a wavelength of 4000 pm that provide 1 J of energy?
Concept. Total energy = (number of photons) × (energy of one photon). The energy of one photon of wavelength λ is E = hc/λ. So the number of photons providing 1 J is N = 1 J / (hc/λ).
N = (total energy)/(hc/λ) = λ × (total energy)/(hc)
- λ = 4000 pm = 4000 × 10−12 m = 4.0 × 10−9 m.
- Energy of one photon: E = (6.626 × 10−34 J s)(3.0 × 108 m s−1)/(4.0 × 10−9 m) = 4.969 × 10−17 J.
- Number of photons: N = 1 J / (4.969 × 10−17 J) = 2.01 × 1016 photons.
| Step | Expression | Result |
|---|---|---|
| λ in metres | 4000 × 10−12 m | 4.0 × 10−9 m |
| Energy of 1 photon | hc/λ | 4.969 × 10−17 J |
| Photons in 1 J | 1 J/(4.969 × 10−17 J) | 2.01 × 1016 |
Extra depth. A 4000 pm (= 4 nm) photon is an X-ray/extreme-UV photon; the shorter the wavelength, the more energy each photon carries, hence the fewer photons are needed for 1 J. Compare Problem 2.7 (visible light of 400 nm needs 2 × 1018 photons for 1 J).
Conclusion: About 2.01 × 1016 photons of wavelength 4000 pm are needed to provide 1 J of energy.
Ex 2.9 — A photon of wavelength 4 × 10−7 m strikes on a metal surface, the work function of the metal being 2.13 eV. Calculate (i) the energy of the photon (eV), (ii) the kinetic energy of the emission, and (iii) the velocity of the photoelectron (1 eV = 1.6020 × 10−19 J).
Concept. In the photoelectric effect Einstein’s equation states: photon energy hν = work function W0 + kinetic energy of the ejected electron. So K.E. = hν − W0 = ½ mev2, valid only if hν > W0.
Ephoton = hc/λ K.E. = Ephoton − W0 v = √(2 K.E./me)
- (i) Photon energy: E = hc/λ = (6.626 × 10−34)(3.0 × 108)/(4 × 10−7) = 4.9695 × 10−19 J. In eV: 4.9695 × 10−19/1.6020 × 10−19 = 3.10 eV.
- (ii) Kinetic energy: K.E. = 3.102 − 2.13 = 0.972 eV = 0.972 × 1.6020 × 10−19 J = 1.557 × 10−19 J.
- (iii) Velocity: v = √(2 × 1.557 × 10−19 J / 9.109 × 10−31 kg) = √(3.419 × 1011) = 5.85 × 105 m s−1.
| Quantity | Value in eV | Value in J |
|---|---|---|
| Photon energy | 3.102 | 4.9695 × 10−19 |
| Work function W0 | 2.13 | 3.412 × 10−19 |
| Kinetic energy | 0.972 | 1.557 × 10−19 |
Extra depth. The electron speed of 5.85 × 105 m s−1 is only 0.2% of the speed of light, so the non-relativistic formula K.E. = ½ mev2 is justified. If the photon energy were smaller than 2.13 eV (i.e. λ > 583 nm), no electron would be emitted at all.
Conclusion: (i) 3.10 eV; (ii) K.E. = 0.972 eV = 1.557 × 10−19 J; (iii) v = 5.85 × 105 m s−1.
Ex 2.10 — Electromagnetic radiation of wavelength 242 nm is just sufficient to ionise the sodium atom. Calculate the ionisation energy of sodium in kJ mol−1.
Concept. “Just sufficient” means the photon energy equals the minimum energy needed to remove one electron — the ionisation energy per atom. Multiplying by Avogadro’s number gives the molar ionisation energy.
IE per atom = hc/λ IE per mole = NA × hc/λ
- λ = 242 nm = 2.42 × 10−7 m.
- Energy per atom: E = (6.626 × 10−34 J s)(3.0 × 108 m s−1)/(2.42 × 10−7 m) = 8.214 × 10−19 J.
- Per mole: 8.214 × 10−19 J × 6.022 × 1023 mol−1 = 4.946 × 105 J mol−1 = 494.6 kJ mol−1.
| Step | Calculation | Result |
|---|---|---|
| Photon energy | hc/λ | 8.214 × 10−19 J |
| Per mole | × 6.022 × 1023 | 4.946 × 105 J mol−1 |
| In kJ | ÷ 1000 | 494.6 kJ mol−1 |
Extra depth. The accepted first ionisation enthalpy of sodium is 496 kJ mol−1, so the calculation reproduces the experimental value — an example of how spectroscopic data give ionisation energies (Chapter 3 on periodic trends). The radiation (242 nm) is in the ultraviolet.
Conclusion: The ionisation energy of sodium is about 494.6 kJ mol−1 (≈ 495 kJ mol−1).
Ex 2.11 — A 25 watt bulb emits monochromatic yellow light of wavelength of 0.57 µm. Calculate the rate of emission of quanta per second.
Concept. Power is energy emitted per second (1 W = 1 J s−1). The number of quanta (photons) emitted per second is therefore the power divided by the energy of one photon, E = hc/λ (as in Problem 2.7 of the chapter).
Rate of emission = Power/(hc/λ)
- λ = 0.57 µm = 0.57 × 10−6 m = 5.7 × 10−7 m.
- Energy of one photon: E = (6.626 × 10−34)(3.0 × 108)/(5.7 × 10−7) = 3.487 × 10−19 J.
- Rate = 25 J s−1 / 3.487 × 10−19 J = 7.17 × 1019 quanta s−1.
| Quantity | Value |
|---|---|
| Power | 25 W = 25 J s−1 |
| Photon energy | 3.487 × 10−19 J |
| Photons per second | 7.17 × 1019 |
Extra depth. About 7 × 1019 photons leave the lamp each second — a huge number because each visible photon carries only 3.5 × 10−19 J. The calculation assumes that all the electrical power is converted to yellow light; a real bulb is far less efficient.
Conclusion: The bulb emits about 7.17 × 1019 quanta per second.
Ex 2.12 — Electrons are emitted with zero velocity from a metal surface when it is exposed to radiation of wavelength 6800 Å. Calculate threshold frequency (ν0) and work function (W0) of the metal.
Concept. Electrons are ejected with zero kinetic energy exactly when the photon energy equals the work function. Thus the given radiation is at the threshold: its frequency is ν0 and its energy is W0 = hν0.
ν0 = c/λ W0 = hν0
- λ = 6800 Å = 6800 × 10−10 m = 6.8 × 10−7 m.
- Threshold frequency: ν0 = (3.0 × 108 m s−1)/(6.8 × 10−7 m) = 4.41 × 1014 s−1.
- Work function: W0 = (6.626 × 10−34 J s)(4.41 × 1014 s−1) = 2.92 × 10−19 J (≈ 1.82 eV).
| Quantity | Value |
|---|---|
| Threshold wavelength | 6800 Å = 6.8 × 10−7 m |
| Threshold frequency ν0 | 4.41 × 1014 Hz |
| Work function W0 | 2.92 × 10−19 J = 1.82 eV |
Extra depth. A 6800 Å threshold lies in the red region, so the metal is photoelectrically sensitive even to red light — typical of the alkali metals with low work functions (compare K = 2.25 eV and Cs = 1.9 eV in Table 2.2 / Ex 2.51). Radiation of longer wavelength than 6800 Å cannot eject electrons at all.
Conclusion: Threshold frequency ν0 = 4.41 × 1014 Hz and work function W0 = 2.92 × 10−19 J.
Ex 2.13 — What is the wavelength of light emitted when the electron in a hydrogen atom undergoes transition from an energy level with n = 4 to an energy level with n = 2?
Concept. In Bohr’s model the energy of the nth level of hydrogen is En = −2.18 × 10−18/n2 J. When the electron falls from ni to nf a photon is emitted whose energy equals the energy difference, ΔE = hν = hc/λ.
ΔE = 2.18 × 10−18 J (1/nf2 − 1/ni2) λ = hc/ΔE
- ni = 4, nf = 2: ΔE = 2.18 × 10−18(1/4 − 1/16) = 2.18 × 10−18 × 3/16 = 4.0875 × 10−19 J (energy emitted).
- λ = hc/ΔE = (6.626 × 10−34 J s)(3.0 × 108 m s−1)/(4.0875 × 10−19 J) = 4.863 × 10−7 m = 486 nm.
- Check with the Rydberg formula: ν̄ = 1.09677 × 107 m−1(1/4 − 1/16) = 2.056 × 106 m−1, λ = 1/ν̄ = 486 nm.
| Quantity | Value |
|---|---|
| Transition | n = 4 → n = 2 (Balmer series) |
| ΔE (emitted) | 4.0875 × 10−19 J |
| λ | 486 nm (blue-green, visible) |
Extra depth. This is the second line (Hβ) of the Balmer series, the only series in the visible region. The first line (3 → 2) is red at 656 nm (Ex 2.17) and the third line (5 → 2) is at 434 nm (Problem 2.10).
Conclusion: The emitted light has wavelength λ = 4.86 × 10−7 m (486 nm), in the visible (Balmer) region.
Ex 2.14 — How much energy is required to ionise a H atom if the electron occupies n = 5 orbit? Compare your answer with the ionization enthalpy of H atom (energy required to remove the electron from n = 1 orbit).
Concept. Ionisation means taking the electron from level n to n = ∞ (where E = 0). The energy required is therefore |En| = 2.18 × 10−18/n2 J. For the ground state (n = 1) this is the ionisation enthalpy of hydrogen.
Energy required = E∞ − En = 0 − (−2.18 × 10−18/n2) = 2.18 × 10−18/n2 J
- From n = 5: ΔE = 2.18 × 10−18/25 = 8.72 × 10−20 J per atom (≈ 52.5 kJ mol−1).
- From n = 1: ΔE = 2.18 × 10−18 J per atom (≈ 1312 kJ mol−1).
- Comparison: (2.18 × 10−18)/(8.72 × 10−20) = 25. Ionising an atom whose electron is in n = 5 needs only 1/25 (one twenty-fifth, i.e. n2 times less) of the ground-state ionisation energy.
| Initial orbit | Energy to ionise (J atom−1) | Per mole (kJ mol−1) |
|---|---|---|
| n = 1 | 2.18 × 10−18 | ≈ 1312 |
| n = 5 | 8.72 × 10−20 | ≈ 52.5 |
Extra depth. An electron in a higher orbit is farther from the nucleus and less tightly bound, so it is easier to remove — the energy needed falls as 1/n2. This is why excited atoms are ionised more easily than ground-state atoms.
Conclusion: Ionising H from n = 5 needs 8.72 × 10−20 J, which is 1/25 of the ionisation enthalpy from n = 1 (2.18 × 10−18 J).
Ex 2.15 — What is the maximum number of emission lines when the excited electron of a H atom in n = 6 drops to the ground state?
Concept. An electron in n = 6 can return to n = 1 either directly or in steps through any intermediate level. Every different pair (ni > nf) is a different transition and gives a different spectral line. Counting all possible pairs from n levels gives n(n − 1)/2 lines.
Number of lines = n(n − 1)/2 = 6 × 5/2 = 15
| Series (final level) | Transitions | Lines |
|---|---|---|
| Lyman (nf = 1) | 6→1, 5→1, 4→1, 3→1, 2→1 | 5 |
| Balmer (nf = 2) | 6→2, 5→2, 4→2, 3→2 | 4 |
| Paschen (nf = 3) | 6→3, 5→3, 4→3 | 3 |
| Brackett (nf = 4) | 6→4, 5→4 | 2 |
| Pfund (nf = 5) | 6→5 | 1 |
| Total | 15 |
Counting shows 5 + 4 + 3 + 2 + 1 = 15 lines.
Extra depth. A single atom can show only one transition at a time, but a sample contains a huge number of atoms in all excited states, so all 15 lines appear together (the chapter notes that a collection of atoms contains all possible excited states). The lines belong to the Lyman (UV), Balmer (visible) and Paschen, Brackett, Pfund (infrared) series.
Conclusion: A maximum of 15 emission lines can be observed when the electron falls from n = 6 to the ground state.
Ex 2.16 — (i) The energy associated with the first orbit in the hydrogen atom is −2.18 × 10−18 J atom−1. What is the energy associated with the fifth orbit? (ii) Calculate the radius of Bohr’s fifth orbit for hydrogen atom.
Concept. In Bohr’s theory, for the hydrogen atom, En = E1/n2 (equation 2.13) and the radius of the nth orbit is rn = n2a0 where a0 = 52.9 pm is the radius of the first (Bohr) orbit.
- (i) Energy of the fifth orbit: E5 = −2.18 × 10−18 J/52 = −2.18 × 10−18/25 = −8.72 × 10−20 J atom−1.
- (ii) Radius of the fifth orbit: r5 = 52 × 52.9 pm = 25 × 52.9 pm = 1322.5 pm = 1.3225 nm (= 1.3225 × 10−9 m).
| n | En (J atom−1) | rn (pm) |
|---|---|---|
| 1 | −2.18 × 10−18 | 52.9 |
| 2 | −5.45 × 10−19 | 211.6 |
| 3 | −2.42 × 10−19 | 476.1 |
| 4 | −1.36 × 10−19 | 846.4 |
| 5 | −8.72 × 10−20 | 1322.5 |
Extra depth. As n increases the orbit becomes larger (r ∝ n2) and the energy less negative (E ∝ −1/n2), i.e. higher in energy and less tightly bound. The radius 1322.5 pm reappears in Ex 2.56.
Conclusion: E5 = −8.72 × 10−20 J atom−1 and r5 = 1322.5 pm (1.3225 nm).
Ex 2.17 — Calculate the wavenumber for the longest wavelength transition in the Balmer series of atomic hydrogen.
Concept. The Balmer series ends at nf = 2 and begins at n = 3, 4, 5 … (Table 2.3). The longest wavelength corresponds to the smallest energy difference, i.e. the transition 3 → 2. The wavenumber is given by Rydberg’s equation.
ν̄ = 109,677 cm−1 (1/n12 − 1/n22) with n1 = 2, n2 = 3
- ν̄ = 109,677 (1/22 − 1/32) = 109,677 (1/4 − 1/9) = 109,677 × 5/36.
- ν̄ = 1.523 × 104 cm−1 (= 1.523 × 106 m−1).
- The corresponding wavelength is λ = 1/ν̄ = 6.565 × 10−5 cm = 656.5 nm (red).
| Balmer transition | ν̄ (cm−1) | λ (nm) |
|---|---|---|
| 3 → 2 (longest λ) | 15,233 | 656.5 (red) |
| 4 → 2 | 20,564 | 486.3 |
| 5 → 2 | 23,032 | 434.1 |
Extra depth. The longest wavelength means the smallest wavenumber, so the answer is the first line of the series (Hα, red). The series limit (n = ∞ → 2) has ν̄ = 109,677/4 = 27,419 cm−1 (λ = 364.6 nm) and is the shortest wavelength of the series.
Conclusion: The wavenumber of the longest-wavelength Balmer line (3 → 2) is 1.523 × 104 cm−1 (1.523 × 106 m−1).
Ex 2.18 — What is the energy in joules, required to shift the electron of the hydrogen atom from the first Bohr orbit to the fifth Bohr orbit and what is the wavelength of the light emitted when the electron returns to the ground state? The ground state electron energy is −2.18 × 10−11 ergs.
Concept. The energy needed to raise the electron from n1 to n2 is ΔE = E2 − E1 with En = E1/n2. When the electron returns to the ground state the same energy is released as a photon of wavelength λ = hc/ΔE. Convert ergs to joules first: 1 erg = 10−7 J.
- E1 = −2.18 × 10−11 erg = −2.18 × 10−11 × 10−7 J = −2.18 × 10−18 J.
- E5 = −2.18 × 10−18/25 = −8.72 × 10−20 J.
- Energy required: ΔE = E5 − E1 = −8.72 × 10−20 + 2.18 × 10−18 = 2.093 × 10−18 J.
- Wavelength on returning (5 → 1): λ = hc/ΔE = (6.626 × 10−34)(3.0 × 108)/(2.093 × 10−18) = 9.50 × 10−8 m = 95 nm (ultraviolet, Lyman series).
| Step | Value |
|---|---|
| E1 | −2.18 × 10−18 J |
| E5 | −8.72 × 10−20 J |
| ΔE (1 → 5) | 2.093 × 10−18 J |
| λ (5 → 1) | 9.50 × 10−8 m = 95.0 nm |
Extra depth. The direct 5 → 1 return gives the 95 nm Lyman line. If the electron returns in steps (e.g. 5 → 2 and then 2 → 1) several lines of longer wavelength are emitted instead (see Ex 2.15); the textbook answer refers to the direct return to the ground state.
Conclusion: The electron needs 2.093 × 10−18 J to go from n = 1 to n = 5, and on falling back to n = 1 it emits light of wavelength about 9.5 × 10−8 m (95 nm).
Ex 2.19 — The electron energy in hydrogen atom is given by En = (−2.18 × 10−18)/n2 J. Calculate the energy required to remove an electron completely from the n = 2 orbit. What is the longest wavelength of light in cm that can be used to cause this transition?
Concept. Removing the electron completely from n = 2 means taking it to n = ∞ where E = 0. The minimum energy required is ΔE = 0 − E2. The photon that supplies exactly this energy has the longest wavelength that can still cause the transition (longer wavelengths carry less energy): λmax = hc/ΔE.
- E2 = −2.18 × 10−18/22 = −5.45 × 10−19 J.
- Energy required: ΔE = E∞ − E2 = 5.45 × 10−19 J per atom.
- Longest wavelength: λ = hc/ΔE = (6.626 × 10−34 J s)(3.0 × 108 m s−1)/(5.45 × 10−19 J) = 3.647 × 10−7 m = 3.647 × 10−5 cm (≈ 365 nm).
| Quantity | Value |
|---|---|
| E2 | −5.45 × 10−19 J |
| Energy to remove electron from n = 2 | 5.45 × 10−19 J |
| Longest wavelength | 3.65 × 10−5 cm (365 nm, near-UV) |
Extra depth. 365 nm is the Balmer series limit (n = ∞ → 2) found in Ex 2.17. Any light with λ ≤ 365 nm can ionise an H atom from n = 2; light of longer wavelength cannot, however intense it is — the same threshold idea as in the photoelectric effect.
Conclusion: Removing the electron from n = 2 needs 5.45 × 10−19 J; the longest wavelength that can do this is 3.647 × 10−5 cm.
Ex 2.20 — Calculate the wavelength of an electron moving with a velocity of 2.05 × 107 m s−1.
Concept. According to de Broglie, a moving particle of mass m and velocity v has an associated wave of wavelength λ = h/(mv) (equation 2.22). The mass of the electron is 9.109 × 10−31 kg.
λ = h/(me v)
- λ = 6.626 × 10−34 J s / (9.109 × 10−31 kg × 2.05 × 107 m s−1).
- Denominator = 9.109 × 10−31 × 2.05 × 107 = 1.867 × 10−23 kg m s−1.
- λ = 6.626 × 10−34/1.867 × 10−23 = 3.55 × 10−11 m (= 35.5 pm = 3.55 × 10−9 cm).
| Quantity | Value |
|---|---|
| Momentum p = mev | 1.867 × 10−23 kg m s−1 |
| Wavelength λ | 3.55 × 10−11 m |
Extra depth. The wavelength (35.5 pm) is comparable to atomic spacings (about 100–300 pm) and is why electron beams are diffracted by crystals and why the electron microscope can resolve very small features. A 0.1 kg ball moving at 10 m s−1 has λ = 6.6 × 10−34 m (Problem 2.12), far too small to detect.
Conclusion: The de Broglie wavelength of the electron is 3.55 × 10−11 m.
Ex 2.21 — The mass of an electron is 9.1 × 10−31 kg. If its K.E. is 3.0 × 10−25 J, calculate its wavelength.
Concept. The wavelength needs the velocity, which follows from the kinetic energy K.E. = ½ mv2. Then λ = h/mv. (Equivalent shortcut: λ = h/√(2m K.E.).)
v = √(2 K.E./m) λ = h/(mv)
- v = √(2 × 3.0 × 10−25 J / 9.1 × 10−31 kg) = √(6.59 × 105) = 812 m s−1.
- λ = 6.626 × 10−34/(9.1 × 10−31 × 812) = 6.626 × 10−34/7.39 × 10−28 = 8.97 × 10−7 m (= 896.7 nm).
| Step | Result |
|---|---|
| Velocity from K.E. | 812 m s−1 |
| Momentum m v | 7.39 × 10−28 kg m s−1 |
| de Broglie wavelength | 8.97 × 10−7 m ≈ 897 nm |
Extra depth. This slow electron has a wavelength (897 nm) longer than visible light — the slower the electron, the longer the wave. Fast electrons (Ex 2.20) have picometre wavelengths. This is exactly Problem 2.13 of the chapter.
Conclusion: The electron has a speed of 812 m s−1 and de Broglie wavelength 8.97 × 10−7 m (897 nm).
Ex 2.22 — Which of the following are isoelectronic species i.e., those having the same number of electrons? Na+, K+, Mg2+, Ca2+, S2−, Ar.
Concept. Isoelectronic species contain the same number of electrons. For a neutral atom electrons = Z; for a cation electrons = Z − charge; for an anion electrons = Z + charge.
| Species | Z | Charge | Electrons | Configuration |
|---|---|---|---|---|
| Na+ | 11 | +1 | 11 − 1 = 10 | 1s22s22p6 |
| Mg2+ | 12 | +2 | 12 − 2 = 10 | 1s22s22p6 |
| K+ | 19 | +1 | 19 − 1 = 18 | 1s22s22p63s23p6 |
| Ca2+ | 20 | +2 | 20 − 2 = 18 | 1s22s22p63s23p6 |
| S2− | 16 | −2 | 16 + 2 = 18 | 1s22s22p63s23p6 |
| Ar | 18 | 0 | 18 | 1s22s22p63s23p6 |
- Group 1 (10 electrons, like Ne): Na+ and Mg2+.
- Group 2 (18 electrons, like Ar): K+, Ca2+, S2− and Ar.
Extra depth. Isoelectronic species have the same electron configuration but different nuclear charges, so their sizes differ: among the 18-electron species the radius decreases as Z increases, S2− > Ar > K+ > Ca2+ (a theme of Chapter 3). The 10-electron pair is Na+ and Mg2+, isoelectronic with Ne, F− and O2−.
Conclusion: Na+ and Mg2+ are isoelectronic (10 electrons); K+, Ca2+, S2− and Ar are isoelectronic (18 electrons).
Ex 2.23 — (i) Write the electronic configurations of the following ions: (a) H− (b) Na+ (c) O2− (d) F−. (ii) What are the atomic numbers of elements whose outermost electrons are represented by (a) 3s1 (b) 2p3 and (c) 3p5? (iii) Which atoms are indicated by the following configurations? (a) [He] 2s1 (b) [Ne] 3s2 3p3 (c) [Ar] 4s2 3d1.
Concept. Write the configuration of the neutral atom with the aufbau order (1s, 2s, 2p, 3s, 3p, 4s, 3d …), Pauli exclusion principle and Hund’s rule, then add electrons for an anion or remove them (from the outermost shell) for a cation. For (ii) and (iii) count all the electrons in the configuration; for a neutral atom this number is the atomic number Z.
(i) Configurations of ions
| Ion | Electrons | Electronic configuration |
|---|---|---|
| (a) H− | 1 + 1 = 2 | 1s2 |
| (b) Na+ | 11 − 1 = 10 | 1s2 2s2 2p6 |
| (c) O2− | 8 + 2 = 10 | 1s2 2s2 2p6 |
| (d) F− | 9 + 1 = 10 | 1s2 2s2 2p6 |
(ii) Atomic numbers from the outermost electron. The outermost electron(s) together with the filled inner shells give the full configuration:
- 3s1: 1s22s22p63s1 → 11 electrons → Z = 11 (Na).
- 2p3: 1s22s22p3 → 7 electrons → Z = 7 (N).
- 3p5: 1s22s22p63s23p5 → 17 electrons → Z = 17 (Cl).
(iii) Atoms from the configuration (core [He] = 2, [Ne] = 10, [Ar] = 18 electrons):
- [He] 2s1: 2 + 1 = 3 electrons → Li.
- [Ne] 3s2 3p3: 10 + 2 + 3 = 15 electrons → P.
- [Ar] 4s2 3d1: 18 + 2 + 1 = 21 electrons → Sc (scandium).
Extra depth. Na+, O2− and F− are all isoelectronic with neon (1s22s22p6, a stable octet); H− has the helium configuration. In (ii) the answers assume a neutral atom with the outermost electrons shown. Note that in scandium the 4s orbital is written before 3d in [Ar]4s23d1 because 4s fills first, though 3d is written first in the conventional order [Ar]3d14s2.
Conclusion: (i) H−: 1s2; Na+, O2−, F−: 1s22s22p6. (ii) 3s1 → Z = 11; 2p3 → Z = 7; 3p5 → Z = 17. (iii) Li, P and Sc respectively.
Ex 2.24 — What is the lowest value of n that allows g orbitals to exist?
Concept. Azimuthal quantum number l takes values 0 to (n − 1); the subshell notation is l = 0 (s), 1 (p), 2 (d), 3 (f), 4 (g), 5 (h). A g subshell therefore needs l = 4, and since l ≤ n − 1, we need n − 1 ≥ 4.
- g orbitals: l = 4.
- Condition: l ≤ n − 1 ⇒ 4 ≤ n − 1 ⇒ n ≥ 5.
- Lowest n = 5 (the 5g subshell, with 2l + 1 = 9 orbitals).
| n | Possible l | Subshells present |
|---|---|---|
| 1 | 0 | s |
| 2 | 0, 1 | s, p |
| 3 | 0, 1, 2 | s, p, d |
| 4 | 0, 1, 2, 3 | s, p, d, f |
| 5 | 0, 1, 2, 3, 4 | s, p, d, f, g |
Extra depth. The 5g subshell holds up to 18 electrons (9 orbitals), but no known ground-state atom has electrons in g orbitals; they would appear only in very heavy elements (Z ≈ 121). For the same reason d orbitals first appear in n = 3 (Section 2.6.2) and f orbitals in n = 4.
Conclusion: g orbitals first occur in the fifth shell; the lowest value of n is 5.
Ex 2.25 — An electron is in one of the 3d orbitals. Give the possible values of n, l and ml for this electron.
Concept. The label “3d” carries two of the quantum numbers: the number 3 is the principal quantum number n, and the letter d means azimuthal quantum number l = 2 (s = 0, p = 1, d = 2, f = 3). The magnetic quantum number ml can take (2l + 1) values from −l to +l, one for each of the five d orbitals.
n = 3 l = 2 ml = −2, −1, 0, +1, +2
| Quantum number | Value for a 3d electron | Reason |
|---|---|---|
| n | 3 | number before the letter |
| l | 2 | d subshell |
| ml | −2, −1, 0, +1, +2 | 2l + 1 = 5 values |
So the electron may be in any one of the five orbitals (n, l, ml) = (3, 2, −2), (3, 2, −1), (3, 2, 0), (3, 2, +1) or (3, 2, +2); in addition its spin quantum number ms is +½ or −½.
Extra depth. The five 3d orbitals (dxy, dyz, dxz, dx²−y², dz²) are degenerate, and the particular ml value does not correspond one-to-one to an axis (Section 2.6.2). The shorthand “3d” is therefore the compact way of writing n = 3 and l = 2.
Conclusion: For a 3d electron n = 3, l = 2 and ml = −2, −1, 0, +1 or +2.
Ex 2.26 — An atom of an element contains 29 electrons and 35 neutrons. Deduce (i) the number of protons and (ii) the electronic configuration of the element.
Concept. The question refers to an atom, which is electrically neutral, so the number of protons equals the number of electrons (= atomic number Z). The mass number A = protons + neutrons identifies the isotope. The configuration follows from the aufbau principle.
- (i) Protons = electrons = 29 (neutral atom), so Z = 29 — the element is copper; mass number A = 29 + 35 = 64, i.e. 6429Cu.
- (ii) Electronic configuration: by the aufbau order 1s22s22p63s23p64s23d9 would be expected, but a completely filled 3d subshell is extra stable, so one electron moves from 4s to 3d: 1s2 2s2 2p6 3s2 3p6 3d10 4s1 = [Ar]3d104s1.
| Quantity | Value |
|---|---|
| Electrons | 29 |
| Protons | 29 |
| Neutrons | 35 |
| Mass number | 64 |
| Element | Copper (Cu), exceptional configuration |
| Configuration | [Ar] 3d10 4s1 |
Extra depth. Copper is one of the exceptional configurations marked * in Table 2.6, along with chromium (3d54s1). Section 2.6.6 explains that the extra stability comes from the symmetrical distribution and the larger exchange energy of a completely filled 3d10. Copper therefore has one unpaired electron (in 4s).
Conclusion: The element has 29 protons (copper, 64Cu) and the configuration 1s22s22p63s23p63d104s1.
Ex 2.27 — Give the number of electrons in the species H2+, H2 and O2+.
Concept. The number of electrons in a molecule or ion = (sum of the atomic numbers of all atoms) − (positive charge) or + (negative charge). Atomic numbers: H = 1, O = 8.
| Species | Sum of Z | Charge | Electrons |
|---|---|---|---|
| H2+ | 1 + 1 = 2 | +1 | 2 − 1 = 1 |
| H2 | 1 + 1 = 2 | 0 | 2 |
| O2+ | 8 + 8 = 16 | +1 | 16 − 1 = 15 |
- H2+ — 2 protons, 1 electron (the hydrogen molecule-ion).
- H2 — 2 protons, 2 electrons.
- O2+ — 16 protons, 16 − 1 = 15 electrons (an odd number of electrons: the species has an unpaired electron).
Extra depth. The positive charge means fewer electrons than protons, so subtract the charge. H2+ is the simplest molecular ion: one electron holds two protons together. With 15 electrons, O2+ is paramagnetic (Chapter 4 on chemical bonding).
Conclusion: H2+ has 1 electron, H2 has 2 electrons and O2+ has 15 electrons.
Ex 2.28 — (i) An atomic orbital has n = 3. What are the possible values of l and ml? (ii) List the quantum numbers (ml and l) of electrons for 3d orbital. (iii) Which of the following orbitals are possible? 1p, 2s, 2p and 3f.
Concept. The quantum numbers are related: n = 1, 2, 3 …; l = 0, 1, … (n − 1); ml = −l, …, 0, …, +l. An orbital “nl” exists only if l ≤ n − 1.
(i) n = 3: l = 0, 1, 2 and for each l the ml values are:
| l | Subshell | ml values | Orbitals |
|---|---|---|---|
| 0 | 3s | 0 | 1 |
| 1 | 3p | −1, 0, +1 | 3 |
| 2 | 3d | −2, −1, 0, +1, +2 | 5 |
Total orbitals = 1 + 3 + 5 = 9 = n2.
(ii) 3d orbitals: l = 2 and ml = −2, −1, 0, +1, +2 (five orbitals).
(iii) Which orbitals are possible?
| Orbital | n | l | Condition l ≤ n − 1 | Possible? |
|---|---|---|---|---|
| 1p | 1 | 1 | 1 ≤ 0 is false | Not possible (n = 1 has only l = 0, i.e. 1s) |
| 2s | 2 | 0 | 0 ≤ 1 | Possible |
| 2p | 2 | 1 | 1 ≤ 1 | Possible |
| 3f | 3 | 3 | 3 ≤ 2 is false | Not possible (n = 3 has only s, p, d) |
Extra depth. An f subshell first appears at n = 4 and a p subshell at n = 2. The same rule makes sets such as n = 1, l = 1 forbidden in Ex 2.30.
Conclusion: (i) l = 0, 1, 2 with ml = 0; −1, 0, +1; −2 to +2; (ii) for 3d: l = 2, ml = −2, −1, 0, +1, +2; (iii) 2s and 2p are possible; 1p and 3f are not.
Ex 2.29 — Using s, p, d notations, describe the orbital with the following quantum numbers. (a) n = 1, l = 0; (b) n = 3, l = 1; (c) n = 4, l = 2; (d) n = 4, l = 3.
Concept. An orbital is described by the principal quantum number n followed by the letter for l: l = 0 → s, 1 → p, 2 → d, 3 → f.
| Part | n | l | Letter | Orbital |
|---|---|---|---|---|
| (a) | 1 | 0 | s | 1s |
| (b) | 3 | 1 | p | 3p |
| (c) | 4 | 2 | d | 4d |
| (d) | 4 | 3 | f | 4f |
All four sets are allowed because l ≤ n − 1 in each case (0 ≤ 0, 1 ≤ 2, 2 ≤ 3, 3 ≤ 3).
Extra depth. The letters come from the descriptions of spectral lines — sharp, principal, diffuse and fundamental; after f the letters continue alphabetically (g, h …). The number of orbitals in these subshells is 1, 3, 5 and 7 and their shapes were described in Section 2.6.2.
Conclusion: (a) 1s; (b) 3p; (c) 4d; (d) 4f.
Ex 2.30 — Explain, giving reasons, which of the following sets of quantum numbers are not possible. (a) n = 0, l = 0, ml = 0, ms = +½ (b) n = 1, l = 0, ml = 0, ms = −½ (c) n = 1, l = 1, ml = 0, ms = +½ (d) n = 2, l = 1, ml = 0, ms = −½ (e) n = 3, l = 3, ml = −3, ms = +½ (f) n = 3, l = 1, ml = 0, ms = +½
Concept. A valid set must satisfy four rules: (1) n is a positive integer (n ≥ 1); (2) l = 0, 1, …, (n − 1); (3) ml runs from −l to +l; (4) ms = +½ or −½. Test each set against these rules in order.
| Set | n | l | ml | ms | Check | Verdict |
|---|---|---|---|---|---|---|
| (a) | 0 | 0 | 0 | +½ | n = 0 violates n ≥ 1 | Not possible |
| (b) | 1 | 0 | 0 | −½ | l = 0 ≤ n − 1 = 0; ml = 0 allowed | Possible (1s electron) |
| (c) | 1 | 1 | 0 | +½ | l = 1 > n − 1 = 0 | Not possible |
| (d) | 2 | 1 | 0 | −½ | l = 1 ≤ 1; ml = 0 allowed | Possible (2p electron) |
| (e) | 3 | 3 | −3 | +½ | l = 3 > n − 1 = 2 (so ml = −3 is invalid as well) | Not possible |
| (f) | 3 | 1 | 0 | +½ | l = 1 ≤ 2; ml = 0 allowed | Possible (3p electron) |
- (a) n cannot be zero — the principal quantum number starts at 1.
- (c) For n = 1 only l = 0 is allowed (l = 0 to n − 1); l = 1 is not.
- (e) For n = 3 the maximum l is 2; l = 3 (f) cannot occur in the third shell.
Extra depth. Sets (b), (d) and (f) correspond to the 1s, 2p and 3p orbitals. Each ms value is acceptable, because the spin can be +½ or −½.
Conclusion: Sets (a), (c) and (e) are not possible; (b), (d) and (f) are allowed.
Ex 2.31 — How many electrons in an atom may have the following quantum numbers? (a) n = 4, ms = −½ (b) n = 3, l = 0.
Concept. Each orbital (fixed n, l, ml) can hold at most two electrons, one with ms = +½ and one with ms = −½ (Pauli exclusion principle). The number of orbitals in the nth shell is n2 and in a subshell 2l + 1.
- (a) n = 4 and ms = −½: the fourth shell has n2 = 16 orbitals (one 4s, three 4p, five 4d, seven 4f). Each orbital can contain exactly one electron with ms = −½, so at most 16 electrons (when the shell is full: 2n2 = 32 electrons in total, half of them with ms = −½).
- (b) n = 3 and l = 0: this is the 3s subshell, which has only one orbital (ml = 0); it can hold 2 electrons (ms = +½ and −½).
| Part | Orbitals involved | Electrons per orbital | Maximum electrons |
|---|---|---|---|
| (a) n = 4, ms = −½ | 16 | 1 (only one spin) | 16 |
| (b) n = 3, l = 0 | 1 (3s) | 2 | 2 |
Extra depth. These are maximum numbers; they apply only if the orbitals are filled. In a real ground-state atom the number is smaller: potassium (Z = 19), for example, has only its single 4s electron in the fourth shell. (Part (b) of Ex 2.67 asks the same question for the 4th shell.)
Conclusion: (a) 16 electrons (at most); (b) 2 electrons.
Ex 2.32 — Show that the circumference of the Bohr orbit for the hydrogen atom is an integral multiple of the de Broglie wavelength associated with the electron revolving around the orbit.
Concept. Bohr’s fourth postulate says that the angular momentum of the electron in a stationary orbit is quantised, mevr = nh/2π (n = 1, 2, 3 …). De Broglie’s relation gives the wavelength of the electron as λ = h/(mev). Combining the two shows that an orbit fits a whole number of electron waves.
- Bohr’s quantum condition: mevr = n h/2π.
- Multiply both sides by 2π and divide by mev: 2πr = n h/(mev).
- De Broglie: h/(mev) = λ. Substituting, 2πr = nλ.
- The left side, 2πr, is the circumference of the orbit. Hence the circumference of the Bohr orbit = n × (de Broglie wavelength), an integral multiple (n = 1, 2, 3 …). ∎
2πr = nλ (n = 1, 2, 3 …)
| Orbit (n) | Circumference 2πr | Number of electron wavelengths on the orbit |
|---|---|---|
| 1 | 1 λ | 1 (standing wave) |
| 2 | 2 λ | 2 |
| 3 | 3 λ | 3 |
Extra depth. This shows that Bohr’s allowed orbits are exactly those on which the electron wave is a standing wave — the wave closes on itself in phase. If the circumference were not a whole number of wavelengths the wave would interfere destructively after each revolution and die out. This idea (standing electron waves) was a stepping stone to the Schrödinger equation; the circumference of the first orbit (2π × 52.9 pm = 332 pm) equals the electron’s wavelength there (Ex 2.59).
Conclusion: Using Bohr’s quantisation condition and de Broglie’s relation, 2πr = nλ: the orbit circumference is an integral multiple of the electron’s wavelength.
Ex 2.33 — What transition in the hydrogen spectrum would have the same wavelength as the Balmer transition n = 4 to n = 2 of He+ spectrum?
Concept. For a hydrogen-like species the transition energy is ΔE = 2.18 × 10−18 Z2(1/n12 − 1/n22) J (equation 2.14), and λ = hc/ΔE. The same wavelength therefore means the same energy difference.
- He+ (Z = 2), n = 4 → 2: ΔE = 2.18 × 10−18 × 4 × (1/4 − 1/16) = 2.18 × 10−18 × 4 × 3/16 = 1.635 × 10−18 J.
- Hydrogen (Z = 1): 2.18 × 10−18(1/n12 − 1/n22) = 1.635 × 10−18 ⇒ (1/n12 − 1/n22) = 0.75 = 3/4.
- The only integers giving 3/4 are n1 = 1 and n2 = 2 (1 − 1/4 = 3/4).
- Wavelength (both): λ = hc/ΔE = 1.988 × 10−25/1.635 × 10−18 = 1.216 × 10−7 m = 121.6 nm.
| Species | Transition | ΔE (J) | λ |
|---|---|---|---|
| He+ (Z = 2) | 4 → 2 (Balmer-type) | 1.635 × 10−18 | 121.6 nm |
| H (Z = 1) | 2 → 1 (Lyman, first line) | 1.635 × 10−18 | 121.6 nm |
Extra depth. A general result: because E ∝ Z2/n2, a transition (n1 → n2) in He+ has the same energy as the transition (n1/2 → n2/2) in H when n1 and n2 are even. Here 4 → 2 in He+ equals 2 → 1 in H — the first line of the Lyman (UV) series.
Conclusion: The n = 2 → n = 1 transition of hydrogen (Lyman series) has the same wavelength (121.6 nm) as the n = 4 → 2 transition of He+.
Ex 2.34 — Calculate the energy required for the process He+(g) → He2+(g) + e−. The ionization energy for the H atom in the ground state is 2.18 × 10−18 J atom−1.
Concept. He+ is a hydrogen-like (one-electron) ion, so Bohr’s theory applies with nuclear charge Z = 2: En = −2.18 × 10−18 Z2/n2 J. The energy needed to remove the electron from the ground state (n = 1) to infinity is the negative of E1.
- For He+: E1 = −2.18 × 10−18 × (2)2/(1)2 = −8.72 × 10−18 J.
- Ionisation energy = E∞ − E1 = 0 − (−8.72 × 10−18) = 8.72 × 10−18 J per ion.
| Species | Z | Ionisation energy (J) | Ratio to H |
|---|---|---|---|
| H | 1 | 2.18 × 10−18 | 1 |
| He+ | 2 | 8.72 × 10−18 | 4 (= Z2) |
| Li2+ | 3 | 1.962 × 10−17 | 9 |
Extra depth. Doubling the nuclear charge makes the 1s electron four times more tightly bound (Z2). Per mole this is 8.72 × 10−18 × 6.022 × 1023 = 5251 kJ mol−1, which matches the experimental second ionisation enthalpy of helium (5250 kJ mol−1).
Conclusion: The energy required for He+ → He2+ + e− is 8.72 × 10−18 J per ion.
Ex 2.35 — If the diameter of a carbon atom is 0.15 nm, calculate the number of carbon atoms which can be placed side by side in a straight line across length of scale of length 20 cm long.
Concept. When atoms are placed side by side in a line, each occupies a length equal to its diameter. The number of atoms = (length of the line)/(diameter of one atom). Convert both lengths to the same unit (metres).
- Diameter of carbon atom = 0.15 nm = 0.15 × 10−9 m = 1.5 × 10−10 m.
- Length of scale = 20 cm = 20 × 10−2 m = 0.20 m.
- Number of atoms = 0.20 m / 1.5 × 10−10 m = 1.33 × 109.
| Quantity | Value |
|---|---|
| Atom diameter | 1.5 × 10−10 m |
| Scale length | 0.20 m |
| Number of atoms | 1.33 × 109 |
Extra depth. More than a billion carbon atoms would fit along a 20 cm scale — an illustration of how small atoms are (their diameter is about 10−10 m, Section 2.2.2). Cross-check: 1.33 × 109 × 0.15 nm = 2.0 × 108 nm = 20 cm.
Conclusion: About 1.33 × 109 carbon atoms can be placed side by side along the 20 cm scale.
Ex 2.36 — 2 × 108 atoms of carbon are arranged side by side. Calculate the radius of carbon atom if the length of this arrangement is 2.4 cm.
Concept. For atoms in a row, the total length = (number of atoms) × (diameter of one atom). The radius is half the diameter.
- Length = 2.4 cm = 2.4 × 10−2 m; number of atoms = 2 × 108.
- Diameter = (2.4 × 10−2 m)/(2 × 108) = 1.2 × 10−10 m.
- Radius = diameter/2 = 6.0 × 10−11 m = 60 pm (0.060 nm = 0.6 Å).
| Quantity | Value |
|---|---|
| Total length | 2.4 cm = 2.4 × 10−2 m |
| Diameter | 1.2 × 10−10 m |
| Radius | 6.0 × 10−11 m = 60 pm |
Extra depth. Note the difference from Ex 2.35: there the diameter was given and the number of atoms was asked; here the number is given and the radius is asked. The value 60 pm is smaller than the covalent radius of carbon (77 pm), because the numbers in the exercise are idealised.
Conclusion: The radius of the carbon atom is 6.0 × 10−11 m (60 pm).
Ex 2.37 — The diameter of zinc atom is 2.6 Å. Calculate (a) radius of zinc atom in pm and (b) number of atoms present in a length of 1.6 cm if the zinc atoms are arranged side by side lengthwise.
Concept. Radius = diameter/2; 1 Å = 10−10 m = 100 pm. The number of atoms in a line = length/diameter.
- (a) Radius: diameter = 2.6 Å = 260 pm, so radius = 260/2 = 130 pm (1.3 Å).
- (b) Number of atoms: length = 1.6 cm = 1.6 × 10−2 m; diameter = 2.6 × 10−10 m. Number = 1.6 × 10−2/2.6 × 10−10 = 6.15 × 107.
| Quantity | Value |
|---|---|
| Diameter | 2.6 Å = 260 pm = 2.6 × 10−10 m |
| Radius | 130 pm |
| Atoms in 1.6 cm | 6.15 × 107 |
Extra depth. The radius of 130 pm agrees with the order of magnitude of metallic radii (Zn: about 134 pm). The same unit conversions (Å, pm, nm, cm) appear throughout this chapter: 1 Å = 0.1 nm = 100 pm.
Conclusion: (a) Radius of zinc atom = 130 pm; (b) about 6.15 × 107 zinc atoms fit in 1.6 cm.
Ex 2.38 — A certain particle carries 2.5 × 10−16 C of static electric charge. Calculate the number of electrons present in it.
Concept. Charge is quantised: the total charge q = n e where e = 1.602 × 10−19 C is the charge of one electron (Millikan). So the number of electrons n = q/e.
- n = (2.5 × 10−16 C)/(1.602 × 10−19 C per electron).
- n = 1.56 × 103 ≈ 1561 electrons (about 1.56 × 103).
| Quantity | Value |
|---|---|
| Total charge q | 2.5 × 10−16 C |
| Charge of one electron | 1.602 × 10−19 C |
| Number of electrons | 1.56 × 103 |
Extra depth. With e = 1.6 × 10−19 C the answer is 1562.5, so the result is correctly quoted as about 1.56 × 103. A real particle carries a whole number of electrons; the slight non-integer value arises because the given charge is rounded to two significant figures.
Conclusion: The particle contains about 1.56 × 103 (≈ 1561) electrons.
Ex 2.39 — In Millikan’s experiment, static electric charge on the oil drops has been obtained by shining X-rays. If the static electric charge on the oil drop is −1.282 × 10−18 C, calculate the number of electrons present on it.
Concept. Millikan found that the charge on an oil drop is always an integral multiple of the electronic charge: q = n e, n = 1, 2, 3 …, with e = 1.602 × 10−19 C. The X-rays ionise the air; the drop acquires electrons by collision with gaseous ions.
n = q/e = 1.282 × 10−18 C / 1.602 × 10−19 C
- n = 12.82 × 10−19/1.602 × 10−19 = 8.002.
- Since n must be an integer, n = 8 electrons.
| Quantity | Value |
|---|---|
| Charge on the drop | −1.282 × 10−18 C |
| Charge of one electron | −1.602 × 10−19 C |
| Number of excess electrons | 8 |
Extra depth. The fact that the ratio comes out so close to a whole number (8.00) is the experimental evidence for the quantisation of charge; had charge been continuous, every drop would give an arbitrary ratio. Millikan used the charges on many drops and found each was a multiple of the same smallest charge, which he took as e (Section 2.1.3).
Conclusion: The oil drop carries 8 excess electrons (q = 8e).
Ex 2.40 — In Rutherford’s experiment, generally the thin foil of heavy atoms, like gold, platinum etc. have been used to be bombarded by the α-particles. If the thin foil of light atoms like aluminium etc. is used, what difference would be observed from the above results?
Concept. The deflection of an α-particle (charge +2e, mass 4 u) arises from the electrostatic repulsion between it and the positive nucleus, and that force is proportional to the product of the charges, 2e × Ze. A heavier nucleus also stays in place when struck, whereas a light nucleus is pushed aside (recoils).
| Foil | Nuclear charge Z | Repulsion on α (∝ 2Z) | Mass of nucleus (relative to α) | Expected scattering |
|---|---|---|---|---|
| Gold | 79 | 158 (large) | 197 u (about 50 times the α-particle) | Many small deflections; a very few rebound by ~180° |
| Aluminium | 13 | 26 (about 6 times smaller) | 27 u (about 7 times the α-particle) | Mostly undeflected or very small deflections; practically no large-angle scattering |
- Much less deflection: the nuclear charge of Al (+13) is much smaller than that of Au (+79), so the repulsive force on the α-particle is about six times weaker; most α-particles pass almost straight through.
- Few or no large-angle deflections: the very rare rebounds at ~180° would essentially disappear, because the α-particle cannot be turned back by such a weakly charged, light nucleus (the nucleus is also pushed aside).
- Consequence for the model: with an aluminium foil the experiment would not so clearly reveal that the positive charge and mass are concentrated in a tiny, massive nucleus — which is why Rutherford, Geiger and Marsden chose a heavy metal such as gold, which can also be beaten into a very thin foil.
Extra depth. In Rutherford scattering the number of particles scattered through a given angle is proportional to Z2, so the scattering from Al is smaller than from Au by a factor of (13/79)2 ≈ 1/37 per nucleus. The qualitative result — “mostly undeflected” — is what the question expects.
Conclusion: With an aluminium (light-atom) foil the α-particles would be deflected much less — most would pass straight through and large-angle (back) scattering would be practically absent.
Ex 2.41 — Symbols 7935Br and 79Br can be written, whereas symbols 3579Br and 35Br are not acceptable. Answer briefly.
Concept. In the notation AZX the superscript is the mass number A (protons + neutrons) and the subscript is the atomic number Z (number of protons). The atomic number of an element is fixed — it is what defines the element — and always A ≥ Z. For bromine Z = 35.
| Symbol | Meaning | Acceptable? | Reason |
|---|---|---|---|
| 7935Br | A = 79, Z = 35 | Yes | Br has Z = 35; 79 is the mass number (45 neutrons), a real isotope of bromine |
| 79Br | A = 79 (Z implied by the symbol Br) | Yes | The symbol Br already tells that Z = 35, so the subscript may be omitted |
| 3579Br | A = 35, Z = 79 | No | Z = 79 is gold, not bromine, and A = 35 < Z = 79 is impossible (neutrons would be negative) |
| 35Br | A = 35 (Z = 35 implied) | No | A = Z = 35 would mean no neutrons; bromine does not occur with mass number 35 (its isotopes are 79Br and 81Br) |
- The atomic number of bromine is 35 (35 protons). Mass number = 35 + neutrons; the known isotopes have 44 and 46 neutrons, i.e. A = 79 and 81.
- The atomic number (subscript) is optional because the symbol of the element fixes it, but the mass number must be correct for an isotope of that element.
- 3579Br interchanges A and Z; 35Br gives a mass number that does not exist for bromine.
Extra depth. The position matters: A is written at the top left, Z at the bottom left. A symbol such as 35Cl (chlorine-35) is perfectly acceptable because 35 is the mass number of chlorine (Z = 17); the same number 35 appears as the atomic number of bromine.
Conclusion: 7935Br and 79Br are correct because Z = 35 for Br and A = 79; 3579Br and 35Br are wrong because the atomic number and mass number are interchanged / A = 35 is not a mass number of bromine.
Ex 2.42 — An element with mass number 81 contains 31.7% more neutrons as compared to protons. Assign the atomic symbol.
Concept. Mass number A = protons (Z) + neutrons (n). If the neutrons are 31.7% more than the protons, then n = Z + 0.317 Z = 1.317 Z.
A = Z + n = Z + 1.317 Z = 2.317 Z
- 2.317 Z = 81 ⇒ Z = 81/2.317 = 34.96 ≈ 35.
- Neutrons n = 81 − 35 = 46.
- Check: 46/35 = 1.314, i.e. about 31.4–31.7% more neutrons than protons (rounding of the data).
- Atomic number 35 is bromine. Symbol: 8135Br.
| Quantity | Value |
|---|---|
| Mass number A | 81 |
| Protons Z | 35 |
| Neutrons | 46 |
| Element | Bromine (Br) |
| Symbol | 8135Br |
Extra depth. 81Br is one of the two stable isotopes of bromine (the other is 79Br); the pair occurs in nearly equal abundance (about 50.7% and 49.3%), giving bromine its average atomic mass of 79.9 u.
Conclusion: The element is bromine and the atomic symbol is 8135Br.
Ex 2.43 — An ion with mass number 37 possesses one unit of negative charge. If the ion contains 11.1% more neutrons than the electrons, find the symbol of the ion.
Concept. For an ion carrying a charge, the number of electrons differs from the number of protons: for an anion with one negative charge, electrons = protons + 1. Let the number of electrons be e; then neutrons n = 1.111 e and protons Z = e − 1.
- Mass number A = Z + n = (e − 1) + 1.111 e = 2.111 e − 1 = 37.
- 2.111 e = 38 ⇒ e = 38/2.111 = 18.0.
- Electrons = 18; protons Z = 18 − 1 = 17; neutrons = 37 − 17 = 20 (check: 20/18 = 1.111, i.e. 11.1% more).
- Z = 17 is chlorine. The species has one extra electron, so it is the chloride ion: 3717Cl−.
| Quantity | Value |
|---|---|
| Mass number | 37 |
| Protons | 17 |
| Neutrons | 20 |
| Electrons | 18 |
| Charge | −1 |
| Symbol | 3717Cl− |
Extra depth. The chloride ion has 18 electrons, the argon configuration 1s22s22p63s23p6 (it is isoelectronic with Ar, K+ and Ca2+ in Ex 2.22). 37Cl is the heavier stable isotope of chlorine (about 24% natural abundance).
Conclusion: The ion is the chloride ion, 3717Cl−.
Ex 2.44 — An ion with mass number 56 contains 3 units of positive charge and 30.4% more neutrons than electrons. Assign the symbol to this ion.
Concept. For a cation with charge +3, the electrons are three fewer than the protons: protons Z = electrons + 3. Let electrons = e; then neutrons n = 1.304 e and Z = e + 3.
- A = Z + n = (e + 3) + 1.304 e = 2.304 e + 3 = 56.
- 2.304 e = 53 ⇒ e = 53/2.304 = 23.0.
- Electrons = 23; protons Z = 23 + 3 = 26; neutrons = 56 − 26 = 30 (check: 30/23 = 1.304).
- Z = 26 is iron, so the ion is 5626Fe3+.
| Quantity | Value |
|---|---|
| Mass number | 56 |
| Protons | 26 |
| Neutrons | 30 |
| Electrons | 23 |
| Charge | +3 |
| Symbol | 5626Fe3+ |
Extra depth. Fe3+ has the configuration [Ar]3d5 — a half-filled d subshell, which is why iron(III) is a particularly stable oxidation state (Section 2.6.6). 56Fe is the most abundant isotope of iron (91.7%).
Conclusion: The ion is 5626Fe3+ (iron(III) ion).
Ex 2.45 — Arrange the following type of radiations in increasing order of frequency: (a) radiation from microwave oven (b) amber light from traffic signal (c) radiation from FM radio (d) cosmic rays from outer space and (e) X-rays.
Concept. In the electromagnetic spectrum (Fig. 2.7) the order of increasing frequency (decreasing wavelength) is: radio waves < microwaves < infrared < visible light < ultraviolet < X-rays < γ-rays/cosmic rays. Place each radiation in its region.
| Radiation | Region | Typical frequency |
|---|---|---|
| (c) FM radio | Radio waves | ~108 Hz (88–108 MHz) |
| (a) Microwave oven | Microwaves | ~109–1010 Hz (2.45 GHz) |
| (b) Amber light of traffic signal | Visible light | ~5 × 1014 Hz (λ ≈ 590 nm) |
| (e) X-rays | X-rays | ~1017–1019 Hz (λ ≈ 0.1 nm) |
| (d) Cosmic rays | γ-rays / cosmic | > 1020 Hz |
(c) FM radio < (a) microwave oven < (b) amber light < (e) X-rays < (d) cosmic rays
Extra depth. Frequency and energy go together (E = hν), so cosmic rays are the most energetic and FM radio waves the least; wavelength decreases in the same order. Microwave ovens operate near 2.45 GHz, FM radio at about 100 MHz, amber light at about 5 × 1014 Hz, X-rays at about 3 × 1018 Hz (λ ≈ 0.1 nm, Section 2.2).
Conclusion: Increasing order of frequency: (c) FM radio < (a) microwave oven < (b) amber light < (e) X-rays < (d) cosmic rays.
Ex 2.46 — Nitrogen laser produces a radiation at a wavelength of 337.1 nm. If the number of photons emitted is 5.6 × 1024, calculate the power of this laser.
Concept. The energy of one photon is E = hc/λ; the total energy of N photons is N hc/λ. Power is energy per unit time (1 W = 1 J s−1). The question does not state the time; as in the standard solution we take the photons to be emitted in one second, so that the numerical value of the energy emitted equals the power (W).
- λ = 337.1 nm = 3.371 × 10−7 m.
- Energy of one photon: E = (6.626 × 10−34)(3.0 × 108)/(3.371 × 10−7) = 5.897 × 10−19 J.
- Total energy of 5.6 × 1024 photons: 5.6 × 1024 × 5.897 × 10−19 = 3.30 × 106 J.
- If this is emitted per second: power = 3.30 × 106 J s−1 = 3.30 × 106 W (≈ 3.3 MW).
| Quantity | Value |
|---|---|
| Energy of one photon | 5.897 × 10−19 J |
| Number of photons | 5.6 × 1024 |
| Total energy | 3.30 × 106 J |
| Power (assuming 1 s) | 3.30 × 106 W |
Extra depth. Data note: the exercise gives no emission time, so the power of 3.3 × 106 W is valid when the photons are emitted in 1 s; for a time t seconds the power would be 3.30 × 106/t W. Such megawatt powers are reached by pulsed lasers during very short pulses. 337.1 nm is an ultraviolet line.
Conclusion: Total energy = 3.30 × 106 J, i.e. a power of about 3.3 × 106 W if the photons are emitted in one second.
Ex 2.47 — Neon gas is generally used in the sign boards. If it emits strongly at 616 nm, calculate (a) the frequency of emission, (b) distance traveled by this radiation in 30 s (c) energy of quantum and (d) number of quanta present if it produces 2 J of energy.
Concept. Use c = νλ for the frequency, distance = speed × time for (b), E = hν for the quantum energy, and N = (total energy)/(energy of one quantum) for (d).
- (a) Frequency: ν = c/λ = 3.0 × 108/(616 × 10−9) = 4.87 × 1014 s−1.
- (b) Distance in 30 s: d = c t = 3.0 × 108 m s−1 × 30 s = 9.0 × 109 m.
- (c) Energy of a quantum: E = hν = 6.626 × 10−34 × 4.87 × 1014 = 3.23 × 10−19 J.
- (d) Number of quanta in 2 J: N = 2 J/3.227 × 10−19 J = 6.2 × 1018.
| Part | Quantity | Value |
|---|---|---|
| (a) | Frequency | 4.87 × 1014 Hz |
| (b) | Distance in 30 s | 9.0 × 109 m |
| (c) | Energy of a quantum | 3.23 × 10−19 J |
| (d) | Quanta in 2 J | 6.2 × 1018 |
Extra depth. 616 nm is orange-red, the colour of neon signs. All electromagnetic radiation travels at c in vacuum, so the distance in (b) depends only on time and not on the wavelength. The result N = 6.2 × 1018 shows how many photons carry just 2 J of light.
Conclusion: (a) 4.87 × 1014 Hz; (b) 9.0 × 109 m; (c) 3.23 × 10−19 J; (d) 6.2 × 1018 quanta.
Ex 2.48 — In astronomical observations, signals observed from the distant stars are generally weak. If the photon detector receives a total of 3.15 × 10−18 J from the radiations of 600 nm, calculate the number of photons received by the detector.
Concept. Number of photons = (total energy received)/(energy of one photon), with E = hc/λ.
- λ = 600 nm = 6.0 × 10−7 m.
- Energy of one photon: E = (6.626 × 10−34)(3.0 × 108)/(6.0 × 10−7) = 3.313 × 10−19 J.
- N = 3.15 × 10−18 J/3.313 × 10−19 J = 9.5 ≈ 10 photons.
| Quantity | Value |
|---|---|
| Energy of one 600 nm photon | 3.313 × 10−19 J |
| Total energy detected | 3.15 × 10−18 J |
| Number of photons | ≈ 9.5 → about 10 |
Extra depth. Only about ten photons give a measurable signal — modern detectors can respond to individual photons. The calculation gives 9.5 rather than a whole number because the data are rounded (3.15 × 10−18 J corresponds to between 9 and 10 photons); since photons cannot be split, the answer is quoted as about 10 photons.
Conclusion: The detector receives about 10 photons (calculated value 9.5).
Ex 2.49 — Lifetimes of the molecules in the excited states are often measured by using pulsed radiation source of duration nearly in the nano second range. If the radiation source has the duration of 2 ns and the number of photons emitted during the pulse source is 2.5 × 1015, calculate the energy of the source.
Concept. The energy of the source = (number of photons) × (energy of one photon) = N hν. The question gives no wavelength or frequency, so the standard NCERT solution takes the frequency of the radiation to be the reciprocal of the pulse duration: ν = 1/t.
- t = 2 ns = 2 × 10−9 s; ν = 1/t = 1/(2 × 10−9 s) = 5 × 108 s−1.
- Energy = N hν = (2.5 × 1015)(6.626 × 10−34 J s)(5 × 108 s−1).
- Energy = 8.28 × 10−10 J.
| Quantity | Value |
|---|---|
| Pulse duration t | 2 ns |
| Frequency taken as 1/t | 5 × 108 Hz |
| Photons N | 2.5 × 1015 |
| Energy N hν | 8.28 × 10−10 J |
Extra depth. Data note: a frequency of 5 × 108 Hz is a radio-frequency value, so this exercise is best read as a dimensional-analysis exercise rather than a realistic optical pulse; the exercise as printed does not provide the wavelength, and the answer 8.28 × 10−10 J follows the textbook’s convention.
Conclusion: Taking ν = 1/(2 ns) = 5 × 108 Hz, the energy of the source is N hν = 8.28 × 10−10 J.
Ex 2.50 — The longest wavelength doublet absorption transition is observed at 589 and 589.6 nm. Calculate the frequency of each transition and energy difference between two excited states.
Concept. Each wavelength gives a frequency ν = c/λ. The two closely spaced lines (a doublet) correspond to two slightly different excited-state energies; the energy difference is ΔE = h(ν1 − ν2). These are the sodium D1 and D2 lines, caused by the spin of the electron (Section 2.6.1).
- ν1 = c/λ1 = 3.0 × 108/(589 × 10−9) = 5.093 × 1014 Hz.
- ν2 = 3.0 × 108/(589.6 × 10−9) = 5.088 × 1014 Hz.
- Δν = ν1 − ν2 = 5.18 × 1011 Hz.
- ΔE = h Δν = 6.626 × 10−34 × 5.18 × 1011 = 3.43 × 10−22 J.
| Line | λ (nm) | ν (Hz) |
|---|---|---|
| D2 (shorter λ) | 589.0 | 5.093 × 1014 |
| D1 (longer λ) | 589.6 | 5.088 × 1014 |
| Difference | 0.6 | 5.18 × 1011 (ΔE = 3.43 × 10−22 J) |
Extra depth. The small energy difference of 3.43 × 10−22 J (about 2 meV) is the fine-structure splitting of the 3p level of sodium — two energy levels so close that the lines look like one yellow line to the eye. Bohr’s model could not explain such doublets (Section 2.4.2); the electron-spin quantum number ms does.
Conclusion: ν1 = 5.093 × 1014 Hz, ν2 = 5.088 × 1014 Hz; the energy difference is ≈ 3.43 × 10−22 J.
Ex 2.51 — The work function for caesium atom is 1.9 eV. Calculate (a) the threshold wavelength and (b) the threshold frequency of the radiation. If the caesium element is irradiated with a wavelength 500 nm, calculate the kinetic energy and the velocity of the ejected photoelectron.
Concept. The work function W0 = hν0 = hc/λ0. For radiation of wavelength 500 nm the kinetic energy of the photoelectron is K.E. = hc/λ − W0 and v = √(2 K.E./me). Use 1 eV = 1.602 × 10−19 J.
- W0 = 1.9 eV = 1.9 × 1.602 × 10−19 = 3.044 × 10−19 J.
- (b) Threshold frequency: ν0 = W0/h = 3.044 × 10−19/6.626 × 10−34 = 4.59 × 1014 Hz.
- (a) Threshold wavelength: λ0 = c/ν0 = 3.0 × 108/4.594 × 1014 = 6.53 × 10−7 m = 653 nm.
- Photon of 500 nm: E = hc/λ = 1.988 × 10−25/5.0 × 10−7 = 3.976 × 10−19 J (2.48 eV > 1.9 eV, so emission occurs).
- Kinetic energy: K.E. = 3.976 × 10−19 − 3.044 × 10−19 = 9.3 × 10−20 J (0.58 eV).
- Velocity: v = √(2 × 9.32 × 10−20/9.109 × 10−31) = 4.52 × 105 m s−1.
| Quantity | Value |
|---|---|
| Work function W0 | 1.9 eV = 3.044 × 10−19 J |
| Threshold frequency ν0 | 4.59 × 1014 Hz |
| Threshold wavelength λ0 | 653 nm (red) |
| Energy of 500 nm photon | 3.976 × 10−19 J (2.48 eV) |
| K.E. of photoelectron | 9.3 × 10−20 J |
| Speed of photoelectron | 4.52 × 105 m s−1 |
Extra depth. Caesium has the lowest work function among the common metals (Table 2.2 lists K = 2.25 eV and Na = 2.3 eV), so it responds even to red light — hence its use in photocells. Radiation with λ > 653 nm cannot eject electrons however intense it is.
Conclusion: λ0 = 653 nm, ν0 = 4.59 × 1014 Hz; for 500 nm light K.E. = 9.3 × 10−20 J and v = 4.52 × 105 m s−1.
Ex 2.52 — Following results are observed when sodium metal is irradiated with different wavelengths. Calculate (a) threshold wavelength and, (b) Planck’s constant. λ (nm): 500, 450, 400; v × 10−5 (cm s−1): 2.55, 4.35, 5.35.
Concept. Einstein’s equation: hc/λ = W0 + ½ mev2, i.e. ½ mev2 = hc(1/λ) − W0. A graph (or any two points) of K.E. against 1/λ is a straight line with slope hc and intercept −W0. The threshold wavelength is where K.E. = 0, λ0 = hc/W0.
Data note on units. The velocities are printed as “v × 10−5 (cm s−1)”. Read literally (2.55 × 105 cm s−1 = 2.55 × 103 m s−1) the kinetic energies are 104 times smaller and give an impossible Planck constant (≈ 10−38 J s). The data give the correct h and a sensible work function only if v is taken as 2.55 × 105, 4.35 × 105, 5.35 × 105 m s−1, which is how it is solved below.
- K.E. = ½ mev2 with me = 9.109 × 10−31 kg: 500 nm → 2.96 × 10−20 J; 450 nm → 8.62 × 10−20 J; 400 nm → 1.304 × 10−19 J.
- 1/λ: 2.000 × 106, 2.222 × 106, 2.500 × 106 m−1.
- Slope of K.E. against 1/λ (least-squares line through the three points) = hc = 1.998 × 10−25 J m ⇒ h = slope/c = 6.66 × 10−34 J s (the accepted value is 6.626 × 10−34 J s).
- Intercept = −W0 = −3.66 × 10−19 J, i.e. W0 = 3.66 × 10−19 J (2.28 eV).
- Threshold wavelength: λ0 = hc/W0 = 1.998 × 10−25/3.66 × 10−19 = 5.46 × 10−7 m = 546 nm.
| λ (nm) | 1/λ (106 m−1) | v (105 m s−1) | K.E. (10−20 J) |
|---|---|---|---|
| 500 | 2.000 | 2.55 | 2.96 |
| 450 | 2.222 | 4.35 | 8.62 |
| 400 | 2.500 | 5.35 | 13.04 |
Extra depth. Two-point check with the 500 nm and 400 nm data: slope = (13.04 − 2.96) × 10−20/(0.500 × 106) = 2.02 × 10−25 J m ⇒ h = 6.7 × 10−34 J s. The result agrees with the accepted h and gives a work function of 2.3 eV, matching Table 2.2 (Na: 2.3 eV) — this confirms the intended unit of v.
Conclusion: Threshold wavelength ≈ 546 nm and Planck’s constant ≈ 6.6 × 10−34 J s (work function ≈ 2.28 eV).
Ex 2.53 — The ejection of the photoelectron from the silver metal in the photoelectric effect experiment can be stopped by applying the voltage of 0.35 V when the radiation 256.7 nm is used. Calculate the work function for silver metal.
Concept. A retarding (stopping) voltage V0 just stops the most energetic photoelectron, so the maximum kinetic energy of the photoelectrons is K.E. = eV0. Einstein’s equation then gives the work function: W0 = hc/λ − eV0.
- Photon energy: E = hc/λ = (6.626 × 10−34)(3.0 × 108)/(256.7 × 10−9) = 7.744 × 10−19 J = 4.83 eV.
- Maximum K.E. = eV0 = 1 e × 0.35 V = 0.35 eV = 5.6 × 10−20 J.
- Work function: W0 = 4.83 − 0.35 = 4.48 eV = 7.18 × 10−19 J.
| Quantity | In eV | In J |
|---|---|---|
| Photon energy | 4.83 | 7.744 × 10−19 |
| Stopping energy eV0 | 0.35 | 5.6 × 10−20 |
| Work function W0 | 4.48 | 7.18 × 10−19 |
Extra depth. The value 4.48 eV agrees with the work function of silver in Table 2.2 (4.3 eV) to within experimental scatter; silver needs ultraviolet light (256.7 nm) to emit electrons, since its threshold lies in the UV (λ0 = hc/W0 ≈ 277 nm).
Conclusion: The work function of silver is about 4.48 eV (7.18 × 10−19 J).
Ex 2.54 — If the photon of the wavelength 150 pm strikes an atom and one of its inner bound electrons is ejected out with a velocity of 1.5 × 107 m s−1, calculate the energy with which it is bound to the nucleus.
Concept. Energy conservation: photon energy = binding energy of the electron + kinetic energy of the ejected electron. Therefore binding energy = hc/λ − ½ mev2.
- λ = 150 pm = 1.5 × 10−10 m: Ephoton = (6.626 × 10−34)(3.0 × 108)/(1.5 × 10−10) = 1.325 × 10−15 J.
- K.E. = ½ (9.109 × 10−31 kg)(1.5 × 107 m s−1)2 = 1.025 × 10−16 J.
- Binding energy = 1.325 × 10−15 − 1.025 × 10−16 = 1.22 × 10−15 J (≈ 7.6 keV).
| Quantity | Value |
|---|---|
| Photon energy | 1.325 × 10−15 J |
| K.E. of ejected electron | 1.025 × 10−16 J |
| Binding energy | 1.22 × 10−15 J |
Extra depth. A 150 pm photon is an X-ray; it can eject an inner (core) electron which is bound far more strongly (thousands of eV) than the outer electrons (a few eV, Ex 2.51). This is the principle of X-ray photoelectron spectroscopy. The electron speed of 1.5 × 107 m s−1 is 5% of c, so the non-relativistic K.E. formula is still a good approximation.
Conclusion: The inner electron is bound to the nucleus with an energy of about 1.22 × 10−15 J.
Ex 2.55 — Emission transitions in the Paschen series end at orbit n = 3 and start from orbit n and can be represented as ν = 3.29 × 1015 (Hz) [1/32 − 1/n2]. Calculate the value of n if the transition is observed at 1285 nm. Find the region of the spectrum.
Concept. Convert the wavelength to frequency, ν = c/λ, then solve the given Paschen expression for n.
- ν = c/λ = 3.0 × 108 m s−1/(1285 × 10−9 m) = 2.335 × 1014 Hz.
- 2.335 × 1014 = 3.29 × 1015 (1/9 − 1/n2) ⇒ 1/9 − 1/n2 = 0.0710.
- 1/n2 = 0.1111 − 0.0710 = 0.0401 ⇒ n2 = 24.9 ≈ 25 ⇒ n = 5.
- The transition is 5 → 3 of the Paschen series; λ = 1285 nm lies in the infrared region.
| Quantity | Value |
|---|---|
| Series | Paschen (nf = 3) |
| Frequency observed | 2.335 × 1014 Hz |
| Starting orbit n | 5 |
| Spectral region | Infrared (λ = 1285 nm > 750 nm) |
Extra depth. All lines of the Paschen series (nf = 3) are in the infrared (Table 2.3): the first line (4 → 3) is at 1875 nm and the series limit at 820 nm. The wavelength 1285 nm lies between them — the 5 → 3 line.
Conclusion: n = 5 (the 5 → 3 transition of the Paschen series), observed in the infrared region.
Ex 2.56 — Calculate the wavelength for the emission transition if it starts from the orbit having radius 1.3225 nm and ends at 211.6 pm. Name the series to which this transition belongs and the region of the spectrum.
Concept. The radius of the nth Bohr orbit of hydrogen is rn = n2 × 52.9 pm. So n = √(r/52.9 pm). The wavelength then follows from ΔE = 2.18 × 10−18(1/nf2 − 1/ni2) and λ = hc/ΔE.
- Initial orbit: r = 1.3225 nm = 1322.5 pm; ni2 = 1322.5/52.9 = 25 ⇒ ni = 5.
- Final orbit: r = 211.6 pm; nf2 = 211.6/52.9 = 4 ⇒ nf = 2.
- ΔE = 2.18 × 10−18 (1/4 − 1/25) = 2.18 × 10−18 × 0.21 = 4.578 × 10−19 J.
- λ = hc/ΔE = 1.988 × 10−25/4.578 × 10−19 = 4.34 × 10−7 m = 434 nm.
- The transition 5 → 2 ends at n = 2: it belongs to the Balmer series, in the visible region (violet).
| Quantity | Value |
|---|---|
| ni (r = 1322.5 pm) | 5 |
| nf (r = 211.6 pm) | 2 |
| λ | 434 nm |
| Series | Balmer |
| Region | Visible (violet) |
Extra depth. 434 nm is the Hγ line — the third line of the Balmer series (see Ex 2.13 and Problem 2.10 for the 4 → 2 and 5 → 2 lines; 5 → 2 is 434 nm). The radius 1322.5 pm of the fifth orbit was found in Ex 2.16.
Conclusion: The transition is n = 5 → n = 2 (Balmer series); λ = 434 nm, in the visible region.
Ex 2.57 — Dual behaviour of matter proposed by de Broglie led to the discovery of electron microscope often used for the highly magnified images of biological molecules and other type of material. If the velocity of the electron in this microscope is 1.6 × 106 m s−1, calculate de Broglie wavelength associated with this electron.
Concept. The de Broglie wavelength is λ = h/(mev). Because electrons travelling fast have very short wavelengths, an electron microscope can resolve details far smaller than an ordinary (light) microscope.
- mev = 9.109 × 10−31 kg × 1.6 × 106 m s−1 = 1.457 × 10−24 kg m s−1.
- λ = 6.626 × 10−34/1.457 × 10−24 = 4.55 × 10−10 m (455 pm = 4.55 Å).
| Quantity | Value |
|---|---|
| Electron speed | 1.6 × 106 m s−1 |
| Momentum | 1.457 × 10−24 kg m s−1 |
| Wavelength | 4.55 × 10−10 m (455 pm) |
Extra depth. Visible light has λ = 400–750 nm, whereas the electron wave here is about 1000 times shorter (0.455 nm), so a microscope using it can resolve structures near atomic dimensions. The chapter notes that the magnification can reach about 15 million times.
Conclusion: The de Broglie wavelength of the electron is 4.55 × 10−10 m (about 455 pm).
Ex 2.58 — Similar to electron diffraction, neutron diffraction microscope is also used for the determination of the structure of molecules. If the wavelength used here is 800 pm, calculate the characteristic velocity associated with the neutron.
Concept. From λ = h/(mv) the velocity is v = h/(mλ). The mass of a neutron is 1.675 × 10−27 kg (Table 2.1).
- λ = 800 pm = 800 × 10−12 m = 8.0 × 10−10 m.
- v = h/(mnλ) = 6.626 × 10−34/(1.675 × 10−27 × 8.0 × 10−10).
- v = 6.626 × 10−34/1.34 × 10−36 = 4.94 × 102 m s−1 (≈ 494 m s−1).
| Quantity | Value |
|---|---|
| Neutron mass | 1.675 × 10−27 kg |
| Wavelength | 8.0 × 10−10 m |
| Velocity | 494 m s−1 |
Extra depth. Thermal neutrons moving at a few hundred m s−1 have wavelengths of about 0.1–1 nm — comparable to interatomic distances — so they are diffracted by crystals; since neutrons are neutral, they are scattered by nuclei (and are especially good at locating hydrogen atoms). A 1836 times lighter electron would need to travel much faster for the same wavelength (about 9 × 105 m s−1).
Conclusion: The neutron has a velocity of about 494 m s−1 (4.94 × 102 m s−1).
Ex 2.59 — If the velocity of the electron in Bohr’s first orbit is 2.19 × 106 m s−1, calculate the de Broglie wavelength associated with it.
Concept. The de Broglie wavelength of the electron is λ = h/(mev).
- mev = 9.109 × 10−31 × 2.19 × 106 = 1.995 × 10−24 kg m s−1.
- λ = 6.626 × 10−34/1.995 × 10−24 = 3.32 × 10−10 m (332 pm).
| Quantity | Value |
|---|---|
| Speed in first Bohr orbit | 2.19 × 106 m s−1 |
| de Broglie wavelength | 3.32 × 10−10 m = 332 pm |
| Circumference 2πr1 = 2π(52.9 pm) | 332 pm |
Extra depth. The wavelength 332 pm equals the circumference of the first Bohr orbit (2π × 52.9 pm = 332 pm), which confirms Ex 2.32 for n = 1: 2πr = nλ with n = 1. The electron wave just fits once around the first orbit.
Conclusion: The de Broglie wavelength of the electron in the first Bohr orbit is 3.32 × 10−10 m (332 pm).
Ex 2.60 — The velocity associated with a proton moving in a potential difference of 1000 V is 4.37 × 105 m s−1. If the hockey ball of mass 0.1 kg is moving with this velocity, calculate the wavelength associated with this velocity.
Concept. The de Broglie relation λ = h/(mv) applies to every moving object. The question compares a proton with a hockey ball moving at the same speed: the wavelength is inversely proportional to the mass, so the heavy ball has a vanishingly small wavelength.
- m = 0.1 kg, v = 4.37 × 105 m s−1: mv = 4.37 × 104 kg m s−1.
- λ = 6.626 × 10−34 J s/4.37 × 104 kg m s−1 = 1.52 × 10−38 m.
| Object | Mass | Speed | Wavelength |
|---|---|---|---|
| Proton (Table 2.1) | 1.673 × 10−27 kg | 4.37 × 105 m s−1 | 9.06 × 10−13 m (0.9 pm) |
| Hockey ball | 0.1 kg | 4.37 × 105 m s−1 | 1.52 × 10−38 m |
Extra depth. The ball’s wavelength (10−38 m) is about 1025 times smaller than a proton’s at the same speed (the ratio of the masses is 6 × 1025) and far smaller than anything measurable — which is why the wave nature of macroscopic bodies is never observed (Problem 2.12), whereas for electrons and protons it is.
Conclusion: The wavelength associated with the hockey ball is about 1.52 × 10−38 m — far too small to be detected.
Ex 2.61 — If the position of the electron is measured within an accuracy of ± 0.002 nm, calculate the uncertainty in the momentum of the electron. Suppose the momentum of the electron is h/(4π) × 0.05 nm, is there any problem in defining this value.
Concept. Heisenberg’s uncertainty principle: Δx · Δp ≥ h/4π, so the minimum uncertainty in momentum is Δp = h/(4π Δx). If the uncertainty in momentum is as large as, or larger than, the momentum itself, the momentum cannot be defined meaningfully.
- Δx = 0.002 nm = 2 × 10−12 m.
- Δp = h/(4π Δx) = 6.626 × 10−34/(4 × 3.1416 × 2 × 10−12) = 2.64 × 10−23 kg m s−1.
- Momentum given in the question (read as p = h/(4π × 0.05 nm)): p = 6.626 × 10−34/(4 × 3.1416 × 0.05 × 10−9) = 1.05 × 10−24 kg m s−1.
- Compare: Δp/p = 2.64 × 10−23/1.05 × 10−24 ≈ 25. The uncertainty is about 25 times the momentum itself.
| Quantity | Value |
|---|---|
| Δx | 2 × 10−12 m |
| Minimum Δp | 2.64 × 10−23 kg m s−1 |
| Given momentum p | 1.05 × 10−24 kg m s−1 |
| Δp/p | ≈ 25 (> 1) |
Yes, there is a problem. The uncertainty in the momentum (2.64 × 10−23) is much larger than the momentum value (1.05 × 10−24), so a value of the momentum cannot be assigned to the electron when its position is fixed this precisely — the momentum is effectively undefined.
Extra depth. Data note: the printed expression “h/4πm × 0.05 nm” is ambiguous; we read it as h/(4π × 0.05 nm), the form used in the standard solution (the units kg m s−1 confirm this reading). The conclusion does not depend on small changes in the interpretation: for the momentum to be well defined, Δp must be much smaller than p, which requires Δx to be much larger than 0.05 nm.
Conclusion: Δp = 2.64 × 10−23 kg m s−1; since this is ~25 times larger than the given momentum (1.05 × 10−24), the momentum cannot be defined — there is a problem.
Ex 2.62 — The quantum numbers of six electrons are given below. Arrange them in order of increasing energies. If any of these combination(s) has/have the same energy lists: 1. n = 4, l = 2, ml = −2, ms = −1/2; 2. n = 3, l = 2, ml = 1, ms = +1/2; 3. n = 4, l = 1, ml = 0, ms = +1/2; 4. n = 3, l = 2, ml = −2, ms = −1/2; 5. n = 3, l = 1, ml = −1, ms = +1/2; 6. n = 4, l = 1, ml = 0, ms = +1/2.
Concept. In a multi-electron atom the energy of an electron depends on n and l only (not on ml or ms). By the (n + l) rule, the lower the value of (n + l) the lower the energy; if (n + l) is the same, the electron with the lower n has the lower energy.
| No. | n | l | Orbital | n + l |
|---|---|---|---|---|
| 1 | 4 | 2 | 4d | 6 |
| 2 | 3 | 2 | 3d | 5 |
| 3 | 4 | 1 | 4p | 5 |
| 4 | 3 | 2 | 3d | 5 |
| 5 | 3 | 1 | 3p | 4 |
| 6 | 4 | 1 | 4p | 5 |
- Electron 5 (3p, n + l = 4) has the lowest energy.
- Electrons 2, 3, 4 and 6 all have n + l = 5; among them the lower n (n = 3: the 3d electrons 2 and 4) is lower than n = 4 (the 4p electrons 3 and 6).
- Electron 1 (4d, n + l = 6) has the highest energy.
5 < 2 = 4 < 3 = 6 < 1
Same energy: electrons 2 and 4 (both in the 3d subshell, different only in ml and ms) and electrons 3 and 6 (both in the 4p subshell) have the same energy.
Extra depth. Electrons 3 and 6 have identical quantum numbers (4, 1, 0, +½), which Pauli’s principle forbids in the same atom; the question treats them only as a list of combinations. In an isolated multi-electron atom the 3d orbitals (5 of them) are degenerate regardless of ml, and so are the three 4p orbitals.
Conclusion: Increasing energy: 5 < 2 = 4 < 3 = 6 < 1; electrons 2 & 4 (3d) and 3 & 6 (4p) have the same energy.
Ex 2.63 — The bromine atom possesses 35 electrons. It contains 6 electrons in 2p orbital, 6 electrons in 3p orbital and 5 electron in 4p orbital. Which of these electron experiences the lowest effective nuclear charge?
Concept. The effective nuclear charge Zeff is the nuclear charge (+35 for Br) minus the screening produced by the other electrons. Electrons in the outer shells are shielded by all the inner-shell electrons, so Zeff decreases as the distance from the nucleus (principal quantum number) increases.
| Electrons | Shell | Position | Shielding by inner electrons | Zeff |
|---|---|---|---|---|
| 2p (6 electrons) | n = 2 | closest to the nucleus | little (only 1s and 2s) | highest of the three |
| 3p (6 electrons) | n = 3 | intermediate | 1s, 2s, 2p, 3s | intermediate |
| 4p (5 electrons) | n = 4 | outermost | all inner shells (1s–3d) | lowest |
The 4p electrons are the farthest from the nucleus and are screened by the largest number of inner-shell electrons (28 core electrons plus partial screening by 4s and other 4p electrons), so they feel the smallest effective nuclear charge.
Extra depth. This is also why the outermost electrons are the ones that are lost or shared in chemical reactions: the lowest Zeff means the weakest attraction. Across a period Zeff of the valence shell increases (Ex 2.65); down a group it is shielded more and the valence electrons are held less tightly.
Conclusion: The 4p electrons (the outermost electrons of bromine) experience the lowest effective nuclear charge.
Ex 2.64 — Among the following pairs of orbitals which orbital will experience the larger effective nuclear charge? (i) 2s and 3s, (ii) 4d and 4f, (iii) 3d and 3p.
Concept. Two trends decide Zeff: (1) for the same type of orbital, Zeff is larger for the shell closer to the nucleus (smaller n, less shielding); (2) in the same shell, Zeff decreases in the order s > p > d > f because penetration towards the nucleus decreases with l (Section 2.6.3).
| Pair | Deciding factor | Orbital with larger Zeff |
|---|---|---|
| (i) 2s and 3s | same l; 2s is closer to the nucleus (smaller n, less shielding) | 2s |
| (ii) 4d and 4f | same n; l = 2 (d) < l = 3 (f), d penetrates more | 4d |
| (iii) 3d and 3p | same n; l = 1 (p) < l = 2 (d), p penetrates more | 3p |
Extra depth. The same reasoning gives the energy order in multi-electron atoms: the orbital with larger Zeff is more tightly bound and has lower energy, so E(2s) < E(3s), E(4d) < E(4f) and E(3p) < E(3d).
Conclusion: (i) 2s; (ii) 4d; (iii) 3p experience the larger effective nuclear charge.
Ex 2.65 — The unpaired electrons in Al and Si are present in 3p orbital. Which electrons will experience more effective nuclear charge from the nucleus?
Concept. Al (Z = 13) is [Ne]3s23p1 and Si (Z = 14) is [Ne]3s23p2. In both atoms the electrons are in the same shell (n = 3), shielded by the same 10 core electrons (1s22s22p6) and in the same subshell, so shielding is almost the same. The nuclear charge is the decisive difference.
| Atom | Nuclear charge | Core electrons shielding | 3p electrons | Zeff on 3p |
|---|---|---|---|---|
| Al | +13 | 10 (+ 3s electrons partly) | 1 | smaller |
| Si | +14 | 10 (+ 3s electrons partly) | 2 | larger |
Si has one more proton, but the extra electron enters the same 3p subshell, where it shields only slightly. So the net attraction on the 3p electrons is greater in silicon: the 3p electrons of Si experience the larger effective nuclear charge.
Extra depth. This is the reason for the periodic trends: across a period (Na → Ar) Zeff on the valence electrons increases, atomic radii decrease and ionisation energies generally increase (Chapter 3).
Conclusion: The 3p electrons of silicon experience the greater effective nuclear charge than those of aluminium.
Ex 2.66 — Indicate the number of unpaired electrons in: (a) P, (b) Si, (c) Cr, (d) Fe and (e) Kr.
Concept. Write the ground-state configuration (aufbau principle, Pauli exclusion principle and Hund’s rule: electrons occupy degenerate orbitals singly with parallel spins before pairing) and count the singly occupied orbitals.
| Atom (Z) | Electronic configuration | Orbital diagram of the valence subshells | Unpaired electrons |
|---|---|---|---|
| (a) P (15) | [Ne] 3s2 3p3 | 3s: ↑↓; 3p: ↑ ↑ ↑ | 3 |
| (b) Si (14) | [Ne] 3s2 3p2 | 3s: ↑↓; 3p: ↑ ↑ _ | 2 |
| (c) Cr (24) | [Ar] 3d5 4s1 | 3d: ↑ ↑ ↑ ↑ ↑; 4s: ↑ | 6 |
| (d) Fe (26) | [Ar] 3d6 4s2 | 3d: ↑↓ ↑ ↑ ↑ ↑; 4s: ↑↓ | 4 |
| (e) Kr (36) | [Ar] 3d10 4s2 4p6 | all orbitals full | 0 |
- P: the three 3p electrons occupy three different orbitals (Hund’s rule) — half-filled p subshell; 3 unpaired.
- Si: two 3p electrons in two different orbitals — 2 unpaired.
- Cr: the exceptional configuration 3d54s1 (half-filled d and half-filled s) gives 6 unpaired electrons — the maximum for the 3d series.
- Fe: 3d6: one 3d orbital has a pair and four are singly occupied — 4 unpaired.
- Kr: noble gas with completely filled subshells — no unpaired electron (diamagnetic).
Extra depth. The number of unpaired electrons determines paramagnetism: P, Si, Cr and Fe are paramagnetic, Kr is diamagnetic. If chromium followed the regular order (3d44s2) it would have only 4 unpaired electrons.
Conclusion: Unpaired electrons: P = 3, Si = 2, Cr = 6, Fe = 4, Kr = 0.
Ex 2.67 — (a) How many subshells are associated with n = 4? (b) How many electrons will be present in the subshells having ms value of −1/2 for n = 4?
Concept. The number of subshells in the nth shell equals n (l = 0 to n − 1). The number of orbitals in the shell is n2, and each orbital can hold only one electron with ms = −½ (the other has +½).
- (a) Subshells for n = 4: l = 0, 1, 2, 3, i.e. four subshells: 4s, 4p, 4d and 4f.
- (b) Electrons with ms = −½ in n = 4: orbitals = 1 (4s) + 3 (4p) + 5 (4d) + 7 (4f) = 16 (= n2). Each orbital has one electron with ms = −½, so 16 electrons (when the shell is completely filled: 32 electrons in all, half with ms = −½).
| Subshell | l | Orbitals | Electrons with ms = −½ |
|---|---|---|---|
| 4s | 0 | 1 | 1 |
| 4p | 1 | 3 | 3 |
| 4d | 2 | 5 | 5 |
| 4f | 3 | 7 | 7 |
| Total | 16 | 16 |
Extra depth. The maximum capacity of the fourth shell is 2n2 = 32 electrons. The answer 16 is a maximum (it applies when all the 4s, 4p, 4d and 4f orbitals are occupied); in a real atom such as potassium only the 4s orbital of the fourth shell is occupied. This exercise is the same counting as part (a) of Ex 2.31.
Conclusion: (a) 4 subshells (4s, 4p, 4d, 4f); (b) 16 electrons (one in each of the 16 orbitals) have ms = −½.