Electrochemistry: Complete Notes for NEET, JEE, IIT-JAM, BITSAT, GATE and CSIR-NET
Electrochemistry sits at the intersection of thermodynamics and redox chemistry, and once you see that connection clearly, most of the chapter stops feeling like a pile of formulas to memorize and starts feeling like one continuous argument. A spontaneous redox reaction wants to release free energy; if we physically separate the oxidation and reduction half-reactions and force the electrons to travel through an external wire to get from one to the other, that released energy shows up as electrical work instead of just heat. Run the same idea backward — push electrons in from an outside source — and you can force a non-spontaneous redox reaction to occur. The first process is what happens inside a galvanic (voltaic) cell; the second is electrolysis. Almost everything in this chapter is a consequence of that one idea, dressed up in different notations for different situations.
I want to build this chapter the way you'll actually need it for exams: starting from cell construction and notation, moving into the thermodynamics that connects cell potential to Gibbs energy and equilibrium constants, then the Nernst equation and its applications, electrode types, concentration cells, electrolysis and Faraday's laws, batteries, and finally conductance — which, despite appearing in the same chapter, is really a separate but related topic about how well solutions carry current.
Contents
- Electrochemical Cells
- Electrode Potential
- Measurement of Electrode Potential
- Thermodynamics of a Cell
- The Nernst Equation
- Calculating E°cell
- Types of Electrodes
- Concentration Cells
- Electrolytic Cells, Electrolysis and Faraday's Laws
- Applications of Electrolysis
- Batteries and Fuel Cells
- Electrical Conductance
- Conductance in Electrolyte Solutions and Kohlrausch's Law
- Conductometric Titrations
- Practice MCQs (35 Questions with Answers)
1 | Electrochemical Cells
An electrochemical cell is a device that interconverts chemical and electrical energy. There are two fundamentally different kinds, and confusing them is one of the most common sources of exam errors, so it's worth fixing the distinction early: a galvanic cell (also called a voltaic cell) uses a spontaneous redox reaction to generate electrical energy, while an electrolytic cell consumes electrical energy to drive a non-spontaneous redox reaction. Galvanic cells split further into chemical cells, where the two electrodes involve genuinely different chemical species, and concentration cells, where the electrodes are chemically identical but differ only in the concentration of the electrolyte or the pressure of a gas.
Galvanic Cells and the Daniell Cell
The classic teaching example is the Daniell cell, built from a zinc electrode dipped in ZnSO4 solution and a copper electrode dipped in CuSO4 solution, the two half-cells connected by a salt bridge. Zinc has a much greater tendency to lose electrons than copper does, so left to itself the system reacts as:
Splitting this into half-reactions:
Reduction (at copper): Cu2+(aq) + 2e− → Cu(s)
Zinc dissolves, releasing electrons that travel through the external wire to the copper electrode, where they reduce Cu2+ ions to metallic copper. This particular cell develops about 1.1 V under standard conditions. If you apply an external voltage that opposes the cell exactly at 1.1 V, the net current drops to zero — the cell is momentarily balanced. Push the opposing voltage higher than 1.1 V and something interesting happens: the reaction reverses direction entirely, copper now dissolves and zinc gets deposited, and the galvanic cell has effectively become an electrolytic cell running on borrowed electrical energy. This reversibility is central to understanding why Ecell shows up as a switch point in so many later derivations.
Cell Terminology and Conventions
A working vocabulary here will save you time throughout the chapter:
- Half-cell: One electrode dipped in its electrolyte solution — the physical compartment where one half-reaction occurs.
- Half-reaction: The oxidation or reduction reaction occurring at a single electrode.
- Cathode: The electrode where reduction occurs (electrons are consumed).
- Anode: The electrode where oxidation occurs (electrons are released).
- Cell reaction: The overall reaction, obtained by scaling the two half-reactions so the electrons cancel and then adding them.
In a galvanic cell, the cathode is the positive terminal and the anode is negative — this is a point students frequently get backward, so it's worth anchoring firmly: at the anode, atoms are leaving the metal as cations, stranding electrons behind and giving that electrode a slight negative charge; at the cathode, cations from solution are picking up electrons and depositing as neutral atoms, which leaves that electrode slightly positive. Cations in the bulk solution migrate toward the cathode (hence the name — they move toward the negatively-charged-relative attractor) and anions migrate toward the anode.
Cell notation follows fixed rules. A single vertical line (or semicolon) marks a phase boundary across which a potential develops — for instance, a copper electrode in 1 M CuSO4 is written Cu | Cu2+(1 M). By convention, the oxidation electrode (anode) is written on the left and the reduction electrode (cathode) on the right, separated by a double vertical line representing the salt bridge:
and the cell potential is defined as:
where both E values are standard reduction potentials, regardless of which electrode is actually undergoing oxidation in practice. This "always use reduction potentials, always read right minus left" convention removes the guesswork of manually tracking signs — commit it to memory rather than re-deriving it each time.
Solution: The left side is the anode (oxidation), the right side is the cathode (reduction).
Anode: Ni(s) → Ni2+(aq) + 2e−
Cathode: Au3+(aq) + 3e− → Au(s)
To balance electrons, multiply the nickel half-reaction by 3 and the gold half-reaction by 2, giving 6 electrons on each side:
3Ni(s) → 3Ni2+(aq) + 6e−
2Au3+(aq) + 6e− → 2Au(s)
Adding and cancelling electrons: 3Ni(s) + 2Au3+(aq) → 3Ni2+(aq) + 2Au(s)
The Salt Bridge and Liquid Junction Potential
Without an internal connection between the two half-cells, charge would build up almost immediately — the anode compartment would accumulate excess positive charge as cations form, and the cathode compartment would accumulate excess negative charge as cations are consumed — and the current would stop within moments. The salt bridge, typically a U-tube of agar gel saturated with an inert electrolyte such as KCl, solves this by allowing ions to migrate and maintain electroneutrality in both compartments without letting the two solutions mix directly.
KCl is the standard choice for a reason worth understanding rather than memorizing: K+ and Cl− have almost identical ionic mobilities, so they migrate out of the salt bridge at essentially the same rate. If two electrolyte solutions of different composition or concentration are placed in direct contact without a salt bridge, the ions diffuse across the junction at different rates (since different ions have different mobilities), and this unequal diffusion sets up a small potential difference called the liquid junction potential. The measured EMF of such a cell is then
A properly functioning KCl salt bridge drives ELJP to essentially zero, which is precisely why salt bridges are used: they let you measure the "clean" potential difference between the two half-cells without a confounding junction contribution.
2 | Electrode Potential
When a metal is placed in a solution of its own ions, a potential difference develops at the metal-solution interface — this is the electrode potential. Physically it arises because the metal has some characteristic tendency either to send its atoms into solution as cations (leaving electrons behind) or to pull cations out of solution and deposit them (consuming electrons). Different metals have different tendencies, and it's exactly this difference in tendency between two coupled electrodes that produces a working cell.
The standard electrode potential is measured with all species at unit activity (1 M for dissolved ions, 1 bar for gases) at 298 K — this defines the standard state used throughout the chapter. By IUPAC convention, we tabulate electrode potentials as standard reduction potentials: the potential associated with the half-reaction written as a reduction. Recall the definition of the volt itself, since it occasionally shows up in derivation-based questions: 1 V corresponds to 1 joule of work done per coulomb of charge transported, 1 V = 1 J/C.
Oxidation and Reduction Potential
Every electrode can, in principle, be written either as an oxidation half-reaction or a reduction half-reaction; the two potentials are equal in magnitude and opposite in sign for the same electrode:
For example, a zinc electrode in 1 M ZnSO4 at 298 K has an oxidation potential of +0.76 V (favoring Zn → Zn2+ + 2e−) and a reduction potential of −0.76 V (for Zn2+ + 2e− → Zn). Comparing these two values for a given electrode tells you which direction is spontaneous at that electrode in isolation — for zinc, since the oxidation potential is more positive, oxidation is the spontaneous direction. Keep in mind, though, that once an electrode is wired into an actual cell, whether it behaves as anode or cathode depends on what it's paired with, not on this isolated comparison.
Cell EMF and Reversibility
The maximum potential a cell can deliver, measured when no current flows, is the electromotive force (EMF). The moment current actually flows, some of that potential is lost overcoming the cell's own internal resistance, so the measured terminal voltage under load is always somewhat less than the EMF. EMF is measured with a potentiometer (a null-deflection method that draws essentially zero current), while ordinary potential differences under load can be read with a voltmeter.
A cell is called reversible if two conditions hold: applying an external EMF exactly equal and opposite to the cell's own EMF brings the reaction to a complete stop, and applying an infinitesimally larger opposing EMF reverses the direction of the reaction. The Daniell cell satisfies both conditions cleanly. Cells that don't satisfy this — for instance, a Zn–Ag cell in dilute H2SO4, where reversing the applied potential produces an entirely different reaction (silver dissolving and hydrogen evolving) rather than simply running the original reaction backward — are classified as irreversible.
3 | Measurement of Electrode Potential
Here's a subtlety that trips a lot of students up: you cannot measure the potential of a single electrode in isolation. Any attempt to connect a measuring probe directly to one half-cell effectively creates a second electrode-solution interface, introducing a new equilibrium and a new, unwanted potential. The only workable approach is to couple the electrode of interest to a second electrode whose potential is already known — a reference electrode — measure the EMF of the resulting cell, and back out the unknown potential by subtraction.
A good reference electrode needs two properties: its potential must be reliably known under the conditions used, and that potential should vary as little as possible with temperature (a large temperature coefficient makes the reference unreliable as conditions drift slightly during an experiment).
The Standard Hydrogen Electrode
The standard hydrogen electrode (SHE), also called the normal hydrogen electrode (NHE), is the universal primary reference against which every other electrode potential is ultimately measured. It consists of a platinum foil (coated with finely divided platinum black to promote adsorption) immersed in 1.0 M HCl, with pure hydrogen gas bubbled over it at 1 bar pressure and 298 K. The platinum itself doesn't participate chemically — it just provides a conducting surface where adsorbed H2 and H+ in solution can equilibrate:
By convention — not by any actual physical measurement, since an absolute single-electrode potential can't be measured — the SHE is assigned a potential of exactly 0.00 V at all temperatures. Every tabulated standard reduction potential is really the EMF of a cell formed by coupling that electrode to a SHE, reported as if the SHE contributes nothing. Because building and maintaining a hydrogen electrode (controlling gas purity, pressure, and platinum surface condition precisely) is experimentally demanding, chemists usually calibrate more convenient secondary reference electrodes — most commonly the calomel electrode — against the SHE once, and then use those secondary electrodes for routine measurements.
Solution: Since the silver electrode is positive, it is the cathode (reduction occurs there), and the hydrogen electrode is the anode (oxidation).
Anode: H2(g) → 2H+(aq) + 2e−; Cathode: Ag+(aq) + e− → Ag(s)
E°cell = E°cathode − E°anode = E°Ag+/Ag − 0 = 0.80 V, so E°Ag+/Ag = +0.80 V.
Calomel Electrode and the Electrochemical Series
The calomel electrode (mercurous chloride electrode) is the most widely used secondary reference because it's compact, robust, easy to transport, and gives a highly reproducible potential that barely shifts with temperature — properties that make it ideal for routine lab work and corrosion studies, where a bulky hydrogen-gas setup would be impractical. It consists of pure mercury at the bottom of a container, covered by a paste of Hg, Hg2Cl2, and KCl, with the rest of the vessel filled with KCl solution saturated with Hg2Cl2:
The reduction half-reaction is Hg2Cl2(s) + 2e− → 2Hg(l) + 2Cl−(aq). For working out a half-cell reaction from a compact notation like this one, a reliable three-step method is: (1) assign oxidation numbers to every element in the notation, (2) read left to right and identify which oxidation number changes, and (3) balance that fundamental change using the species actually present in the half-cell.
Once enough half-reactions have been measured against the SHE (directly or via a calibrated secondary reference), they can be tabulated as an electrochemical series — a ranked list of standard reduction potentials, conventionally arranged from most positive (strongest oxidizing agents, top of the table) to most negative (strongest reducing agents, bottom). Species written on the left of each half-reaction (e.g., F2) are oxidizing agents because they get reduced going forward; species on the right (e.g., Li) are reducing agents because they get oxidized going in reverse. This ordering has real predictive power:
- A metal higher in the series (more negative/lower reduction potential) can displace, from solution, any metal that sits below it — this is exactly why zinc shavings displace copper from CuSO4 solution.
- The lower the reduction potential of a couple, the greater its reducing power; the higher the reduction potential, the greater the tendency to get reduced (the stronger the oxidizing power).
- Given any two half-cells, you can immediately predict the polarity of each electrode and the spontaneity of the overall combination without further calculation.
4 | Thermodynamics of a Cell
This is where electrochemistry connects back to the thermodynamics you already know, and understanding the connection makes the rest of the chapter's equations feel derived rather than dropped from nowhere. The electrical work a spontaneous cell can deliver is the maximum useful (non-expansion) work available from the reaction, and by the standard thermodynamic identification of maximum useful work with the Gibbs energy change:
where n is the number of moles of electrons transferred per mole of reaction as written, F is Faraday's constant (charge per mole of electrons, 96,500 C mol−1), and Ecell is the cell potential. Under standard conditions this becomes
The negative sign matters and is worth internalizing rather than just memorizing: a spontaneous cell reaction (ΔG < 0) must correspond to a positive Ecell, which lines up with the everyday fact that a working battery has a positive voltage.
Now bring in the general thermodynamic relation between ΔG and the reaction quotient, ΔG = ΔG° + RT ln Q, and substitute both Gibbs energy expressions:
Dividing through by −nF gives the Nernst equation, which we'll return to in detail in the next section:
At equilibrium, Ecell = 0 and Q = Keq, so the Nernst equation collapses to a direct link between the standard cell potential and the equilibrium constant of the cell reaction:
This single relation is enormously useful on exams because it lets you move freely between three quantities that otherwise look unrelated: a measured cell voltage, a Gibbs energy change, and an equilibrium constant for a redox reaction that might otherwise be tedious to evaluate directly.
Enthalpy and Entropy from the Temperature Dependence of EMF
If you know how Ecell varies with temperature at constant pressure, you can extract ΔH and ΔS for the cell reaction as well, using the Gibbs–Helmholtz equation ΔG = ΔH + T[∂(ΔG)/∂T]p. Substituting ΔG = −nFE and differentiating:
ΔS = nF(∂E/∂T)p
The quantity (∂E/∂T)p is called the temperature coefficient of the cell. Its sign tells you something physically meaningful: if the coefficient is positive, the cell's EMF (and hence ΔS of the reaction) increases with temperature; a coefficient of essentially zero, as in the calomel electrode, is precisely what makes an electrode attractive as a stable reference.
Solution: With n = 2, F = 96,500 C mol−1:
ΔG° = −nFE° = −2 × 96500 × 0.42 = −81,060 J mol−1 = −81.06 kJ mol−1
ΔS° = nF(∂E/∂T)p = 2 × 96500 × 1.5 × 10−4 = 28.95 J K−1 mol−1
ΔH° = ΔG° + TΔS° = −81060 + (298 × 28.95) = −81060 + 8627.1 = −72.43 kJ mol−1
5 | The Nernst Equation
Standard electrode potentials assume every species is at unit concentration (or unit pressure for gases) — a convenient but artificial condition that real solutions rarely satisfy exactly. The Nernst equation tells us how the potential shifts away from the standard value as concentrations deviate from 1 M. We already derived the cell-level form above; the same logic applies to a single electrode. For a general reduction half-reaction Mn+ + ne− → M at equilibrium, the electrode potential at any concentration is:
(using [M] = 1 for a pure solid). Substituting R = 8.314 J K−1 mol−1, F = 96,500 C mol−1, T = 298 K, and converting to base-10 logarithms gives the version you'll actually use for calculations:
A few points about applying this correctly are worth being explicit about, since they're exactly where marks are lost in numerical problems:
- Q is built the same way as any reaction quotient — products over reactants, each raised to its stoichiometric coefficient — with pure solids and liquids taken as unity, and gas-phase species entered as partial pressures (in atm) rather than concentrations.
- Any half-cell reaction always carries an explicit e− term; a full-cell reaction never does, because the electrons from oxidation and reduction cancel exactly.
- n is the number of electrons that cancel when the two balanced half-reactions are combined into the overall cell reaction — not simply "the charge on the ion," which is a frequent source of arithmetic slips.
Solution: The half-reaction is Ag+ + e− → Ag, so n = 1.
E = E° − (0.0591/1) log(1/[Ag+]) = 0.80 − 0.0591 × log(1/0.015)
= 0.80 − 0.0591 × log(66.67) = 0.80 − 0.0591 × 1.824 = 0.80 − 0.1078 = 0.692 V
Solution: E°cell = E°cathode − E°anode = −0.13 − (−0.40) = +0.27 V
Cell reaction: Cd(s) + Pb2+(aq) → Cd2+(aq) + Pb(s), so n = 2 and Q = [Cd2+]/[Pb2+] = 0.05/0.2 = 0.25
Ecell = 0.27 − (0.0591/2) log(0.25) = 0.27 − 0.02955 × (−0.602) = 0.27 + 0.0178 = 0.288 V
Equilibrium Constant from the Nernst Equation
Returning to the equilibrium relation E°cell = (0.0591/n) log Keq at 298 K: this is one of the most exam-favoured results in the whole chapter because it converts a redox equilibrium constant — which could otherwise require awkward independent measurement — into something obtainable purely from tabulated electrode potentials. Practically, once you have E°cell and n, solving for log Keq and then taking the antilog gives Keq directly.
Solution: n = 2 (from the Ni → Ni2+ + 2e− half-reaction).
log K = nE°cell/0.0591 = (2 × 1.05)/0.0591 = 35.53
K = antilog(35.53) ≈ 3.4 × 1035 — confirming the reaction proceeds essentially to completion.
6 | Calculating E°cell
There's a subtlety in combining half-cell potentials that catches many students, and it's worth stating as a clean rule rather than re-deriving it every time: electrode potential (E°) is an intensive property — it does not scale with the number of electrons or the stoichiometric coefficients you multiply through by when balancing a reaction. Gibbs energy (ΔG°), by contrast, is extensive and does scale. This distinction produces two different combination rules depending on what you're combining.
Case 1: Two Half-Cells Combine to Give a Full Cell
Here you simply subtract the two standard reduction potentials directly — you do not multiply either one by the number of electrons, even if you had to multiply the half-reactions themselves to balance electrons:
This is exactly the rule used throughout the worked examples above.
Case 2: Two Half-Cells Combine to Give a Third Half-Cell
This case is different and is a frequent source of error: when you're not forming a complete cell but instead deriving one half-reaction's potential from two others (for example, finding E° for Fe3+/Fe from the known potentials of Fe3+/Fe2+ and Fe2+/Fe), you must work through Gibbs energies, because ΔG° — unlike E° — is a state function that adds directly along a path of half-reactions:
−n3FE°3 = −n1FE°1 − n2FE°2
E°3 = (n1E°1 + n2E°2) / n3
Solution: This is Case 2 — we're building one new half-reaction (Cr3+ → Cr, n = 3) from two others (n = 1 and n = 2 respectively).
E°Cr3+/Cr = [(1)(−0.41) + (2)(−0.91)] / 3 = (−0.41 − 1.82)/3 = −2.23/3 = −0.743 V
7 | Types of Electrodes
Electrodes are classified by what's physically present at the metal-solution interface. Recognizing the type quickly tells you how to write the half-reaction and how to set up the Nernst equation, so it's worth being able to sort any electrode you're given into one of these five buckets.
Metal–Metal Ion Electrode
The simplest case: a metal rod dipped directly in a solution of its own ions, e.g., Zn2+/Zn or Ag+/Ag. The metal can serve as either anode or cathode depending on what it's coupled with.
Gas–Gas Ion Electrode
Since gases don't conduct electricity on their own, an inert metal (typically platinum, often coated with platinum black to increase surface area and catalyze the equilibrium) provides electrical contact between the gas and its ions in solution. The SHE is the standard example of this type; the general notation is Pt | Gas(p atm) | Ion(C M).
Redox Electrode
Here the electrode potential arises purely from the presence of two different oxidation states of the same species in solution, with an inert platinum wire simply providing the electrical contact — the platinum itself never changes oxidation state. A classic example is Pt | Fe2+(C1 M), Fe3+(C2 M), where the potential depends on the ratio of the two concentrations via the Nernst equation. The quinhydrone electrode, used historically to measure pH, is another example: quinhydrone dissolves to give an equimolar mixture of quinone and hydroquinone, and the quinone/hydroquinone couple behaves as a reversible redox electrode.
Metal Insoluble Salt–Anion Electrode
Built by coating a metal with a paste of one of its sparingly soluble salts and immersing it in a solution containing the salt's anion — the Ag/AgCl electrode (silver coated with saturated AgCl, dipped in NaCl solution) is the standard example. Because the electrode potential ends up depending on the solubility product of the coating salt, this type is useful for measuring Ksp values. The derivation runs through the Gibbs-energy-addition logic from Section 6: writing AgCl(s) → Ag+(aq) + Cl−(aq) (governed by Ksp) and Ag+(aq) + e− → Ag(s) as two steps that add to give the overall electrode reaction AgCl(s) + e− → Ag(s) + Cl−(aq), you arrive at:
Amalgam Electrode
A modification of the metal–metal ion electrode where the metal is dissolved in mercury (an amalgam) rather than existing as pure solid metal — for instance Zn(Hg) | Zn2+(x M). Since the metal in the amalgam is not at unit activity the way a pure solid is, the Nernst equation for this electrode explicitly retains a concentration term for the metal:
8 | Concentration Cells
A concentration cell generates a (typically small, and rapidly decaying) EMF purely from a difference in concentration or pressure between two otherwise identical electrodes — there is no net chemical transformation of one substance into another the way there is in the Daniell cell; the "reaction" is simply the transport of the electroactive species from the more concentrated side to the more dilute side. Because both half-cells involve the same reduction potential formula with the same E° value, E°cell for any concentration cell is exactly zero, and the entire observed EMF comes from the log(Q) term in the Nernst equation.
Electrode Concentration Cells
Here the electrolyte concentration is identical in both compartments, but the two electrodes themselves differ in some measurable way — most commonly, two hydrogen electrodes with H2 maintained at different pressures p1 and p2 (p1 > p2), both dipped in the same HCl solution:
Since E°cell = 0 for identical hydrogen electrodes, the Nernst equation reduces directly to:
Electrolyte Concentration Cells
Here it's the electrolyte concentration itself that differs between the two compartments containing otherwise identical electrodes, with the two solutions connected directly (through a porous membrane) rather than via a salt bridge — no salt bridge is needed here because there's no risk of unwanted chemical reaction between the two identical species, only a driving force toward equalizing concentration. Because ions are free to migrate directly across the junction, the EMF expression carries an extra factor for the transport number of the moving ion:
Solution: For a hydrogen electrode concentration cell, n = 2 and E°cell = 0.
Ecell = (0.0591/2) log(2.5/0.5) = 0.02955 × log(5) = 0.02955 × 0.699 = 0.0207 V
Applications of Concentration Cells
Concentration cells aren't practical power sources — their EMF collapses quickly as the concentration difference driving them equalizes — but they have genuine analytical value:
- Determining ionic valency: build a concentration cell from two solutions of the same ion at known but different concentrations C1 and C2, measure Ecell, and solve Ecell = (0.0591/n) log(C2/C1) for n. This is historically how the doubly-charged nature of the mercurous ion, Hg22+, was confirmed experimentally.
- Determining solubility of a sparingly soluble salt: couple a silver electrode in a saturated AgCl solution (concentration unknown, call it x) against a silver electrode in a known AgNO3 concentration. Measuring Ecell lets you solve for x, and from x you can get Ksp and hence the solubility of AgCl.
Solution: n = 2 for Pb2+/Pb. Ecell = (0.0591/2) log(x/0.001)
0.0295 = 0.02955 × log(x/0.001) ⇒ log(x/0.001) ≈ 1.0 ⇒ x/0.001 = 10
x = 0.01 M
9 | Electrolytic Cells, Electrolysis and Faraday's Laws
Where a galvanic cell harnesses a spontaneous reaction to produce electrical energy, an electrolytic cell runs the whole idea in reverse: an external power source forces electrons through the system, driving a redox reaction that would never occur on its own. Both electrodes now sit in the same container in a single electrolyte (there's no need to physically separate the half-reactions, since nothing is spontaneous here that needs protecting from a competing back-reaction), and the polarity of each electrode is dictated entirely by which terminal of the external battery it's connected to.
| Galvanic Cell | Electrolytic Cell |
|---|---|
| Converts chemical energy to electrical energy | Converts electrical energy to chemical energy |
| Redox reaction is spontaneous | Redox reaction is non-spontaneous; driven externally |
| Two electrodes in separate compartments, joined by a salt bridge | Two electrodes share a single container/electrolyte |
| Anode is negative, cathode is positive | Anode is positive, cathode is negative |
| Electron source: the species undergoing reaction itself | Electron source: the external battery |
Faraday's First Law
The mass of a substance deposited or liberated at an electrode is directly proportional to the quantity of charge passed:
Z, the electrochemical equivalent, is the mass deposited by exactly 1 coulomb of charge. Since 1 mole of electrons carries 96,500 C (one Faraday, F), and Z relates to molar mass through Z = M/(n × F), Faraday's first law is most usefully rearranged as:
where E = M/n-factor is the equivalent weight of the substance. This form is what you'll actually reach for in numerical problems, since it directly connects current, time, and mass through the number of equivalents.
Faraday's Second Law
When the same quantity of charge is passed through different electrolytic cells connected in series, the masses of different substances deposited or dissolved are proportional to their equivalent weights:
This follows immediately from the first law once you notice that It/96500 — the number of equivalents — is the same for both cells if the same charge passes through each.
Solution: Ca2+ + 2e− → Ca, so equivalent weight E = 40/2 = 20 g equiv.−1
Q = It = 2.5 × 40 × 60 = 6000 C
w = (E × Q)/96500 = (20 × 6000)/96500 = 120000/96500 = 1.244 g
Solution: EAg = 108/1 = 108; ECr = 52/3 = 17.33
By Faraday's second law: wAg/EAg = wCr/ECr
wCr = wAg × (ECr/EAg) = 3.05 × (17.33/108) = 0.489 g
What Actually Gets Discharged: Preferential Discharge
When an electrolyte solution contains more than one type of cation or anion — which, in aqueous solution, is essentially always the case since water itself contributes H+ and OH− — several competing electrode reactions become possible, and predicting which one actually occurs requires weighing a few factors together rather than applying just one rule.
- Standard electrode potential: at the cathode, the species with the highest (most positive) reduction potential is reduced preferentially; at the anode, the species with the lowest reduction potential (i.e., most easily oxidized) is oxidized preferentially. This is the electrochemical series doing its predictive work again, now applied to electrolysis.
- Nature of the electrolyte — molten vs. aqueous: electrolyzing molten NaCl gives sodium metal and chlorine gas cleanly, because there's no competing water. Electrolyzing aqueous NaCl gives entirely different products — H2 at the cathode and Cl2 at the anode, with NaOH accumulating in solution — because water's own reduction (to H2) is thermodynamically preferred over Na+ reduction, and even though water's oxidation to O2 is thermodynamically preferred over Cl− oxidation, Cl− is observed to be oxidized instead due to overpotential — the extra potential beyond the thermodynamic minimum needed to actually drive a kinetically sluggish reaction, and O2 evolution from water is kinetically very slow.
- Nature of the electrodes: inert electrodes like platinum act only as a source or sink of electrons and don't influence the products; reactive electrodes participate directly. Using a mercury cathode for aqueous NaCl electrolysis, for instance, suppresses H2 evolution (mercury has an unusually high overpotential for hydrogen) and allows Na+ to be reduced instead, forming a sodium amalgam — the basis of the industrial chlor-alkali process.
- Concentration: since concentration enters the Nernst equation, the effective electrode potential (not just the standard value) shifts with concentration, and this can flip which reaction is preferred. In sulphuric acid electrolysis, dilute acid gives O2 at the anode, while concentrated acid favors formation of peroxydisulphate, S2O82−.
Thickness of an Electroplated Layer
Faraday's first law can be adapted to find how thick a coating becomes in electroplating. If a metal sheet of dimensions l × b (cm) is coated to thickness h (cm), the volume coated is l × b × h, and the mass deposited is that volume times the metal's density ρ:
Transport (Transference) Number
During electrolysis, current is carried jointly by both cations and anions, and the transport number of an ion is simply the fraction of the total current it carries:
Since the current an ion carries depends on its charge, speed, and concentration, and since electroneutrality requires m+Q+ = m−Q− for the electrolyte as a whole, the transport numbers simplify to a ratio of ionic speeds (equivalently, ionic conductances):
10 | Applications of Electrolysis
Corrosion and Its Prevention
Rusting is the most familiar example of corrosion, and it's fundamentally an electrochemical process — not a simple direct chemical attack — which is why iron rusts readily in the presence of both oxygen and moisture together, but resists rusting if either one alone is absent. At an anodic region on the metal surface, iron oxidizes: Fe(s) → Fe2+(aq) + 2e−. The released electrons travel through the metal to a separate cathodic region, where dissolved oxygen is reduced: ½O2(aq) + H2O(l) + 2e− → 2OH−(aq). The Fe2+ and OH− formed at separate locations diffuse together and precipitate as Fe(OH)2, which atmospheric O2 further oxidizes and partially dehydrates into the hydrated oxide we recognize as rust, roughly Fe2O3·xH2O.
Two main prevention strategies follow directly from this electrochemical picture:
- Sacrificial protection (protective coatings): covering iron with a more reactive metal — zinc in galvanization is the standard example — so the coating metal oxidizes preferentially and protects the iron underneath, even if the coating is scratched.
- Cathodic protection: connecting the iron structure to a more easily oxidized metal (again, commonly zinc, attached e.g. to a ship's rudder), which forces the iron to behave as the cathode of the resulting galvanic pair. Since corrosion occurs at anodic sites, converting the entire iron structure into one large cathodic surface protects it, at the cost of the sacrificial anode gradually corroding away and needing periodic replacement.
Electroplating
Electroplating deposits a thin protective or decorative layer of one metal onto another using electrolysis — silver-plating cutlery is the classic example. The object to be plated is made the cathode, the plating metal forms the anode, and the electrolyte contains a complex ion of the plating metal (e.g., [Ag(CN)2]− rather than free Ag+) because such complexes deposit a smoother, more uniform layer than direct reduction of the free metal ion would give.
Electrolytic Refining of Metals
Impure metal (e.g., blister copper containing Zn, Fe, Ag, and Au as impurities) is made the anode in a bath of its own salt solution, with a thin sheet of pure metal as the cathode. At the correct applied voltage, the base metal and any impurity metals more easily oxidized than it (here Zn and Fe) dissolve into solution, while impurities that are harder to oxidize than the metal itself (Ag, Au) simply detach as solid particles and fall to the bottom as "anode mud" — this anode mud is, incidentally, an economically important byproduct precisely because it concentrates the precious metal impurities. At the cathode, only the target metal ion is reduced, since the more easily-reduced target ion is thermodynamically favored over the less-easily-reduced impurity ions (Zn2+, Fe2+) left behind in solution.
Electrometallurgy and Compound Preparation
Highly reactive metals — the alkali metals, alkaline earth metals, and aluminium — sit so low in the electrochemical series that their aqueous salt solutions can't be electrolyzed to give the free metal at all; water itself gets reduced/oxidized preferentially. These metals must instead be extracted by electrolysis of a fused (molten) salt, as in the Hall–Héroult process for aluminium or the Down's process for sodium. Electrolysis is also used industrially to manufacture a range of important compounds, including NaOH, Na2CO3, KMnO4, and various organic compounds via processes like Kolbe's electrolysis of carboxylate salts.
11 | Batteries and Fuel Cells
A battery is simply a practical, portable packaging of one or more galvanic cells. Batteries split into two broad classes based on whether the underlying chemical reaction can be reversed: primary cells are used until their active materials are exhausted and then discarded, while secondary (storage) cells can be recharged by driving the discharge reaction backward with an external current — meaning a secondary cell behaves as a galvanic cell while discharging and as an electrolytic cell while charging. Every battery, regardless of type, is built from the same four basic components: an anode (where oxidation occurs), a cathode (where reduction occurs), an electrolyte that carries ions between them, and a separator that physically keeps the electrode products from mixing while still allowing ion transport.
Primary Cells
Dry cell (Leclanché cell): a zinc container serves as both the physical casing and the anode, with a central graphite rod surrounded by a manganese dioxide paste acting as cathode, and a moist paste of NH4Cl and ZnCl2 as electrolyte.
Cathode: 2MnO2(s) + H2O(l) + 2e− → Mn2O3(s) + 2OH−(aq)
It delivers about 1.5 V, but the voltage drifts downward with use as products accumulate at the electrodes, and the acidic NH4Cl slowly corrodes the zinc casing even when the cell sits unused, which limits shelf life.
Alkaline dry cell: essentially the same construction, but NH4Cl is replaced by NaOH or KOH, which doesn't corrode zinc (zinc is stable in basic medium) and gives a more stable voltage over the cell's life.
Cathode: 2MnO2 + 2e− + H2O(l) → Mn2O3(s) + 2OH−(aq)
Mercury cell (Ruben–Mallory cell): amalgamated zinc powder as anode, a paste of HgO and graphite as cathode, and a paste of ZnO/KOH as electrolyte. Because the electrolyte composition doesn't change as the reaction proceeds — KOH is regenerated as fast as it's consumed — this cell delivers an unusually flat, constant voltage (about 1.35 V) throughout its working life, which makes it valuable in devices like watches and hearing aids where voltage stability matters more than raw energy density.
Cathode: HgO(s) + H2O(l) + 2e− → Hg(l) + 2OH−(aq)
Secondary (Storage) Cells
Lead storage battery (the standard car battery): a lead grid packed with spongy lead metal is the anode; a lead grid packed with PbO2 is the cathode; roughly 20% sulphuric acid is the electrolyte.
Cathode: PbO2(s) + 4H+(aq) + SO42−(aq) + 2e− → PbSO4(s) + 2H2O(l)
Notice that H2SO4 is consumed by the overall discharge reaction, which is exactly why the density of the acid — a direct proxy for its concentration — is used as a practical, quick way to check a lead battery's state of charge. Recharging simply reverses both half-reactions, converting the PbSO4 deposited on both plates back into Pb and PbO2 respectively and regenerating H2SO4 — behaving, during charging, exactly like an electrolytic cell.
Nickel–cadmium cell: spongy cadmium as anode, nickel oxyhydroxide as cathode, concentrated KOH as electrolyte.
Cathode: 2NiO(OH)(aq) + 2H2O(l) + 2e− → 2Ni(OH)2(aq) + 2OH−(aq)
Delivering about 1.4 V and available in compact button-cell form, it was historically popular for portable electronics before largely being displaced by lithium-based chemistry.
Lithium batteries: lithium is an unusually attractive anode material because it's the lightest metal, has a very negative (favorable) electrode potential, and conducts well — a combination that yields both high voltage and high energy density per unit mass. In the lithium–manganese dioxide cell, lithium metal is the anode and heat-treated MnO2 the cathode, with the electrolyte a mixture of lithium salts dissolved in an organic solvent (aqueous electrolytes can't be used since lithium reacts violently with water):
Cathode: MnIVO2 + Li+ + e− → Li+[MnIIIO2]−
delivering roughly 3.0 V — noticeably higher than either the dry cell or Ni–Cd cell — while being lighter and more compact, which is why lithium chemistry now dominates portable electronics.
Solution: Q = It = 4.0 × 3 × 3600 = 43200 C
At the cathode, PbO2 + 4H+ + SO42− + 2e− → PbSO4 + 2H2O, so n = 2, giving equivalent weight of PbSO4 = 303/2 = 151.5
w = (E × Q)/96500 = (151.5 × 43200)/96500 = 6,544,800/96500 ≈ 67.8 g
Fuel Cells
A conventional route to electricity — burning a fuel to release heat, using the heat to raise steam, and using the steam to spin a turbine-generator — loses a substantial fraction of the fuel's chemical energy at each conversion step, with overall efficiencies often only around 40%. A fuel cell sidesteps this entirely by converting the chemical energy of a fuel directly into electrical energy through a continuously-fed, catalytically-activated redox reaction, avoiding the intermediate heat-engine step altogether — which is exactly why fuel cells can reach substantially higher thermodynamic efficiency, typically in the 70–75% range.
A fuel cell differs from an ordinary battery in one crucial respect: the reactants (fuel and oxidant) are not stored inside the cell itself but are continuously supplied from outside, so the cell keeps producing current as long as the feed continues, rather than running down as its own internal stock of reactants depletes.
The hydrogen–oxygen fuel cell is the most widely discussed example, historically significant for its use in crewed spaceflight. Hydrogen flows over one porous carbon electrode (the anode) and oxygen over the other (the cathode), separated by an ion-conducting electrolyte such as concentrated aqueous NaOH:
Cathode: O2(g) + 4H+(aq) + 4e− → 2H2O(l)
Overall: 2H2(g) + O2(g) → 2H2O(l)
The only byproduct is water, which is precisely why this technology is attractive wherever both power and potable water are valuable, as on a spacecraft.
The thermodynamic efficiency of a fuel cell is defined as the ratio of the useful electrical work actually obtained to the enthalpy change of the overall reaction:
Solution: Since ΔG = wuseful under ideal (reversible) conditions, efficiency = ΔG°/ΔH°
Efficiency = (−237/−286) × 100 = 82.9%
12 | Electrical Conductance
Conductance is really a story about two entirely different physical mechanisms that happen to share the same vocabulary and units. Metallic (electronic) conductors carry current via the drift of essentially free, delocalized electrons through a fixed lattice of metal cations — no matter is transported, and no chemical change accompanies the flow of current. Electrolytic conductors carry current via the physical migration of ions through a solution or molten salt toward the oppositely charged electrode — here, matter genuinely moves, and a chemical change (the electrode reaction) is an unavoidable part of sustaining current flow, which is the deep reason electrolysis exists as a phenomenon at all.
This mechanistic difference produces opposite temperature dependences, a fact that's tested often enough to be worth stating plainly: raising the temperature of a metal increases lattice vibrations, which scatter the drifting electrons more and so decreases metallic conductance; raising the temperature of an electrolyte solution decreases the solution's viscosity and increases ion mobility (and, for weak electrolytes, increases the degree of dissociation too), so electrolytic conductance increases with temperature.
Based on how completely they ionize, electrolytes are classified as strong (essentially complete dissociation in solution — HCl, NaOH, KCl) or weak (only partial dissociation, with an equilibrium persisting between ions and undissociated molecules — CH3COOH, NH4OH).
Resistance, Resistivity, and Conductance
Like any conductor, an electrolytic solution offers resistance to current flow, following the same geometric dependence as a metallic wire: resistance is proportional to path length l and inversely proportional to cross-sectional area A, R = ρ(l/A), where ρ is the resistivity (specific resistance) — the resistance of a sample exactly 1 m long with 1 m2 cross-section. Conductance G is simply the reciprocal of resistance, G = 1/R, measured in siemens (S), also historically called the mho (ohm spelled backward). The reciprocal of resistivity is conductivity (specific conductance), κ = 1/ρ = (1/R)(l/A), representing the conductance of exactly 1 cm³ of solution.
Measuring Solution Resistance: The Conductivity Cell
A direct-current Wheatstone bridge can't be used on an ionic solution, because passing DC current through the solution itself would electrolyze it and steadily change its composition mid-measurement. The workaround is to use an alternating current source together with a purpose-built conductivity cell — typically two fixed platinum electrodes, coated with platinum black to reduce polarization effects, forming one arm of an AC-fed Wheatstone bridge. The cell's geometry (length/area ratio) is a fixed characteristic called the cell constant:
determined experimentally by measuring the resistance of a KCl solution of precisely known conductivity, and then applied to compute the conductivity of any unknown solution measured afterward in the same cell.
13 | Conductance in Electrolyte Solutions and Kohlrausch's Law
Because different electrolytes dissociate into different numbers and charges of ions, comparing raw conductivity values across electrolytes isn't very meaningful on its own — a more useful quantity accounts for how much electrolyte is actually present. Molar conductance is the conductance contributed by all the ions from exactly 1 mole of electrolyte at a given concentration:
where C is the molar concentration. The related equivalent conductance uses gram-equivalents instead of moles in the same expression.
Why Molar Conductance Increases on Dilution — and Differently for Strong vs. Weak Electrolytes
Both types of electrolyte show increasing Λm as concentration drops, but for genuinely different physical reasons, and distinguishing those reasons is exactly what exam questions on this topic tend to probe.
For a weak electrolyte, the number of ions actually present in solution is small at higher concentration simply because dissociation is incomplete. Diluting the solution shifts the dissociation equilibrium further toward completion (more ions per mole of original electrolyte), so Λm rises sharply and continues rising all the way to very low concentrations. On a plot of Λm against √C, a weak electrolyte traces a curve that shoots up steeply near C = 0 without ever quite leveling off at an experimentally accessible point — meaning Λm0 for a weak electrolyte can't be found by extrapolating the graph and must instead be obtained indirectly (see Kohlrausch's law below).
For a strong electrolyte, essentially full dissociation already exists even in a fairly concentrated solution — the rise in Λm on dilution isn't about creating more ions, but about the ions already present interfering with each other less. Each ion is surrounded by a loose cloud of oppositely-charged neighbours that creates a retarding "drag" on its motion; diluting the solution spreads the ions farther apart, weakening this interionic drag and letting each ion move more freely. Kohlrausch found this behavior follows a clean empirical relation at low concentration:
so a plot of Λm against √C gives a straight line for a strong electrolyte, with slope −k and y-intercept Λm0 — meaning, unlike the weak-electrolyte case, Λm0 for a strong electrolyte genuinely can be read straight off the graph by extrapolating to C = 0.
Kohlrausch's Law of Independent Ionic Migration
At infinite dilution, interionic effects vanish entirely and each ion migrates completely independently of whatever counter-ion it happens to be paired with — so each ion makes a fixed, characteristic contribution to the total molar conductance, regardless of which specific salt it came from:
where λ+0 and λ−0 are the limiting (infinite-dilution) ionic conductances of the cation and anion, and v+, v− are the number of each ion per formula unit. This is precisely the tool that solves the weak-electrolyte problem flagged above: since λ0 values are additive and transferable between different salts, you can build up Λm0 for a weak electrolyte from the (graphically obtainable) Λm0 values of related strong electrolytes that share ions with it.
Solution: By Kohlrausch's law, Λm0(CH3COOH) = λ°CH3COO− + λ°H+
= [Λm0(CH3COOK) + Λm0(HCl) − Λm0(KCl)]
= 114.4 + 426.2 − 149.9 = 390.7 S cm2 mol−1
Once Λm0 for a weak electrolyte is known this way, the degree of dissociation α at any working concentration C can be found from the ratio of the actual molar conductance to the limiting one:
and substituting this α into the standard weak-electrolyte equilibrium expression K = Cα²/(1 − α) gives the dissociation constant purely from conductance data:
Solution: α = Λm/Λm0 = 19.6/380 = 0.0516
K = Cα²/(1−α) = (0.02 × 0.0516²)/(1 − 0.0516) = (0.02 × 0.002663)/0.9484 = 5.62 × 10−5
Other Applications of Kohlrausch's Law
- Ionic conductance from transport number: t+ = λ+0/Λ0, so knowing the transport number and the overall limiting molar conductance gives the individual ionic conductance.
- Solubility of a sparingly soluble salt: a saturated solution of a very insoluble salt (like AgCl) is dilute enough that its molar conductance essentially equals Λm0 (built up from tabulated ionic values via Kohlrausch's law); measuring the solution's conductivity κ then gives the concentration, and hence the solubility, via Λm0 = κ/(1000C).
14 | Conductometric Titrations
A conductometric titration tracks how a solution's conductance changes as one ion is progressively replaced by another during a titration, exploiting the fact that different ions carry current with markedly different efficiency (different ionic conductances/mobilities). Instead of relying on a color-change indicator, the equivalence point shows up as a sharp change in slope on a plot of conductance versus volume of titrant added — which makes this method valuable for colored or turbid solutions where a visual indicator would be hard to read.
Strong Acid vs. Strong Base (e.g., HCl titrated with NaOH)
Initially, conductance is high because of the very mobile H+ ion. As NaOH is added, fast-moving H+ is progressively replaced by the much slower Na+ (via H+ + OH− → H2O), so conductance falls steadily until the equivalence point, where the solution contains only NaCl. Beyond that point, further NaOH adds free, highly mobile OH− ions directly to the solution, so conductance rises again — producing a sharp, easily located V-shaped minimum right at the equivalence point.
Weak Acid vs. Strong Base (e.g., CH3COOH titrated with NaOH)
Because acetic acid is only weakly ionized to begin with, initial conductance is low. As NaOH is added, the common-ion effect from the sodium acetate being formed actually suppresses the acid's own dissociation further, but the acetate ion produced by neutralization is still a better conductor than the barely-dissociated acid was, so conductance rises steadily (rather than falling, as in the strong-acid case) right up to the equivalence point. Past equivalence, added free OH− drives an even steeper rise. The curve therefore has a gentler, upward-only shape rather than a sharp V, and the equivalence point is located at the kink where the slope changes rather than at a minimum.
Weak Base vs. Strong Acid (e.g., NH4OH titrated with HCl)
Highly mobile H3O+ is progressively replaced by the much less mobile NH4+, so conductance falls up to the equivalence point, then stays nearly flat afterward — since excess NH4OH is only weakly ionized and contributes little additional conductance — with only a slight upward curvature very close to the endpoint due to hydrolysis of the NH4+ formed.
Precipitation Titrations (e.g., AgNO3 titrated with NaCl)
As NaCl is added, Ag+ is removed from solution as insoluble AgCl precipitate essentially as fast as it's added, so conductance stays roughly flat (Na+ simply substitutes for the departing Ag+ at similar mobility) until all the Ag+ is consumed. Beyond that point, further NaCl simply accumulates as free, dissociated electrolyte in solution, so conductance rises noticeably.
15 | Practice MCQs (35 Questions with Answers)
These questions are original and target the concepts covered above — mechanism-level understanding, not just formula recall. Work through them without looking at the answer key first; the point is to find out what you don't yet have solid, not to confirm what you already do.
- (a) Cathode, and it is the positive terminal
- (b) Anode, and it is the negative terminal
- (c) Cathode, and it is the negative terminal
- (d) Anode, and it is the positive terminal
- (a) They are colorless
- (b) They have nearly equal ionic mobilities
- (c) They form an insoluble precipitate
- (d) They have equal molar masses
- (a) EZn2+/Zn − ESn2+/Sn
- (b) ESn2+/Sn − EZn2+/Zn
- (c) EZn2+/Zn + ESn2+/Sn
- (d) 2ESn2+/Sn − EZn2+/Zn
- (a) Because it genuinely has no tendency to gain or lose electrons
- (b) By international convention, as a reference point
- (c) Only at 273 K
- (d) Because hydrogen is the lightest element
- (a) Sn2+ is oxidized by Fe3+
- (b) Fe2+ is oxidized by Sn4+
- (c) No reaction occurs between these species
- (d) Fe3+ is reduced by Sn4+
- (a) Ecell = E°cell and ΔG = 0
- (b) Ecell = 0 and Q = K
- (c) Ecell = 0 and ΔG° = 0
- (d) Q = 0 and Ecell = E°cell
- (a) Very small, close to zero
- (b) Exactly 1
- (c) Very large, favoring products
- (d) Negative
- (a) Simply add the two E° values
- (b) Subtract the two E° values
- (c) Add the nE° (proportional to ΔG°) products, then divide by the target n
- (d) Average the two E° values regardless of electron count
- (a) Concentration in mol/L for the gas
- (b) Mole fraction of the gas
- (c) Partial pressure of the gas in atm
- (d) Density of the gas
- (a) 1
- (b) 2
- (c) 3
- (d) 4
- (a) Metal–metal ion electrode
- (b) Gas–gas ion electrode
- (c) Redox electrode
- (d) Amalgam electrode
- (a) Increase the electrode potential
- (b) Decrease the electrode potential
- (c) Have no effect on the electrode potential
- (d) Cause the electrode to stop functioning
- (a) Positive
- (b) Negative
- (c) Zero
- (d) Dependent on which side has higher concentration
- (a) Because no current flows in such a cell
- (b) Because both electrodes and electrolytes are chemically identical, so direct contact poses no risk of an unwanted reaction
- (c) Because the electrodes are inert
- (d) Because the electrolyte is a solid
- (a) Dissolve into solution along with the copper
- (b) Are deposited at the cathode before copper
- (c) Fall to the bottom as anode mud
- (d) Form a soluble complex with sulphate ions
- (a) The higher standard reduction potential of the Cl2/Cl− couple compared to O2/H2O
- (b) Overpotential, which makes O2 evolution kinetically slow despite being thermodynamically favored
- (c) Chlorine being a heavier gas
- (d) Sodium ions blocking oxygen evolution
- (a) The current alone
- (b) The time alone
- (c) The quantity of charge passed
- (d) The square of the current
- (a) 1:1
- (b) 1:2
- (c) 2:1
- (d) 1:4
- (a) 0.2 F
- (b) 0.6 F
- (c) 0.067 F
- (d) 3 F
- (a) Zinc physically blocks water from reaching the iron
- (b) Zinc is a better conductor than iron
- (c) Zinc is more easily oxidized than iron, so it corrodes preferentially and iron becomes the protected cathode
- (d) Zinc reacts with dissolved oxygen to remove it from the water
- (a) Free Ag+ does not conduct electricity
- (b) The complex ion gives a smoother, more uniform metal deposit
- (c) CN− is required to balance the charge of the spoon
- (d) Free Ag+ is too expensive
- (a) Increases, because H2SO4 is produced
- (b) Decreases, because H2SO4 is consumed and water is produced
- (c) Remains constant throughout discharge
- (d) Increases only at the cathode
- (a) It is the cheapest available metal
- (b) It is chemically inert and doesn't react with water
- (c) It is very light, has a highly negative electrode potential, and gives high energy density
- (d) It has the highest melting point among metals
- (a) It cannot produce direct current
- (b) Reactants are continuously supplied from outside rather than stored internally
- (c) It requires no electrolyte
- (d) It only works with molten salts
- (a) ΔH/ΔG
- (b) ΔG/ΔH (i.e., −nFE/ΔH)
- (c) ΔS/ΔH
- (d) E°cell/ΔS
- (a) Electrons are destroyed at high temperature
- (b) Increased lattice vibration scatters the drifting electrons more
- (c) The metal expands and becomes less dense
- (d) Free electrons recombine with metal cations
- (a) Electrolyte solutions have infinite resistance
- (b) DC current would electrolyze the solution, changing its composition during the measurement
- (c) Wheatstone bridges only work with solid conductors
- (d) Electrolyte solutions are always at the wrong temperature
- (a) The degree of dissociation increases, creating more ions per mole of electrolyte
- (b) Interionic attraction decreases
- (c) The solvent becomes a better conductor
- (d) Water molecules dissociate more readily
- (a) Weak electrolytes only
- (b) Strong electrolytes only
- (c) Both strong and weak electrolytes equally well
- (d) Neither; it must always be calculated from Kohlrausch's law
- (a) Ions stop moving entirely
- (b) Each ion's contribution to molar conductance is fixed, independent of the counter-ion it is paired with
- (c) All electrolytes have identical molar conductance
- (d) Only cations contribute to conductance
- (a) A steady increase throughout
- (b) A steady decrease throughout
- (c) A decrease to a minimum at the equivalence point, followed by an increase
- (d) No change until the equivalence point, then a sharp rise
- (a) Falls sharply, mirroring the strong-acid case
- (b) Rises gradually, as the poorly-conducting acid is converted to the better-conducting acetate salt
- (c) Stays exactly constant
- (d) Falls to zero
- (a) Anode, since it has higher concentration
- (b) Cathode, since reduction is favored at the more concentrated side
- (c) Neither; no current flows in a concentration cell
- (d) Both simultaneously
- (a) The total charge on the ion
- (b) The fraction of total current carried by that ion
- (c) The ion's molar mass divided by its charge
- (d) The ion's diffusion coefficient
- (a) 26.2 S cm2 mol−1
- (b) 126.4 S cm2 mol−1
- (c) 63.2 S cm2 mol−1
- (d) 152.8 S cm2 mol−1
