DUET

Course Code: CHE 2122 Chemistry

Topic: Class Test 02 Solutions

Answer to Question Number 1

Law of Mass Action

The Law of Mass Action (āĻ­āϰ āĻ•ā§āϰāĻŋāϝāĻŧāĻž āϏ⧂āĻ¤ā§āϰ) states that at a constant temperature, the rate at which a chemical reaction proceeds is directly proportional (āϏāϰāĻžāϏāϰāĻŋ āϏāĻŽāĻžāύ⧁āĻĒāĻžāϤāĻŋāĻ•) to the product of the active masses (āϏāĻ•ā§āϰāĻŋāϝāĻŧ āĻ­āϰ) or molar concentrations of the reacting substances.

For a general reversible reaction (āωāĻ­āĻŽā§āĻ–ā§€ āĻŦāĻŋāĻ•ā§āϰāĻŋāϝāĻŧāĻž):

\[aA + bB \rightleftharpoons cC + dD\]

According to the law:

  • Rate of forward reaction (\(R_f\)) \(\propto [A]^a [B]^b \implies R_f = k_f [A]^a [B]^b\)
  • Rate of backward reaction (\(R_b\)) \(\propto [C]^c [D]^d \implies R_b = k_b [C]^c [D]^d\)

Here, \(k_f\) and \(k_b\) are the rate constants (āĻ—āϤāĻŋ āĻ§ā§āϰ⧁āĻŦāĻ•) for forward and backward reactions.

Derivation of Relationship Between \(K_p\) and \(K_c\)

At chemical equilibrium (āϰāĻžāϏāĻžāϝāĻŧāύāĻŋāĻ• āϏāĻžāĻŽā§āϝāĻžāĻŦāĻ¸ā§āĻĨāĻž), the rate of forward reaction becomes equal to the rate of backward reaction (\(R_f = R_b\)):

\[k_f [A]^a [B]^b = k_b [C]^c [D]^d\]
\[\frac{k_f}{k_b} = \frac{[C]^c [D]^d}{[A]^a [B]^b}\]
\[K_c = \frac{[C]^c [D]^d}{[A]^a [B]^b}\]

Where \(K_c\) is the equilibrium constant in terms of concentration (āϘāύāĻŽāĻžāĻ¤ā§āϰāĻž).

If the reactants and products are in gaseous state, we express equilibrium constant in terms of partial pressure (āφāĻ‚āĻļāĻŋāĻ• āϚāĻžāĻĒ), denoted as \(K_p\):

\[K_p = \frac{P_C^c \cdot P_D^d}{P_A^a \cdot P_B^b}\]

From the ideal gas equation (āφāĻĻāĻ°ā§āĻļ āĻ—ā§āϝāĻžāϏ āϏāĻŽā§€āĻ•āϰāĻŖ), \(PV = nRT\):

\[P = \left(\frac{n}{V}\right) RT = C R T = [\text{Concentration}] RT\]

So, we write the partial pressures of each component as:

  • \(P_A = [A]RT\)
  • \(P_B = [B]RT\)
  • \(P_C = [C]RT\)
  • \(P_D = [D]RT\)

Now substituting these partial pressure values in the \(K_p\) expression:

\[K_p = \frac{([C]RT)^c \cdot ([D]RT)^d}{([A]RT)^a \cdot ([B]RT)^b}\]
\[K_p = \frac{[C]^c [D]^d}{[A]^a [B]^b} \cdot \frac{(RT)^{c+d}}{(RT)^{a+b}}\]
\[K_p = K_c (RT)^{(c+d)-(a+b)}\]
\[K_p = K_c (RT)^{\Delta n}\]

Where \(\Delta n = (c+d) - (a+b)\) represents the difference between total number of moles of gaseous products and gaseous reactants.

Answer to Question Number 2

Degree of Ionization

Degree of ionization or dissociation (āĻŦāĻŋāϝāĻŧā§‹āϜāύ āĻŽāĻžāĻ¤ā§āϰāĻž) is defined as the fraction of the total number of moles of a reactant that undergoes dissociation or splitting into simpler ions or molecules at equilibrium. It is denoted by the Greek letter \(\alpha\) (alpha).

\[\alpha = \frac{\text{Number of moles dissociated}}{\text{Total number of initial moles}}\]

Mathematical Derivation of \(K_p\) Equation for Dissociation of \(\text{PCl}_5\)

Let us consider the dissociation of Phosphorus Pentachloride (\(\text{PCl}_5\)) gas in a closed container:

\[\text{PCl}_5(g) \rightleftharpoons \text{PCl}_3(g) + \text{Cl}_2(g)\]
  • Initial moles at time \(t = 0\):
  • Moles of \(\text{PCl}_5 = 1\)
  • Moles of \(\text{PCl}_3 = 0\)
  • Moles of \(\text{Cl}_2 = 0\)

  • Moles at equilibrium:

  • Moles of \(\text{PCl}_5 = 1 - \alpha\)
  • Moles of \(\text{PCl}_3 = \alpha\)
  • Moles of \(\text{Cl}_2 = \alpha\)

Total number of moles at equilibrium (\(N_{total}\)):

\[N_{total} = (1 - \alpha) + \alpha + \alpha = 1 + \alpha\]

Let total pressure of the system at equilibrium be \(P\). Now we calculate the partial pressure of each gas using mole fraction (āĻŽā§‹āϞ āĻ­āĻ—ā§āύāĻžāĻ‚āĻļ):

  • \(P_{\text{PCl}_5} = \left(\frac{1 - \alpha}{1 + \alpha}\right) P\)
  • \(P_{\text{PCl}_3} = \left(\frac{\alpha}{1 + \alpha}\right) P\)
  • \(P_{\text{Cl}_2} = \left(\frac{\alpha}{1 + \alpha}\right) P\)

The equilibrium constant \(K_p\) expression for the reaction is:

\[K_p = \frac{P_{\text{PCl}_3} \cdot P_{\text{Cl}_2}}{P_{\text{PCl}_5}}\]

Substituting the partial pressure values:

\[K_p = \frac{\left(\frac{\alpha}{1 + \alpha} P\right) \cdot \left(\frac{\alpha}{1 + \alpha} P\right)}{\left(\frac{1 - \alpha}{1 + \alpha} P\right)}\]
\[K_p = \frac{\alpha^2 P^2}{(1 + \alpha)^2} \cdot \frac{1 + \alpha}{(1 - \alpha) P}\]
\[K_p = \frac{\alpha^2 P}{(1 + \alpha)(1 - \alpha)}\]
\[K_p = \frac{\alpha^2 P}{1 - \alpha^2}\]

This is the required mathematical expression for \(K_p\) for the dissociation of \(\text{PCl}_5\).

Answer to Question Number 3

Le Chatelier's Principle

Le Chatelier's principle (āϞāĻž āĻļāĻžāϤ⧇āϞāĻŋāϝāĻŧ⧇āϰ āύ⧀āϤāĻŋ) states that if a system at equilibrium is subjected to any change in stress parameters like temperature, pressure, or concentration, the equilibrium position will shift in such a direction so as to counteract or nullify (āĻĒā§āϰāĻļāĻŽāĻŋāϤ āĻ•āϰāĻž) the effect of that change.

Temperature Effect on the Synthesis of Ammonia

Ammonia (\(\text{NH}_3\)) is synthesized by Haber process according to the following reversible reaction:

\[\text{N}_2(g) + 3\text{H}_2(g) \rightleftharpoons 2\text{NH}_3(g) \quad \Delta H = -92.4 \text{ kJ/mol}\]

Key analysis of temperature effect:

  • The forward reaction is exothermic (āϤāĻžāĻĒāĻ‰ā§ŽāĻĒāĻžāĻĻā§€), meaning heat is released during the formation of ammonia.
  • According to Le Chatelier's principle, if we increase the temperature, the system will try to reduce the heat by shifting in the backward direction (āĻĒāĻļā§āϚāĻžā§ŽāĻŽā§āĻ–ā§€). This decreases the yield (āĻ‰ā§ŽāĻĒāĻžāĻĻāύ) of ammonia.
  • Conversely, if we decrease the temperature, the system shifts in the forward direction (āϏāĻŽā§āĻŽā§āĻ–āĻŽā§āĻ–ā§€) to produce more heat, which increases the yield of ammonia.
  • However, at very low temperatures, the rate of reaction (āĻŦāĻŋāĻ•ā§āϰāĻŋāϝāĻŧāĻžāϰ āĻ—āϤāĻŋ) becomes extremely slow and impractical for commercial synthesis.

To solve this problem, an optimum temperature (āĻ…āύ⧁āϕ⧂āϞ āϤāĻžāĻĒāĻŽāĻžāĻ¤ā§āϰāĻž) of around \(450^\circ\text{C}\) to \(500^\circ\text{C}\) is maintained along with an iron catalyst (āĻ…āύ⧁āϘāϟāĻ•) to get maximum yield at a good speed.

Assignment Answers: Atomic Structure and Quantum Mechanics

Answer to Question 1

Isotopes

Isotopes (āφāχāϏ⧋āĻŸā§‹āĻĒ / āϏāĻŽāĻ¸ā§āĻĨāĻžāύāĻŋāĻ•) are defined as atoms of the same chemical element having the same atomic number (\(Z\), number of protons) but different mass numbers (\(A\), total protons and neutrons). Because they have the same atomic number, they possess identical chemical properties but slightly different physical properties.

  • Example: Hydrogen has three well-known isotopes:
  • Protium (\(^1_1\text{H}\)): \(1\) proton, \(0\) neutrons
  • Deuterium (\(^2_1\text{H}\)): \(1\) proton, \(1\) neutron
  • Tritium (\(^3_1\text{H}\)): \(1\) proton, \(2\) neutrons

Isotones

Isotones (āφāχāϏ⧋āĻŸā§‹āύ / āϏāĻŽāύāĻŋāωāĻŸā§āϰāύāĻ•) are defined as atoms of different chemical elements having the same number of neutrons (\(A - Z\)) in their nucleus, but different atomic numbers (\(Z\)) and different mass numbers (\(A\)). Because they belong to different elements, their chemical and physical properties are completely different.

  • Example: Carbon-14 (\(^{14}_6\text{C}\)) and Oxygen-16 (\(^{16}_8\text{O}\)):
  • For Carbon-14: Neutrons = \(14 - 6 = 8\)
  • For Oxygen-16: Neutrons = \(16 - 8 = 8\)

Isobars

Isobars (āφāχāϏ⧋āĻŦāĻžāϰ / āϏāĻŽāĻ­āϰāϝ⧁āĻ•ā§āϤ) are defined as atoms of different chemical elements having the same mass number (\(A\)), but different atomic numbers (\(Z\)). Since they possess different atomic numbers, they belong to different elements and exhibit completely different chemical properties.

  • Example: Argon-40 (\(^{40}_{18}\text{Ar}\)) and Calcium-40 (\(^{40}_{20}\text{Ca}\)):
  • Argon-40: Mass number \(A = 40\), Atomic number \(Z = 18\)
  • Calcium-40: Mass number \(A = 40\), Atomic number \(Z = 20\)

Answer to Question 2

Statement of Hund's Rule

Hund's Rule of Maximum Multiplicity (āϏāĻ°ā§āĻŦā§‹āĻšā§āϚ āϗ⧁āĻŖāύ āύ⧀āϤāĻŋ) states that:

During the filling of electrons into degenerate orbitals (āϏāĻŽāĻļāĻ•ā§āϤāĻŋ āϏāĻŽā§āĻĒāĻ¨ā§āύ āĻ…āϰāĻŦāĻŋāϟāĻžāϞ) belonging to the same subshell, pairing of electrons will not take place until each available orbital is singly occupied by an electron with parallel spin (āϏāĻŽāĻŽā§āĻ–ā§€ āĻ¸ā§āĻĒāĻŋāύ).

Explanation of Hund's Rule

Electrons are negatively charged particles, so two electrons placed in the same orbital experience electrostatic repulsion (āĻ¸ā§āĻĨāĻŋāϰāĻŦ⧈āĻĻā§āϝ⧁āϤāĻŋāĻ• āĻŦāĻŋāĻ•āĻ°ā§āώāĻŖ). To minimize this inter-electronic repulsion and achieve maximum stability, electrons prefer to occupy separate degenerate orbitals (such as \(2p_x, 2p_y, 2p_z\)) individually first. Furthermore, these single electrons keep their spin directions parallel to gain exchange energy (āĻŦāĻŋāύāĻŋāĻŽāϝāĻŧ āĻļāĻ•ā§āϤāĻŋ), which makes the atom more stable. Only after every orbital of a subshell gets one electron each, does the pairing up of electrons begin with opposite spins.

Example

Consider the electronic configuration of Nitrogen (\(Z = 7\)):

Total electrons = \(7\).

  • \(1s^2 2s^2 2p^3\)

Here, the \(2p\) subshell has three degenerate orbitals (\(2p_x, 2p_y, 2p_z\)).

  • Incorrect filling: \(2p_x^2 2p_y^1 2p_z^0\) (violates Hund's rule because pairing happens before all \(p\)-orbitals get one electron).
  • Correct filling according to Hund's rule: \(2p_x^1 2p_y^1 2p_z^1\) (all three \(2p\) orbitals get one electron each with parallel spins).

Answer to Question 3

Definition of Quantum Numbers

Quantum numbers (āĻ•ā§‹ā§ŸāĻžāĻ¨ā§āϟāĻžāĻŽ āϏāĻ‚āĻ–ā§āϝāĻž) are a set of four mathematical values used to completely define the quantum state, exact address, energy level, orbital shape, orientation, and spin direction of an electron residing inside an atom.

The Four Quantum Numbers and Their Significance

1. Principal Quantum Number (\(n\))

  • Definition: Represents the main energy shell (āĻĒā§āϰāϧāĻžāύ āĻļāĻ•ā§āϤāĻŋāĻ¸ā§āϤāϰ) or orbit level in which the electron is revolving around the nucleus.
  • Allowed Values: Positive integers \(n = 1, 2, 3, 4, \dots\) (corresponding to \(K, L, M, N\) shells).
  • Significance: It determines the size of the electron cloud and the average distance of the electron from the nucleus. It also dictates the overall energy of the shell. The maximum electron capacity of any shell is calculated using \(2n^2\).

2. Azimuthal Quantum Number (\(l\))

  • Definition: Also called the orbital angular momentum quantum number, it defines the subshell (āωāĻĒāĻļāĻ•ā§āϤāĻŋāĻ¸ā§āϤāϰ) to which the electron belongs.
  • Allowed Values: \(l = 0 \text{ to } (n-1)\) for a given value of \(n\).
  • If \(l = 0\), it is \(s\)-subshell (Spherical shape)
  • If \(l = 1\), it is \(p\)-subshell (Dumbbell shape)
  • If \(l = 2\), it is \(d\)-subshell (Double dumbbell shape)
  • If \(l = 3\), it is \(f\)-subshell (Complex shape)

  • Significance: It determines the three-dimensional geometric shape of the orbital and the orbital angular momentum of the electron.

3. Magnetic Quantum Number (\(m_l\))

  • Definition: Represents the spatial orientation (āĻ¤ā§āϰāĻŋāĻŽāĻžāĻ¤ā§āϰāĻŋāĻ• āĻĻāĻŋāĻ•āĻŦāĻŋāĻ¨ā§āϝāĻžāϏ) of an orbital in three-dimensional space when placed under an external magnetic field.
  • Allowed Values: \(m_l = -l \text{ through } 0 \text{ to } +l\). Total values \(= (2l + 1)\).
  • For \(p\)-subshell (\(l=1\)), \(m_l = -1, 0, +1\) (gives 3 degenerate \(p\)-orbitals: \(p_x, p_y, p_z\)).

  • Significance: It determines the number of preferred spatial orientations or distinct degenerate orbitals present within a given subshell.

4. Spin Quantum Number (\(m_s\))

  • Definition: Describes the intrinsic spin direction (āύāĻŋāϜāĻ¸ā§āĻŦ āĻ˜ā§‚āĻ°ā§āĻŖāύ āĻĻāĻŋāĻ•) of an electron rotating around its own axis while orbiting the nucleus.
  • Allowed Values: \(m_s = +\frac{1}{2}\) (representing spin-up or clockwise rotation) and \(m_s = -\frac{1}{2}\) (representing spin-down or anti-clockwise rotation).
  • Significance: It distinguishes between two electrons occupying the exact same orbital, ensuring compliance with Pauli's Exclusion Principle (āĻĒāĻžāωāϞāĻŋāϰ āĻŦāĻ°ā§āϜāύ āύ⧀āϤāĻŋ) which states that no two electrons in an atom can have all four quantum numbers identical.