2011 h2 chemistry paper 3 suggested solutions
TRANSCRIPT
2011 H2 CHEMISTRY 9647/03 SUGGESTED SOLUTIONS
1 (a) Let the oxidation number of iodine in ICl4– be x.
–1 = –4 + x
x = +3
(b) ClF5: 5 bond pairs; 1 lone pair; square pyramidal
ICl4–: 4 bond pairs; 2 lone pairs; square planar
(c)(i) HClO + H+ + 2I
– Cl
– + I2 + H2O
(ii) Mass of NCS = 0.5 × 6.0 × 10–3
× 0.0050 × [4(12.0) + 4(1.0) + 35.5 + 14.0
+ 2(16.0)] = 0.00200 g
(d)(i) R–CONH2 + Br2 R–CONHBr + HBr
(ii) +1
(iii) 8 electrons (2 inner electrons and 6 valence electrons)
(iv) The other product is CO32–
. R–N=C=O + 2OH– R–NH2 + CO3
2–
(e) V: FeBr3/Br2, room temperature
VI: KMnO4(aq)/H2SO4(aq), heat
VII: PCl5, room temperature
VIII: NH3, room temperature
C: 4-bromobenzoic acid
D: 4-bromobenzamide
2 (a)(i) Mr = (0.562 × 8.31 × 298) / (1.00 × 105 × 386 × 10
–6) = 36.1
(ii) carbon dioxide
(iii) Mr = 2(36.1 – 44/2) = 28.2 carbon monoxide
(iv) E: CaC2O4 CaC2O4 CaO + CO + CO2
(b)(i) HO2CCH2CO2– has an electron-withdrawing –CH2CO2H which disperses
the negative charge, in addition to resonance stability (electron
delocalisation) of the carboxylate ion, making it more stable than the
ethanoate ion (which only has resonance stability).
(ii) –O2CCH2CO2
– is more negatively charged (2–) compared to ethanoate ion
(1–), which makes it more likely to accept a proton back to form
HO2CH2CO2–.
(iii) [H+]2 = K1[HA] = (10
–2.85)(0.10) = 0.000141 mol
2 dm
–6
pH = –log10[H+] = 1.93
(iv) Key features of titration curve sketch:
Initial pH = 1.93 at 0 cm3 (as calculated in part (iii))
pH at MBC1 = pK1 = 2.85 at 5 cm3 ([HO2CCH2CO2
–] = [HO2CCH2CO2H])
pH at 1st equiv. point = 0.5 log10(10–5.70
)(0.050) = 3.50 at 10 cm3
pH at MBC2 = pK2 = 5.70 at 15 cm
3 ([HO2CCH2CO2
–] = [
–O2CCH2CO2
–])
pH at 2nd equiv. point = 14 + 0.5 log10(10–8.30
)(0.0333) = 9.11 at 20 cm3
pH beyond 2nd equiv. point = 14 + log10(0.001/0.04) = 12.40 at 30 cm3
(c)(i) F: O=C=C=C=O linear with respect to all atoms
(ii) NH3(g): H2NOCCH2CONH2
HCl(g): ClOCCH2COCl
(d) BrCH2CH2Br HO2C–CO2H
1. NaOH(aq), heat
2. K2Cr2O7(aq)/H2SO4(aq), heat
BrCH2CH2Br HO2C–CH2CH2–CO2H
1. ethanolic KCN, heat
2. H2SO4(aq), heat
3 (a)(i) [Ca2+
] = 0.0080/40.1= 2.00 × 10–4
mol dm–3
[Mg2+
] = 0.0049/24.3 = 2.00 × 10–4
mol dm–3
[Cl–] = 0.0071/35.5 = 2.00 × 10
–4 mol dm
–3
[HCO3–] = 0.0366 / [1.0 + 12.0 + 3(16.0)] = 6.00 × 10
–4 mol dm
–3
CaCl2 : MgCl2 : Ca(HCO3)2 : Mg(HCO3)2 = 1 : 1 : 3 : 3
(ii) calcium carbonate
When the sample was partially evaporated, [HCO3–] increased. This
caused the position of the equilibrium CO2(g) + H2O(l) + CO32–
(aq)
2HCO3–(aq) to shift to the left, forming more CO3
2–. Since CaCO3 is more
insoluble than MgCO3, the Ksp value for CaCO3 is smaller than that for
MgCO3. The increased [CO32–
] caused the ionic product [Ca2+
][CO32–
] to
increase to a value more than Ksp(CaCO3) first, with [Mg2+
][CO32–
]
remaining less than Ksp(MgCO3). Thus, CaCO3 is precipitated first.
(iii) The rock is probably made up of calcium carbonate and magnesium
carbonate. Rainwater contains dissolved carbon dioxide and the following
equilibrium is established:
CO2(g) + H2O(l) + CO32–
(aq) 2HCO3–(aq)
When rainwater percolates through the rock, carbon dioxide reacts with
some of the dissolved CO32–
from the partial dissolution of calcium and
magnesium carbonates to form HCO3– as present in the mineral water.
The decrease in concentration of CO32–
causes the position of the next
equilibrium
MCO3(s) M2+
(aq) + CO32–
(aq) where M = Ca or Mg
to shift to the right, enabling more carbonate to dissolve to produce the
metal cations present in the mineral water.
(b)(i) 6Ca5(PO4)3F + SiO2 + H2O SiF4 + 2HF + 3CaO + 9Ca3(PO4)2
(ii) Ksp = [Ca2+
]3[PO4
3–]2 units: mol
5 dm
–15
(iii) 1 × 10–26
= (3x)3(2x)
2 = 108x
5
[Ca2+
] = 3x = 3(2.47 × 10–6
) = 7.42 × 10–6
mol dm–3
(c)(i) PCl3 can be made by refluxing chlorine with phosphorus, with continuous
removal of PCl3 as it is formed.
PCl5 can be made by reacting PCl3 further with excess chlorine.
(ii) G: POCl3 tetrahedral with respect to central P
(iii) H: sulfur dioxide
PCl3 + SO3 POCl3 + SO2
PCl5 + H2O POCl3 + 2HCl
4 (a) The secondary structure of proteins is the arrangement of a polypeptide
chain in space around a single axis. It is formed and stabilised by the
interactions of amino acids that are fairly close to one another on the
polypeptide chain, through hydrogen bonding between C=O group of one
peptide and N-H group of another.
The tertiary structure of proteins refers to the way in which the polypeptide
with its primary and secondary structures can be organised in space to
form a more complex polypeptide configuration through the formation of
interactions between the R-groups of the amino acids, such as hydrogen
bonding, disulfide bridges, van der Waals’ forces and ionic linkages.
The quaternary structure of proteins consists of more than one
polypeptide chain coming together to form the complete protein
maintained by the same forces which are responsible for tertiary structure.
(b) ΔG should be negative because the reaction is spontaneous.
ΔH should be negative due to the formation of various interactions (e.g.
hydrogen bonding, disulfide bridges, van der Waals’ forces and ionic
linkages) between the R-groups of the constituent amino acids, which is
an exothermic process.
ΔS should be negative due to the coalescence of a more ordered
haemoglobin molecule, which reduces the number of ways in which the
energy can be distributed.
(c)(i) Fe2+
: [Ar] 3d6
Fe2+
has incompletely filled d-orbitals. In an octahedral environment, the
d-orbitals are split into two energy levels. When white light shines, the
electron in a d-orbital of the lower energy level will absorb a quantum of
light and jump to one of the partially filled d-orbitals of higher energy. The
energy gap E between the two levels corresponds to a range of
wavelengths in the visible spectrum. The red colour observed is the
complementary colour of the light absorbed during this d-d transition.
(ii)
‘high spin’ state ‘low spin’ state
(iii) Electrons prefer to occupy orbitals singly to minimise inter-electronic
repulsion.
(iv) Oxyhaemoglobin (‘low spin’ state) will contain the larger energy gap, E,
between its d-orbitals.
Where the energy gap is larger, the energy required to overcome the
energy gap, E, in adding subsequent electrons to the higher energy d-
orbitals is more than that required to overcome inter-electronic repulsion in
adding electrons to the partially filled lower energy d-orbitals. Thus, the
lower energy d-orbitals are filled first, before higher energy d-orbitals are
used (i.e. ‘low spin’ state).
Conversely, where the energy gap is smaller, the energy required to
overcome E in adding subsequent electrons to the higher energy d-
orbitals is less than that required to overcome inter-electronic repulsion in
adding electrons to the partially filled lower energy d-orbitals. Thus, the
electrons occupy all the d-orbitals singly, before pairing up in the lower
energy d-orbitals (i.e. ‘high spin’ state).
(d)(i) Acidic/alkaline conditions, heat.
H+/OH
– acts as a catalyst during hydrolysis.
(ii) met-asp-gly-ser-ala-gly-glu-ser-lys-tyr
5 (a) Acidity increases from ethanol to water to phenol.
The electron-donating ethyl group in ethanol intensifies the negative
charge on the ethoxide ion, compared to hydroxide (from water). This
destabilises the ethoxide ion, making ethanol a weaker acid than water.
The p-orbital of oxygen overlaps with the π-electron cloud of the benzene
ring. The negative charge on oxygen is delocalised into the benzene ring.
This dispersion of charge stabilises the phenoxide ion, making phenol a
stronger acid than water.
(b) dilute nitric acid, room temperature
(c) 4-nitrophenol is likely to be more acidic than phenol due to the presence of
the electron-withdrawing –NO2 group on the para-position which further
disperses the charge, stabilising the 4-nitrophenoxide ion even further.
(d)(i) I: Sn, concentrated HCl, heat; then NaOH(aq), room temperature
II: excess NaOH(aq), room temperature
IV: CH3COCl, room temperature
(ii) I: reduction
II: deprotonation / acid-base / neutralisation
III: nucleophilic (aliphatic) substitution (bimolecular)
IV: nucleophilic (acyl) substitution
(iii) To make it a better nucleophile
(e) Cl2(aq), room temperature
(f)(i) 3Cl2 + 6NaOH NaClO3 + 5NaCl + 3H2O
(ii) n(Fe2+
) = 11.3 × 10–3 × 0.500 = 0.00565 mol
ClOx– + 2xH
+ + 2xe Cl
– + xH2O
Mole ratio of ClOx– : e = 1 : 2x
0.150 / (39.1 + 35.5 + 16.0x) = 0.00565 / 2x x = 2
KClO2 + 4Fe2+
+ 4H+ KCl + 4Fe
3+ + 2H2O