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Solids, Liquids, Energy & Heat. Intermolecular Forces “Inter” => between “molecular” => molecules Intermolecular forces apply only to covalent bonds.

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Presentation on theme: "Solids, Liquids, Energy & Heat. Intermolecular Forces “Inter” => between “molecular” => molecules Intermolecular forces apply only to covalent bonds."— Presentation transcript:

1 Solids, Liquids, Energy & Heat

2 Intermolecular Forces “Inter” => between “molecular” => molecules Intermolecular forces apply only to covalent bonds

3 Intermolecular Forces vs. Intramolecular Forces Intermolecular Forces Intramolecular Forces Intermolecular forces are between neighboring molecules Weaker than intramolecular forces Types: London dispersion forces dipole-dipole forces hydrogen bonding Intramolecular forces are within one molecule a.k.a. Bonding Stronger than intermolecular forces Types: Ionic Bonding Covalent Bonding

4 Intermolecular Forces Intermolecular forces vary in strength and properties: Hydrogen bonds Dipole-dipole London dispersion bond strength incr. properties incr. Boiling point, melting point, surface tension, and viscosity and

5 London Dispersion Forces (van der Waals Forces) Very weak forces Occurs when an electron cloud temporarily gets distorted and forms a temporary positive and negative charge. The ONLY forces of attraction that exist between nonpolar molecules (e.g. Ar, C 8 H 18 )

6 London Dispersion Forces

7 Dipole-Dipole Attraction Polar molecules that orient themselves so that + and – ends of the dipoles are close to each other.

8 Hydrogen Bonding Strongest dipole-dipole attraction when hydrogen is bound with either: N, O, F. Molecule would contain –NH, -OH, or -FH

9 Hydrogen Bonding in DNA

10 Steps to Determine Intermolecular Forces 1) Draw & determine the VSEPR Shape for each molecule: I 2 H 2 SeNH 3 II Se H H NHH H linear bent pyramid

11 2) Determine if each molecule is a polar or non- polar structure: Options: (a) There are no polar bonds  non-polar structure (b) Every polar bond has an opposite (no lone pairs on center)  non-polar structure (c) Not every polar bond has an opposite (lone pairs on center)  polar structure I 2 H 2 SeNH 3 non-polar polar II Se H H NHH H

12 3) Determine the type of intermolecular force for each molecule: Options: (a) non-polar structure  London dispersion forces (b) polar structure with H-O, H-N, or H-F bond(s)  hydrogen bonding (c) polar structure without H-O, H-N, or H-F bond(s)  dipole-dipole forces I 2 H 2 SeNH 3 London dispersion forces dipole-dipole forces hydrogen bonding

13 Energy * + & - indicate whether the heat is flowing into or out of the system* Energy is the capacity to do work. Energy allows us to “do things”, such as drive, cook eggs, and read the words on this page. Often energy is used to change the temperature of a substance. When you change the temperature of a substance, you are reflecting the random motion of the molecules. There are two common units of energy – the calorie and the joule.

14 A calorie (cal) is defined as the amount of energy required to raise the temperature of one gram of water by 1  C. The joule (J) is the unit of energy in the SI System. 1 calorie = 4.184 J Example – Express 22.4 cal of energy in joules. 1 kcal = 1000 cal1 kJ = 1000 J 22.4 cal X _________________ cal J 1 4.184 = 93.7 J

15 The amount of energy required to raise the temperature of a substance depends on three things: 1. amount of substance (mass) 2. the amount of the temperature change 3. type or identity of the substance Different substances respond to heat differently – 4.184 J raises 1 g of water - 1  C BUT 4.184 J raises gold 32  C Specific Heat Capacity – the amount of energy required to change the temperature of one gram of a substance by 1  C

16 Formula to calculate energy requirements- Q = (s)(m)(  T) Q = energy required, J s = specific heat capacity, J/g  C m = mass of substance, g  T = change in temperature,  C  T = T final - T initial Include: Given, formula, setup, answer, SF, units

17 Specific Heat, Heat of Fusion, and Heat of Vaporization of Some Selected Substances SubstanceSpecific Heat (J/g°C) Heat of Fusion ΔH fus ( J/g) Heat of Vaporization ΔH vap ( J/g) alcohol - ethanol2.51109879 aluminum0.90039510800 benzene1.42126548 chloroform0.97179.5264 copper0.3852055310 ice2.093342260 iron0.4602677450 lead0.13024.7946 magnesium1.023726070 mercury0.13811.3285 steam2.023342260 water4.1843342260 gold0.13063.01580 silver0.2401112360

18 Ex. – A 5.63 g sample of solid copper is heated from 21  C to 32  C. How much energy in joules is required? m = 5.63 g  T = T f – T i  T = 32  C - 21  C = 11  C Q = ? s = 0.385 J/g  C Q = s m  T Q = (0.385 J/g  C) (5.63 g) (11  C ) Q = 24 J

19 Example – A 2.8 g sample of pure metal requires 10.1 J of energy to change its temperature from 21  C to 36  C. What is the metal? m = 2.8 g Q = 10.1 J  T = T f – T i  T = 36  C - 21  C = 15  C s = ? s = __Q__ m  T s = ___10.1 J___ (2.8 g)(15  C) s = 0.24 J/g  C Look on chart Silver

20 Heating Curve for Water

21 When a substance melts or boils, there is no change in temperature (no ∆T). Heat of Fusion (∆H fus ) is the amount of energy required to melt a substance Heat of Vaporization (∆H fus ) is the amount of energy required to boil a substance The formulas to use are: For melting or freezing, Q=m∆H fus For boiling or condensing, Q=m∆H vap

22 Molar Heat of Fusion and Molar Heat of Vaporization have units of J/mol Heat of Fusion, Heat of Vaporization, and Specific Heat capacity are characteristic properties and can be used to identify a substance. Ex. How much energy is required to melt 8.93 moles of gold with no change in temperature? Ex. How much energy is absorbed when 5.34 g of chloroform condenses from a gas? m = 8.93 mol Au  H fus Au = q=m∆H fus q = (1760 g)(63.0 J/g) q = 111000 J x _________ g Au 1 196.97 mol Au 63.0 J/g = 1760 g Au m = 5.34 g  H vap chloroform = q=m∆H vap q = (5.34 g)(264 J/g) q = 1410 J 264 J/g

23 Enthalpy (H) – Heat of reaction -  H = exothermic reaction - heat flows out of the system +  H = endothermic reaction - heat flows into the system feels hot or gives off light feels cold

24 Entropy (S) – Disorder Second law of thermodynamics - the entropy of the universe is always increasing Solid  liquid  gas Ordered  disordered Also: # of moles and number of bonds

25 Ex: Which of the following has more entropy? a.solid or gaseous phosphorus b.KBr (s) or KBr (aq) c.CH 4 (g) or C 3 H 8 (g)

26 Ex: Does entropy increase or decrease for each of the following reactions? a.(NH 4 ) 2 Cr 2 O 7 (s)  Cr 2 O 3 (s) + 4 H 2 O (l) + N 2 (g) b. Mg(OH) 2 (s)  MgO (s) + H 2 O (g) c. PCl 3 (g) + Cl 2 (g)  PCl 5 (g) INCREASE DECREASE

27 Phase Diagram Triple point is the temperature and pressure at which all three phases can exist in equilibrium. Above the critical point, molecules are unable to liquefy.

28 Phase Changes: Melting Freezing Boiling Condensing Sublimation Deposition Normal Boiling Point: Normal Freezing Point the temperature at which a liquid boils at 1 atmosphere of pressure. the temperature at which a liquid freezes at 1 atmosphere of pressure. solid  liquid liquid  solid liquid  gas gas  liquid solid  gas gas  solid


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