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Changes in Matter Chapter 4.

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Presentation on theme: "Changes in Matter Chapter 4."— Presentation transcript:

1 Changes in Matter Chapter 4

2 Characteristic properties are altered.
Physical Changes -Characteristic properties and the nature of the substance remain unchanged. Ex: snow melting, ripping paper, crushing a can 2. Chemical Changes Bonds between atoms in molecules are rearranged, leading to the formation of new substances. Characteristic properties are altered. Ex: burning wood, cooking an egg, cellular respiration, explosions 3. Nuclear Transformations Protons and neutrons are rearranged inside an atom’s nucleus creating new elements. Ex: Deuterium + tritium  helium

3 Try This!

4 Chemical Changes Signs of a chemical change:
-release of a gas -release or absorption of heat -emission of light -change in colour -formation of a precipitate (residue) Chemical changes are also called chemical reactions. They can be represented in chemical equations. STATE

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6 The Law of Conservation of Mass
Matter cannot be created or destroyed. Mass of the reactants must equal mass of products. Ex: If you react 16 g of H2 to produce 50 g of H2O, how much O2 did you use? 2 H2 +O2  2 H2O ***** DO NOT MULTIPLY MASSES BY THE COEFFICIENTS!!!!! *******

7 Try This! During a chemical reaction 15 g of hydrochloric acid (HCl) reacts with 25 g of aluminum (Al) to produce 29 g of aluminum chloride (AlCl3) and some hydrogen gas (H2) is released. The balanced equation for this reaction is as follows: 6 HCl + 2 Al → 2 AlCl3 + 3 H2 What mass of hydrogen gas was released?

8  See Particle Model Worksheet!
Conservation of Mass Atoms cannot be created or destroyed! Particle Model Atoms: smallest particle of matter Molecule: a group of 2 or more atoms Ex: H2O  this is a molecule composed of 2 hydrogen atoms and 1 oxygen atom. Subscripts tell us how many atoms of each type are in a molecule. H2SO4  2 hydrogen, 1 sulfur, 4 oxygen Coefficients tell us how many molecules there are. 2 CO2  2 carbon dioxide molecules, 2 carbon atoms and 4 oxygen atoms  See Particle Model Worksheet!

9 Using Symbols Examples: H2O AlCl3 H3PO4 2 NO2 3 PO4
Pick a shape to represent each type of atom Use a line to show the bond between the atoms. Examples: H2O AlCl3 H3PO4 2 NO2 3 PO4

10 Balancing Chemical Equations
Rules: Place coefficients in front of reactants or products. DO NOT change subscripts. Coefficients must be whole numbers. Reduce coefficients to lowest possible form. Count atoms of each type on both sides of arrow. Draw pictures if it helps! Example: N2 + H2  NH3 CH4 + O2  CO2 + H2O

11 Stoichiometry Used to determine the number of moles/mass of reactants or products in a chemical reaction. Ex. Calculate the amount of oxygen needed to react completely with 1.00 g of hydrogen in the following equation: 2 H2 + O2  2 H2O Molar Ratio: Mass: MM: mols:

12 Try This! Iron oxide, Fe2O3, reacts with carbon, C, to produce iron, Fe, according to the following balanced equation: Fe2O3 + 3 C → 2 Fe + 3 CO What mass of carbon is required for every 6.0 moles of Fe2O3 reacted?

13 Endothermic and Exothermic Reactions
Endothermic reaction: Chemical reaction where energy (heat) is absorbed. Requires constant source of energy Energy is taken in from the surrounding environment (it can be written as a reactant in a chemical equation). Exothermic reaction: Chemical reaction where energy (heat) is released. Requires energy only to be initiated. Energy released is absorbed by the surrounding environment (it can be written as a product in a chemical reaction)

14 Chemical Bonds Breaking chemical bonds in molecules requires energy.
Forming a chemical bond releases energy. Determining whether a reaction is exothermic or endothermic Calculate the amount of energy required to break the bonds of the reactants. Calculate the amount of energy released by the formation of the new bonds of the products. Step 1 – Step 2

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16 Try This! CH4 + 2 O2  CO2 + 2H2O Step 1: Find the energy needed to break the bonds of the reactants CH4 + 2 O2 (4 x 414 kJ) + (2 x 498 kJ) = 2652 kJ Step 2: Find the energy released by the formation of the new bonds in the products CO2 + 2H2O (2 x 741 kJ) + (2 x 2 x 464 kJ) = 3338 kJ Step 3: Find out whether the overall reaction has taking in or given off heat. Step 1 – Step kJ – 3338 kJ = -686 kJ Because the overall result is negative, this means that the bonds of the products released more energy than the amount that was taken in to break the bonds of the reactants.  A negative result indicated an exothermic reaction.

17 Try This! Calculate the reaction energy for the electrolysis of water. Determine whether it is an endothermic or exothermic reaction. 2 H2O  2 H2 + O2

18 Reaction Energy

19 Endothermic vs. Exothermic Reaction Energy Diagrams

20 Calculating Reaction Energy using Stoichiometry
Determine the reaction energy if 32g of methane react with sufficient oxygen using the equation below: CH4 + 2 O2  CO2 + 2 H2O kJ

21 Types of Chemical Change
Acid-Base Neutralization We can neutralize an acid with a base and vice versa. A neutralization reaction always produces water and a salt. Acid (aq) + Base (aq)  Water (l) + Salt (aq) Reminder: How can you identify an acid, base, salt and water by the molecular formula? How does it work? The H+ ions from the acid and the OH- ions from the base will join together to form H2O (water). The remaining metal from the base and the non-metal from the acid will join together to form the salt.

22 Try This! How do we recognize a neutralization reaction?
Are the following equations balanced? HCl + NaOH  H2O + NaCl HF + KOH  H2O + KF H2SO4 + Mg(OH)2  2 H2O + MgSO4 2 HBr + Ca(OH)2  2 H2O + CaBr2

23 2. Combustion Reaction requiring oxygen (oxidation reaction) that releases energy Products are always CO2, H2O and Energy Ex: wood burning, iron rusting, cellular respiration Fuel + O2  CO2 + H2O + Energy There are 3 things necessary for combustion to occur: Oxidizing agent (oxygen) Fuel (wood, gas) Ignition Temperature (heat, spark)

24 Types of Combustion Type 1: Rapid Fast
Releases a lot of heat and light Ex: log fire, burning candle, combustion of gasoline in a car engine Type 2: Spontaneous No energy from an outside source is required Often unpredictable Ex: forest fire Type 3: Slow Occurs over a very long period of time Slow release of energy Ex: rusting, decomposition, fermentation, cellular respiration

25 Sugar + Oxygen  Carbon dioxide + Water + Energy
3. Cellular Respiration Glucose and oxygen react to form carbon dioxide, water and energy. The energy produced allows your cells to work and keeps your body temperature stable. Sugar + Oxygen  Carbon dioxide + Water + Energy C6H12O6 + 6 O2  6 CO2 + 6 H2O + Energy

26 Carbon dioxide + water + energy  glucose + oxygen
4. Photosynthesis Plants use solar energy, carbon dioxide and water to produce glucose and oxygen. Plants produce glucose to feed themselves (producers) and oxygen that we benefit from. Carbon dioxide + water + energy  glucose + oxygen 6 CO2 + 6 H2O + Energy  C6H12O6 + 6 O2

27 Nuclear Transformations
Reactions that occur in the nucleus of an atom. Natural process in which unstable atoms spontaneously transform into more stable atom(s). Energy is released in the form of ionizing radiation. There are 3 types of radiation: Type Charge Symbol Penetrating Ability Alpha + 2 α Stopped by paper Beta -1 β Stopped by foil (at least 3mm) Gamma None γ Stopped by concrete

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29 Nuclear Stability The nucleus of an atom is composed of protons and neutrons. Protons repel each other (like-charges), however the neutrons act like glue keeping the protons together in the nucleus. Most nuclei remain stable because the force of attraction between neutrons and protons (nuclear force) is greater than the electrical repulsion between protons. If the force of repulsion of protons is greater than the nuclear force, the atom is unstable and will decay.

30 The Stability of the Nucleus Depends on:
Size of the atom (all atoms with atomic # greater than 83 are unstable) The larger the atom, the more protons are found in the nucleus. Because of a larger number of protons, it is very difficult to offset the repulsion. 2. The number of neutrons in the atom. (The more neutrons, the more stable the atom as it increases the space between protons, thus reducing repulsion.) Reminder: How do we calculate the number of neutrons an element contains? What is an isotope?

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32 Half-Life The time required for half of the nuclei in a sample of radioactive material to decay. Each substance has a specific half-life. The longer the half-life, the longer it takes to eliminate that element from the environment.

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34 Types of Nuclear Transformation
Nuclear Fission Neutron hits a nucleus of atom which is split to form two lighter nuclei. Neutrons are released which bombard other nuclei (chain reaction). Difficult to control # protons and mass conserved throughout the reaction.

35 2. Nuclear Fusion The principal source of energy in stars (sun). Occurs when 2 small nuclei collide and join to form a heavier one and a neutron is released. Can only occur at extreme temperatures ( one million degrees)


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