chem 161 chapter 1: matter, energy, and the origins of the universe problems: 1.1-1.10, 1.14-1.22,...

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Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

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Page 1: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Chem 161Chapter 1: Matter, Energy,

and the Origins of the Universe

Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Page 2: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Chapter 1: Matter, Energy, and the Origins of the

Universe• Science: study of nature that results in a

logical explanation of the observations

• Chemistry: study of matter, its properties, and the changes it undergoes

• In what fields is chemistry used today? How is it used? 

Page 3: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

1.2 Matter: An Atomic View• We study matter at different levels:

– macroscopic: the level which we can observe with the naked eye (geologists study rocks at the macroscopic level)

– microscopic: the level which we can observe using a microscope (scientists study tiny animals, plants, or crystals at the microscopic level)

– atomic or molecular (also called particulate): • at the level of atoms and molecules• can only be “observed” using the most

powerful microscopes• most atoms and molecules are a few

nanometers in size The term “nanotechnology” refers to materials created or developed by manipulating atoms and/or molecules

Page 4: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96
Page 5: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

1.1 Classes of Matter• matter: anything that has

mass and occupies volume

• Types of matter we deal with:– pure substances

(elements & compounds): a single chemical consisting of only one kind of matter

– mixtures (homogeneous & heterogeneous): Two or more pure substances can combine to form mixtures

Page 6: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Pure Substances• Two types of pure substances:

– elements:• consist of only one type of atom• atoms cannot be broken down into smaller

components by chemical reaction– Examples: copper wire (Cu), sulfur powder

(S8), sodium (Na), barium (Ba), hydrogen gas (H2), oxygen gas (O2), and chlorine gas (Cl2).

– compounds:• consist of more than one type of atom and have

a specific chemical formula– Examples include hydrogen chloride (HCl),

water (H2O), sodium chloride (NaCl) [table salt], barium chloride (BaCl2)

Page 7: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Mixtures• Two or more pure substances can combine

to form mixtures.– mixtures:

• consist of many compounds and/or elements, with no specific formula

• matter having variable composition with definite or varying properties can be separated into component elements and/or compounds

• Examples: Any alloy like brass, steel, 10-K to 18-K gold (anything less than 24K gold); course mixtures like sea water, carbonated soda; air is a mixture consisting of nitrogen (~78%), oxygen (21%), and other trace gases.

Page 8: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Mixtures

• Mixtures can be homogeneous or heterogeneous:– Homogeneous mixtures have a

uniform appearance and composition. • e.g. solutions (salt water, soda,

etc.), metallic alloys, homogenized milk

– Heterogeneous mixtures do not have a uniform composition• e.g. chocolate chip cookie, coarse

mixture of sand and iron filings, raw (non-homogenized) milk

Page 9: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

1.6 States of Matter• Matter exists in one of three physical states:

solid, liquid, gas– Example 1: A few drops of food coloring is

added to a beaker of water. How would you expect the water to appear after a few minutes? Why?

– Example 2: If you add a drop of food coloring on top of an ice cube, would you expect the same result? Why?

To understand matter, we must recognize how particles behave at the molecular level.

Page 10: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

States of Matter

Page 11: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Gas

• Volume is variable, particles are widely spaced

• Takes the shape of the container because particles are moving– If container volume expands,

particles move apart to fill container

– If container volume decreases, particles move closer together

• Particles are in constant random motion

Page 12: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Liquid

• Fixed (or constant) volume, but shape can change

• Takes the shape of the container because particles are moving

• Particles are packed closely together but move around each other

Page 13: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Solid

• Has definite shape, rigid volume• Particles can only vibrate in

place

Page 14: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Dep

ositio

nGas

Liquid

Solid

Vaporization

Freezing

Changes of State

Melting

Condensation

Su

blim

ati

on

Page 15: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Properties of Matter

• Intensive Properties: properties independent of quantity– Density– Boiling point– Freezing point

• Extensive Properties: properties that depend on quantity– Mass– Volume

Page 16: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Physical and Chemical Properties and Changes

• Physical Properties:– physical state (solid, liquid, gas)– electrical and heat conductivity– color– solubility (amount of solid that dissolves in

liquid)– density– hardness– melting and boiling points– odor

• Chemical Properties: how a substance reacts with other substances– e.g. hydrogen reacts explosively with oxygen

Page 17: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Chemical vs. Physical Changes

Physical Change:• a process that does not alter the chemical

makeup of the starting materials– changing shape, changing physical state,

dissolving– boiling water, melting ice, hammering gold

into foil, dissolving salt in water

Note: In the images here, the chemical makeup of H2O does not change as it goes from a solid to a liquid and to a gas.

Page 18: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Chemical Change:• a process that does changes the chemical

makeup of the starting materials • We can use space-filling models to show what

happens at the molecular-level when H2 and O2 react to form water (H2O) of each molecule.

Notice that the H2O has a different chemical makeup than H2 and O2.

Chemical vs. Physical Changes

Page 19: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

The following examples are all chemical changes that convert the reactants to completely different compounds and/or elements.

Chemical vs. Physical Changes

release of gas bubbles(fizzing)

formation of insoluble solid (precipitation) oxidation of matter

(burning or rusting)

Page 20: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Example Problem 1Consider the following molecular-level representations of different substances:

A B C

D F

E

For each figure above, indicate if it represents an element, a compound, or a mixture AND if it represents a solid, liquid, or gas.

Page 21: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Example Problem 2Match the following substances with the correct molecular-level representation.

_____ ammonia (NH3) _____ air _____hydrogen_____ sodium chloride _____ mercury _____ copper

A B C

D F

E

Page 22: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Example Problem 3

Which of the following are chemical changes?

burning condensing dissolving

melting vaporizing rusting

Page 23: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Making Measurements and Expressing Results

Accuracy vs. Precision• accuracy: indicates how close a

measurement is to the true value• precision: refers to how closely two or more

measurements agree with one another

For each diagram (above), what is the level of accuracy and precision?

accurate inaccurate precise imprecise

Page 24: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

Testing a Hypothesis – The Big Bang Revisited

• In the 1960s, the US launched the first communication satellites, called Echo and Telstar, which were basically reflective spheres that bounced microwave signals from transmitters to receivers back on Earth.

• Bell Labs in NJ had built an antenna to receive such signals, and two Bell Lab scientists, Robert W. Wilson and Arno A. Penzias, were trying to improve the antenna’s reception.

• But they kept picking up a background signal, no matter where they directed the antenna.

Page 25: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

• Assuming the signal was just an artifact, even attributing it to pigeons roosting on the antenna, the pair continued testing the equipment until they finally realized their original hypothesis must have been wrong, that the nuisance signal was not an artifact but actually significant.

Testing a Hypothesis – The Big Bang Revisited

Page 26: Chem 161 Chapter 1: Matter, Energy, and the Origins of the Universe Problems: 1.1-1.10, 1.14-1.22, 1.24-1.93, 1.96

• Wilson and Penzias learned that a Princeton University physicist named Robert Dicke had predicted residual energy left over from the Big Bang.

• Their nuisance signal matched Professor Dicke’s predicted Big Bang microwave echo Wilson and Penzias shared the Nobel Prize in Physics in 1978 for discovering the cosmic microwave background radiation of the universe.

Testing a Hypothesis – The Big Bang Revisited