Matter and It's Changes Quiz
Chemistry is the study of
The structure and composition of matter
The changes that occur in this composition of matter
The mechanisms that bring about these changes
Different Kinds of Chemistry
Biochemistry: living things
Organic chemistry: carbon containing compounds
Inorganic chemistry: non carbon containing compounds (metals)
Physical chemistry: chemistry and energy
Analytical chemistry: the chemistry of unknowns (forensic chemistry)
Nuclear chemistry: chemistry of the nucleus
Matter: anything that has mass and occupies space
States of Matter
Solid: has a definite volume, definite shape
Liquid: has a definite volume, no definite shape
Gas: has neither a definite volume or definite shape
Plasma: high temperature and energy state wherein most atoms now have charges
Theory: an explanation of how/why something occurs based on a wide body of evidence which is not yet disproven
Law: an observation that tells you what happens, but not the why, and is also not yet disproven
The Kinetic Theory of Matter
The particles of matter are always in motion and this motion has consequences
Used to determine the states of matter
Properties of Matter
Inertia: resistance to change in state of motion
Mass: measure of the quantity of matter = measure with a balance
Weight: measure of Earth’s gravitational attraction = measure with a scale
Types of Properties
Extensive: depends on the amount of matter that is present = dependent on amount
Ex: Mass
Intensive: does not depend on the amount of matter that is present = independent on amount
Ex: Density
Physical Property: characteristic that can be observed or measured without changing the identity of substance
Chemical Property: characteristic that relates to a substance’s ability to undergo changes that transform it into different substances
Physical Change
Reversible process
Identifying properties of the substance remain unchanged
No atoms or molecules are destroyed, but the spacing between them changes
Chemical Change
Can be a reversible or irreversible processes
Different substances with new properties are formed
Atoms and moleules are rearranged
Nuclear Change
Most are irreversible change
Different substances with new properties are formed
Atoms are destroyed and new ones are made
5 Signs of a Chemical Reaction
Production of light
Color Change
Production of a gas
Precipitate is formed - insoluble solid
Production of heat
Reaction = Undergo a Chemical Change
Reactants → Products
In → Out
Before → After
Energy of reactions
Exothermic: process that gives off energy
Endothermic: process that absorbs energy
Chemical: any substance that has a definite composition (synonym - substance)
3 Other Classes of Matter
Mixtures: a material consisting of 2 or more kinds of matter, each retaining its own characteristic properties
Heterogeneous
Different from point to point
Matter that has parts with different properties
Homogeneous
Same from point to point
Matter that has similar properties throughout
Pure Substances
Elements
A substance that cannot be further decomposed
Compounds
A substance that may be decomposed into 2 or more simpler substances
Mixture vs. Compound
Mixture
Components may be present in any proportion
Components do not lose their “identity”
Components can be separated by physical means
In preparation there is no evidence of a chemical reaction taking place
Compounds and Elements
Components always have a definite proportion (can’t change the ingredient amounts)
Components lose their identity
Components can be separated by chemical means
In preparation evidence of a chemical reaction is usually apparent
Has a chemical a formula NaCl, H20, C12H22O11
Element Symbols
1st letter = always capitalized, usually 1st letter of name
2nd letter = never capitalized
All element symbols come from the Latin version of the element name
The States of Elements at Room Temperature
Color of symbol tells state
Black = solid
Blue = liquid
Red = gas
Outline = manmade
The Nucleus
Comprised of the 2 nucleons
Protons
Neutrons
Isotopes
Not all atoms of the same element have the same mass due to different numbers of neutrons in those atoms
Radioactivity
Some nuclides of an element may be unstable, or radioactive
Referred to as radioisotopes
Types of Radioactive Decay
2 Main Types
Nuclear Fission
Splitting apart of nuclei
Results in two smaller atoms
Does not normally occur in nature
Takes little energy to split -- releases energy 1,000,000 times greater than a chemical reaction (lower than nuclear fusion)
Ex: Atomic Bomb
Nuclear Fusion
Joining together of nuclei
Results in larger atoms
Often needs a “trigger” to start process -- requires a lot of energy and high temperature
Energy released 3-4 times larger than fission (so about 4,000,000 times that of a chemical reaction)
Ex: the Sun, Hydrogen bombs
Alpha Decay: The loss of an a-particle (a helium nucleus)
Beta Decay: The loss of a B-particle (a high energy or fast moving electron)
Positron Emission
Some nuclei decay by emitting a positron, a particle that has the same mass as but an opposite charge to that of an electron
Gamma Emission
Loss of a y-ray, which is high-energy radiation that almost always accompanies the loss of a nuclear particle
Gamma rays are not charged particles like a and B particles
Gamma rays are electromagnetic radiation with high frequency
When atoms decay by emitting a or B particles to form a new atom, the nuclei of the new atom formed may still have too much energy to be completely stable
This excess energy is emitted as gamma rays
Electron Capture
Addition of an electron to a proton in the nucleus
The result of this process is that a proton is transformed into a neutron
Neutron-Proton Ratios
Any element with more than one proton (i.e., anything but hydrogen) will have repulsions between the protons in the nucleus
A strong nuclear force helps keep the nucleus from flying apart
Neutrons play a key role in stabilizing the nucleus (more neutrons = more strong force)
Therefore, the ratio of neutrons to protons is an important factor
For smaller nuclei (#protons <= 20) stable nuclei have a neutron-to-proton ratio close to 1:1
As nuclei get larger, it takes a greater number of neutrons to stabilize the nucleus
Stable Nuclei
There are no stable nuclei with an atomic number greater than 83
Nuclei with such large atomic numbers tend to decay by alpha emission
Half-Life
The time it takes for half of your isotope to decay into another element
Electrons in Atoms
Electrons can only orbit the nucleus in specific, allowed pathways
They move toward and away from the nucleus by “steps” or discrete amounts of energy that are released or absorbed
Electrons farther from the nucleus have more energy. Those closer to the nucleus have less energy
Ground State: lowest energy state
This means that electrons are found in shells closer to the nucleus
Excited State: higher potential energy of an atom
A form of heat, light, electrical or mechanical energy is needed to go from the ground to an excited state
As electrons increase in energy, they move away from the nucleus and into outer shells
Absorption: moves electrons from a ground state to a higher energy state
Emission: lets electrons fall back down to a lower energy state
Usually light
The kind of light emitted by each element is unique because each element has a unique arrangement of electrons
Carbon footprint is the summation of all emissions, as a result of activities
Ex: the fuel burned by cars or buses to get to school
Chemicals in carbon, such as carbon dioxide, are harmful
Should be taken seriously because of its effect on the temperature.
Energy comes from the sun
Solar power/sunlight can be converted into electricity
The Sun influences all forms of energy like coal and other renewable sources
The Sun also influences things like heat, wind, and plants
Elements in the Sun
Predominant one is Hydrogen
Small amount of Helium is present, with traces of other elements
Life cycle of a star
Formation of stars occurs as a result of gravitational centers with nebulas that draw minerals together
Hydrogen in stars (the fuel) can run out, and they collapse → explosion by increasing temperature and presure, counteracting gravity
Larger stars have shorter lifespans because of their mass
Death of stars
Different deaths can occur due to their shape and size
Occurs due to the exhaustion of reactants/fission energy
Normal stars become white dwarfs
Large stars turn into black holes or nebulas
Particles found in the center of the atom: Protons and neutrons
Neutral atoms have the same number of protons and electrons
Positive ions have more protons than electrons
Negative ions have less protons than electrons
The ratio of protons to electrons is based on the charge of the atom
The rule for determining the mass number of an atom or ion is protons and neutrons that are present in the nucleus
Element symbol is determined by the number of protons
The letters representing the chemical element
Charge is determined by the protons and electrons
The value difference between protons and electrons
Atomic number is determined by the number of protons
Mass number is determined by the protons and netrons
Isotopes
Protons and neutrons affect the stability of the atom
Electrons do not affect the stability of the atom
Requirements for 2 atoms to be isotopoes of each other
They have to have the same number of protons but a different number of neutrons
They need to have the same charge
Similarities/Differences between an atom, ion, and isotope
They have the same number of protons
Isotopes have a different amount of neutrons
Ions have a different amount of electrons
Order of the Periodic Table
Column (verticle) = Group or Family
Alkali Metals
Alkaline Earth Metals
Transition Metals
Boron Family
Carbon Family
Nictides (Nitrogen Family)
Chalcogens (Oxygen Family)
Halogens
Noble Gases
Row (horizontal) = Period or Series
Actinide
Lanthanide
Metals/Mettaloids/Nonmetals
Left
Zigzag
Right
Matter and It's Changes Quiz
Chemistry is the study of
The structure and composition of matter
The changes that occur in this composition of matter
The mechanisms that bring about these changes
Different Kinds of Chemistry
Biochemistry: living things
Organic chemistry: carbon containing compounds
Inorganic chemistry: non carbon containing compounds (metals)
Physical chemistry: chemistry and energy
Analytical chemistry: the chemistry of unknowns (forensic chemistry)
Nuclear chemistry: chemistry of the nucleus
Matter: anything that has mass and occupies space
States of Matter
Solid: has a definite volume, definite shape
Liquid: has a definite volume, no definite shape
Gas: has neither a definite volume or definite shape
Plasma: high temperature and energy state wherein most atoms now have charges
Theory: an explanation of how/why something occurs based on a wide body of evidence which is not yet disproven
Law: an observation that tells you what happens, but not the why, and is also not yet disproven
The Kinetic Theory of Matter
The particles of matter are always in motion and this motion has consequences
Used to determine the states of matter
Properties of Matter
Inertia: resistance to change in state of motion
Mass: measure of the quantity of matter = measure with a balance
Weight: measure of Earth’s gravitational attraction = measure with a scale
Types of Properties
Extensive: depends on the amount of matter that is present = dependent on amount
Ex: Mass
Intensive: does not depend on the amount of matter that is present = independent on amount
Ex: Density
Physical Property: characteristic that can be observed or measured without changing the identity of substance
Chemical Property: characteristic that relates to a substance’s ability to undergo changes that transform it into different substances
Physical Change
Reversible process
Identifying properties of the substance remain unchanged
No atoms or molecules are destroyed, but the spacing between them changes
Chemical Change
Can be a reversible or irreversible processes
Different substances with new properties are formed
Atoms and moleules are rearranged
Nuclear Change
Most are irreversible change
Different substances with new properties are formed
Atoms are destroyed and new ones are made
5 Signs of a Chemical Reaction
Production of light
Color Change
Production of a gas
Precipitate is formed - insoluble solid
Production of heat
Reaction = Undergo a Chemical Change
Reactants → Products
In → Out
Before → After
Energy of reactions
Exothermic: process that gives off energy
Endothermic: process that absorbs energy
Chemical: any substance that has a definite composition (synonym - substance)
3 Other Classes of Matter
Mixtures: a material consisting of 2 or more kinds of matter, each retaining its own characteristic properties
Heterogeneous
Different from point to point
Matter that has parts with different properties
Homogeneous
Same from point to point
Matter that has similar properties throughout
Pure Substances
Elements
A substance that cannot be further decomposed
Compounds
A substance that may be decomposed into 2 or more simpler substances
Mixture vs. Compound
Mixture
Components may be present in any proportion
Components do not lose their “identity”
Components can be separated by physical means
In preparation there is no evidence of a chemical reaction taking place
Compounds and Elements
Components always have a definite proportion (can’t change the ingredient amounts)
Components lose their identity
Components can be separated by chemical means
In preparation evidence of a chemical reaction is usually apparent
Has a chemical a formula NaCl, H20, C12H22O11
Element Symbols
1st letter = always capitalized, usually 1st letter of name
2nd letter = never capitalized
All element symbols come from the Latin version of the element name
The States of Elements at Room Temperature
Color of symbol tells state
Black = solid
Blue = liquid
Red = gas
Outline = manmade
The Nucleus
Comprised of the 2 nucleons
Protons
Neutrons
Isotopes
Not all atoms of the same element have the same mass due to different numbers of neutrons in those atoms
Radioactivity
Some nuclides of an element may be unstable, or radioactive
Referred to as radioisotopes
Types of Radioactive Decay
2 Main Types
Nuclear Fission
Splitting apart of nuclei
Results in two smaller atoms
Does not normally occur in nature
Takes little energy to split -- releases energy 1,000,000 times greater than a chemical reaction (lower than nuclear fusion)
Ex: Atomic Bomb
Nuclear Fusion
Joining together of nuclei
Results in larger atoms
Often needs a “trigger” to start process -- requires a lot of energy and high temperature
Energy released 3-4 times larger than fission (so about 4,000,000 times that of a chemical reaction)
Ex: the Sun, Hydrogen bombs
Alpha Decay: The loss of an a-particle (a helium nucleus)
Beta Decay: The loss of a B-particle (a high energy or fast moving electron)
Positron Emission
Some nuclei decay by emitting a positron, a particle that has the same mass as but an opposite charge to that of an electron
Gamma Emission
Loss of a y-ray, which is high-energy radiation that almost always accompanies the loss of a nuclear particle
Gamma rays are not charged particles like a and B particles
Gamma rays are electromagnetic radiation with high frequency
When atoms decay by emitting a or B particles to form a new atom, the nuclei of the new atom formed may still have too much energy to be completely stable
This excess energy is emitted as gamma rays
Electron Capture
Addition of an electron to a proton in the nucleus
The result of this process is that a proton is transformed into a neutron
Neutron-Proton Ratios
Any element with more than one proton (i.e., anything but hydrogen) will have repulsions between the protons in the nucleus
A strong nuclear force helps keep the nucleus from flying apart
Neutrons play a key role in stabilizing the nucleus (more neutrons = more strong force)
Therefore, the ratio of neutrons to protons is an important factor
For smaller nuclei (#protons <= 20) stable nuclei have a neutron-to-proton ratio close to 1:1
As nuclei get larger, it takes a greater number of neutrons to stabilize the nucleus
Stable Nuclei
There are no stable nuclei with an atomic number greater than 83
Nuclei with such large atomic numbers tend to decay by alpha emission
Half-Life
The time it takes for half of your isotope to decay into another element
Electrons in Atoms
Electrons can only orbit the nucleus in specific, allowed pathways
They move toward and away from the nucleus by “steps” or discrete amounts of energy that are released or absorbed
Electrons farther from the nucleus have more energy. Those closer to the nucleus have less energy
Ground State: lowest energy state
This means that electrons are found in shells closer to the nucleus
Excited State: higher potential energy of an atom
A form of heat, light, electrical or mechanical energy is needed to go from the ground to an excited state
As electrons increase in energy, they move away from the nucleus and into outer shells
Absorption: moves electrons from a ground state to a higher energy state
Emission: lets electrons fall back down to a lower energy state
Usually light
The kind of light emitted by each element is unique because each element has a unique arrangement of electrons
Carbon footprint is the summation of all emissions, as a result of activities
Ex: the fuel burned by cars or buses to get to school
Chemicals in carbon, such as carbon dioxide, are harmful
Should be taken seriously because of its effect on the temperature.
Energy comes from the sun
Solar power/sunlight can be converted into electricity
The Sun influences all forms of energy like coal and other renewable sources
The Sun also influences things like heat, wind, and plants
Elements in the Sun
Predominant one is Hydrogen
Small amount of Helium is present, with traces of other elements
Life cycle of a star
Formation of stars occurs as a result of gravitational centers with nebulas that draw minerals together
Hydrogen in stars (the fuel) can run out, and they collapse → explosion by increasing temperature and presure, counteracting gravity
Larger stars have shorter lifespans because of their mass
Death of stars
Different deaths can occur due to their shape and size
Occurs due to the exhaustion of reactants/fission energy
Normal stars become white dwarfs
Large stars turn into black holes or nebulas
Particles found in the center of the atom: Protons and neutrons
Neutral atoms have the same number of protons and electrons
Positive ions have more protons than electrons
Negative ions have less protons than electrons
The ratio of protons to electrons is based on the charge of the atom
The rule for determining the mass number of an atom or ion is protons and neutrons that are present in the nucleus
Element symbol is determined by the number of protons
The letters representing the chemical element
Charge is determined by the protons and electrons
The value difference between protons and electrons
Atomic number is determined by the number of protons
Mass number is determined by the protons and netrons
Isotopes
Protons and neutrons affect the stability of the atom
Electrons do not affect the stability of the atom
Requirements for 2 atoms to be isotopoes of each other
They have to have the same number of protons but a different number of neutrons
They need to have the same charge
Similarities/Differences between an atom, ion, and isotope
They have the same number of protons
Isotopes have a different amount of neutrons
Ions have a different amount of electrons
Order of the Periodic Table
Column (verticle) = Group or Family
Alkali Metals
Alkaline Earth Metals
Transition Metals
Boron Family
Carbon Family
Nictides (Nitrogen Family)
Chalcogens (Oxygen Family)
Halogens
Noble Gases
Row (horizontal) = Period or Series
Actinide
Lanthanide
Metals/Mettaloids/Nonmetals
Left
Zigzag
Right