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Chemistry: Reactants and Products
Reactants are the starting substances in a chemical reaction, while products are the new substances formed as a result of the reaction.
Law of Conservation of Mass
States that mass is neither created nor destroyed in a chemical reaction; therefore, \text{Total Mass of Reactants} = \text{Total Mass of Products}.
Bohr Models
A diagram representing an atom that shows the nucleus and the arrangement of electrons in specific energy levels or shells surrounding it.
Valence Electrons
The electrons located in the outermost shell of an atom, which determine the element's chemical reactivity and bonding properties.
Ionic Bonding
A type of chemical bond formed through the transfer of electrons from a metal atom to a non-metal atom, resulting in electrostatic attraction between ions.
Covalent Bonds
Chemical bonds formed when two or more non-metal atoms share pairs of valence electrons to achieve a stable electron configuration.
Physics: Position and Time
Position is the location of an object relative to a reference point, while Time is the interval or duration in which a change or motion occurs.
Distance vs. Displacement
Distance: The total length of the path traveled by an object (scalar).
Displacement: The straight-line change in position from the starting point to the ending point, including direction (vector).
Naming Binary Ionic Compounds
Named by writing the name of the metal first, followed by the non-metal with the suffix changed to -ide (e.g., Sodium Chloride).
Molecular Compounds Prefixes
Numerical prefixes used to indicate the number of atoms in a covalent compound:
1: mono-
2: di-
3: tri-
4: tetra-
5: penta-
Valence Electrons
The electrons located in the outermost shell of an atom, which determine the element's chemical reactivity and bonding properties.
Ionic vs. Molecular Compounds
Ionic: Formed by electron transfer between metals and non-metals; usually solids with high melting points.
Molecular (Covalent): Formed by electron sharing between non-metals; can be solids, liquids, or gases with lower melting points.
Covalent Bonds: Single, Double, Triple
Single Bond: Shares 1 pair of electrons.
Double Bond: Shares 2 pairs of electrons.
Triple Bond: Shares 3 pairs of electrons.
Physics: Position and Time
Position is the location of an object relative to a reference point, while Time is the interval or duration in which a change or motion occurs.
Distance vs. Displacement
Distance: The total length of the path traveled by an object (scalar).
Displacement: The straight-line change in position from the starting point to the ending point, including direction (vector).
Speed vs. Velocity
Speed: The rate at which an object covers distance (scalar, v = d/t).
Velocity: Speed in a specific direction (vector, displacement over time).
Acceleration
The rate at which an object changes its velocity over time, calculated as \text{a} = \frac{\Delta v}{\Delta t}.
Newton's Three Laws of Motion
Inertia: An object remains at rest or in motion unless acted on by a net force.
F=ma: The force acting on an object is equal to its mass times its acceleration.
Action-Reaction: For every action, there is an equal and opposite reaction.
Force and the Newton (N)
A Force is a push or pull. It is measured in Newtons (N), where 1 N = 1 kg \cdot m/s^2.
Pressure
Defined as force acting on a unit area. It is calculated using the formula: P = \frac{F}{A}. Standard unit is the Pascal (Pa).
Pressure in States of Matter
Solids, liquids, and gases all exert pressure. In fluids, pressure is affected by factors such as density, gravity, depth/height, and temperature.
Earth and Space Science: Ozone (O_3)
A molecule composed of three oxygen atoms. It forms the ozone layer in the stratosphere, which protects life on Earth by absorbing harmful ultraviolet (UV) radiation.
Ionic vs. Molecular Compounds
Ionic: Formed by electron transfer between metals and non-metals; usually solids with high melting points.
Molecular (Covalent): Formed by electron sharing between non-metals; can be solids, liquids, or gases with lower melting points.
Properties of Solids, Liquids, and Gases
Solids: Definite shape and volume; particles vibrate in fixed positions.
Liquids: Definite volume but take the shape of their container; particles move past each other.
Gases: No definite shape or volume; particles move rapidly and independently.
Systematic Naming of Compounds
IUPAC naming ensures global consistency. Binary Ionic Compounds use the metal name followed by the non-metal with an -ide suffix. Molecular Compounds use numerical prefixes (e.g., mono-, di-, tri-).
Physics: Position and Time
Position is the location of an object relative to a reference point, while Time is the interval or duration in which a change or motion occurs.
Distance vs. Displacement
Distance: The total length of the path traveled by an object (scalar).
Displacement: The straight-line change in position from the starting point to the ending point, including direction (vector).
Speed vs. Velocity
Speed: The rate at which an object covers distance (scalar, v = d/t).
Velocity: Speed in a specific direction (vector, displacement over time).
Acceleration
The rate at which an object changes its velocity over time, calculated as a = \frac{\Delta v}{\Delta t}.
Newton's Three Laws of Motion
Inertia: An object remains at rest or in motion unless acted on by a net force.
F = ma: The force acting on an object is equal to its mass times its acceleration.
Action-Reaction: For every action, there is an equal and opposite reaction.
Force and the Newton (N)
A Force is a push or pull measured in Newtons (N), where 1 N = 1 kg \cdot m/s^2. Force is a vector quantity.
Pressure (P)
Defined as force acting on a unit area (P = F/A). The standard unit is the Pascal (Pa).
Pressure in States of Matter
All states exert pressure. In fluids, pressure is affected by density, gravity, depth, and temperature.
Ozone (O_3): Composition and Formation
Ozone is a molecule made of 3 oxygen atoms. It forms in the stratosphere when ultraviolet (UV) radiation splits O_2 into free oxygen atoms that then bond with other oxygen molecules.
Ozone Layer and UV Radiation
The ozone layer blocks harmful ultraviolet (UV) radiation from the sun, protecting life on Earth from skin cancer and ecological damage.
Ozone Depletion: CFCs and the Ozone Hole
Chlorofluorocarbons (CFCs) break down ozone. An Ozone Hole is a region where the ozone layer has become exceptionally thin, primarily over Antarctica.
The Montreal Protocol
An international environmental treaty designed to phase out the production of ozone-depleting substances like CFCs. Global cooperation has successfully reduced ozone damage.
Factors Influencing Earth's Climate
Latitude: Determines the intensity of solar energy.
Landscape: Mountains affect precipitation and wind.
Ocean Currents & Winds: Distribute heat globally.
The Coriolis Effect
The apparent deflection of winds and ocean currents to the right in the Northern Hemisphere and left in the Southern Hemisphere due to Earth's rotation.
The Greenhouse Effect
The natural process where gases (like CO_2 and Methane) trap heat in the atmosphere. Human activities, specifically burning fossil fuels, intensify this effect.
Consequences of Climate Change
Extreme weather and wildfires
Melting polar ice and rising sea levels
Ocean acidification
Flooding and desertification
Natural Resources: Definition and Types
Materials from nature used by society. Includes fossil fuels (coal, oil), ores, minerals, and metals. They are extracted via mining or drilling.
Astronomical Units of Distance
AU: Distance from Earth to Sun (1.5 \times 10^8 \text{ km}).
Light Year: Distance light travels in a year.
Parsec: Approximately 3.26 light years.
Evidence for the Big Bang Theory
Supported by the Cosmic Microwave Background Radiation (CMBR) and the observed Redshift (Doppler shift) of distant galaxies.
Doppler Shift
A change in wavelength of light due to motion. Redshift indicates galaxies are moving away, proving the universe is expanding.
Solar System Formation: Gravity and Accretion
Gravity collapsed a nebula into a disk. Accretion is the process where dust and gas particles clumped together to form planets.
Ages: Universe, Solar System, and Earth
Stars: Formation and Energy
Stars form in nebulae when gravity collapses gas until Nuclear Fusion begins. Fusion converts Hydrogen into Helium, releasing massive energy.
Types of Stars
Stars are classified by mass and temperature; common types include Average stars (like the Sun), Red Giants, White Dwarfs, and Neutron Stars.
Gravity and Celestial Objects
Gravity is the fundamental force that keeps planets and moons in orbit, governs the motion of galaxies, and drives the life cycle of stars.
Meteor Activity
Meteoroid: A small rocky body in space.
Meteor: The streak of light in the atmosphere.
Meteorite: A rock that survives atmosphere entry and hits the ground.
Life Beyond Earth
No scientific evidence of life has been found beyond Earth yet, primarily due to extreme planetary environments and the vast distances between stars.
Chemistry: Reactants and Products
Reactants are the starting substances in a chemical reaction, while products are the new substances formed as a result of the reaction.
Law of Conservation of Mass
States that mass is neither created nor destroyed in a chemical reaction; therefore, \text{Total Mass of Reactants} = \text{Total Mass of Products}.
Bohr Models
A diagram representing an atom that shows the nucleus and the arrangement of electrons in specific energy levels or shells surrounding it.
Valence Electrons
The electrons located in the outermost shell of an atom, which determine the element's chemical reactivity and bonding properties.
Ionic Bonding
A type of chemical bond formed through the transfer of electrons from a metal atom to a non-metal atom, resulting in electrostatic attraction between ions.
Covalent Bonds
Chemical bonds formed when two or more non-metal atoms share pairs of valence electrons to achieve a stable electron configuration.
Physics: Position and Time
Position is the location of an object relative to a reference point, while Time is the interval or duration in which a change or motion occurs.
Distance vs. Displacement
Distance: The total length of the path traveled by an object (scalar).
Displacement: The straight-line change in position from the starting point to the ending point, including direction (vector).
Naming Binary Ionic Compounds
Named by writing the name of the metal first, followed by the non-metal with the suffix changed to -ide (e.g., Sodium Chloride).
Molecular Compounds Prefixes
Numerical prefixes used to indicate the number of atoms in a covalent compound:
1: mono-
2: di-
3: tri-
4: tetra-
5: penta-
Ionic vs. Molecular Compounds
Ionic: Formed by electron transfer between metals and non-metals; usually solids with high melting points.
Molecular (Covalent): Formed by electron sharing between non-metals; can be solids, liquids, or gases with lower melting points.
Covalent Bonds: Single, Double, Triple
Single Bond: Shares 1 pair of electrons.
Double Bond: Shares 2 pairs of electrons.
Triple Bond: Shares 3 pairs of electrons.
Speed vs. Velocity
Acceleration
The rate at which an object changes its velocity over time, calculated as a = \frac{\Delta v}{\Delta t}.
Newton's Three Laws of Motion
Inertia: An object remains at rest or in motion unless acted on by a net force.
F = ma: The force acting on an object is equal to its mass times its acceleration.
Action-Reaction: For every action, there is an equal and opposite reaction.
Force and the Newton (N)
A Force is a push or pull measured in Newtons (N), where 1 N = 1 kg \cdot m/s^2. Force is a vector quantity.
Pressure (P)
Defined as force acting on a unit area (P = F/A). The standard unit is the Pascal (Pa).
Pressure in States of Matter
All states exert pressure. In fluids, pressure is affected by density, gravity, depth, and temperature.
Earth and Space Science: Ozone (O_3)
A molecule composed of three oxygen atoms. It forms the ozone layer in the stratosphere, which protects life on Earth by absorbing harmful ultraviolet (UV) radiation.
Properties of Solids, Liquids, and Gases
Solids: Definite shape and volume; particles vibrate in fixed positions.
Liquids: Definite volume but take the shape of their container; particles move past each other.
Gases: No definite shape or volume; particles move rapidly and independently.
Systematic Naming of Compounds
IUPAC naming ensures global consistency. Binary Ionic Compounds use the metal name followed by the non-metal with an -ide suffix. Molecular Compounds use numerical prefixes (e.g., mono-, di-, tri-).
Ozone (O_3): Composition and Formation
Ozone is a molecule made of 3 oxygen atoms. It forms in the stratosphere when ultraviolet (UV) radiation splits O_2 into free oxygen atoms that then bond with other oxygen molecules.
Ozone Layer and UV Radiation
The ozone layer blocks harmful ultraviolet (UV) radiation from the sun, protecting life on Earth from skin cancer and ecological damage.
Ozone Depletion: CFCs and the Ozone Hole
Chlorofluorocarbons (CFCs) break down ozone. An Ozone Hole is a region where the ozone layer has become exceptionally thin, primarily over Antarctica.
The Montreal Protocol
An international environmental treaty designed to phase out the production of ozone-depleting substances like CFCs. Global cooperation has successfully reduced ozone damage.
Factors Influencing Earth's Climate
Latitude: Determines the intensity of solar energy.
Landscape: Mountains affect precipitation and wind.
Ocean Currents & Winds: Distribute heat globally.
The Coriolis Effect
The apparent deflection of winds and ocean currents to the right in the Northern Hemisphere and left in the Southern Hemisphere due to Earth's rotation.
The Greenhouse Effect
The natural process where gases (like CO_2 and Methane) trap heat in the atmosphere. Human activities, specifically burning fossil fuels, intensify this effect.
Consequences of Climate Change
Natural Resources: Definition and Types
Materials from nature used by society. Includes fossil fuels (coal, oil), ores, minerals, and metals. They are extracted via mining or drilling.
Astronomical Units of Distance
Evidence for the Big Bang Theory
Supported by the Cosmic Microwave Background Radiation (CMBR) and the observed Redshift (Doppler shift) of distant galaxies.
Doppler Shift
A change in wavelength of light due to motion. Redshift indicates galaxies are moving away, proving the universe is expanding.
Solar System Formation: Gravity and Accretion
Gravity collapsed a nebula into a disk. Accretion is the process where dust and gas particles clumped together to form planets.
Ages: Universe, Solar System, and Earth
Stars: Formation and Energy
Stars form in nebulae when gravity collapses gas until Nuclear Fusion begins. Fusion converts Hydrogen into Helium, releasing massive energy.
Types of Stars
Stars are classified by mass and temperature; common types include Average stars (like the Sun), Red Giants, White Dwarfs, and Neutron Stars.
Gravity and Celestial Objects
Gravity is the fundamental force that keeps planets and moons in orbit, governs the motion of galaxies, and drives the life cycle of stars.
Meteor Activity
Life Beyond Earth
No scientific evidence of life has been found beyond Earth yet, primarily due to extreme planetary environments and the vast distances between stars.
Ecology: Ecosystems and Biodiversity
Ecological Hierarchy
The levels of biological organization in ecology:
Food Webs and Ecological Pyramids
Trophic Levels
Steps in a food chain or web (Producers, Primary Consumers, Secondary Consumers, Tertiary Consumers).
Niche and Competition
A niche is a species' unique role and use of resources. Different niches allow species to coexist by reducing direct competition for the same resources.
Biotic vs. Abiotic Factors
Carbon and Nitrogen Cycles
Carrying Capacity and Limiting Factors