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Collision
An event where two or more objects come into contact and exert forces on each other.
Kinetic Energy (KE)
The energy an object has due to its motion, calculated as 𝐾𝐸=1/2𝑚𝑣^2
Momentum (p)
The product of an object’s mass and velocity; a measure of how hard it is to stop the object.
Elastic Collision
A collision in which both momentum and kinetic energy are conserved; objects bounce off each other.
Ex. Two marbles colliding on a smooth surface and bouncing apart without losing energy.
Inelastic Collision
A collision in which momentum is conserved but kinetic energy is not; some energy is converted to heat, sound, or deformation.
Ex. A hockey puck hitting a goalie’s glove and stopping; momentum is conserved but some kinetic energy is lost.
Perfectly Inelastic Collision
A special case of an inelastic collision where the colliding objects stick together after impact.
Ex. Two blocks colliding and sticking together on a frictionless surface.
Momentum in Collisions
Total momentum of the system is conserved in all types of collisions.
Kinetic Energy in Collisions
Conserved only in elastic collisions; partially lost in inelastic collisions.
Total Momentum
The sum of the momenta of all objects in a system before and after a collision; remains constant in isolated systems.
Impulse
The change in momentum caused by a force applied over a period of time.
𝐽=𝐹Δ𝑡
Average Force (F)
The net force applied to an object over a time interval.
Time Interval (Δt)
The length of time during which a force acts on an object.
Impulse–Momentum Theorem
The impulse applied to an object equals its change in momentum.
Change in Momentum (Δp)
The difference between an object’s final momentum and initial momentum.
Longer Contact Time
Results in a smaller average force for the same impulse.
Shorter Contact Time
Results in a larger average force for the same impulse.
Impulse as a Vector Quantity
Impulse has both magnitude and direction, matching the direction of the applied force.
Impulse in Collisions
Determines how much an object’s momentum changes during an impact.
Momentum Formula
Momentum equals mass times velocity: p=m⋅v.
Units of Momentum
Kilogram meters per second (kg·m/s).
Mass (m)
The amount of matter in an object; measured in kilograms.
Velocity (v)
The speed of an object in a given direction; measured in meters per second.
Mass and Momentum
As mass increases, momentum increases if velocity stays the same.
Relationship between…
Relationship Between Velocity and Momentum
As velocity increases, momentum increases if mass stays the same.
High Momentum
Objects that are very massive, moving very fast, or both.
Low Momentum
Objects that are light, slow-moving, or both.
Changing Momentum
Momentum changes when an object’s velocity changes due to a force.
Force and Momentum Equation
Net force equals change in momentum divided by time: 𝐹=Δ𝑝/Δ𝑡
Stopping an Object
Requires removing all of its momentum using external forces.
Impulse
The effect of a force acting over a period of time that changes momentum (related to Δp).
Acceleration and Momentum
Acceleration is a change in velocity, which also means a change in momentum.
Vector Quantity
A quantity that has both magnitude and direction (momentum is a vector).
Law of Conservation of Momentum
In an isolated system, the total momentum remains constant.
Isolated System
A system where no external forces act and no mass enters or leaves.
Total Momentum
The sum of the momenta of all objects in a system.
Collision
An interaction where objects exert forces on each other, changing individual momenta.
Momentum Transfer
When one object loses momentum and another gains the same amount.
Frictionless Surface
An ideal surface with no external forces, allowing momentum to be conserved.
External Forces
Forces from outside a system that can change total momentum.
Why Momentum Is Useful
It helps analyze collisions and interactions without needing to track complex forces.
Atom
The basic building block of matter, made of a nucleus surrounded by electrons.
Nucleus
The dense center of an atom that contains protons and neutrons and most of the atom’s mass.
Proton
A positively charged particle found in the atomic nucleus.
Neutron
A neutral particle found in the atomic nucleus with no electric charge.
Electron
A negatively charged particle that exists in energy levels around the nucleus.
Electron Shells (Energy Levels)
Regions around the nucleus where electrons are likely to be found.
Electrostatic Repulsion
The force that causes positively charged protons to repel each other.
Nuclear Forces
Forces that act inside the atomic nucleus to hold protons and neutrons together.
Strong Nuclear Force
The strongest of the four fundamental forces; binds quarks together and holds protons and neutrons in the nucleus.
Purpose of the Strong Nuclear Force
Prevents the nucleus from flying apart due to electrostatic repulsion between protons.
Range of the Strong Nuclear Force
Extremely short; only works at very small (nuclear) distances.
Quarks
Fundamental particles that make up protons and neutrons.
Up Quark
A type of quark found in protons and neutrons.
Down Quark
A type of quark found in protons and neutrons.
Proton Quark Composition
Two up quarks and one down quark.
Neutron Quark Composition
Two down quarks and one up quark.
Gluons
Particles that carry the strong nuclear force and “glue” quarks together.
Weak Nuclear Force
A fundamental force responsible for radioactive decay and particle transformations.
Purpose of the Weak Nuclear Force
Allows quarks to change type, such as turning a proton into a neutron.
Radioactive Decay
A process in which unstable atoms release energy or particles due to the weak nuclear force.
Element Transformation
When an atom changes into a different element due to particle changes caused by the weak force.
Relative Strength of Forces
Strong nuclear force > electromagnetic force > weak nuclear force > gravitational force.
Why We Don’t Feel Nuclear Forces
They act only at extremely short distances inside atoms.
Nuclear Fusion
A process where light atomic nuclei combine to form a heavier nucleus, releasing large amounts of energy.
Fusion in Stars
Occurs when the strong nuclear force overcomes electromagnetic repulsion between nuclei.
Role of Gravity in Star Formation
Pulls gas and dust together to form a dense core.
Role of Electromagnetic Force in Stars
Helps atoms form and electrons stay bound to nuclei.
Role of Strong Nuclear Force in Stars
Allows nuclei to fuse, releasing energy that makes stars shine.
Role of Weak Nuclear Force in Stars
Enables particle changes that keep fusion reactions going.
Four Fundamental Forces
Gravitational force, electromagnetic force, strong nuclear force, and weak nuclear force.
Why Stars Shine
Energy released from nuclear fusion powered by the strong and weak nuclear forces.
Electromagnetic Force
The force that acts between charged particles; includes both electric and magnetic effects.
Why Electromagnetic Force Matters
It explains interactions between small objects where gravity is too weak to have a noticeable effect.
Electric Charge
A property of matter that can be positive or negative and causes electromagnetic interactions.
Point Charge
An electric charge treated as if all its charge is concentrated at a single point with no physical size.
Coulomb’s Law
An equation that describes the electrostatic force between two charged objects based on charge and distance.
Electrostatic Force (F)
The force of attraction or repulsion between two electric charges, measured in newtons.
Coulomb’s Constant (k)
A physical constant used in Coulomb’s law that determines the strength of the electrostatic force.
Charge Magnitude (q)
The amount of electric charge on an object, measured in coulombs (C).
Distance (r)
The separation between two charges, measured between their centers.
Like Charges Repel
Two charges with the same sign (both positive or both negative) push away from each other.
Opposite Charges Attract
A positive charge and a negative charge pull toward each other.
Direction of Electromagnetic Force
Depends on the signs of the charges; repulsive for like charges and attractive for opposite charges.
Direct Relationship (Charge)
Increasing the magnitude of either charge increases the electromagnetic force.
Inverse Square Relationship (Distance)
Increasing the distance between charges decreases the force by the square of the distance.
Inverse Square Law
Doubling the distance between charges reduces the electromagnetic force to one-fourth its original value.
Comparison to Gravity
Electromagnetic force is much stronger than gravitational force for small, charged objects.
Electric Field
A region around a charged object where other charges experience an electric force.
Magnetic Field
A region around moving charges or magnets where magnetic forces act.
Electromagnetism
The connection between electricity and magnetism as different aspects of the same force.
Michael Faraday
Scientist who discovered that changing magnetic fields can create electric currents.
Electromagnetic Induction
The process by which a changing magnetic field produces an electric current in a conductor.
Faraday’s Law
States that a changing magnetic field induces an electric current.
Changing Magnetic Field
A requirement for inducing current; a constant magnetic field does not produce current.
Induced Current
Electric current created by a changing magnetic field.
Heinrich Lenz
Scientist who explained the direction of induced current.
Lenz’s Law
The induced current always opposes the change in magnetic field that created it.
Opposition to Change
Induced currents resist increases or decreases in magnetic fields.
Alternating Current (AC)
Electric current that repeatedly changes direction, often produced by changing magnetic fields.
Coil and Magnet Interaction
Moving a magnet near a coil changes the magnetic field and induces current.