Physics Lecture Notes: Momentum, Energy, and Motion

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Flashcards covering physics concepts including momentum, energy, work, rotational motion, gravity, and Newton's laws based on lecture notes from Lectures 1-10.

Last updated 8:05 PM on 6/14/26
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101 Terms

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Momentum

Inertia in motion; a property that quantifies the motion of an object.

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Momentum Vector

A property indicating that momentum has both a magnitude and a direction.

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Momentum (Symbol)

pp

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Momentum Units

kgm/skg \cdot m/s or NsNs

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Momentum Equation

p=mvp = mv

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Direct Proportionality in Momentum

Both mass and velocity are directly proportional to momentum.

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Impulse

The change in momentum of an object or system of objects.

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Impulse (Symbol)

Δp\Delta p

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Impulse Equation (Change)

Δp=pfinalpinitial\Delta p = p_{final} - p_{initial}

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Impulse Equation (Force)

Δp=FΔt\Delta p = F \Delta t

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Force and Impulse Relationship

Impulse is directly proportional to force.

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Duration of Time and Impulse

Impulse is directly proportional to the duration of time over which force is applied.

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Speeding Up Force Direction

Force needs to be applied in the same direction as the velocity.

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Slowing Down Force Direction

Force needs to be applied in the opposite direction as the velocity.

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Conservation of Momentum

The momentum of a system is conserved in the absence of external forces.

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Momentum Conservation in Dimensions

In the absence of external forces, momentum is conserved in all dimensions (x, y, and z).

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Kinetic Energy (Definition)

The energy that an object has by virtue of its motion.

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Kinetic Energy (Symbol)

KEKE

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Kinetic Energy (Units)

JJ (Joules)

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Kinetic Energy Equation

KE=12mv2KE = \frac{1}{2} mv^2

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Inelastic Collision

A collision where some of the kinetic energy (KEKE) of the system is converted into other forms of energy like heat or sound.

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Elastic Collision

A collision where the kinetic energy (KEKE) of the system is conserved.

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Perfectly Inelastic Collision

A collision where the maximum amount of KEKE is lost and the two objects travel together after the collision.

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Elastic Collision Characteristics

Occur when no heat is generated, no sound is made, and molecules do not physically deform.

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Energy

The capability of an object to do useful work.

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Work

The transfer of energy by applying a force to an object over a distance.

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Work Equation

W=FdW = F_{\parallel} d

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Joule (Definition)

The primary unit for energy and work; 1J=1Nm1\,J = 1\,Nm.

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Newton (Symbol and Unit)

N=kgm/s2N = kg \cdot m/s^2

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Potential Energy

Stored energy.

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Kinetic Energy (Major Type)

Energy of motion.

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Electric Potential Energy

Energy that comes from the arrangement of charged particles.

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Chemical Energy

Energy that comes from the arrangement of atoms or molecules.

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Nuclear Energy

Energy that comes from the nucleus of an atom.

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Elastic Potential Energy

Energy that comes from the configuration of a deformable object.

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Gravitational Potential Energy (Definition)

Energy that comes from the gravitational attraction between the Earth and an object of mass.

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Gravitational Potential Energy (Symbol)

GPEGPE

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Gravitational Potential Energy Equation

GPE=mghGPE = mgh

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Heat

Energy that flows between objects due to a temperature difference.

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Friction Energy Conversion

Friction converts KEKE to heat, which is frequently wasted energy.

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Mechanical Energy (Definition)

Provides a way to describe the amount of GPEGPE and KEKE of an object.

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Mechanical Energy Equation

ME=GPE+KEME = GPE + KE

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Conservation of Mechanical Energy

MEME is conserved in the absence of dissipative forces like friction or air drag.

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Positive Work

Occurs when parallel force points in the same direction as the displacement, causing the object to speed up and gain KEKE.

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Negative Work

Occurs when parallel force points in the opposite direction as the displacement, causing the object to slow down and lose KEKE.

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Work-Energy Theorem

W=ΔKEW = \Delta KE or W=KEfinalKEinitialW = KE_{final} - KE_{initial}

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Power (Definition)

The rate at which work is done.

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Power (Symbol)

PP

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Power Units

WW (Watts) or J/sJ/s

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Power Equation

P=WtP = \frac{W}{t}

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Simple Machines

Devices that change direction or magnitude (or both) of an applied force.

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Mechanical Advantage (Definition)

Multiplication of an input force by a simple machine.

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Mechanical Advantage (Symbol)

MAMA

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Mechanical Advantage Equation

MA=FoutFinMA = \frac{F_{out}}{F_{in}}

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Translational Motion

Motion along a straight line.

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Rotational Speed

The speed at which an object rotates about an axis.

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Radian Measure Relation

2π=1 rotation2\pi = 1\text{ rotation}

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Rotational Speed Units

RPMRPM, degrees/s\text{degrees/s}, or rad/srad/s

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Tangential Velocity (Definition)

Relates to rotational speed and distance from the center of rotation.

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Tangential Velocity (Symbol)

VtV_t

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Tangential Velocity Equation

Vt=2πr/tV_t = 2\pi r / t

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Tangential Velocity Direction

Tangent to the motion of the rotation.

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Rotational Acceleration

Measures the change in rotational speed of an object.

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Rotational Inertia

Measures how much an object resists changes to its rotational motion.

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Torque (Definition)

A twist or a turn that causes an object to change its rotational motion.

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Torque (Symbol)

τ\tau

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Torque Units

NmNm

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Torque Equation

τ=Fr\tau = F_{\perp} r

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Apparent Weight (Definition)

Comes from the support force acting on us.

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Universal Gravitational Constant (G)

6.67×1011Nm2/kg26.67 \times 10^{-11}\,N\cdot m^2/kg^2

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Inverse-Square Law

Mathematical description of physical properties that decrease with the square of the distance (1/d2\propto 1/d^2).

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Newton's Law of Universal Gravitation Equation

F=Gm1m2d2F = G \frac{m_1 m_2}{d^2}

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Gravitational Acceleration (Little g)

The acceleration due to gravity on Earth's surface, equal to 9.8m/s2-9.8\,m/s^2.

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Gravitational Fields

A model describing how objects interact due to gravity using arrows depicting mass movement.

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General Relativity

Theory where motion is influenced by curves in "spacetime" caused by massive objects.

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Projectile Motion

Description of the motion of an object that moves in free-fall, considering only gravity.

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Ballistics

The study of objects that travel in projectile motion.

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Projectile Path Shape

Parabola

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Optimal Launch Angle for Horizontal Range

4545^{\circ}

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Satellite

A projectile that falls around Earth.

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Orbit

Describes the path of a satellite around a planet or star; all are elliptical.

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Circular Orbit

A special case where orbital height does not change and KE+GPE=constantKE + GPE = \text{constant}.

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Science

Systematic pursuit and organization of knowledge through questions, observations, and experiments.

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Scientific Method

The process by which scientists come to answer questions about the universe.

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Hypothesis

A proposed explanation based on observations that can be tested experimentally.

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Theory

An explanation of how the universe works supported by multiple, repeated experiments.

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Quantum Physics

Physical laws describing properties of matter and energy on a very small scale.

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Newton's First Law

An object in motion tends to stay in motion; an object at rest tends to stay at rest, unless acted upon by an outside force.

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Inertia

Describes the difficulty in changing an object's motion; caused by mass.

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Mass

A physical property that relates to inertia.

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Vector

A quantity that contains magnitude (strength) and direction.

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Mechanical Equilibrium

A condition where the sum of all forces is zero and the object experiences no change in motion.

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Displacement

A vector quantity representing the straight-line distance from one point to another.

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Speed

The scalar rate at which an object changes its position.

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Velocity

The vector rate at which an object changes its position.

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Acceleration

The rate at which an object's velocity changes (m/s2m/s^2).

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Newton's Second Law Equation

F=ma\sum F = ma

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Static Friction

The force required to get an object at rest to start moving.

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Kinetic Friction

The force between two objects where there is motion.

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Terminal Speed

The speed at which air resistance equals gravity, resulting in dynamic equilibrium.