Tenth Grade Physics: Mechanics, Energy, and Gravitation

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Vocabulary flashcards based on tenth-grade physics lecture notes covering Newton's three laws of motion, free-body diagrams, work, kinetic and potential energy, conservation principles, and universal gravitation.

14 Terms

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Inertia (Newton's First Law)

The law stating that an object only moves when an external force acts on it, expressed as ∑F⃗=0⇒a⃗=0\sum \vec{F} = 0 \Rightarrow \vec{a} = 0.

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Acceleration / Dinamic Law (Newton's Second Law)

The law stating that the acceleration of an object depends on the net force and its mass, expressed mathematically as ∑F⃗=m⋅a⃗\sum \vec{F} = m \cdot \vec{a}.

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Action and Reaction (Newton's Third Law)

The law stating that every action force has an equal and opposite reaction force acting on another object, represented by F⃗A→B=−F⃗B→A\vec{F}_{A \rightarrow B} = -\vec{F}_{B \rightarrow A}.

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Free-body Diagram

A diagram showing all external forces acting on a single object, commonly including weight (mgmg), normal force (NN), friction (ff), and tension (TT).

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Work

The energy transferred by a force when an object moves through a displacement, calculated as W=F⋅d⋅cos⁡(θ)W = F \cdot d \cdot \cos(\theta); if an object does not move, there is zero work.

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Energy

The capacity of making work.

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Kinetic Energy (EKE_K)

Energy associated with an object's motion that increases with mass and the square of speed, defined by the formula EK=12⋅m⋅v2E_K = \frac{1}{2} \cdot m \cdot v^2.

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Gravitational Potential Energy (EpE_p)

Energy associated with an object's position within a gravitational field, expressed as U=m⋅g⋅hU = m \cdot g \cdot h.

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Conservation of Mechanical Energy

The principle that when only conservative forces do work, total mechanical energy remains constant (EK+Ep=constantE_K + E_p = \text{constant}, or 12mvi2+mghi=12mvf2+mghf\frac{1}{2}m v_i^2 + m g h_i = \frac{1}{2}m v_f^2 + m g h_f).

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Momentum (p⃗\vec{p})

The measure of motion of an object, defined as the product of its mass and velocity (p⃗=mv⃗\vec{p} = m \vec{v}).

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Conservation of Momentum

The principle stating that in an isolated system with zero net external force, total momentum remains constant (∑p⃗i=∑p⃗f\sum \vec{p}_i = \sum \vec{p}_f).

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Momentum Conservation for Two Interacting Objects

The relation expressing momentum conservation during an interaction between two objects: m1v⃗1i+m2v⃗2i=m1v⃗1f+m2v⃗2fm_1 \vec{v}_{1i} + m_2 \vec{v}_{2i} = m_1 \vec{v}_{1f} + m_2 \vec{v}_{2f}.

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Universal Gravitation

The law describing the gravitational attractive force between two objects of masses m1m_1 and m2m_2 separated by a distance rr, given by Fg=Gm1⋅m2r2F_g = G \frac{m_1 \cdot m_2}{r^2}.

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Gravitational Constant (GG)

The proportionality constant in Newton's law of universal gravitation, equal to 6.674×10−116.674 \times 10^{-11}.