Mechanics: Forces and Newton's Laws of Motion

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Vocabulary flashcards covering forces, free-body and force diagrams, friction, inclined plane components, Newton's three laws of motion, and Newton's law of universal gravitation.

Last updated 7:01 PM on 10/11/26
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68 Terms

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Force

A push or pull. It is a vector quantity having both magnitude and direction, denoted by the symbol FF, and measured in the unit Newton (NN).

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Free-Body Diagram

A diagrammatic representation where an object of interest is represented by a dot, and all forces acting upon it are drawn as arrows pointing away from the dot.

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Force Diagram

A visual representation of all the forces acting on an object, drawn as arrows directly on the picture of the object itself rather than on a dot.

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Tension (TT)

A contact force acting on a rope or string.

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Weight (WW)

A non-contact gravitational force exerted by the Earth on an object, directed straight downwards and calculated by the formula W=mgW = mg.

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Normal Force (NN)

The perpendicular force (or component of a force) exerted by a surface on an object in contact with it.

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Frictional Force (ff)

A force that opposes the motion of an object relative to a surface and acts parallel to that surface.

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Kinetic Friction (fkf_k)

The frictional force that opposes the motion of a moving object relative to a surface and acts parallel to the surface, given by f_k = \μ_k N.

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Static Friction (fsf_s)

The frictional force that opposes the tendency of motion of a stationary object relative to a surface and acts parallel to the surface, reaching a maximum value of f_s^{\\text{max}} = \μ_s N.

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Coefficient of Friction (\μ)

A dimensionless ratio (\μ_k or \μ_s) that depends strictly on the contacting surfaces; it does not change unless the nature of the surface changes.

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Perpendicular Component of Weight (F_{g\⊥})

The component of weight acting perpendicular to an inclined surface, calculated as F_{g\⊥} = mg \\cos(\θ), which equals the magnitude of the normal force (NN) on the incline.

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Parallel Component of Weight (F_{g\∥})

The component of weight acting parallel down an inclined surface, calculated as F_{g\∥} = mg \\sin(\θ), which balances static friction (fsf_s) when the object remains stationary.

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Normal Force when Pulling at an Angle

The normal force on a horizontal surface when pulled upward at an angle θ\theta, given by N = F_g - F_y = mg - F_A \\sin(\θ); increasing the angle decreases NN and decreases kinetic friction.

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Normal Force when Pushing at an Angle

The normal force on a horizontal surface when pushed downward at an angle θ\theta, given by N = F_g + F_y = mg + F_A \\sin(\θ); increasing the angle increases NN and increases kinetic friction.

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Newton's First Law of Motion

An object will remain at rest or continue moving at constant velocity unless a non-zero resultant force acts on it.

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Inertia

The tendency of an object to resist a change in its state of motion, which is directly dependent on the mass of the object.

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Newton's Second Law of Motion

When a resultant force acts on an object, the object accelerates in the direction of the force; the acceleration is directly proportional to the resultant force and inversely proportional to the mass (Ftextnet=maF_{\\text{net}} = ma).

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Newton's Third Law of Motion

When object A exerts a force on object B, object B simultaneously exerts an oppositely directed force of equal magnitude on object A.

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Action-Reaction Pair

A pair of simultaneous, equal, and oppositely directed forces acting between two interacting bodies, which holds true regardless of their relative masses.

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Newton's Law of Universal Gravitation

Every particle in the universe attracts every other particle with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres (F=fracGm1m2r2F = \\frac{G m_1 m_2}{r^2}).

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Universal Gravitational Constant (GG)

The constant of proportionality in Newton's Law of Universal Gravitation, with a value equal to 6.67 \× 10^{-11}\\,\\text{N}\·\\text{m}^2/\\text{kg}^2.

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Gravitational Acceleration on Earth (gg)

The downward acceleration due to Earth's gravity at its surface, determined by g = \\frac{G M_{\\text{Earth}}}{r_{\\text{Earth}}^2} = 9.8\\,\\text{m}\·\\text{s}^{-2}.

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Force

A push or pull. It is a vector quantity (having both magnitude and direction) represented by the symbol FF and measured in Newtons (N\text{N}).

24
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Tension (TT)

A contact force acting on a rope or string.

25
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Weight (ww or FgF_g)

A non-contact gravitational force exerted by the Earth on an object, acting straight downwards.

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Normal Force (NN or FNF_N)

The force or component of a force exerted by a surface on an object in contact with it, acting perpendicular to the surface.

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Frictional Force (ff)

A force that opposes the motion or tendency of motion of an object relative to a surface and acts parallel to the surface.

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Kinetic Friction (fkf_k)

A force that opposes the motion of a moving object relative to the surface and acts parallel to the surface, calculated as fk=μkNf_k = \mu_k N.

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Static Friction (fsf_s)

A force that opposes the tendency of motion of a stationary object relative to the surface and acts parallel to the surface, with a maximum value given by fsmax⁡=μsNf_s^{\max} = \mu_s N.

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Coefficient of Friction (μ\mu)

A unitless ratio (μk\mu_k or μs\mu_s) that depends on the surface properties and remains constant as long as the surface does not change.

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Free-Body Diagram

A diagram where the object of interest is represented by a dot, and all forces acting on it are drawn as arrows pointing away from the dot and labeled.

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Force Diagram

A diagram representing all forces acting on an object drawn as arrows, where the object itself is drawn instead of being represented by a dot.

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Parallel Component of Weight (Fg∥F_{g\parallel})

The component of gravitational force acting parallel to an inclined plane, given by Fg∥=mgsin⁡(θ)F_{g\parallel} = mg \sin(\theta).

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Perpendicular Component of Weight (Fg⊥F_{g\perp})

The component of gravitational force acting perpendicular to an inclined plane, given by Fg⊥=mgcos⁡(θ)F_{g\perp} = mg \cos(\theta), which equals the normal force magnitude on the incline.

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Pulling at an Angle (θ\theta)

A scenario where an applied pulling force reduces the normal force (N=Fg−FyN = F_g - F_y), which in turn decreases the frictional force.

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Pushing at an Angle (θ\theta)

A scenario where an applied pushing force increases the normal force (N=Fg+FyN = F_g + F_y), which in turn increases the frictional force.

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Newton's First Law

An object will remain at rest or continue moving at constant velocity unless a non-zero resultant force acts on it.

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Inertia

The tendency of an object to resist a change in its state of motion, which is dependent on the mass of the object.

39
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Newton's Second Law

When a resultant force acts on an object, the object will accelerate in the direction of the force; the acceleration is directly proportional to the resultant force and inversely proportional to the mass (Fnet=maF_{\text{net}} = ma).

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Newton's Third Law

When object A exerts a force on object B, object B simultaneously exerts an oppositely directed force of equal magnitude on object A.

41
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Action-Reaction Pair

Two simultaneous forces of equal magnitude and opposite direction that act between two interacting objects, holding true irrespective of their relative masses.

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Newton's Law of Universal Gravitation

Every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres (F=Gm1m2r2F = \frac{G m_1 m_2}{r^2}).

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Universal Gravitational Constant (GG)

The proportionality constant in Newton's Law of Universal Gravitation, with an experimental value of 6,67×10−11 N⋅m26{,}67 \times 10^{-11}\,\text{N}\cdot\text{m}^2.

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Acceleration Due to Gravity on Earth (gg)

The downward acceleration at Earth's surface caused by gravity, calculated as g=GMEarthrEarth2=9,8 m⋅s−2g = \frac{G M_{\text{Earth}}}{r_{\text{Earth}}^2} = 9{,}8\,\text{m}\cdot\text{s}^{-2}.

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Gravitational Acceleration on Another Planet (gpg_p)

The acceleration due to gravity on another planet of mass MpM_p and radius rpr_p, calculated as gp=GMprp2g_p = \frac{G M_p}{r_p^2}, used to find weight via W=mgpW = m g_p.

46
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Force

A push or a pull exerted on an object. It is a vector quantity (having both magnitude and direction), denoted by the symbol FF, and measured in Newtons (N\text{N}).

47
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Tension (TT)

A contact force acting on a rope, string, or cable.

48
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Weight (ww or FgF_g)

A non-contact gravitational force exerted by the Earth on an object, acting straight downwards with magnitude calculated as w=mgw = mg.

49
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Normal Force (NN or FNF_N)

The force (or component of a force) exerted by a surface on an object in contact with it, acting perpendicular to the surface.

50
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Frictional Force (ff)

A force that opposes the motion of an object relative to the surface and acts parallel to the surface. It is directly proportional to the normal force (NN).

51
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Kinetic Friction (fkf_k)

The friction force that opposes the motion of a moving object relative to the surface, acting parallel to the surface and calculated using fk=μkNf_k = \mu_k N.

52
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Static Friction (fsf_s)

The friction force that opposes the tendency of motion of a stationary object relative to the surface, acting parallel to the surface with a maximum value given by fsmax⁡=μsNf_s^{\max} = \mu_s N.

53
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Coefficients of Friction (μk\mu_k and μs\mu_s)

Unitless ratios representing the roughness between two interacting surfaces. Their values depend only on the surface materials and do not change if the surface remains the same.

54
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Free-Body Diagram

A diagram where the object of interest is represented by a single dot, and all forces acting on it are drawn as arrows pointing away from that dot.

55
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Force Diagram

A diagram representing all the forces acting on an object, where the forces are drawn as arrows directly acting upon a drawing of the object itself.

56
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Newton's First Law of Motion

An object will remain at rest or continue moving at constant velocity unless a non-zero resultant force acts on it.

57
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Inertia

The tendency of an object to resist a change in its state of motion, which is dependent directly on the object's mass.

58
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Newton's Second Law of Motion

When a resultant force acts on an object, the object accelerates in the direction of the force; this acceleration is directly proportional to the resultant force and inversely proportional to the mass (Fnet=maF_{\text{net}} = ma).

59
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Newton's Third Law of Motion

When object A exerts a force on object B, object B simultaneously exerts an oppositely directed force of equal magnitude on object A, irrespective of their relative masses.

60
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Action-Reaction Pair

A pair of simultaneous forces of equal magnitude and opposite directions exerted between two interacting bodies (e.g., a block pushing downward on a table while the table pushes upward on the block).

61
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Newton's Law of Universal Gravitation

Every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres: F=Gm1m2r2F = \frac{G m_1 m_2}{r^2}.

62
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Universal Gravitational Constant (GG)

The proportionality constant in Newton's gravitational formula, with a value of 6,67×10−11 N⋅m2/kg26{,}67 \times 10^{-11}\,\text{N}\cdot\text{m}^2/\text{kg}^2.

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Gravitational Acceleration on Earth (gg)

The acceleration due to Earth's gravity, given by g=GMEarthrEarth2=9,8 m⋅s−2g = \frac{G M_{\text{Earth}}}{r_{\text{Earth}}^2} = 9{,}8\,\text{m}\cdot\text{s}^{-2} downwards.

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Perpendicular Component of Weight (Fg⊥F_{g\perp})

The component of weight perpendicular to an inclined surface, calculated as Fg⊥=mgcos⁡(θ)F_{g\perp} = mg\cos(\theta), which equals the normal force (NN) on the incline.

65
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Parallel Component of Weight (Fg∥F_{g\parallel})

The component of weight directed down an inclined plane, given by Fg∥=mgsin⁡(θ)F_{g\parallel} = mg\sin(\theta), which equals the static friction force (fsf_s) when the object remains stationary.

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Normal Force When Pulling at an Angle

Given by N=Fg−Fy=mg−Fsin⁡(θ)N = F_g - F_y = mg - F\sin(\theta). As the angle θ\theta increases, the normal force decreases, which consequently causes the frictional force to decrease.

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Normal Force When Pushing at an Angle

Given by N=Fg+Fy=mg+Fsin⁡(θ)N = F_g + F_y = mg + F\sin(\theta). As the angle θ\theta increases, the normal force increases, which consequently causes the frictional force to increase.

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Two-Body System Analysis

The problem-solving approach of drawing separate free-body diagrams for each connected block and applying Newton's second law (Fnet=maF_{\text{net}} = ma) individually to blocks moving with the same acceleration.