Forces and Motion: Forces, Inclined Planes, and Tension

Net forces and basic definitions

  • fnet = ∑ F = sum of all forces acting on an object. In vertical direction this often involves the normal force FN (up) and the force of gravity F_g (down).

  • If the normal force and gravity have equal magnitude and opposite directions, the net force is zero: f_net = 0.

  • By Newton’s second law, fnet = m a, so if fnet = 0, the acceleration a = 0 (no change in velocity).

  • If an object is above a surface (no contact force), the only force is gravity, so f_net = m g downward and the object accelerates downward at a = g ≈ 9.8 m/s^2.

  • Net force equals mass times acceleration in the direction of motion (or the net acceleration): f_net = m a.

Terminal velocity and air resistance

  • Terminal velocity occurs when an object falling through a fluid (like air) reaches a constant speed and stops speeding up.

  • In this situation the upward drag force Fdrag opposes gravity and can balance it: Fdrag ≈ F_g.

  • If Fdrag = m g, then fnet = 0 and acceleration a = 0 even though the object is still moving downward.

  • Example intuition: if gravity is 100 N and drag is also 100 N, the net force is zero and the speed remains constant.

Acceleration and velocity concepts

  • Acceleration is the rate of change of velocity: a=v<em>fv</em>iΔt.a = \frac{v<em>f - v</em>i}{\Delta t}.

  • Acceleration is zero when vf = vi (no net change in velocity).

  • You can have nonzero velocity with zero acceleration if velocity is constant (inertial reference frame). In a car at constant speed you don’t feel a force unless your velocity changes (e.g., turning). If you suddenly decelerate, you feel a strong force due to a large negative acceleration.

  • Forceful deceleration (e.g., hitting a wall) causes a large force: F = m a, and that force is transmitted to you (and to the wall) via the interaction.

Normal force and friction on surfaces

  • Normal force F_N is exerted by a surface to prevent an object from passing through it; it acts perpendicular to the surface.

  • On a flat surface (theta = 0), F_N = m g.

  • On an inclined plane (angle theta), the normal force is reduced: FN=mgcosθ.F_N = m g \cos\theta. If there is no acceleration perpendicular to the plane, the component of gravity perpendicular to the plane is balanced by the normal force.

  • The component of gravity along the plane (down the incline) is Fg,x=mgsinθ.F_{g,x} = m g \sin\theta. This drives the motion down the ramp when friction is present or absent.

  • Friction opposes motion along the surface and depends on the normal force: F<em>frictionμF</em>N.F<em>\text{friction} \le \mu F</em>N. The direction is opposite to the motion (up the ramp if the block would slide down). Friction depends on the normal force; we’ll discuss friction in more detail in Chapter 5.

Free-body diagrams (FBD) and force decomposition

  • A free-body diagram places all forces on the object being analyzed to visualize what enters the equations.

  • For an object on a ramp, key forces are gravity (downwards), the normal force (perpendicular to the ramp), and friction (opposite to motion along the ramp).

  • When weighing components, choose a coordinate system that simplifies calculations (e.g., rotate coordinates so x is along the ramp and y is perpendicular to the ramp).

  • In the rotated frame:

    • Gravity decomposes into components: F<em>g,y=mgcosθF<em>{g,y} = m g \cos\theta (perpendicular to ramp) and F</em>g,x=mgsinθF</em>{g,x} = m g \sin\theta (along the ramp, down the incline).

    • If there is no acceleration perpendicular to the ramp, then: F<em>g,yF</em>N=ma<em>y=0F</em>N=mgcosθ.F<em>{g,y} - F</em>N = m a<em>y = 0 \Rightarrow F</em>N = m g \cos\theta.

    • The friction force acts along the ramp and is opposite the motion.

  • For the x-direction along the ramp: F<em>x=ma</em>x.\sum F<em>x = m a</em>x. If there is no friction, F<em>x=mgsinθ=ma</em>xax=gsinθ.F<em>x = m g \sin\theta = m a</em>x \Rightarrow a_x = g \sin\theta.

  • Special case: when theta = 90°, the ramp is vertical and the down-ramp component becomes the full weight: Fx=mgsin90°=mg.F_x = m g \sin 90° = m g.

  • If there is friction, include the friction term in the x-direction: the net along-plane force is F<em>g,xF</em>friction=maxF<em>{g,x} - F</em>\text{friction} = m a_x (signs depend on chosen direction).

Inclined plane and angle-specific notes

  • For a flat surface (\theta = 0):

    • F<em>N=mgF<em>N = m g, F</em>g,x=mgsin0°=0.F</em>{g,x} = m g \sin 0° = 0. No acceleration along the plane due to gravity alone.

  • For a typical incline (0 < \theta < 90°):

    • Gravity components: F<em>g,x=mgsinθ,F</em>g,y=mgcosθ.F<em>{g,x} = m g \sin\theta, \quad F</em>{g,y} = m g \cos\theta.

    • Normal force: FN=mgcosθ.F_N = m g \cos\theta.

    • If friction is present, friction force opposes motion and its maximum magnitude is F<em>friction,max=μF</em>N.F<em>\text{friction,max} = \mu F</em>N.

  • Example with a 30° incline (illustrative): Fg,x=mgsin30°=12mg.F_{g,x} = m g \sin 30° = \tfrac{1}{2} m g.

Weight, mass, and unit considerations

  • Weight is the force due to gravity: W=Fg=mg.W = F_g = m g. It is the same physical quantity referred to as force due to gravity in many introductory contexts.

  • Mass is the amount of matter in an object and is invariant (measured in kilograms). It does not change with location, unlike weight.

  • On different planets or moons, the acceleration due to gravity g changes, so weight changes but mass does not. For example, on the Moon, g is smaller, so you weigh less but have the same mass.

  • Units note: force is in newtons (N). 1 N = 1 kg·m/s². Weight in pounds is a force unit in customary systems; 1 N ≈ 0.2248 lb_f. Mass is measured in kg; the same mass on Earth or the Moon has different weights due to g differences.

Two-block/rope tension intuition (connected bodies)

  • When two blocks are connected by a rope, the rope transmits tension. In an ideal (massless) rope, the tension magnitude is the same along the rope.

  • At each end of the rope, the rope exerts a force of magnitude T in opposite directions on the connected bodies (one end pulls forward on one block, the other end pulls backward on the other block).

  • If you pull on a system and all pieces accelerate together as a unit, each segment experiences the same acceleration, and the external force must overcome the internal tensions to achieve that acceleration.

  • The transcript discusses a scenario where, for a system of connected pieces, one asks how much force is needed to produce a given acceleration for the entire system. In such a case you sum the external forces and set them equal to the total mass times the common acceleration: Fexternal = (mtotal) a. The details depend on the configuration (e.g., how tensions distribute across interfaces).

  • Important caveat discussed in the talk: a single rope in an idealized setup yields a single tension value along the rope. If a diagram shows two tensions (T1 and T2) on the same rope segment, that would indicate a non-ideal situation or a particular pulley/attachment arrangement; in an ideal rope, T1 = T2 = T.

Practical applications and takeaways

  • Draw a clear free-body diagram before writing equations to identify which forces act and their directions.

  • Always check directions: gravity acts downward; normal force acts perpendicular to the contact surface; friction acts opposite the direction of motion along the surface; components on an incline separate gravity into sin and cos components with respect to the ramp.

  • Choose coordinates that simplify the problem (e.g., along the ramp for motion down a ramp).

  • Use the relation f_net = m a to connect forces to the motion you want to describe.

  • Remember the distinction between mass (in kg) and weight (a force in N), and how weight changes with g across environments, while mass stays the same.

  • Understand terminal velocity conceptually as a balance of forces (drag equals weight). Use this to reason about why acceleration becomes zero even though the object is moving.

  • When analyzing a system of connected bodies (e.g., blocks connected by a rope), recognize that internal forces (like tension) affect each piece, but the overall external force determines the system’s acceleration. In an ideal rope, tension is uniform along the rope; the forces on connected bodies are equal in magnitude and opposite in direction at each connection.