🔋College Physics I – Introduction Unit 4 Review
4.3 Newton’s Second Law of Motion: Concept of a System
4.3 Newton’s Second Law of Motion: Concept of a System
Unit & Topic Study Guides
The Nature of Science and Physics
Kinematics
Two–Dimensional Kinematics
Force and Newton's Laws of Motion
Newton's Laws: Friction, Drag, and Elasticity
Circular Motion and Gravity
Work and Energy in Physics
Linear Momentum and Collisions
Statics and Torque
Rotational Motion & Angular Momentum
Fluid Statics
Fluid Dynamics: Biological & Medical Uses
Temperature and Gas Laws
Heat and Heat Transfer Methods
Thermodynamics
Oscillatory Motion and Waves
Physics of Hearing
Electric Charge and Fields
Electric Potential & Field
Electric Current, Resistance, and Ohm's Law
Circuits and DC Instruments
Magnetism
Electromagnetic Induction & AC Circuits
Electromagnetic Waves
Geometric Optics
Vision and Optical Instruments
Wave Optics
Special Relativity
Quantum Physics
Atomic Physics
Radioactivity and Nuclear Physics
Nuclear Physics in Medicine
Particle Physics
Newton's Second Law of Motion: Concept of a System
Newton's Second Law connects force, mass, and acceleration in one equation. It gives you the tool to predict exactly how an object will move when you know the forces acting on it, making it the most widely used law in classical mechanics.
Net Force and System Concepts
Net force is the vector sum of all forces acting on an object or system. It's the net force, not any single force, that determines acceleration. The relationship is captured by:
An external force is any force that originates from outside the system you've defined. Gravity, friction, and an applied push are all common examples. Only external forces can change the motion of the system.
A system is whatever collection of objects you choose to analyze. How you draw the boundary matters: it determines which forces count as external (affecting the system's motion) and which are internal (forces between objects inside the system that cancel out). For example, if you define two connected blocks as your system, the tension between them is internal and doesn't appear in your net force calculation.
The center of mass is the point where you can treat the entire mass of a system as concentrated. When you apply Newton's Second Law to a system, the acceleration you calculate is the acceleration of this point.
Newton's Second Law Implications
The law tells you three things at once:
- Acceleration is proportional to net force. Double the net force on an object and its acceleration doubles.
- Acceleration is inversely proportional to mass. The same force applied to an object with twice the mass produces half the acceleration.
- Direction matters. The acceleration always points in the same direction as the net force.
If the net force on an object is zero, its acceleration is zero. That means it either stays at rest or keeps moving at constant velocity. This is actually Newton's First Law, which you can think of as a special case of the Second Law.
Newton's Third Law also plays a role here. Every force is part of an interaction: if object A pushes on object B, then B pushes back on A with equal magnitude and opposite direction. When defining your system, Third Law pairs between objects inside the system cancel out. Third Law pairs where one force is on the system and the other is on something outside are the external forces you need to account for.
Weight vs. Mass Calculations
Mass is a measure of an object's inertia, its resistance to acceleration. It's an intrinsic property that doesn't change with location and is measured in kilograms (kg).
Weight is the gravitational force acting on an object, calculated with:
- is the object's mass (kg)
- is the acceleration due to gravity (approximately on Earth's surface)
- is the weight, measured in newtons (N)
Because weight depends on , it changes with location. A 70 kg person weighs about 686 N on Earth but only about 114 N on the Moon (where ). Their mass stays 70 kg in both places.
A quick way to remember the distinction: you can measure mass with a balance (comparing to a known mass), but you measure weight with a scale (which reads the force of gravity pulling you down).
Forces and Interactions
Several common forces show up repeatedly in Newton's Second Law problems:
- Normal force is the perpendicular contact force a surface exerts on an object resting on it. On a flat surface with no other vertical forces, the normal force equals the object's weight.
- Friction opposes the relative motion (or attempted motion) between two surfaces in contact. It acts parallel to the surface.
- Tension is the pulling force transmitted through a rope, string, or cable. It acts along the length of the rope and pulls equally on both ends.
You'll also encounter momentum (), which is the product of mass and velocity. Newton's Second Law can actually be stated more generally as: the net force equals the rate of change of momentum. For constant mass, this reduces back to .