Introductory Physics Concepts
Topics Covered
- Unit Conversion
- Kinematics
- Vectors
- Projectile Motion
- Newton's Laws of Motion
- Circular Motion
- Work and Energy
- Linear Momentum
- Rotational Motion
Unit Conversions
Common Conversions
- **Mass and Length: **
- 1 kilogram = 1000 grams
- 1 kilometer = 1000 meters
- 1 mile = 5280 feet
- 1 inch = 2.54 centimeters
- 12 inches = 1 foot
- 3 feet = 1 yard
- 1 meter = 100 centimeters
Conversion Examples
- **Grams to Kilograms: **
- 470 grams = 0.47 kilograms
- **Centimeters to Meters: **
- **Kilometers per Hour to Meters per Second: **
Units of Length, Area, and Volume
- Distance: meters (m)
- Area: square meters (m²)
- Volume: cubic meters (m³)
Examples:
- Square Feet to Square Yards:
- Cubic Inches to Cubic Feet:
Metric System Prefixes
- Terra (T): 10¹²
- Giga (G): 10⁹
- Mega (M): 10⁶
- Kilo (k): 10³
- Hecto (h): 10²
- Deca (da): 10¹
- Base Unit (meters, liters, grams, etc.)
- Deci (d): 10⁻¹
- Centi (c): 10⁻²
- Milli (m): 10⁻³
- Micro (μ): 10⁻⁶
- Nano (n): 10⁻⁹
- Pico (p): 10⁻¹²
Metric System Examples
- Millimeters to Micrometers:
- Micrometers to Kilometers:
Kinematics
Distance vs Displacement
- Distance: Scalar, always positive
- Displacement: Vector, has magnitude and direction
Speed vs Velocity
- Speed: Scalar, distance/time
- Velocity: Vector, displacement/time
Acceleration
- Acceleration: rate of change of velocity; a = Δv/Δt
Kinematic Equations for Constant Acceleration
- v = u + at
- s = ut + ½at²
- v² = u² + 2as
- s = vt - ½at²
- s = ½(u + v)t
Example Problems
Newton's Laws of Motion
Newton's 1st Law
- Law of Inertia:
- An object at rest stays at rest, and an object in motion remains in motion unless acted on by a net external force.
Newton's 2nd Law
- F = ma:
- Force = mass × acceleration
Newton's 3rd Law
- Action/Reaction:
- For every action, there is an equal and opposite reaction.
Friction
- Static Friction: When objects are not moving relative to each other.
- Kinetic Friction: When objects are moving relative to each other.
- **Formulas: **
Energy
Types of Energy
- Kinetic Energy (KE): ½mv²
- Potential Energy (PE): mgh
- Mechanical Energy (ME): KE + PE
Conservation of Mechanical Energy
- Gravity: Conservative force. Mechanical energy remains constant when only gravity does work.
- Friction: Non-conservative force. Reduces mechanical energy.
Work
- Definition:
- Work-Energy Theorem:
- Work done = Change in kinetic energy
Momentum
Linear Momentum
- Definition: p = mv
- Impulse-Momentum Theorem:
Conservation of Momentum
- Elastic Collisions: Kinetic energy is conserved.
- Inelastic Collisions: Kinetic energy is not conserved, but momentum is.
- Formula:
- m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂'
Circular Motion
Centripetal Force
- Definition:
- Centripetal Acceleration:
Gravitational Force and Orbital Motion
- Formula:
- F_gravity = G(m₁m₂/r²)
- G = 6.67430 × 10⁻¹¹ m³⋅kg⁻¹⋅s⁻²
- Speed of Orbiting Object:
Miscellaneous
- **Maximum Safe Speed for a Car in a Curve: **
- Force in Horizontal Circular Motion:
- T = mv²/r (Tension provides the force)
Rotational Motion
Key Equations
- Torque: τ = F × l
- Rotational Work: W = τθ
- Angular Displacement: θ = ωt
- Angular Velocity: ω = ω₀ + αt
- Angular Acceleration: α = Δω/Δt
Inertia
- Formula for a disk: I = ½mR²
- Formula for a sphere: I = ²/₅ mR²
For additional practice problems and detailed videos, refer to the channel's physics playlists.