Oscillations are parallel to the direction of energy transfer, consisting of compressions and rarefactions
Longitudinal Waves
Sound
Ultrasound (Ultrasonic)
Infrasound
Time Period
Time taken to complete 1 round of wave, inverse of frequency
Time Period
1. time period = time taken / number of waves
2. time period = 1 / frequency
Law of Reflection
angle of incidence = angle of reflection
Refraction
The change in the speed and direction of a wave once it passes through different mediums
In refraction, the frequency ALWAYS remains the same
Dispersion
The refraction of light with different wavelengths at different angles, resulting in different colors of the rainbow
Greater frequency
Higher pitch
Gas
Non-fixed shape, Non-fixed volume, Particles move at high speed, freely, at random
Evaporation
Occurs over a range of temperatures, Occurs ONLY at the liquid's surface, Causes cooling effect
Brownian Motion
When small particles (such as pollen or smoke particles) are suspended in fluids, the particles can be observed moving at random through a microscope. This motion is caused by the fluid molecules colliding at high speeds with the small particles.
The effects of thermal expansion include length increases, area increases, and volume increases
Gas
Expand significantly (due to there being no bonds holding the molecules together)
Shiny and white things do not reflect heat, they reflect radiation. And vice versa with matt black things
Types of energy stores
Magnetic
Internal (thermal)
Chemical
Kinetic
Electrostatic
Elastic potential
Gravitational potential
Nuclear
Work done
Whenever a force acts on an object that moves in the direction of the force, there is work done. Whenever any work is done, energy gets transferred from one form to another.
Power (P)
The amount of energy transferred every second, unit watt (W) or joules per second.
P = energy transferred / time taken
Mass and Weight
Mass is related to the amount of matter in an object, measured in kilograms (kg). Weight is the force of gravity on a mass, measured in newtons (N).
Weight = mass x gravitational field strength
Average speed (ms-1)
distance (m) / time (s)
Average velocity (ms-1)
displacement (m) / time (s)
Period of a pendulum (s)
total time (s) / number of swings
Weight (N)
mass (kg) × gravitational field strength (ms-2)
Force (N)
mass (kg) × acceleration (ms-2)
Density (kgm-3)
mass (kg) / volume (m3)
Hooke's law: Force (N)
constant (Nm-1) × extension (m)
Pressure (Pa)
force (N) / area (m2)
Fluid Pressure (Pa)
density (kgm-3) × gravitational field strength (ms-2 or Nkg-1) × height (m)
Work (J)
force (N) × distance moved (m)
Power (W)
work (J) / time (s)
Kinetic Energy (J)
1/2 × mass (kg) × velocity2 (ms-1)
Gravitational potential energy (J)
mass (kg) × gravitational field strength (ms-2 or Nkg-1) × height (m)
Efficiency (%)
useful power output (W) / total power input (W) × 100
Efficiency (%)
useful energy output (J) / total energy input (J) × 100