• Shuffle
    Toggle On
    Toggle Off
  • Alphabetize
    Toggle On
    Toggle Off
  • Front First
    Toggle On
    Toggle Off
  • Both Sides
    Toggle On
    Toggle Off
  • Read
    Toggle On
    Toggle Off
Reading...
Front

Card Range To Study

through

image

Play button

image

Play button

image

Progress

1/17

Click to flip

Use LEFT and RIGHT arrow keys to navigate between flashcards;

Use UP and DOWN arrow keys to flip the card;

H to show hint;

A reads text to speech;

17 Cards in this Set

  • Front
  • Back
Geocentric model
The belief that the Sun, Moon, planets and stars all orbited the Earth in perfect circles
Heliocentric model
States that the Earth and planets all orbit the Sun at the centre of the Universe (replaced the Geocentric model)
Galileo's observations of Jupiter's moons
Showed not everything was in orbit around the Earth proving the Geocentric model wrong
Wavelength
The distance from one peak to the next
Frequency
How many complete waves pass a point per second (measured in Hz)
Amplitude
The height of the wave
Speed (m/s) =
Frequency (Hz) x Wavelength (m)
Wave speed (m/s)
Distance (m) / Time (s)
Transverse waves
S-waves on strings and springs e.g. ripples on water.
Includes all EM waves and Light
Longitudinal waves
P-waves including sound and ultrasound e.g. a slinky spring
Angle of reflection (r) =
Angle of incidence (i)
Focal point
Where the rays hitting the lens parallel to the axis all meet
Focal length
The distance from the lens to its focal point
Normal
The line at right angles to the surface
Refracting telescope
Made up of an objective lens and an eyepiece lens and uses two converging lenses
Reflecting telescope
Uses concave mirrors and a converging lens
Converging eyepiece lens
Used to magnify the image