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P1A Topic 1
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P1A Topic 1
Solar System
- Geocentric Model
- Ancient greeks
- Everything orbited the earth in circles
- Heilocentric model
- Introduced Copernicus 1543
- Condemned by the church
- Galileos observation of Jupiter's moons
- Sun
- Current model
- Ellipiticals
- Geocentric Model
Waves
- Properties
- Amplitude (height of the wave)
- Frequency (waves per second)
- Wavelength (distance of one peak to the next)
- Speed (How fast)
- 2 types
- Transverse (the vibrations are 90 degrees to the direction of travel)
- Longitudinal (the vibrations are along the same direction of travel)
- Waves transfer energy and information without transferring matter.
- Properties
Reflection
- Wave hits boundary between one medium and another.
- The angle of reflection r is the same as the angle of incidence i
- Occurs because of a change in density.
- air to glass.
Refraction
- EM waves travel slower in more dense.
- Hits face on, no refraction, same direction.
- Hits at a angle wave changes direction.
- bending effect
- Air to glass bends towards the normal
- Glass to air bends away from the normal
Lenses
- Converging lens (convex)
- Causes rays to converge to a focus
- Diverging lens (concave)
- Causes rays to diverge
- Focal point one at the front, one at the back.
- Focal length
- Distance from the lens to its focal point
- A real image is there (projected on a screen) a virtual is not (can not be projected on a screen)
- Converging lens (convex)
Telescopes
- Refracting telescope
- In a refracting telescope, the objective lens forms a image inside the tube. Eyepiece then magnify's it.
- Objective lens = Convex lens
- The rays are so far away they're pretty much parellel
- In a refracting telescope, the objective lens forms a image inside the tube. Eyepiece then magnify's it.
- Reflecting telescope
- Uses two mirrors and a eyepiece lens.
- Refracting telescope
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- Summary of the topic with everything you need for the exam
- Created by
- James Disley
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