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643209
The earth in the universe
Descripción
GCSE (P1) Physics Mapa Mental sobre The earth in the universe, creado por zakbarwell el 17/03/2014.
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p1
physics
physics
p1
gcse
Mapa Mental por
zakbarwell
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Resumen del Recurso
The earth in the universe
The Solar System
Formed around 5000 million years ago
Started off as clouds of dust and gas
Pulled together by forces of gravity
Nuclear fusion created the sun
Smaller masses of the solar system:
Planets - 8 large masses that orbit the sun
Moons - small masses orbit planets
Asteroids - rocky masses orbit the sun
The Sun
Suns energy comes from nuclear fusion
Hydrogen nuclei fuse together to produce nucleus with larger mass
Speed of Light
Speed of light: 300,000km/s
Vast distance measured in Light Years
We see things as it was in the past
Nearest galaxy 2.2 million light years away
Measuring Distances in Space
Relative Brightness
Dimmer the star is further away it is
But stars vary in brightness so can never be 100%
Parallax
Stars measured at 6 month intervals
Measurements then used to calculate distance from earth
The closer a star the more it will move
Distant Stars
Everything we know about stars are from; Radiation (Ultraviolet and infrared), Visible Light.
Light pollution from all our electric lights make it hard to see stars
Redshift
If a wave is moving away/towards a observer, there will be a change in frequenxy and wavelength
If a source of light moves away from an observer, the wavelengths of light in its spectrum are longer than if it wasn't moving
This is known as REDSHIFT, because the wave lengths 'shift' towards the red end of the spectrum.
Continental Drift
Alfred Wegener came up with the theory
he saw that all continents fitted together like a jigsaw
he found that the rock types and fossils were the same as if they did all fit together
Waves
Longitudinal
The motion of the wave is backwards and forwards
Sound travels in longitudinal waves
Transverse
The motion of the wave, angles of the particles are 90 degrees
Light and water travel in transverse waves
Features
Amplitude - From the undisturbed position line to the crest.
Wavelength - Distance between corresponding points on 2 adjacent disturbances
Frequency - Number of waves passing through a point in one second
Tectonic Plates
Conservative Plate boundaries - When plates slide past each other and huge stress and strain builds up and is eventually released
Constructive Plate Boundaries - when the plates move away from each other leaving the magma to rise the solidifying creating more land
Destructive Plate Boundaries - As plater move towards eachother one is forced under and the other one is pushed up creating volcanoes
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