Visible Light And The Solar System Flashcards

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1
Q

What is the geocentric model

A

A model of the solar system in which everything orbits the earth

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2
Q

What is a heliocentric model

A

A model of the solar system where everything orbits the sun

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3
Q

How did Galileo realise the heliocentric model was true

A

Using an early telescope, he discovered Jupiter had moons by tracking there paths, this showed that not everything orbited the earth

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4
Q

What is refraction

A

The change of speed and direction of a wave when it enters a new material

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5
Q

What is the interface in refraction

A

The point where refraction occurs, the boundary between two materials

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6
Q

What is the normal

A

A perpendicular line to the interface

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7
Q

What is the incident ray

A

The ray that enters the new medium

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8
Q

What is the refracted ray

A

The ray after the incidence ray has refracted

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9
Q

What is the ange of incidence and angle of refraction

A

Angle of incidence is the angle the incidence ray entered to the normal
Angle of refraction is ange the refracted ray is to the normal

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10
Q

What is a converging/convex lense

A

A lens that is curved outwards on both sides so it become thicker the closer to the middle

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11
Q

Wat are the properties of a convex lens

A

Refracts light inwards, the thicker it is, the greater the angle of refraction and the closer the focal point

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12
Q

What is the focal point

A

The point in which refracted light rays meet

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13
Q

What is the focal length and how can it be found

A

The length between the lens and the focal point, can be found by focussing the image onto a piece of paper and measuring the distance between the paper and the lens

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14
Q

How does a refracting telescope work

A

Light enter the objective ( a convex lens) lens that’s in a tube, this refracts the light and an eyepiece lens the magnifies the image

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15
Q

What is the difference between a real and virtual image

A

A real image. The rays actually meet where the image is seen, it can be put onto a screen such as paper
A virtual image, the rays appear to come from the image but don’t, it can’t be shown on a screen. E.g. Mirrors make virtual images

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16
Q

What are the problems with refracting telescopes

A

They need to be very long for a good magnification
If the lens insnt perfect, the colours wont be correct, it’s hard to make a large lens perfect
As some light is always reflected as well as refracted on the boundary, it’s hard for them to magnify faint images such as distant stars

17
Q

How does a reflecting telescope work

A

Light enters the tube and reflects of a curved primary mirror, this focuses the parallel rays towards the secondary mirror, this reflects the light into the magnifying eyepiece

18
Q

What are transverse waves

A

Waves in which movement of wave is perpendicular to movement of energy. S waves and electromagnetic waves are transverse

19
Q

What are longitudinal waves,

A

Waves that travel in pulses such as sound and look like this

||| | | | |||||||| | | | | | | |||||

20
Q

What is frequency and its unit and formula

A

Amount of waves per second, measured in Hz hertz. Formula is

Amount of waves divided by time in seconds

21
Q

What is wavelength

A

Length of one wave, distance between two crests or two troughs

22
Q

What is amplitude

A

Furthest distance from middle of wave, crest to the middle

23
Q

Wave length formulas

A

Distance(M)/time(S)

Frequency(Hz)*wavelength(M)