Topic 1 - Visible light and the solar system Flashcards

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1
Q

What is the geocentric model?

A

Everything orbited the earth.

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2
Q

What is the heliocentric model?

A

All planets orbit the sun, which is at the centre of the universe.

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3
Q

who thought of the heliocentric model?

A

Copernicus

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4
Q

What evidence helped support the heliocentric model?

A

Galileo discovered moons orbiting jupiter which showed that not everything was orbiting the earth proving the geocentric model wrong

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5
Q

what does the current model state?

A

all the planets in our solar system orbit the sun but these orbits are elliptical rather than circular

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6
Q

What did early astronomers use to study the stars

A

naked eye but this was only useful for mapping things positions

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7
Q

What are the advantages of telescopes?

A

magnify images so they can be seen in more detail.
see objects at larger distances
help learn what the universe is made of.
Can be sent into space to avoid light being absorbed by the atmosphere
Can use cameras

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8
Q

What advantages are there for using digital cameras with telescopes

A

Can ‘zoom in’ to see things in more detail
makes it easier to monitor an object by taking pictures at different times.
Can see faint objects by allowing a long exposure time.

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9
Q

What is wavelength

A

the distance from one peak to the next

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10
Q

What is frequency

A

how many complete waves there are per second. Measured in hertz

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11
Q

What is amplitude

A

The height of the wave from the midline to the peak

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12
Q

What do waves transfer

A

energy and information without transferring matter

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13
Q

What is a transverse wave

A

the vibrations are perpendicular to the direction of travel

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14
Q

give examples of transverse waves

A

EM waves

S-Waves

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15
Q

What is a longitudinal wave

A

the vibrations are parallel to the direction of travel

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16
Q

give examples of longitudinal waves

A

Sound

P-Waves

17
Q

What is an oscilloscope

A

shows things as transverse waves even sound

18
Q

what is the relationship between the angle of incidence and the angle of reflection when a wave is reflected

A

i = r

19
Q

Why is light reflected

A

when theres a change in destiny some of the wave is reflected

20
Q

What happens when a wave is refracted?

A

the material its travelling in changes density so the speed changes and sometime the direction of the wave

21
Q

What happens when a wave goes into a denser material

A

it slows down and the direction moves towards the normal

22
Q

What is a real image

A

When the light from an object comes together to form an image on a ‘screen’

23
Q

What is a virtual image

A

When rays of light are diverging so the light from the object appears to be coming from a completely different place

24
Q

Give an example of a virtual image

A

Magnifying glass

Reflection

25
Q

What is a converging lens

A

convex (blues outwards)
Causes parallel rays of light to move together (converge) and focus
Focal point is where rays hitting the lens parallel to the axis meet
Image is flipped

26
Q

Describe an experiment to find the focal length of a lens

A

Clamp lens to one end of a track, clamp piece of white card further down the track.
Set up the equipment near a window with the lens directed at a distant object.
Move card along the track until the image is focused and clamp it so it doesn’t move.
Measure the distance between the centre of the lens and the card and thats the focal length

27
Q

Describe a refracting telescope

A

Objective lens focuses the rays of light to form a real image at the focal point. the eyepiece lens then magnifies the image so you can see it

28
Q

describe a reflecting telescope

A

A large concave mirror (primary mirror) collects the light and reflects the light onto a smaller concave mirror in front of the focal point. The smaller mirror (secondary mirror) reflects light through a hole in the centre of the primary mirror and an eyepiece lens magnifies the image so you can see it.