Telescopes Flashcards

1
Q

Give four optical advantages which a reflecting telescope has over a refracting telescope?

A

Collects more light as mirrors can be larger than lens, better revolving power as diameter of mirrors larger, no chromatic aberration and no spherical aberration

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2
Q

Explain chromatic aberration

A

Different wavelengths of light are refracted by different amounts meaning the image is blurred and has coloured edges

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3
Q

Explain spherical aberration

A

When axial rays converge to different focal points at different distances from the axis

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4
Q

Define quantum efficiency and state the value of it for a CCD and the eye

A

Ratio of the number of photons incident on a detector that are being detected to the total number of photons incident on the detector, >80% for CCD, 1% for eye

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5
Q

Describe a CCD and how it produces an image

A

Silicon chip divided into pixels, incident photons causes electrons to be released (number released proportional to intensity), which are trapped I potential wells forming a pattern which is processed to give an image

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6
Q

State the Rayleigh criterion

A

The resolution of two point objects is not possible if any part of the central spot of either image lies inside the first dark ring of the other image

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7
Q

What is the maximum mesh spacing of the reflector of a radio telescope (which is made from wire mesh) for effective reflection?

A

Wavelength/20

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8
Q

What is the angle alpha in a telescope in normal adjustment?

A

Angle sub tended by object at unaided eye

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9
Q

What is the angle beta in a telescope in normal adjustment?

A

Angle subtended by image at eye

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10
Q

Why can you see more stars when looking through a telescope than using the naked eye?

A

Telescopes have greater diameter objective lenses compared to pupil of the eye, meaning greater collecting power

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11
Q

Why are the images of stars never magnified by telescopes?

A

They are point objects

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12
Q

Explain why the image of a planet viewed using a telescope is not significantly brighter than the planet when it is viewed directly

A

This is because, although more light per second enters the eye when a telescope is used, the virtual image is magnified, so it is spread over a larger part of the field of view. As a result, the amount of light per second per unit area of the virtual image is unchanged

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13
Q

Give two disadvantages of using CCDs in astronomy

A

Expensive as they need to have a large number of pixels in a small area and need to be cooled to low temperatures to prevent the random emission of electrons (which cause ‘dark’ currents) which does not depend on intensity of light

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14
Q

Give two examples of objects in space which can be detected by infrared telescopes

A

Dust clouds and planets which are not hot enough to emit visible light

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15
Q

Give two disadvantages of infrared telescopes

A

Need the be cooled to stop infrared radiation from its own surface affecting measurements and some infrared radiation absorbed by water vapour in the atmosphere

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16
Q

Why must UV telescopes be on satellites and use reflectors?

A

UV radiation absorbed by atmosphere and glass (which lenses often made from)

17
Q

What range of radio waves can be transmitted through the Earth’s atmosphere?

A

0.001m - 10m