3.9 Astrophysics Flashcards

1
Q

How do you calculate the magnification of a refracting telescope?

A

(Angle subtended by image at eye) / (angle subtended by object at unaided eye)

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2
Q

What is normal adjustment?

A

Eye views parallel rays as if they’ve come from an object at infinity.

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3
Q

What are the disadvantages of refracting telescopes?

A

Chromatic aberration - Different wavelengths are refracted by different amounts so, the edges of an image appear coloured.
Spherical aberration
Light, usually blue/UV, are absorbed by the lens
Tube length must be very long for a good magnification
Distortion of lens
Lenses are heavy

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4
Q

What is spherical aberration?

A

When the shape of a lens isn’t fully parabolic, then light doesn’t converge at a single point.

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5
Q

What are the advantages of a cassegarian telescope?

A

Lighter and more compact
The mirror has no chromatic aberration
The objective can be made much bigger- better resolution

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6
Q

What are the disadvantages of a cassegarian telescope?

A

The secondary mirror obstructs light- there’s less light entering the telescope which decreases the brightness of the image.
Costly to maintain- recoating the mirror and cleaning
The eyepiece lens has spherical and chromatic aberration

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7
Q

What is the relationship between collecting power and the diameter objective lens?

A

Collecting power ∝ diameter^2

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8
Q

What property of the telescope does collecting power effect?

A

The higher the collecting power, the brighter the image.

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9
Q

What is angular resolution?

A

The smallest angle of separation between 2 objects which can be distinguished.

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10
Q

What happens to a wave when it passes through an aperture?

A

The wave is diffracted which can result in circular interference fringes. This leads to a loss of detail.

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11
Q

What is an airy disc?

A

The large central maximum on a diffraction pattern when light is diffracted. It is twice as wide as the other maxima in the pattern.

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12
Q

What is the Rayleigh criterion?

A

2 objects are resolvable when the first minimum of one airy disc coincides with the central maximum of the other.

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13
Q

What is quantum efficiency?

A

A measure of the effectiveness of an imaging device to convert incident photons into electrons

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14
Q

What is the quantum efficiency of a CCD?

A

> 70%

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15
Q

What is the quantum efficiency of the eye?

A

1% - 10%

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16
Q

What is the resolution of a CCD?

A

> 200 MP

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17
Q

What is the resolution of the eye?

A

Approximately 100m light sensitive cells in the retina.

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18
Q

What is the ‘convenience of use’ of a CCD?

A

It can be used in low temperatures of space
It can be used remotely
Detects a wider range of wavelengths
Exposure can last longer

19
Q

What is the ‘convenience of use’ of the eye?

A

You experience a loss of colour vision at low light levels

20
Q

Why are CCDs better than the naked eye?

A

Quantum efficiency is higher so, dimmer stars can be seen more easily.
CCDs can detect a wider range of wavelengths so, objects emitting non-visible light can be seen.
More convenient- image can be viewed remotely and recorded
Pixel size is smaller so, stars can be more easily seen as separate.

21
Q

How does a single dish radio telescope work?

A

It uses a big parabolic dish as a reflector and an aerial picks up the signal.
The larger the dish, the more energy per second it collects. Collecting power ∝ diameter^2

22
Q

What are the similarities between a radio telescope and an optical telescope?

A

The larger the diameter, the larger the collecting power, the larger the resolving power.

23
Q

What are the differences between a radio telescope and an optical telescope?

A

Wavelength used be a radio telescope are much longer so, is resolution is much lower than an optical telescope.

24
Q

What are the advantages of a radio telescope?

A

They are manoeuvrable, allowing the source of the wave to be tracked.

25
Q

How can radio telescopes be modified to increase resolution?

A

Multiple telescopes are linked together and their data can be combined to produce a single image. So, a resolution that is a thousand times better than an optical telescope can be produced.

26
Q

What are the disadvantages of radio telescopes?

A

They are affected by man-made interference from:
Radio transmissions
Mobile phones
Radar systems
Microwave ovens

27
Q

What is an alternative way in which radio telescopes can be made to make them cheaper?

A

Instead of a mirror, a wire mesh can be used where the precision of the dish must be about lambda/20 to avoid spherical aberration.
This makes construction easier and cheaper than optical telescopes.

28
Q

What is the structure of an IR or UV telescope?

A

Similar to an optical reflecting telescope.
But, CCDs are used as radiation detectors.
The mirrors have to be more perfectly made as the light has a shorter wavelength and therefore more affected by imperfections.

29
Q

Where are IR telescopes located and why?

A

They must be positioned at high altitudes in dry places as most IR is absorbed by water vapour in the atmosphere. But, ideally they are sent to pace.

30
Q

Where are UV and x-ray telescopes located and why?

A

They can be strapped to high altitude weather balloons, aeroplanes or sent into space as the radiation is absorbed by most of the upper atmosphere.

31
Q

What are the disadvantages of IR telescopes?

A

Can only be built in specific locations
They must be heat resistant and have its components cooled by liquid nitrogen to operate effectively.

32
Q

What are IR telescopes used for?

A

They’re useful for imaging relatively cool objects that don’t emit much visible light, like clouds of gas and dust where new stars are forming.

34
Q

What are UV telescopes used for?

A

Used to observe very hot stars with temperatures above 1000k that are dim and mostly emit UV.

35
Q

What are the disadvantages of x-ray telescopes?

A

They’re difficult to manufacture.
X-rays are either fully absorbed by or fully penetrate most materials. So, you need special components.
They must be outside the earths atmosphere.

36
Q

What are x-ray telescopes used for?

A

Observing extremely high energy emissions of matter entering a black hole.

37
Q

What is the structure of an x-ray telescope?

A

Grazing telescope. X-rays reflect if they graze the surface of a mirror. You can use multiple mirrors to gradually focus x-rays.

38
Q

What is the Hipparcos scale?

A

A first magnitude star is the brightest
A sixth magnitude star is the dimmest

39
Q

What is the difference in intensity between a first and sixth magnitude star?

A

A magnitude 1 star has an intensity 100 times greater than a magnitude 6 star.

40
Q

What is the intensity of a star?

A

The effective brightness

41
Q

Which factors affect the brightness of a star?

A

Luminosity- total energy emitted per second
Distance from earth

42
Q

How do you calculate the difference in brightness using the Hipparcos scale?

43
Q

What is a parsec?

A

The distance a star is from earth whne the angle of parallax is 1 arc second.