Chapter 5 Flashcards

1
Q

What is collecting power in a telescope

A

It is how big a telescope is and how much light it collects

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2
Q

What is focusing power in a telescope

A

It is how it uses its mirrors and lenses to bend the path of light and create images

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3
Q

What is resolving power in a telescope

A

It is how clear the image is and how many details show

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4
Q

How does the size of the telescope affect the image

A

The size is directly proportional to the light collected, more light collected means a brighter image is shown.

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5
Q

What two methods does focusing power use

A

Refraction and reflection

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6
Q

What is refraction

A

It is the bending of light due to it shifting between one medium to another and changing speed

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7
Q

What telescopes are called refractors

A

Ones that use lenses to collect and focus light

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8
Q

What are disadvantages of refractors

A

Large lenses are extremely expensive, a large lens is only supported in the middle and will sag, dispersion causes images to have colored fringes, many lens materials absorb short-wavelength light

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9
Q

What are reflecting telescopes

A

What astronomers mainly use today, are telescopes that use mirrors to focus the light

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10
Q

How do reflecting mirrors work

A

A secondary mirror may be used to deflect the light through a hole in the primary mirror and focus the light

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11
Q

How do astronomers deal with large mirrors in reflecting telescopes

A

They developed multi-mirror instruments and extremely thin mirrors

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12
Q

What are the 3 styles of reflectors

A

Prime focus, cassegrain focus, and Newtonian focus

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13
Q

How does a prime focus reflector work

A

Light comes in and bounces off the primary mirror into a mounted camera hanging in the middle of the telescope

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14
Q

How does a cassegrain focus reflector work

A

Light comes in and bounces off the primary mirror, and then bounces off again off of a hanging secondary mirror in the middle back to the observer

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15
Q

How does a Newtonian reflector work

A

Light comes in and bounces off the primary mirror, it then hits a diagonal hanging mirror in the middle and into the observers eyes

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16
Q

What is diffraction

A

It is when waves pass through a narrow opening

17
Q

How does diffraction affect how we see an object

A

A diffracted point source of light appears as a point surrounded by rings of light. EX: the sun

18
Q

What is resolving power and what limits it

A

Resolving power is the ability for a telescope to gather detail, it is limited by the wave nature of light and its diffraction

19
Q

How can resolution be increased

A

It can be increased by a larger telescope diameter

20
Q

How can a larger resolution diameter be achieved

A

By the use of an interferometer which simultaneously combines the observations from two or more widely spaced telescopes

21
Q

What are the 3 ways of detecting light

A

The human eye, photographic film, electronic detectors

22
Q

What is photographic film

A

It chemically stores data to increase sensitivity to dim light. Very inefficient as only 4% of photons are recorded

23
Q

What are electronic detectors

A

Incoming photons strike an array of semiconductor pixels that are connected to a computer. Efficiencies of 75% possible

24
Q

What are the non visible wavelengths and what emits them

A

Cold gas= emits radio, dust clouds= emit infrared, hot gases= x-rays

25
Q

What are false color images

A

They are images typically used to depict wavelengths and distributions in non visible observations

26
Q

What are advantages of space based telescopes

A

Freedom from atmospheric blurring , freedom from atmospheric absorption

27
Q

What are advantages from ground bass telescopes

A

Larger collecting power, can be easily fixed

28
Q

What is scintillation (twinkling)

A

It is the refraction of light from stars, it can be caused by temperature and density in pockets of air that are constantly shifting

29
Q

What can improve distorted seeing for telescopes

A

Adaptive optics that employ a powerful laser correcting scintillation

30
Q

How do computers help telescopes gather data

A

Solve equations, move telescopes and feed information to detectors, convert data into useful form, creates networks for communication and data exchange