Chapter 6 Flashcards

1
Q

What is an astronomer’s most important tool?

A

A telescope

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2
Q

What are the two primary types of optical telescopes?

A
  1. Refracting

2. Reflecting

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3
Q

What does a reflecting telescope use for collecting and focusing incoming light?

A

A primary mirror, a secondary mirror, and an eyepiece on the side of the telescope

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4
Q

What does a refracting telescope use for collecting and focusing incoming light?

A

An objective lens & eyepiece

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5
Q

What is the focal plane?

A

The plane, perpendicular to the optical axis of a lens or mirror, on which an image is formed

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6
Q

What is the focal point?

A

The point at which light from a very distant object converges after being refracted or reflected

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7
Q

What is the focal length?

A

The distance from the lens or mirror to its focal point

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8
Q

What type of telescope does chromatic aberration occur in?

A

Refracting telescopes

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9
Q

How can chromatic aberration be corrected?

A

You add in a second lens that is made from a different kind of glass

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10
Q

What is chromatic aberration?

A

Its when the lens acts slightly like a prism. It bends different colored lights by different amounts

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11
Q

What is the best resolution that a given telescope can achieve?

A

Diffraction limit

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12
Q

What’s the advantage of launching a telescope above earth’s atmosphere?

A

They aren’t affected by astronomical seeing

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13
Q

Which dimensions of the refracting telescope determine its magnification?

A

Focal lengths of the objective lens / focal length of the eyepiece

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14
Q

Describe the advantages of reflecting telescopes over refracting telescopes

A
  1. No chromatic aberration

2. The mirror can be supported by a bracket on it’s back

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15
Q

What is spherical aberration?

A

Light from different parts of the mirror converge at different focal points due to the shape of the mirror

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16
Q

What are the two ways that you can correct spherical aberration?

A
  1. You can use a parabolic mirror instead of a spherical one

2. You can put a correcting lens in front of the mirror

17
Q

What criteria would you employ to evaluate a telescope when you want to buy one? Explain

A
  1. Light-gathering power - Provides a brighter image

2. Resolving power - Provides sharp and crisp images

18
Q

Compare an optical reflecting telescope and a radio telescope. How are they different?

A

Since radio waves are much longer, radio telescopes have to be bigger. Also, optical telescopes work during the night while radio telescopes work during the day

19
Q

Compare an optical reflecting telescope and a radio telescope. What do they have in common?

A

They both use a curved reflecting surface to focus the incoming radiation

20
Q

What is the optical window and the radio window?

A

They are wavelength regions where our atmosphere is transparent

21
Q

Why isn’t there an X-ray window or an ultraviolet window?

A

Our atmosphere is not transparent to these wavelength ranges, so the waves aren’t able to reach the earth’s surface

22
Q

Why do we need Gamma-ray, X-ray, UV and Infrared telescopes? Explain.

A

So we can study extremely hot objects

23
Q

How do you find the magnification of a reflecting telescope?

A

Focal length of primary mirror / focal length of eyepiece

24
Q

Explain the different designs of reflecting telescopes

A

You have a primary mirror and a secondary mirror, so your head doesn’t block some of the light