telescopes and Doppler Effect Flashcards

1
Q

refracting telescopes

A

use a lens to focus light

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Light is ref racted when

A

when it mov es from air to
glass or f rom glass to air

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

A curv ed lens will focus

A

A curv ed lens will focus parallel ray s of
light to a focal point

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

problem with lenses

A

(1) Lenses absorb light.
(2) Lenses sag.
(3) Good lenses expensiv e
and dif f icult to make.
(4) Chromatic aberration

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Largest refracting telescope

A

Yerkes Observatory, 102 cm in diameter

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Reflecting telescopes use a mirror to focus light

A

For a mirror, equal angles of incidence and
ref lection (independent of wav elength!)
A mirror shaped like a parabola
f ocuses parallel rays of light to a point

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

The primary purpose of a
telescope

A

is to gather light.
Telescope is a
“light bucket.”

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

of photons collected
each second is

A

proportional to the area
of lens (or mirror)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Area = pi/2 D2

A

where D is the diameter of
the lens or mirro

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Angular measures

A

360 degrees (360°) in a circle
60 arcminutes (60’) in a degree
60 arcseconds (60”) in an arcminute

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

The secondary purpose of a
telescope is to resolve fine detail.

A

two stars are resolved if they are seen as
two separate points.
Smallest angle resolv ed is proportional to
o stars are resolved if they are seen as
D = 1 inch 4.6 arcseconds
2.3 arcsecondsD = 2 inch
resolved

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Larger diameter mean

A

more light, higher
resolution

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Charge-coupled devices (CCDs)

A

capture images electronically

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Atmospheric blurring

A

Due to movements of
warmer and colder ‘cells’ in the atmosphere

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Modern telescopes use mirrors rather than lenses for all
of these reasons EXCEPT

A

Reflecting telescopes aren’t affected by the atmosphere
as much.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Telescope A has a diameter of 4 meters. Telescope B
has a diameter of 8 meters.
The light gathering power of B is ___ times
the light gathering power of A

A

4

17
Q

The angular resolution of an 8-inch diameter telescope
is better than a 2-inch diameter telescope by a factor of

A

4

18
Q

Observatory Sites

A

Best observatory sites are high, dry mountain peaks.
* dark skies, f ar from city lights
* many clear nights
* dry conditions (f or infrared observations)
* steady atmosphere (less ‘twinkling’)

19
Q

Radio telescopes use

A

reflecting
dish to focus waves onto an antenna.
For radio telescopes, as f or optical telescopes,
BIGGER is BETTER.

20
Q

Visible light

A

 = 500 nanometers

21
Q

microwave

A

> 1 millimeter

22
Q

radio

A

> 10 centimeters

23
Q

Two or more radio telescopes can be
combined to

A

to make a radio interferometer.
Example:
Very Large Array ,
New Mexico
27 dishes, each 25-m across
Light-gathering power =
Resolv ing power =
VLA, Socorro, NM
dish 130 meters across
dish 36 kilometers across

24
Q

Hubble Space Telescope

A

Height abov e ground: 600 kilometers
Diameter of mirror = 2.4 meters
Resolution =
0.05 arcseconds
(Resolution on ground is limited
to 0.5 arcseconds)

25
Q

Not all EM radiation can penetrate Earth’s atmosphere.

A

only radio and visible can fully penetrate

26
Q

Earth’s atmosphere is transparent in

A

“visual
window” and “radio window.

27
Q

Infrared light is absorbed by

A

water vapor in the atmosphere.
IR light is less af fected by gas and dust

28
Q

Ultraviolet

A

Emitted by hot stars, gas (50,000 K)
* Absorbed in the ozone lay er, 25 kilometers up

29
Q

X-rays

A

X-ray s are absorbed by most molecules in the atmosphere.
X-ray mirrors ref lect at very
shallow angles (‘grazing incidence’)
X-ray s are emitted by
extremely hot gas:
T > 300,000K

29
Q

X-rays

A

X-ray s are absorbed by most molecules in the atmosphere.
X-ray mirrors ref lect at very
shallow angles (‘grazing incidence’)
X-ray s are emitted by
extremely hot gas:
T > 300,000K

30
Q

Gamma rays:

A

absorbed by nearly everything.
Gamma ray s can’t be
f ocused, so images
are low resolution.
Produced by exotic
objects in v ery energetic
processes.

31
Q

The tendency of a wave to bend as it passes from one
transparent medium to another is called

A

refraction

32
Q

What causes stars to twinkle?

A

turbulence in the atmosphere

33
Q

doppler Effect

A

Christian Doppler (1842): If a source of waves moves toward you or
away f rom you, the wavelength is changed

34
Q

radial velocity

A

how f ast an object is moving
toward y ou or away f rom you

35
Q

The Doppler Effect in Light

A

The Doppler Effect in Light
Shif t depends upon the radial speed of the object:
Source moving toward you:
– Wav elength gets shorter = BLUESHIFT
Source moving away:
– Wav elength gets longer = REDSHIFT

36
Q

The Doppler Ef f ect causes light from a source moving away to

A

be shifted to longer wavelengths