Chapter 5 Flashcards

(48 cards)

1
Q

Order of waves (left to right)

A
gamma rays,
x-rays, 
ultraviolet, 
infrared, 
radio.
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2
Q

all light… (speed)

A

travels at same speed (300,000 km/s.)

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3
Q

what is wavelength?

A

the distance between adjacent peaks of the electric (and magnetic) field.

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4
Q

longer wavelength =

A

lower frequency

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5
Q

shorter frequency =

A

higher frequency which is dangerous

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6
Q

higher frequency equals

A

higher energy

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7
Q

c = (equation)

A

3.0 x 10^8 m/s

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8
Q

Atomic number =

A

of protons

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9
Q

Atomic Mass Number =

A

of protons + neutrons

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10
Q

the nucleus is 100,000 times smaller…

A

but contains all masses

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11
Q

Nucleus contains…

A

protons(red) and neutral neutrons (grey)

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12
Q

isotopes :

A

same # of protons but different # of neutrons (4He, 3He)

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13
Q

Molecules:

A

consists of two or more atoms (h2o, CO2)

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14
Q

how do light and matter interact?

A

emission
absorption
transmission
reflection or scattering

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15
Q

Emission means

A

to emit light

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16
Q

Absorption means

A

to absorb light

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17
Q

Transmission means

A

to pass light

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18
Q

why is a rose red?

A

it reflects red light

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19
Q

each type of atom has a ?

A

unique set of energy levels

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20
Q

each transition corresponds to..

A

a unique photon energy, frequency, and wavelength

21
Q

when do energy levels for electrons vary? (hydrogen)

A

from one element to another

22
Q

Downward _________ produce a unique pattern of ________ lines. (Emits a ______ of a specific ______)

A

transitions, emission

Photon, frequency

23
Q

Lower than red

A

Infrared. Slow movements

24
Q

Upward transitions produce

A

A pattern of ABSORPTION lines at the same WAVELENGTH

25
From level 1 to level 2 it needs...
Ultraviolet
26
Amount of nm that can send electron from level 2 to level 4?
486.1 nm
27
Hotter objects emit
More light
28
Hotter objects have
Higher average energy
29
Why is Betelgeuse red?
It's surface is cooler than that of the sun
30
How do we generally measure the Doppler Effect?
From shifts in the wavelengths of spectral lines
31
Doppler shift tells us only about the part of
An objects motion toward or away from us
32
Rotating planet
Gives both red and blue shifted lines
33
How do telescopes help us learn about the universe?
- Telescopes collect more light than our eyes | - telescopes can see more detailed than our eyes
34
More light than our eyes ➡️
Light collecting area
35
More detail than our eyes ➡️
Angular resolution
36
Largest Optical Telescope?
10.4m - Gran Telescopio Canarias (2007)
37
2nd largest optical telescope?
10.2m - South African Large Telescope (2005)
38
3rd largest optical telescope?
10m keck 1, Keck 2 (1993/1996)
39
Diameter of Radio telescope in Puerto Rico?
305 meters
40
Cons of Radio Telescope?
Very limited view, could only see in zenith
41
What emits X-Rays!?
Million degree gas
42
What does the first set of nested mirrors do?
Deflects X-rays to the second set
43
What does the 2nd set do?
Deflects X-rays a second time to the focus point
44
1st reason why we put telescopes into space?
Light pollution (avoid light from human sources)
45
2nd reason why we place telescopes in space
Turbulence causes twinkling which Blurs Images (turbulence is in earths atmosphere)
46
3rd reasons why we put telescopes in space?
Atmosphere absorbs most of EM spectrum, including all UV and Xray and most infrared.
47
What is interferometry?
A technique that allows two or more telescopes to work together TO OBTAIN THE ANGULAR RESOLUTION of a large telescope
48
which is hottest? A) blue star B) red star C) planet that emits only infrared light
A) blue star | Blue stars are hotter than red