THE Milky Way 2 Flashcards

(42 cards)

1
Q

what is the diffuse band of light across the sky

A

Milky Way

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2
Q

what is the “milky light” caused by?

A
  • due to stars

- Galileo, 1610

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3
Q

why does our galaxy have a very flattened (disk-like) shape?

A

to see the concentration of stars

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4
Q

why did Herschels think that sun was approx at center of MWG?

A

they counted roughly same number of stars in all directions

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5
Q

what did Kapteyn discover about motion of stars and how?

A

that they were due to orbit of stars about Galaxy center

-doppler shift

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6
Q

globular clusters

A

extremely compact star cluster

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7
Q

star cluster

A

stars bound together by gravity

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8
Q

what did Harlow Shapley do in order to get distances to globular clusters?

A

used RR Lyrae variable stars

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9
Q

RR Lyrae stars have predictable what….?

A

luminosities

-allows us to measure distances into space

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10
Q

what did the discovery that globular clusters were offset from Sun tell astronomers?

A

sun was at edge of Galaxy and galaxy was much larger than Kapteyn estimated

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11
Q

What did the Kapteyn and Shapley models neglect the effects of in terms of measuring distances to stars?

A

neglected the effects of dust that lies between stars (interstellar medium)

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12
Q

what color brightness does dust reduce more?

A

it reduces blue light brightness more than red light brightness

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13
Q

what is the effect of dust blocking blue light better than red light?

A

stars look redder than they would if there was no dust

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14
Q

what is a very reliable measure of temperature?

A

spectral type

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15
Q

what kind of wavelength makes us able to see past the dust?

A

infrared wavelengths

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16
Q

what is the temperature of dust?

A

cold, 10-20 Kelvin

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17
Q

at what wavelengths does thermal dust emission occur?

A

very long infrared or radio wavelengths

18
Q

interstellar medium contains more gas or dust?

19
Q

does gas produce visible light?

A

no

  • too far away from stars
  • too cold
20
Q

energy difference in atomic hydrogen atoms?

A

energy diff is small, so can be readily excited by collisions in cold interstellar medium

21
Q

how are molecules formed in the denser regions of the interstellar medium?

A

the atomic gas can undergo chemical reactions

22
Q

when were radio spectral lines produced by quantized rotation of molecules detected?

A

1960s and 1970s

23
Q

does it take little or lots of energy to set a molecule into rotation?

A

takes little energy

-this emission can be produced by very cold molecular gas

24
Q

where do stars form?

A

in the dense, molecular clouds

25
how do individual stars and planetary systems form?
gas in molecular clouds fragments and collapses
26
visible material in MWG by mass...
90% stars | 10% gas/dust (interstellar medium)
27
MWG structure
spiral galaxy with a central bar
28
what is the spiral pattern a result of?
spiral density waves
29
"the wave pattern moves thru that galactic disk, but what 3 things do not remain in the spiral arms?
stars, gas, and dust
30
why do stars, gas, and dust bunch up?
due to the spiral density wave
31
what do the spiral arms represent a mixture of?
crowding of stars and interstellar medium
32
what is the spiral density wave?
moves around galaxy, compressing stars/gas/dust and rarifying
33
what does gas compressed in the spiral density wave do?
initiates the gravitational collapse of the gas to form dense molecule clouds and eventually stars
34
what do spiral arms represent?
waves of star formation in the gaseous disk
35
what kind of stars delineate the arms well? (3 characteristics)
young, luminous, massive stars
36
who discovered the two stellar populations and when?
Walter Baade, 1940s | Pop I and Pop II
37
population I stars
young, disk stars | -abundant in elements heavier than H and He
38
population II stars
old, bulge and halo stars
39
what do the two stellar populations have differences in?
age, size, color, orbits, amounts of heavy elements
40
Population I star orbits?
orbits confined to the disk of the Milky Way
41
Population II star orbits?
often have elliptical orbits that extend into the halo
42
recycling in the galaxy
MWG recycles material from gas to stars back to gas and the process repeats -enriches MWG in fusion products (heavy elements)