Chapter 16- Life of Stars Flashcards

1
Q

what are the basic steps in a stars life

A
  • competition between gravity and pressure
  • thermal pressure
  • radiation pressure
  • turbulence
  • rotation (centrifugal force)
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2
Q

first step of stars life

A

stars form a cold dense cloud of dust and gas called nebula

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3
Q

emission nebula

A

RED=HYDROGEN

  • hydrogen atoms in these regions are ionized by high energy radiation =lost an electron
  • this is how fluorescent lights work
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4
Q

Reflection Nebula

A

BLUE=DUST

  • dust cloud surrounding newly formed stars
  • dust scatters visible light causing it to be blue
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5
Q

Dark Nebula

A

BLACK

  • cloud of dust and gas so dense that it blocks out background stars
  • very little material there but cloud covers so much space
  • the most promising site for new stars to form
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6
Q

what can astronomers determine from absorption spectrum lines

A

the composition of interstellar gas

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7
Q

molecular cloud

A
  • most of the matter is molecules

- very very very cold

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8
Q

what causes the compression of molecular clouds

A
  • spiral density waves in galaxies
  • supernova explosion
  • cloud collisions
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9
Q

in the third step, what does the cloud release

A

photons, therefore making it to become a protostar

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10
Q

more massive stars do what?

A

move to the main sequence faster

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11
Q

what would happen if the cloud were not able to radiate away its thermal energy

A

pressure would keep increasing

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12
Q

protostar

A
  • often difficult to see in visible light because it still surrounded by cloud
  • infrared light allows us to see through the cloud because it penetrates dust
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13
Q

what would happen to a protostar that formed without any rotation at all?

A

no rotation=no disk=no planets

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14
Q

final step in becoming a star

A
  • temp and pressure become high enough for thermonuclear fusion t begin
  • pressure balances gravity causing collapse to stop
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15
Q

smaller than ___ can’t sustain fusion

A

0.08Msun

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16
Q

more massive than ___ would blow apart

A

150Msun