lifecycle Flashcards

1
Q
  • large dense cloud of gas and dust
A

stellar nebula

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2
Q
  • early stage in star formation
  • forms when a region of stellar nebula collapses under gravity and heats up.
  • as it grows, it gathers more material and the core gets hotter.
  • core becomes hot and dense enough for nuclear fusion , birthing a new star.
A

protostar

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3
Q
  • stable and long-lasting phase of the lifecycle.
  • fuses hydrogen to helium in its core, producing energy that makes stars shine
  • like our sun
  • eventually evolves into red giants as they exhaust hydrogen fuel.
A

main sequence

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4
Q
  • occurs when a star has exhausted most of hydrogen fuel and has begun the process of dying.
  • star expands and cools, making it appear larger and redder.
  • core contracts the heat up, leading to fusion of heavier elements like helium.
  • large size+low surface temp
  • gravity contracts core, allowing enough pressure for helium to fuse to carbon.
  • outer layers drift away in shockwave, leaving the carbon core.
A

red giant

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5
Q
  • a region of space of cosmic gas and dust formed by the cast-off outer layers of dying stars
  • outer layers drifting away
A

planetary nebula

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6
Q
  • stellar core that’s left behind after a dying star has exhausted its nuclear fuel
  • carbon core
  • maintaining energy from nuclear fusion.
  • no longer fusing and won’t collapse further
  • fades as energy depletes
A

white dwarf

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7
Q
  • small cooled remnant of white dwarf that emits no detectable light energy.
  • dead star made of carbon, now cold due to loss of all remaining energy.
A

black dwarf

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8
Q
  • end of lifecycle and explodes in a burst of light.
  • gravity causes a catastrophic collapse of the core
  • iron atoms are crushed and electrons are pushed into the nuclei
  • rapid increase in temp and repulsive electrical forces in the core cause a massive, bright, short-lived explosion.
A

supernova

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9
Q
  • region of space that has a gravitational field so intense that no matter or radiation can escape.
  • product of massive stars
A

blackhole

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10
Q
  • formed when a massive star runs out of fuel and collapses, crushing together every proton and electron into a neutron
  • remaining extremely dense core
  • strong magnetic field
  • rapid spin
  • no fusion
A

neutron star

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11
Q
  • large star, extremely bright, great luminosity
  • several magnitudes brighter than a giant star and several times greater in diameter
  • large radius for its mass and temp
  • high mass
  • core under high pressure and temps
  • fuses helium to iron (most stable nucleus)
  • fusion stops at iron, and the star can’t release further energy from the core.
A

supergiant

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12
Q

SA and temp is determined by

A

brightness and magnitude

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