lifecycle Flashcards
1
Q
- large dense cloud of gas and dust
A
stellar nebula
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
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
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
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
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
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
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
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
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
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
12
Q
SA and temp is determined by
A
brightness and magnitude