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PSQ4W2ASTRON
STARS
| Question | Answer |
|---|---|
| Hertzsprung-Russell diagram | shows the relationships and differences between stars; plots the luminosities and temperatures of stars. HR diagrams show how red giant stars are more luminous but have lower core temperatures than white dwarf stars. |
| Neutron star | star made almost entirely of neutrons; also called a pulsar when it rotates and emits electromagnetic radiation; what’s left over after a massive star goes supernova. |
| Nova | explosions of extra material off of a white dwarf; lasts for about a week and is much smaller than a supernova. |
| Planetary nebula | collection of gases ejected after a star dies; when a low-mass red giant runs out of helium, it will eject its outer layers and make a planetary nebula. |
| Protostar | formed when a nebula collapses under its own gravity; early stage of star development. |
| White dwarf | object left over after a low mass star runs out of helium; about the size of the Earth, but it is incredibly dense. |
| Luminous | emitting self-generated light; stars are luminous, planets and moons are illuminated |
| Plasma | state beyond gas when particles are ionized; commonly found in stars and neon signs |
| Blue stars | the hottest stars, while cooler stars glow red or yellow. |
| nuclear fusion | reaction on a star which is the result of heat intense enough to fuse hydrogen into helium; source of star’s energy |
| main sequence star | stage when star is doing nuclear fusion |
| pulsar | forms when a neutron star starts rapidly rotating and emits pulses of electromagnetic radiation |