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Astronomy(universe)
Term | Definition |
---|---|
Big Bang theory | A greatly accepted theory on how the Earth was formed. |
The Doppler Shift towards the red end of the spectrum is evidence of what? | That the universe is expanding. |
Solar Nebular theory | Theory on how stars and solar system form. |
How do all stars start off? | As a solar nebula that eventually collapses. |
How do stars form? | They form by condensation and gravitational compression of the nebula. |
Solar Nebula | Huge, vast clouds of ice, gas, and dust. |
What is a star's lifespan? Does the star change? | The lifespan is infinite; star evolves over time. |
What controls a stars lifespan, ultimate fate, and how it evolves. | Its weight |
What is the order of less massive stars? | Nebula, protostar, main sequence star(born), white dwarf, and the black dwarf (death). |
List the order of massive stars. | Nebula, main sequence star (born), supernova, and neutron star (death) |
Define galaxies. | Collection of billions of stars. |
List the types of galaxies. | The spiral, elliptical, and irregular. |
What galaxy is our solar system located in? | The Milky Way |
Define black holes. | The end of the life cycle of some super giant (massive) stars usually after the supernova stage post a supernova explosion. |
How do black holes in the middle of the galaxy effect other stars. | They allow the stars to gain velocity so they can orbit around the black hole rather than get sucked into the center. |
The ground-based information we get about the universe by satellites gather what type of information? | Electromagnetic radiation ( infrared, ultraviolet, and X- rays) |
Light- year | Distance light travels in one year |
What is measured in light years? | Distances in the universe |
Blue giant | Star that put a lot of energy out and lasts only hundreds to millions of years |
When are heavier elements above iron produced? | When the Blue Giant becomes a supernova. |
Russel (H-R) | A diagram that shows the relationship between absolute magnitude in relation to their surface temperatures. |