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Star Notes
| Question | Answer |
|---|---|
| Life Cycle of a Star | All stars begin life in the same way. A cloud of dust and gas, also known as a nebula , becomes a protostar, which goes on to become a main sequence star. |
| Interstellar Medium | Interstellar medium is the space between the stars. |
| Nebula | A cloud of gas and dust in outer space, visible in the night sky either as an indistinct bright patch or as a dark silhouette against other luminous matter. |
| Protostar | A contracting mass of gas which represents an early stage in the formation of a star, before nucleosynthesis has begun |
| Equilibrium | A state in which opposing forces or influences are balanced. |
| Star | Stars are huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores |
| Main Sequence | A series of star types to which most stars belong, represented on a Hertzsprung–Russell diagram as a continuous band extending from the upper left (hot, bright stars) to the lower right (cool, dim stars). |
| Red Giant | A star that has low surface temperature and a diameter that is large relative to the sun. |
| Planetary Nebula | Expnding shells of luminous gas that are from a Planetary nebula, any of a class of bright nebulae that are expanding shells of luminous gas expelled by dying star. |
| White Dwarf | A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula. |
| Black Dwarf | As white dwarfs cool down over the next few trillion years, they'll grow dimmer, eventually freeze solid, and become black dwarf stars that no longer shine. |
| Red Super Giants | A red supergiant is an aging giant star that has consumed its core's supply of hydrogen fuel. |
| Supernova | A supernova happens where there is a change in the core, or center, of a star. One of the stars, a carbon-oxygen white dwarf, steals matter from its companion star. |
| Neutron Star | Neutron star, any of a class of extremely dense, compact stars thought to be composed primarily of neutrons. Neutron stars are typically about 20 km (12 miles) in diameter. |
| Black Hole | A black hole is a place in space where gravity pulls so much that even light can not get out. |
| (H-R) Hertzsprung–Russell diagram | It plots the temperature of stars against their luminosity |
| Luminosity | Luminosity is an absolute measure of radiated electromagnetic power |
| Brightness | The quality or state of giving out or reflecting light |
| Absolute Magnitude | The magnitude (brightness) of a celestial object |