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Stars and Galaxies
| Term | Definition |
|---|---|
| Light-year | the distance light travels in a year, about 9.5 trillion kilometers |
| Apparent-magnitude | the brightness of a star when viewed from Earth |
| Absolute-magnitude | the apparent brightness of a star if it were viewed from a distance of 32.6 light-years; used to compare the true brightness of stars |
| Hertzsprung-Russel Diagram | a plot of stars according to their magnitudes and temperatures |
| Main-sequence star | a star that falls into the main-sequence category on the H-R diagram, contains the majority of stars, and runs diagonally from the upper left to the lower right on the H-R diagram |
| Binary star | one of two stars revolving around a common center of mass under their mutual gravitational attraction |
| Cepheid variable | a star whose brightness varies periodically because it expands and contracts; a type of pulsating star |
| Nova | a star that explosively increases in brightness |
| Protostar | a collapsing cloud of gas and dust destined to become a str; a developing star not yet hot enough to engage in nuclear fusion |
| Supernova | an exploding star that increases in brightness many thousands of times |
| Pulsar | a variable radio source of small size that emits radio pulses in very regular periods |
| Black hole | a massive star that has collapsed to such a small volume that its gravity prevents the escape of everything, including light. |
| Galaxy | a group of stars, dust, and gases held together by gravity |
| Hubble's Law | a law that states that the galaxies are retreating from the Milky Way at a speed that is proportional to their distance |
| Big Bang Theory | the theory that proposes that the universe originated as a single mass, which subsequently exploded |