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ES VOCAB CARDS hec
STUDING FOR EXAM
| Question | Answer |
|---|---|
| Constellation | Group of stars in the night sky. 88 modern constellations. most are seasonal; some are circumpolar. |
| Circumpolar Constellation | A constellation that seems to circle Polaris (The North Star) |
| Absolute Magnitude | The amount of light a star actually gives off. |
| Apparent Magnitude | The amount of light received on Earth. |
| Parallax | Apparent shift in the position of an abject when viewed from two different positions. The nearer an object is to the observer, the greater the parallax is. |
| Light Year | Distance that light can travel in one year; approx. 9.5 trillon Km. per year |
| Astronomical Unit | 1 au = 95 million mi. |
| Photosphere | Lowest layer where sunlight originates Often called the "surface" of the sun. 6000 K temp. |
| Chromoshpere | Above the photosphere 2000 km. thick 2000-10,000 km. "transition zone." |
| Corona | Largest layer of the sun's atmosphere Millions of kilometers thick Temps. are as high as 2 million k. Where solar wind originates. |
| Sunspots | Dark (cooler) areas onthe photosphere Show that the sun rotates, although not like the Earth. Occur in a solar activity cycle of 11 years. |
| Prominence | Magnetic field caused by sunspots Huge arching column of gas Speeds range from 600-1000 Km/s. |
| Solar Flare | Violent eruptions of gases near a sunspot. |
| Coronal Mass Ejection (CME) | Happens when large amounts of electrically charged gas are ejected suddenly from the sun's corona; caused by sunspots. May damage satellites and interfere with radio and power distribution equipment. Cause auroras |
| Our Sun is an Average Star | Middle-aged Yellow light One unique feature: It is not close to any other stars. |
| Hertzprung Russel (H-R) Diagram | Developed in the early 1900's Shows the relationship between temperature and absolute magnitude. |
| Non-Main Sequence Stars | 90% follow the main sequence Hot, dim star= white dwarf Cool, bright star giant Largest giants= supergiants |
| Supernova | the collapsed core of a supergiant |
| Neutron Star | Collapsed core of a star that is 1.4 to 3 times more massive than the sun. |
| Black Hole | Collapsed core of a star that is more than 3 times more massive than the sun; nothing can escape from a black hole. |
| Life of a Star | Main Sequence (low mass star) Nebula, main sequence progression, red giant, white dwarf, black dwarf. Non-main sequence progression, red supergiant, supernova, then Either a neutron star or a black hole. |
| Galaxy | A large group of stars, gas, and dust held together by gravity. Our galaxy= the Milky Way Grouped into clusters; ours is the Local Group which contains about 45 galaxies. |