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CHP 22 Origin
Origin of Modern Astronomy
| Question | Answer |
|---|---|
| astronomy | the scientific study of the universe - observation of clestial bodies and phenomena |
| geocentric | the concept of an Earth centered universe |
| orbit | the path of an object that goes around another object in space. |
| heliocentric | describes the view that the sun is at the center of the solar system |
| retrograde motion | the apparent motion westward motion of the planets with respect to the stars |
| ellipse | an oval - shape of planet orbits around the sun. |
| astronomical unit (AU) | average distance from Earth to the sun. 150 million kilometers |
| rotation | the spinning of a body, such as Earth, about its axis |
| revolution | the motion of one body about another - Earth's movement around the sun |
| precession | a slow motion of Earth's axis that traces out a cone over a period of 26,000 years. |
| perihelion | the point in orbit at which the planet is closest to the sun |
| aphelion | the place in the orbit of a planet where the planet is farthest from the sun |
| perigee | the point at which the moon is closest to earth |
| apogee | the point where the moon is farthest from the Earth |
| phases of the moon | the progression of changes in the moon's appearance during the month |
| solar eclipse | an eclipse of the sun; a solar eclipse occurs when the moon moves in a line directly between Earth and the sun, casting a shadow on Earth |
| lunar eclipse | an eclipse of the moon; a lunar eclipse occurs when the moon passes through Earth's shadow |
| crater | round depressions in the surface of the moon |
| ray | any system of bright elongated streaks, sometimes associated with a crater on the moon. |
| mare | the Latin name for the smooth areas of the moon formerly thought to be seas |
| rille | a long channel associated with lunar Maria - looks similar to a valley or a trench |
| lunar regolith | a thin, gray layer on the surface of the moon, consisting of loosely compacted fragmented material believed to have been formed by repeated impacts of meteorites |