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ES ASTRO 2

Space and our Solar System

TermDefinition
Law of Orbits Kepler's First Law The orbital shape for any satellite is an ellipse
Law of Equal Areas Kepler's Second Law Satellites sweep through equal area in equal time. Practically speaking, this means they move fastest when nearest the orbited body
Law of Periods Kepler's Third Law Satellites further from the orbited body travel slower than those that are closer to the orbited body
Rotation The movement of a body about its axis. The earth, the moon, and the sun each exhibit rotation
Revolution The movement of a body in an orbital path around another body
Tilt The angle of a planetary axis measured against its orbital plane
Solstice When the sun's direct rays fall at either 23.5 degrees North or South latitude; the tropics of Cancer and Capricorn, respectively
Equinox Literally translated equal night. Direct rays of the sun shine directly at earth's equator. Every location on earth receives equal minutes of night and equal minutes of day
Waning Getting smaller
Waxing Geting Larger
Crescent The apparent shape of the moon when it is less than half illuminated
Gibbous The apparent shape of the moon when it is more than half illuminated
Lunar eclipse When the earth's shadow falls on the moon; or better, when the moon travels within the earth's umbra/penumbra. A lunar eclipse can only happen during a full moon.
Solar eclipse When the moon's shadow falls on the earth; or better, when the earth travels across the moon's umbra/penumbra. A solar eclipse can only happen during a new moon.
Maria Regions on the moon that appear darker in color. These are ancient lava beds, yest comprise the youngest rocks on the moon
Highlands Regions on the moon that appear lighter in color. These are the oldest rocks of the moon
Created by: MrGross
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