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m&m 2.2

How We Use Astronomy

QuestionAnswer
Celestial sphere What appears to be a dome to which stars are attached
Horizon Separates the visible portion of the celestial sphere from the part we can't see
Zenith The point on the celestial sphere directly above an observer
Nadir The point on the celestial sphere directly below an observer
Celestial equator An imaginary line that encircles the heavens midway between the celestial poles
Celestial poles The ends of the earth's axis
Day The most basic unit of time
Meridian An imaginary line that is used to measure the motion of celestial objects
Sideral day One rotation of the earth relative to the stars. Also called sidus in Latin
Apparent solar day Equals the amount of time the sun takes to cross the meridian twice
Mean solar day The average length of the apparent solar day
Equation of time The difference between mean solar time and apparent solar time
Standard solar time When a traveler crosses into another time zone, they must their watch by exactly one hour and have the correct time
Ecliptic The path the sun follows in a year
Equinox Where the sun crosses the celestial equator. Two points
Vernal equinox The point when the sun crosses the celestial equator from south to north
Autumnal equinox The point when the sun crosses the celestial equator from north to south
Solstice A point on the ecliptic midway between the two equinoxes
Summer solstice Halfway between the vernal and autumnal equinoxes, the sun reaches its farthest point of the celestial equator
Torrid zone Extremely hot zones that are bounded on the north by an imaginary circle called the Tropic of Cancer and on the south by the Tropic of Capricorn
Frigid zones Extremely cold zones that are bounded on the north by an imaginary circle called the Arctic Circle and on the south by the Antarctic Circle
Seasons Because of the earth's elliptical orbit these are not equal in terms of days. Length depends on orbit and speed of earth
Temperate zones Located between the frigid and torrid zones which are neither hot nor cold
Precession of the equinoxes The process when the earth's axis traces a slow circle and the equinoxes are gradually shifting along the ecliptic. Takes 26,000 years to complete
Month Comes from Latin word for the period between one new moon and the next, moonth
The Gregorian calendar The system we now use because the original calendar we used was several days off
Pope Gregory XIII Issued a proclamation in 1582 which established a new calendar
Year The time it takes for the earth to revolve around the sun
Anno Domini Latin for "in the year of our Lord"
Week Instituted by god at the end of creation when He rested on the 7th day of creation and ordained it as a day of rest
Other calendars All of these calculate moon phases and have different year lengths
Created by: Jer Stephens
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