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Elarth Ch 1 and 2
Celestial Sphere
| Question | Answer |
|---|---|
| ASTRONOMICAL UNIT | AVERAGE DISTANCE FROM EARTH TO THE SUN (15O,OOO,OOO km OR 93,000,000 MILES |
| LIGHT YEAR (LY) | DISTANCE LIGHT TRAVELS IN A YEAR |
| CONSTELLATION (OLD) | ONE OF 88 STELLAR PATTERNS IN THE SKY (USUALLY MYTHOLOGICAL ANIMALS, PEOPLE, GODS, OR OBJECTS |
| CONSTELLATION (NEW) | THE REGIONS OF THE SKY CONTAINING THE 88 CONSTELLATIONS |
| ZENITH | THE POINT ON THE SKY DIRECTLY OVERHEAD |
| NORTH CELESTIAL POLE | THE POINT ON THE CELESTIAL SPHERE DIRECTLY ABOVE THE EARTH'S NORTH POLE |
| SOUTH CELESTIAL POLE | THE POINT ON THE CELESTIAL SPHERE DIRECTLY ABOVE THE EARTH'S SOUTH POLE |
| PRECESSION | THE SLOW CHANGE IN THE DIRECTION OF THE EARTH'S AXIS OF ROTATION, ONE CYCLE TAKES ABOUT 26,000 YEARS |
| ROTATION | THE TURNING OF A BODY ABOUT AN AXIS THAT PASSES THROUGH IT |
| REVOLUTION | THE MOTION OF A BODY IN A CLOSED PATH AROUND A BODY OUTSIDE OF ITS VOLUME |
| ECLIPTIC | THE APPARENT PATH OF THE SUN AROUND THE SKY |
| VERNAL EQUINOX | ONE OF 2 PLACES WHERE THE ECLIPTIC AND THE CELESTIAL EQUATOR CROSS. ABOUT MARCH 21, BEGINNING OF SPRING |
| SUMMER SOLSTICE | POINT ON THE CELESTIAL SPHERE WHERE THE SUN IS AT ITS MOST NORTHERN. BEGINNING OF SUMMER, ABOUT JUNE 22 |
| CELESTIAL EQUATOR | IMAGINARY LINE AROUND THE SKY DIRECTLY ABOVE THE EARTH'S EQUATOR |
| AUTUMNAL EQUINOX | ONE OF 2 PLACES WHERE THE ECLIPTIC AND THE CELESTIAL EQUATOR CROSS. ABOUT SEPT 22, BEGINNING OF FALL |
| ANGULAR DIAMETER | MEASURE OF THE SIZE OF AN OBJECT IN THE SKY |
| PERIHELION | THE POINT WHEN AN OBJECT IS CLOSEST TO THE SUN |
| APHELION | THE POINT AT WHICH AN OBJECT IS FARTHEST FROM THE SUN |
| CIRCUMPOLAR | ANY CONSTELLATION SO CLOSE TO THE POLE IT DOESN'T SET |
| ALTITUDE | DEGREES ABOVE THE HORIZON |
| AZIMUTH | DEGREE MEASUREMENT, BEGINNING AT NORTH, FOLLOWING THE HORIZON THROUGH EAST |