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1. annular eclipse - • the moon is not close enough to the earth to completely block the sun, so the sun rings the moon
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1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

Jan 02, 2016

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Page 1: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

1. annular eclipse -

• the moon is not close enough to the earth to completely block the sun, so the sun rings the moon

Page 2: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

2. autumnal equinox

• when the sun crosses the celestial equator in the fall season, directly over the earth’s equator

Page 3: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

3.celestial coordinates

• points on the celestial sphere defined by declination and right ascension

Page 4: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

4. celestial equator

• line on the celestial sphere directly over the earth’s equator

Page 5: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

5. celestial sphere

• the inside of a sphere where the stars and other objects appear to be fixed

Page 6: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

6. constellation -

• a group of stars that appear to form a pattern

Page 7: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

7. crescent -

• moon phase that appears as a thin sliver, less surface visible than quarter moon

Page 8: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

8. declination -

• degree measure above or below the celestial equator

Page 9: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

9. diurnal -

• The daily progression of the Sun, Moon, planets and stars across the celestial sphere

Page 10: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

10. eclipse -

• event where one body passes in front of another, blocking the light from the light producing body

Page 11: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

11. eclipse season-

• season during which lunar and solar eclipses are possible

Page 12: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

12. ecliptic -

• path the Sun follows through the celestial sphere over the course of a year.

Page 13: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

13. equinox -

• times of the year when the Sun is directly over the equator

Page 14: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

14. full moon -

• all the viewable surface of the Moon is illuminated

Page 15: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

15. gibbous -

• more than half of the viewable surface of the Moon is illuminated

Page 16: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

16. light-year -

• the distance light travels in one year

Page 17: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

17. line of nodes -

• the lines where the plane of the Earth’s orbit and the plane of the Moon’s orbit cross

Page 18: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

18. lunar eclipse

• the shadow of the Earth falls on the Moon

Page 19: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

19. lunar phase -

• the apparent change of shape of the surface of the Moon as different amounts of the illuminated surface are visible

Page 20: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

20. new moon -

• none of the illuminated surface of the Moon is visible

Page 21: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

21. north celestial pole -

• point on the celestial sphere directly over north pole

Page 22: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

22. partial eclipse -

• not all of the surface of the object is covered by the shadow

Page 23: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

23. penumbra -

• the area where all the light from the Sun is not blocked

Page 24: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

24. precession -

• the ‘wobble’ of the Earth on its axis

Page 25: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

25. quarter moon -

• exactly half of the visible surface of the Moon is illuminated or shaded

Page 26: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

26. revolution -

• the movement of any object through its orbit

Page 27: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

27. right ascension

• the position of any object in the celestial sphere east or west of a beginning point

Page 28: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

28. rotation -

• the spinning of any object on its axis

Page 29: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

29. seasons -

• the changes in climatic conditions caused by Earth’s orbit and its tilt on its axis

Page 30: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

30. sidereal day -

• a day measured by the position of the stars

Page 31: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

31. sidereal month

• a month measured by the position of the Moon in the celestial sphere (measured by the stars)

Page 32: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

32. sidereal year -

• a year as measured by the position of the stars

Page 33: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

33. solar day -

• a day measured by the position of the Sun in the sky

Page 34: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

34. solar eclipse -

• the shadow of the Moon falls on the Earth

Page 35: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

35. south celestial pole -

• point on the celestial sphere directly over the south pole

Page 36: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

36. summer solstice -

• date when the Sun is as far north of the celestial equator as it will be

Page 37: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

37. synodic month -

• a month as measured by the phases of the Moon

Page 38: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

38. total eclipse -

• entire surface of the object is blocked,viewers are in the umbra

Page 39: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

39. tropical year -

• time it takes Sun to make one complete trip around the celestial sphere on the ecliptic

Page 40: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

40. umbra -

• eclipse area where all the light from an object is blocked

Page 41: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

41. vernal equinox -

• date in the spring season when the Sun is directly over the equator

Page 42: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

42. universe -

• the totality of all space, time, matter, and energy

Page 43: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

43. wane -

• when the size of the visible, illuminated surface of the Moon appears to shrink from one date to the next

Page 44: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

44. winter solstice -

• date when the Sun is as far south of the celestial equator as it will be

Page 45: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

45. wax -

• when the size of the visible, illuminated surface of the Moon appears to grow from one date to the next

Page 46: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

46. zodiac -

• the constellations through which the Sun passes over the course of a year

Page 47: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

1. Why is it important to astronomical science that the laws of physics as we know them apply equally well throughout the whole universe?

Page 48: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

• It’s the only way we can understand and predict occurrences in other areas of the universe.

Page 49: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

2. Why does the sun rise in the east and set in the west each day? Does the moon also rise in the east and set in the west? Why? Do the stars do the same? Why?

Page 50: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

• The sun, moon, and stars rise in the east and set in the west because the earth rotates from west to east.

Page 51: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

3. How many times in your life have you traveled around the sun?

• How old are you in years?

Page 52: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

4. Why do we have seasons on earth?• The Earth’s axial tilt causes the Sun’s heat

energy to fall more directly and less directly on certain areas of the Earth at different times of the Earth’s yearly orbit.

Page 53: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

5. Why do we see different stars in summer than in winter?• The night time side of the Earth faces

different directions in space at different times of the year.

Page 54: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

6. At what phase of the Moon would you expect there to be the most burglaries? Why?

• At new moon it is darkest.

Page 55: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

7. If one complete hemisphere of the Moon is always lighted by the sun, why do we see different phases of the moon? • The orbit of the moon around the Earth

causes the Sun’s rays to illuminate different areas of the surface of the Moon. We always see the same side of the Moon, so the fraction of that side that is illuminated changes.

Page 56: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

8. What causes a lunar eclipse? A solar eclipse?

• Lunar - Earth between Sun and Moon.

• Solar - Moon between Sun and Earth.

Page 57: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

9. What does the fact that there are both annular and total eclipses tell us about the Moon’s distance from the earth?• The distance from the Earth to the Moon

changes.

Page 58: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

10. Why aren’t there lunar and solar eclipses every month?• The Moon’s orbital plane is at an angle to

the plane of the Earth’s orbit.

Page 59: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

11. From what part’s of the earth is the Pole Star (Polaris) never visible?

• The south pole area.

Page 60: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

1. Cosmology –

• the study and descriptions of the universe

• for example, the geocentric model of the solar system (earth at the center) is one cosmology

Page 61: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

2. deferent -

the orbit of the planet in the Ptolemaic solar system

Page 62: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

3. direct motion -

the normal motion of a planet from west to east from one night to the next

Page 63: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

4. epicycle -

• the smaller circle in the orbit of a planet, in addition to the deferent in the Ptolemaic solar system

• explained the retrograde motion of the planets

Page 64: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

5. geocentric -

• the model of the solar system (cosmology) with the earth at the center

• everything orbited the earth

Page 65: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

6. parallax -

• The apparent shift in position of an object as it is viewed from different positions.

• The lack of observable parallax in the stars was one reason scientists did not believe the earth was moving.

Page 66: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

7. Ptolemaic model -

• Best geocentric model of the solar system.

• Consisted of 80 different circles.

Page 67: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

8. retrograde motion -

• When a planet is observed to move from east to west from one night to the next.

• The opposite of direct motion.

Page 68: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

9. solar system -

• The collection of all objects that orbit the sun.

• In the geocentric system, it was the collection of all objects that orbited the earth.

Page 69: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

10. triangulation -

• Using angles, trigonometry, and parallax to determine the distance to an object.

Page 70: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

1. What is parallax? Give an example.

• Parallax is the apparent shift in position of an object as it is viewed from different positions.

• When riding in a car, distant objects appear to be moving more slowly than nearby objects.

Page 71: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

2. What are epicycles and deferents?

• The deferent is the orbit of a planet; the epicycle is the smaller additional circle.

• Used in the Ptolemaic solar system.

Page 72: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.

3. Give a brief description of the Ptolemaic model of the universe.

• The earth is at the center, geocentric.

• The planets orbited in deferents.

• The planets also orbited in epicycles to explain retrograde motion. (See question 2.)

Page 73: 1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.