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Today! From Earth’s Perspective: Celestial Motion: Stellar Motion

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Presentation on theme: "Today! From Earth’s Perspective: Celestial Motion: Stellar Motion"— Presentation transcript:

1 Today! From Earth’s Perspective: Celestial Motion: Stellar Motion Solar Motion Planetary Motion

2 Celestial Motion Some stars and constellations
Are circumpolar—never rise or set. Celestial Motion

3 Constellation vs Asterism!

4 A constellation is one of
88 listed ‘states’ or regions in the sky: like Orion.

5 An asterism is not on the list
Of 88, but forms a shape In the sky: like the Big Dipper, Part of the constellation Ursa Major.

6 Finding Planets: Once you find the North Star,
Turn around 180 degrees— The Ecliptic and the planets will be in the sky toward the South. Finding Planets:

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8 The stars (at a given time of night) shift 1 degree a day
Because the earth is orbiting the sun. Thus the sidereal day is 23 hours and 56 minutes: It is the time for a star to return to the same place In the sky.

9 Solar motion: Mean solar day--24 hours by definition. Return of sun to same angle of view relative to the horizon.

10 seasons caused by tilt of earth’s axis,
solstices--maximum and minimum light, equinoxes equal light on northern and southern hemisphere.

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12 Planetary motion: retrograde motion--apparent backtracking of
planets in sky from earth's perspective. inner planets--Me and Ve --stay within 'maximum elongation'. conjunction vs opposition

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15 Mercury 8/30/02 Above Cloud Center w/ Venus Upper Left

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