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

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

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

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

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 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 :

7 Circumpolar Constellations at our Latitude.

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

10

11 Solar motion: Mean solar day--24 hours by definition. Average return of sun to same angle relative to the horizon.

12 NOTES: Planetary motion: retrograde 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

13 Mars going RETROGRADE: journeying backward against constellations.

14 Venus: always within 46 degrees of the sun— its MAXIMUM ELONGATION (Mercury within 26 degrees)

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

16 Note conjunction and opposition as seen from the Earth.


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