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Seasonal Motion & Ecliptic. “Motion” Debriefing Stars circle NCP counterclockwise –For circumpolar stars: E  W if above Polaris, but W  E if below Polaris.

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Presentation on theme: "Seasonal Motion & Ecliptic. “Motion” Debriefing Stars circle NCP counterclockwise –For circumpolar stars: E  W if above Polaris, but W  E if below Polaris."— Presentation transcript:

1 Seasonal Motion & Ecliptic

2 “Motion” Debriefing Stars circle NCP counterclockwise –For circumpolar stars: E  W if above Polaris, but W  E if below Polaris Stars move E  W but also up (rising) and down The sun AND the stars move around the observer, so the sun stays (approx.) fixed amongst the stars

3 Daily Motion: View changes in hours

4 Seasonal Motion: View changes in months At the same time, say midnight, different constellations are high in the sky if you observe a month or so later (or earlier)

5 The Apparent Motion of Stars at Different Latitudes Apparent motion: motion as it appears in the sky This is due to the position (latitude) of the observer on earth, and the fact that the earth rotates about its axis This can also be explained by a competing theory: that there is a celestial sphere which rotates around the motionless earth.

6 The observation of these different star movement patterns made it obvious to humans early on that we live on a sphere Change your observation spot on the spherical earth, and you will change the pattern of motion you observe

7 Daily and yearly motion intertwined Solar vs Siderial Day –Earth rotates in 23 h 56 m –also rotates around sun  needs 4 min. to “catch up” Consequence: stars rise 4 minutes earlier each night (or two hours per month, or 12 hours in ½ year)  After 1/2 year we see a completely different sky at night!

8 Seasonal Motion Daily Rising and Setting: –Due to the rotation of the Earth around its axis –Period of rotation: 1 siderial day= 23 h 56 m 4.1 s –1 solar day (Noon to Noon) = 24 h –Stars rotate around the North Star – Polaris (Anim)Anim Seasonal Changes: –Monthly differences caused by Earth’s orbit around sun –AnimationAnimation

9 The Zodiac throughout the Year Example: In Winter sun in Sagittarius, Gemini at night sky; in summer sun in Gemini, Sagittarius at night sky

10 The Sun shifts its position on the Celestial Sphere. Therefore its visibility changes seasonally

11 The Ecliptic plane & the Ecliptic

12 Zodiacal signs vs. Constellations -360/12=30, so each zodiacal sign is exactly 30 degrees “long” -0 degrees: Aries, 30 degrees: Taurus, 60 degrees: Gemini, 90 degrees: Cancer, etc. “Constellation” is a modern, well-defined term - Some constellations are big, some are small on the celestial sphere “Zodiacal sign” is the old way of dividing the year and the Sun’s path into 12 equal parts

13 Homework Figure out maximal altitude of the sun in these steps –Where is NCP (what is its altitude angle)? –Where is therefore the celestial equator? –How high is the sun on the celestial sphere above/below the celestial equator? –Add or subtract this angle from the altitude of the celestial equator

14 Reminder: iSkylab 1 due in two weeks, Sep 23 Observe! Ask questions! Already demonstrated Option 1 measurement (shadow of a stick  altitude of the Sun) Will construct a quadrant

15 iSkylab: Sun Option What: Determine how the height of the sun above the horizon at a specific time is changing as the days pass by measuring the length of the shadow it casts with a gnomon (essentially a stick in the ground). Time: Once you know how to do it, this only takes a minute per observation. Commitment: Do this over several, not necessarily consecutive days, at exactly the same time. Weather: Need to see the shadow for a minute, so can do on partly cloudy, possibly hazy but not overcast days. Shadow Gnommon To Sun

16 iSkylab: Moon Option 1 What: Determine the height of the moon above the horizon with the help of a quadrant (essentially a bob dangling from a protractor), and see how it changes as the days go by. Time: Once you know how to do it, this only takes a minute per observation. Commitment: Do this over several, not necessarily consecutive days, at exactly the same time. Weather: Need to see the moon for a minute, so can do on partly cloudy, possibly hazy but not overcast days.

17 iSkylab: Moon Option 2 What: Determine the position of the moon with respect to the stars by sketching the position and the shape of the moon and the bright stars in the sky. Document changes as the days go by. Time: Once you know how to do it, this takes several minutes per observation. Commitment: Do this over several, not necessarily consecutive days, exact time does not matter. Weather: Need to see the moon and the stars for several minutes, so it needs to be a cloudless night with good seeing.


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