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Seasonal Motion. 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.

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Presentation on theme: "Seasonal Motion. 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."— Presentation transcript:

1 Seasonal Motion

2 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!

3 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 Seasonal Changes: –Monthly differences caused by Earth’s orbit around sun

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

5 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

6 Another Complication: Axis Tilt! The Earth’s rotation axis is tilted 23½ degrees with respect to the plane of its orbit around the sun (the ecliptic) It is fixed in space  sometimes we look “down” onto the ecliptic, sometimes “up” to it Path around sun Rotation axis

7 Position of Ecliptic on the Celestial Sphere Earth axis is tilted w.r.t. ecliptic by 23 ½ degrees Equivalent: ecliptic is tilted by 23 ½ degrees w.r.t. equator!  Sun appears to be sometime above (e.g. summer solstice), sometimes below, and sometimes on the celestial equator

8 Precession of the Equinoxes Precession period about 26,000 years “The dawning of the age of Aquarius”

9 Is the sun rising in the East? Typically NOT! See for yourself! –Study variation of the rising/setting points of the sun over time –Need at least 10 sunrises or sunsets; more is better –Measure time and azimuth (angle relative to North) –Note position of sunrise/sunset on horizon –Measure angle to that position relative to some fixed landmark (mountain, etc.)

10 The Seasons Change of seasons is a result of the tilt of the Earth’s rotation axis with respect to the plane of the ecliptic Sun, moon, planets run along the ecliptic


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