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Learn about the measurement of angles in the sky, the motion of the sun, and how it affects the seasons. Get started on your project and join an astrophotography session. Questions on motion are welcome!
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Miscellaneous announcements… • Homework 1 due today by 5:00. • Pick up Homework 2; solutions are on the web. • Get started on a project soon, if you haven’t already! • Astrophotographers: please see me after class. • Questions on motion of the stars? • Try out Sky View Café and/or Sky Chart III…
The Sun and the Seasons 6 September 2006
Today: • Measuring angles in the sky • How the sun moves through our sky • Seasons
Motion of the Sun • On any given day, the sun’s motion is essentially the same as that of a star (rises in the east, sets in the west). • The sun’s motion doesn’t quite keep up with the stars: It completes a 360º circle in 24 hours. • With respect to the stars, the sun appears to move once a year around a great circle, tipped 23.5º with respect to the celestial equator. • In late June (summer solstice), the sun is farthest north; in late December (winter solstice), the sun is farthest south. In late March and September (equinoxes), it’s on the celestial equator.
Motion of the Sun Facing south
Motion of the Sun Sun’s apparent path among the stars is called the ecliptic
Seasons Summer Winter (A one-square-meter surface, directly facing the sun, receives about 1000 watts of power.)