1. The Sky http://www.phy.ohiou.edu/~mboett/PSC100/spring12/PSC100_spring12.html

2. If you look up into the sky, towards the south, then … 1.east is to your right, north is behind you, west is to your left. 2.east is to your left, north is behind you, west is to your right. 3.east is to your left, west is behind you, north is to your right. 4.east is to your right, west is behind you, and north is to your right. 5.east is behind you, west is to your left, north is to your right.

3. North EastWest South

4. The Celestial Sphere Zenith = Point on the celestial sphere directly overhead Nadir = Point on the c. s. directly underneath (not visible!) Celestial equator = projection of the Earth’s equator onto the c. s. North celestial pole = projection of the Earth’s north pole onto the c.s.

5. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the northern horizon; From geographic latitude – l (southern hemisphere), you see the celestial south pole l degrees above the southern horizon. Celestial equator culminates 90 o – l above the horizon. l 90 o - l

6. Example: New York City: l ≈ 40.7 0 Horizon North Celestial North Pole 40.7 0 South 49.3 0 Celestial Equator The Celestial South Pole is not visible from the northern hemisphere. Horizon

7. Athens, OH, is located at l ≈ +39 o. Where in the sky would you see the highest point of the celestial equator? 1.North, 39 o above the horizon. 2.South, 39 o above the horizon. 3.North, 51 o above the horizon. 4.South, 51 o above the horizon. 5.South, 45 o above the horizon.

8. Athens, OH: l ≈ 39 0 Horizon North Celestial North Pole 39 0 South 51 0 Celestial Equator Horizon

9. The Celestial Sphere (III)

10. Apparent Motion of the Celestial Sphere

11. Apparent Motion of the Celestial Sphere II

12. 1.Far off to the right 2.Far off to the left 3.Near the Zenith 4.Near the Nadir 5.Close to where it is now. Where will the sun be in the evening before sunset? A View of the Sugarloaf Mountain (Rio de Janeiro, Brazil) Sun’s position in the morning

13. The Magnitude Scale First introduced by Hipparchus (160 - 127 B.C.): Brightest stars: ~1 st magnitude (m v = 1) Faintest stars (unaided eye): 6 th magnitude (m v = 6) More quantitative: 1 st mag. stars apear 100 times brighter than 6 th mag. stars 1 mag. difference gives a factor of 2.512 in apparent brightness (larger magnitude => fainter object!)

14. The magnitude scale system can be extended towards negative numbers (very bright) and numbers > 6 (faint objects): Sirius (brightest star in the sky): m v = -1.42 Full moon: m v = -12.5 Sun: m v = -26.5

15. The Sun and its Motions (I) Earth’s rotation is causing the day/night cycle.

16. What is the name for the plane of the Earth’s orbit around the sun? 1.Earth plane 2.Solar plane 3.Epileptic 4.Ecliptic 5.Epiphany

17. The Sun and its Motions (II) Due to Earth’s revolution around the sun, the sun appears to move through the zodiacal constellations. The Sun’s apparent path on the sky is called the Ecliptic. Equivalent: The Ecliptic is the projection of Earth’s orbit onto the celestial sphere.

18. What is causing the seasons? 1.Brightness variations of the sun. 2.The Earth being closer to the sun in the summer and further away in the winter. 3.A steeper angle of incidence of the sun’s rays in the summer than in the winter. 4.A denser cloud cover in the winter than in the summer. 5.Stronger heat output from within the Earth in the summer than in the winter.

19. The Seasons (I) The Earth’s axis of rotation is inclined vs. the normal to its orbital plane by 23.5 0, which is causing the seasons.

20. The Seasons (II) The Seasons are only caused by a varying angle of incidence of the sun’s rays. They are not related to the Earth’s distance from the sun. In fact, the Earth is slightly closer to the sun in (northern- hemisphere) winter than in summer. Light from the sun Steep incidence → Summer Shallow incidence → Winter

21. The Seasons (III) Sun Earth in July Earth in January The Earth’s distance from the sun has only a very minor influence on seasonal temperature variations. Earth’s orbit (eccentricity greatly exaggerated)

22. When it’s summer in the U.S., it is … in Argentina 1.spring 2.summer 3.fall 4.winter 5.midnight

23. The Seasons (IV) Northern summer = southern winter Northern winter = southern summer

24. What happens to a spinning top that you set on a table top slanted? 1.It will immediately fall over 2.It will quickly adjust itself to a perfectly upright position. 3.It will wobble around in a circular motion around the vertical. 4.It will wobble around back and forth through the vertical position. 5.It will take off and become airborne.

25. Precession (I) Gravity is pulling on a slanted top. => Wobbling around the vertical. The Sun’s gravity is doing the same to the Earth. The resulting “wobbling” of the Earth’s axis of rotation around the vertical to the Ecliptic takes about 26,000 years and is called precession.

26. Precession (II) As a result of precession, the celestial north pole follows a circular pattern on the sky, once every 26,000 years. It will be closest to Polaris ~ A.D. 2100. ~ 12,000 years from now, it will be close to Vega in the constellation Lyra. There is nothing peculiar about Polaris at all (neither particularly bright nor nearby etc.)

27. What is the radius of the circle that the celestial north pole traces out on the celestial sphere in the course of a precession cycle? 1.90 o 2.45 o 3.39 o 4.23.5 o 5.66.5 o Radius

28. The Motion of the Planets (I) The planets are orbiting the sun almost exactly in the plane of the Ecliptic. The Moon is orbiting Earth in almost the same plane (Ecliptic). Jupiter Mars Earth Venus Mercury Saturn

29. The Motion of the Planets (II) All outer planets (Mars, Jupiter, Saturn, Uranus, Neptune and Pluto) generally appear to move eastward along the Ecliptic. The inner planets Mercury and Venus can never be seen at large angular distance from the sun and appear only as morning or evening stars.

30. Which planet is the most difficult one to observe? 1.Mercury 2.Venus 3.Mars 4.Jupiter 5.Saturn

31. Mercury appears at most ~28 0 from the sun. It can occasionally be seen shortly after sunset in the west or before sunrise in the east. Venus appears at most ~ 46 0 from the sun. It can occasionally be seen for at most a few hours after sunset in the west or before sunrise in the east.