1. ASTRO 101 Principles of Astronomy

2. Instructor: Jerome A. Orosz (rhymes with “boris”) Contact: Telephone: 594-7118 E-mail: orosz@sciences.sdsu.eduorosz@sciences.sdsu.edu WWW: http://mintaka.sdsu.edu/faculty/orosz/web/ http://mintaka.sdsu.edu/faculty/orosz/web/ Office: Physics 241, hours T TH 3:30-5:00

3. Text: “Discovering the Essential Universe, Fifth Edition” by Neil F. Comins

4. Course WWW Page http://mintaka.sdsu.edu/faculty/orosz/web/ast101_fall2012.html Note the underline: … ast101_fall2012.html … Also check out Nick Strobel’s Astronomy Notes: http://www.astronomynotes.com/

5. Homework/Announcements Homework due Thursday, October 25: Question 6, Chapter 7 (What role did Charon play in enabling astronomers to determine Pluto’s mass?). Exam 2, Thursday November 1

6. Next: Chapter 5 and Chapter 6: Other Planets and Moons.

7. Comparing the Inner Planets

8. Next: The Giant Planets

9. The Giant Planets The giant planets are Jupiter, Saturn, Uranus, and Neptune.

10. The Giant Planets The radii are between about 4 and 11 times that of Earth. The masses are between 14 and 318 times that of Earth.

11. The Giant Planets The radii are between about 4 and 11 times that of Earth. The masses are between 14 and 318 times that of Earth. However, the densities are between 0.7 and 1.8 grams/cc, and the albedos are high.

12. The Giant Planets The radii are between about 4 and 11 times that of Earth. The masses are between 14 and 318 times that of Earth. However, the densities are between 0.7 and 1.8 grams/cc, and the albedos are high. The planets are composed of light elements, mostly hydrogen and helium.

13. The Gas Giants The composition of the giant planets, especially Jupiter, is close to that of the Sun.

14. The Gas Giants The composition of the giant planets, especially Jupiter, is close to that of the Sun. The internal structures of these planets is completely different from that of the Earth.

15. The Gas Giants The composition of the giant planets, especially Jupiter, is close to that of the Sun. The internal structures of these planets is completely different from that of the Earth. In particular, there is no hard surface.

16. The Gas Giants These planets are relatively far from the Sun (more than 5 times the Earth-Sun distance), so heating by the Sun is not a big factor.

17. Jupiter Jupiter is by far the most massive planet in the solar system (it contains about 2/3 of the solar system mass outside the Sun). It has the largest radius of any solar system planet, and it rotates the fastest (once every 10 hours). It has at least 63 moons. In many categories, Jupiter is the most extreme case.

18. Jupiter’s Weather Owing to its rapid rotation, Jupiter has a very turbulent atmosphere, which is composed mostly of methane and ammonia (both hydrogen rich).

19. Jupiter’s Weather Owing to its rapid rotation, Jupiter has a very turbulent atmosphere, which is composed mostly of methane and ammonia (both hydrogen rich).

20. Jupiter’s Weather Owing to its rapid rotation, Jupiter has a very turbulent atmosphere, which is composed mostly of methane and ammonia (both hydrogen rich).

21. Jupiter’s Weather The most famous feature on Jupiter is the Great Red Spot.

22. The Great Red Spot The Spot is at least 150 years old. It is basically a giant hurricane, roughly three times the size of Earth. Smaller features are also evident.

23. The Great Red Spot

24. Similar storm systems have been observed to form recently.

25. Jupiter’s Interior There is no way to directly study the deep interior parts, we rely on computer models. The interior should be hot (35,000 K), with a solid core, possibly surrounded by liquid. The gaseous outer atmosphere surrounds molecular and liquid metallic hydrogen and helium.

26. Jupiter’s Atmosphere The atmosphere of Jupiter (and Saturn) consists of poisonous gas (ammonia and ammonium hydrosulfide) covering a layer of water vapor.

27. Jupiter’s Moons Jupiter has 4 fairly large moons, discovered by Galileo in 1610, and at least 59 other moons, all significantly smaller.

28. Jupiter’s Moons The largest moon is larger than Mercury. Image from Nick Strobel (http://www.astronomynotes.com)http://www.astronomynotes.com

29. Jupiter’s Moons The 4 Galilean moons have small rocky or iron cores. They have similar densities to our Moon, indicating that each contains a thick layer of water and ice.

30. Io The surface of Io is unlike that of any other solar system body. There are no impact craters, so its surface must be young.

31. Io There are active volcanoes on Io, the only place in the solar system outside of Earth where this is the case.

32. Io There are active volcanoes on Io, the only place in the solar system outside of Earth where this is the case.

33. Volcanoes on Io Io’s surface is constantly altered by volcanoes.

34. Volcanoes on Io Io’s surface is constantly altered by volcanoes. On Earth, the energy for geological activity comes from radioactivity.

35. Volcanoes on Io Io’s surface is constantly altered by volcanoes. On Earth, the energy for geological activity comes from radioactivity. However, Io’s mass is relatively small, so it should have no radioactivity left.

36. Volcanoes on Io Io’s surface is constantly altered by volcanoes. On Earth, the energy for geological activity comes from radioactivity. However, Io’s mass is relatively small, so it should have no radioactivity left. The heating source turns out to be Jupiter’s gravity, which compresses Io as its orbits.

37. Europa Europa has a very smooth surface, and it may have an ocean of liquid water underneath the surface.

38. Europa Europa has a very smooth surface, and it may have an ocean of liquid water underneath the surface. Could there be primitive life?

39. Other Jovian Satellites The rest of Jupiter’s moons are small and have an irregular shape. These may be fragments of a once larger body or captured asteroids.

40. Jupiter’s Rings Jupiter also has dark rings, discovered by Voyager in the late 1970s.

41. Next

42. Saturn The most obvious feature of Saturn is its large ring system, which has been known for more than 300 years.

43. Saturn’s Atmosphere The composition of Saturn is similar to that of Jupiter. Saturn also rotates rapidly, once every 10 hours or so. Saturn’s weather is like that on Jupiter, although the contrast between different bands is much less.

44. Saturn Note the band-like structure in the clouds.

45. Saturn Note the band-like structure in the clouds.

46. Saturn The rings are very thin, and gaps are evident, even from the ground. They consist of fragments of ice and ice- covered rocks.

47. Saturn The rings are very thin, and gaps are evident, even from the ground. They consist of fragments of ice and ice- covered rocks.

48. Saturn Small satellites can cause some of the rings to ripple or to have braided structure.

49. Saturn Small satellites can cause some of the rings to ripple or to have braided structure.

50. Saturn’s Rings From Voyager, we know the rings are composed of hundreds or thousands of “ringlets”.

51. Saturn’s Moons Saturn has 1 very large moon (Titan), 10 moderate size moons, and a few dozen much smaller ones.

52. Saturn’s Moons Saturn has 1 very large moon (Titan), 10 moderate size moons, and a few dozen much smaller ones.

53. Saturn’s Moons Saturn has 1 very large moon (Titan), 10 moderate size moons, and a few dozen much smaller ones. Titan is the only moon with an atmosphere.

54. Titan Titan’s atmosphere is mostly hydrogen with a substantial amount of methane. There are organic molecules, but it is probably too cold for life to have evolved.

55. Titan There are lakes of liquid methane, as well as large flat areas.

56. Uranus and Neptune These distant planets were not known before the invention of the telescope. They are each about 4 times the diameter of the Earth, and about 15 times more massive than the Earth. They are made up mostly of H and He, but with a bit more heavy elements.

57. Uranus and Neptune Both planets appear blue-green because of the methane gas mixed in with the hydrogen. The weather patterns are much less apparent. Solar heating is not important since they are far from the Sun.

58. Uranus and Neptune Both planets appear blue-green because of the methane gas mixed in with the hydrogen. The weather patterns are much less apparent. Solar heating is not important since they are far from the Sun.

59. Uranus and Neptune Both planets are believed to have rocky cores surrounded by compressed water and liquid hydrogen and helium.

60. Seasons on Uranus The rotation axis of Uranus is inclined by about 90 degrees relative to its orbital plane. This gives rise to highly exaggerated seasons.

61. Uranus’s Rings Uranus also has rings, which were discovered in 1977 when Uranus passed directly in front of a distant star. They are very dark, reflecting only about 2% of the sunlight.

62. Uranus’s Rings Uranus also has rings, which were discovered in 1977 when Uranus passed directly in front of a distant star. They are very dark, reflecting only about 2% of the sunlight.

63. Uranus’s Rings Uranus also has rings, which were discovered in 1977 when Uranus passed directly in front of a distant star. Recent advances in telescopes and cameras allow for a better view than was previously possible.

64. Uranus’s Rings Recent advances in telescopes and cameras allow for a better view than was previously possible. Note the system of moons that orbit in the equatorial plane. They take their names from Shakespeare’s A Midsummer’s Night Dream and other works.

65. Neptune’s Rings Neptune also has dark rings, discovered by Voyager in the late 1980s.

66. Rings All of the gas giants have rings, although the rings of Saturn are by far the largest. They appear to be relatively short-lived (only millions of years) and composed of material from moons that wandered to close to their parent planets.

67. Neptune’s Moons Neptune has at least 13 moons, most of which appear to be captured asteroids. The largest moon, Triton, was captured into a retrograde orbit, and will soon be destroyed by Neptune’s gravity.

69. Next: Chapter 7 (Dwarf Planets and Small Solar System Bodies)