1. ASTR-1010 Planetary Astronomy Day - 35

2. Solar Surface Close Up

3. Course Announcements Next Lab: 51 Pegasi: Discovery of a New Planet51 Pegasi: Discovery of a New Planet Homework Chapter 10: Due Monday April 19. Homework Chapter 11: Due Friday April 23. Homework Chapter 12: Due Wednesday April 28. Homework Chapter 21: Due Wednesday April 28. -this is extra credit. The last 1 st Quarter moon observing nights are: Tuesday (April 20) & Thursday (April 22) 8:00 pm both nights. Exam 4 and “Final”: Friday, April 30 – 1030 am

4. Uranus has thin rings and several moons

5. The Moons of Uranus

6. Miranda: a broken world

7. The Chevron

8. Grooves and Cracks

9. Ariel

10. Umbriel

11. Titania

12. Oberon

13. The Moons of Neptune

14. Triton

15. Triton has a thin atmosphere

16. Nitrogen Geysers on Triton

17. Proteus

18. Pluto Very small – 1/6 the mass of Earth’s Moon. Binary planet: Pluto/Charon. Has properties like comets: –Eccentric orbit –Icy composition (probably) Member of the Kuiper Belt Objects, maybe not even the largest one.

19. Pluto and Charon Dr. R. Albrecht, ESA/ESO Space Telescope European Coordinating Facility/NASA

23. Pluto: distant ice world

24. Pluto Facts

25. Pluto was discovered by Clyde Tombaugh in 1930

26. Charon was discovered by James Christy in 1978

27. Pluto & Charon System by HST

28. Pluto & Charon are not big

29. Pluto and Charon Eclipsed each other from 1985- 1990

30. Like Uranus, Pluto orbits on its side

31. Pluto Has An Atmosphere!

32. Pluto is covered in Methane Frost

33. Interior of Pluto & Charon?

34. All is speculation until the New Horizons mission arrives in 2016

36. © 2007 W.W. Norton & Company, Inc. 21st CENTURY ASTRONOMY, 2/e 36 Concept Quiz – Pluto Pluto is very different from the gas giants in all ways but: A.Its mass. B.Its composition. C.Its location in the Solar System. D.The shape of its orbit.

37. Chapter 12 Lecture Outline Asteroids, Meteorites, Comets, and other Debris

38. The Debris of the Solar System

39. Titus-Bode Law is a mathematical coincidence Orbital radius = 0.4 + 0.3x2 n-2 where n =2, 3, 4, 5, 6, …

40. The “missing” planet Ceres was discovered in 1801 Diameter 934 km

41. Numerous other asteroids were discovered in the early 1800’s

42. Most (but not all) asteroids orbit between Mars & Jupiter

43. Asteroid Belt Astronomers first discovered the asteroids while searching for a “missing planet”. There was no planet, but there were thousands of asteroids with diameters ranging from a few kilometers up to 1000 kilometers orbiting within a belt between the orbits of Mars and Jupiter. It was first thought that these must be the remains of a planet that was destroyed by a collision. But, the combined mass of these asteroids is nowhere near being enough for a planet-sized object. They are simply debris left over from the formation of the solar system.

44. Locating asteroids Asteroids are being continually discovered at a rate of 10-100 per month. Asteroids are generally discovered using photographic techniques - take a very long exposure of a star field; if something moves, it is probably an asteroid. NASA also has a relatively new program for tracking all known NEOs (Near Earth Objects), in the hopes that we might be able to avoid a collision (http://neo.jpl.nasa.gov).

45. Formation of the belt - Jupiter’s influence Supercomputer simulations indicate that the formation of the asteroid belt was drastically affected by Jupiter’s gravity - in fact, without Jupiter, a 5th terrestrial planet probably would have formed! However, Jupiter’s gravity can’t explain the fact that the asteroids have eccentric inclined orbits rather than circular. Recent theories include a Mars-sized object that did form in the region of the belt, but was then ejected by Jupiter’s gravity. This object would have interacted with the asteroids to produce the observed orbits. Perhaps this is the same object that collided with Earth to produce the Moon!

46. Continuing influence from Jupiter Even today, gravitational perturbations by Jupiter deplete certain orbits within the asteroid belt. The resulting gaps, called Kirkwood gaps, occur at simple fractions of Jupiter’s orbital period.

47. Trojan asteroids The combined effect of the Sun’s and Jupiter’s gravity also captures asteroids in two locations, called Lagrangian points, along Jupiter’s orbit. These are known as trojan asteroids.

48. Appearance and composition 1 Ceres is by far the largest asteroid (it makes up almost one-third of the mass of the asteroid belt by itself). Several of the larger asteroids are able to hold themselves together in a roughly spherical shape. These larger asteroids even show signs of chemical differentiation due to the heat of the impacts that formed them. Some even have “moons” like Ida.

49. Appearance and composition Most asteroids, however, are quite irregular, frequently loosely bound conglomerations of material. This is because of the billions of years of occasional collisions that they have undergone, causing them to break up into smaller fragments. Even though there are a great number of asteroids, they are spread out over a lot of space, so they are not actually that close together (as The Empire Strikes Back would have you believe).

50. Most asteroids are small and irregular shaped

51. Asteroids tumble

52. Some asteroids are piles of debris 253 Mathilde

53. Collisions with Earth Some asteroids (the near-Earth objects), move in elliptical orbits that cross the orbits of Mars and Earth. If such an asteroid strikes the Earth, it forms an impact crater whose diameter depends on both the mass and the speed of the asteroid. It is thought that several particularly large collisions led to the multiple mass extinctions that are observed in the fossil record. The top picture is Barringer Crater in Arizona, the bottom is the aftermath of an “almost collision”. The asteroid exploded in the atmosphere due to the extreme heating above the Tunguska region of Siberia before it actually hit the ground.

54. Asteroids Asteroids are small, irregular bodies. Most are composed of rock or metal. Most orbit between Mars and Jupiter. Some can cross Earth’s orbit. Model conditions in the early Solar System.

55. Asteroids and Meteorites Meteorites are pieces of asteroids that have fallen to Earth. In space it is called a meteroid. While passing through the atmosphere, it is a meteor. Meteorites have different types. The types reflect different physical conditions during formation.

56. Types of Meteorites Most are stony, like Earth rocks. Iron meteorites have high concentrations of metal. Stony-irons are a combination. Some stony meteorites are carbonaceous (they have a lot of carbon). Can date meteorites to the age of the Solar System (4.5 billion years).

57. Types of Meteorites Courtesy of Ron Greeley