1. QUESTIONS 1.How do we form hypotheses about the formation of our Solar System? 2.In what ways can we scientifically test ideas about the Solar System’s formation and early events? 3.What is the Solar System’s destiny?

2. BUILDING A SOLAR SYSTEM

3. STEP 1. FUSE METALS

5. ORIGIN OF MATTER All matter originated at the Big Bang Primordial nucleosynthesis A few minutes after the big bang, protons were highly dense and very energetic, allowing fusion For about 17 minutes, nucleosynthesis could occur

6. BIG BANG NUCLEOSYNTHESIS Discussed by Alpher-Bethe-Gamow in 1940s H + H  D Nearly all deuterium originated in the big bang Also formed 3 He, 4 He, 7 Li ~10:1 H:He ratio Beyond that energy required wasn’t amenable

7. T=1000 s

8. STARS AND FUSION http://webhome.idirect.com/~rsnow/aboutstars.htg/H-RDIAGRAM.gif Less fusion Lots of fusion

9. NUCLEAR FUSION The process of forming a new atomic nucleus by the fusing of two or more nuclei Hydrogen is “burned” to form Helium, and further fusion leads to other elements Fusion only occurs at high temperatures (core of the Sun, nuclear bomb, early big bang) ++ Coulombic Barrier

10. 2 H D D + H 3 He 2 3 He 4 He 2 H H  HE

11. SYNTHESIS OF HEAVIER ELEMENTS Requires bigger, hotter stars High temperature means more energy to overcome coulomb barrier Also means more frequent collisions between nuclei, so short-lived nuclei can act as intermediates

12. MORE BURNING Triple alpha process 2 4 He 8 Be 4 He 12 C 16 O

13. ORIGIN OF HEAVIER ELEMENTS http://www.hacastronomy.com/sn/onion_skin_model.gif

14. From Stellar Nucleosynthesis

15. HEAVIER ELEMENTS Require energy to synthesize No pay for their own nucleosynthesis Supernova Form new elements by proton/neutron capture Result in the periodic table http://magic.mppmu.mpg.de/snr.jpg

17. Anders and Grevasse 1989

18. Most abundant elements easiest to synthesize

19. Anders and Grevasse 1989 Heavy elements much rarer than light elements

20. Anders and Grevasse 1989 Sawtooth pattern from addition of He nuclei

21. Anders and Grevasse 1989 Iron peak- the dead end of nucleosynthesis

22. Anders and Grevasse 1989 Easy to burn light elements so Li, Be, B are depleted

23. STEP 2. DESTROY AN OLD STAR

24. Brightest Explosion since Kepler’s time Guess the year it happened! Ring of expelled gas from earlier Bipolar filaments SUPERNOVA 1987A

25. http://hubblesite.org/newscenter/archive/releases/2004/09/ Brightest Explosion since Kepler’s time Guess the year it happened! Ring of expelled gas from earlier Bipolar filaments Hubble has been watching…

26. Not actually planetary at all: Herschel thought they looked like planets, that they were new planetary systems forming. PLANETARY NEBULA

27. Orion Nebula ~2000 Solar Masses NEBULA

28. STEP 3. CONDENSE A NEW STAR

29. Material condenses from “small” shock waves, perturbations in nebula Spinning increases (Moment of Inertia) Fusion begins when P/T is achieved Materials fall into new star and are ejected This modifies the solar system! YOUNG STARS

30. STEP 4. GET A PROPLYD

31. Material spins out like record, Earth North and South of Sun, material is excavated by jets Orion Nebula proplyds  (PRO)TO(PL)ANETAR(Y D)ISK = PROPLYD

32. STEP 5. BUILD PARTICLES

33. Anders and Grevasse 1989 Take a gas of this composition and cool it. What forms?

34. FIRST THING TO FORM: Ceramics These are high temperature minerals First condensates

35. CALLED CALCIUM-ALUMINUM RICH INCLUSIONS

36. THEN COME SILICATES AND METAL Olivine and iron

37. SILICATES MELTED Formed chondrules

38. VOLATILE MATERIALS Phosphorus Lower temeprature silicates (Na-, K-bearing) Sulfides Ices Where do they go?

39. STEP 6. BUILD MASSES

41. EARTH FORMED FROM SOLAR SYSTEM DEBRIS Earth and other planets form from a mixture of rocky material Meteorites Asteroids Comets Hoba- www.nmm.ac.uk

42. ORIGINS OF THE EARTH’S CONSTITUENTS Volatile components, including key biogenic elements, were in short supply on the early Earth Earth was hot Volatiles were lost or were not delivered Not primordial ( 20 Ne, 36 Ar)

43. LOSS OF VOLATILES ON INNER PLANETS H, C, N, O P

44. Carbonaceous Chondrites, with hydrated minerals, were the last accreted constituent to the early earth Outgassing of volatiles led to hydro + atmosphere Consistent with D/H ratio Something odd going on with PGEs Comets, loaded with H 2 O and organics, were the source of volatiles Loaded with water High flux (possibly) to early Earth D/H ratio is much higher than earth What were early comets really like? DELIVERY OF VOLATILES TO THE EARTH Cometary DeliveryLate Veneer

45. STEP 7. “CRUSH THE MASSES” -Stalin

46. PLANETARY ACCRETION Dust grains and small particles collide and stick together Accumulate, making larger and larger bodies A miracle occurs Planets form http://ircamera.as.arizona.edu/NatSci102/NatSci102/images/accretion.jpg http://blog.stackoverflow.com/wp-content/uploads/then-a-miracle-occurs-cartoon.png

47. STEP 8. DIFFERENTIATE THE PLANETS

48. PROCESSING OF PLANETS Planets accreted and were warmed Radioactive decay of short-lived elements? Impact heating Warming causes differentiation of planets

50. STEP 9. REARRANGE AND WATCH OUT

51. CREATING MOONS AND RINGS From Robin Canup: Gravity is hell Earth-Moon formed from early collision Jupiter kept eating its moons Saturn’s Rings formed from destroyed ice moon? http://www.youtube.com/watch?v=Fwl_JBQtH9o

52. Caused by a turbulent outer Solar System 4.1 - 3.8 Ga THE LATE HEAVY BOMBARDMENT http://physics.uoregon.edu/~jimbrau/astr121/notes/chapter15.html http://www.youtube.com/watch?v=6LzQfR-T5_A The Nice Model  Gomes et al, Nature, 2005 Giants were at 5-17 AU Now at 5-30 AU

53. Caused by a turbulent outer Solar System 4.1 - 3.8 Ga Ended same time as life “?” showed up on Earth Effects still seen nightly THE LATE HEAVY BOMBARDMENT

54. ANNOUNCEMENTS…

55. for METEORITICS MEET IN CHE313 NEXT WEEK!

56. Uploaded to Canvas Read Chapter 8, stopping at 8.8 for next week! Homework: 1.Chapter 8, problems 1 & 2 2.Chelyabinsk Research Paper questions HOMEWORK: DUE SEPT 12 IN CLASS

57. We (The Solar System) is now in a cloud of gas probably blown to us by a group of super-giants. It is called the Local Interstellar Cloud(LIC) or the Local Fluff. Assume: T = 7000 K 0.1 atoms/cubic cm Using the Ideal Gas Law, Calculate its pressure. Give units. EXTRA CREDIT (2pts, due with HW2, 9/12) http://science1.nasa.gov/science-news/science-at-nasa/2003/06jan_bubble/