2. Nucleosynthetic processes: Fusion: Hydrogen Helium Carbon Oxygen After Fe, neutron addition takes place (rapid and slow processes)

6. Summary – Solar abundances of the elements: H and He are the most abundant elements Elements with higher atomic numbers decrease in abundance exponentially Peak at Fe, unusually low abundances for Li, Be, B Isotopes with even atomic numbers and mass numbers more abundant than those with odd atomic numbers Sun is H-burning to form He, solar system contains elements formed in older, more massive stars

7. Meteorites – extraterrestrial rocks that enter the Earth’s atmosphere and strike the Earth’s surface Basic Classification: Stony (silicates) –Chondrites –Achondrites Stony-iron (mixed silicate and metal) Iron (metal) Falls are witnessed falling through the atmosphere (meteors), finds are found. Most finds are irons. http://meteorites.asu.edu/

8. The nebular hypothesis The solar nebula (gas) contracted, cooled and condensed into dust sized particles that accreted (stuck together as the result of collisions) into protoplanets (asteroid sized bodies) and then larger planets http://meteorites.asu.edu/

12. Evidence that chondrites are representative of early solar system materials: 1:1 ratio of non-volatile elements to those in the sun “sedimentary”, non-equilibrated texture - formed by accretion of condensed particles with little subsequent heating or alteration presence of minerals predicted to be formed by condensation of solar nebula, such as corundum, Fe metal, troilite, etc. Also inferred: achondrites, iron and stony-meteorites represent fragments of accreted planetesimals that had heated internally, melted and differentiated

13. The nebular hypothesis The solar nebula (gas) contracted, cooled and condensed into dust sized particles that accreted (stuck together as the result of collisions) into protoplanets (asteroid sized bodies) and then larger planets

16. Measured quantity = Heat of vaporization

17. Hypotheses for the formation of Earth (other planets and moons) Heterogeneous accretion Homogeneous accretion Chondrite mixing

18. Chondrite minerals: Ca-Al inclusions (CAI’s) (corundum, perovskite, melilite, anorthite) Silicates in chondrules: enstatite, diopside, olivine, anorthite Metal: Fe, Ni Troilite (FeS) Serpentine Carbonaceous material