2 Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth What is the bulk composition of the solar system? Where/when/how did the atoms.
Star & Planet Formation Minicourse, U of T Astronomy Dept. Lecture 5 - Ed Thommes Accretion of Planets Bill Hartmann.
The role of laboratory astrophysics in studies of Fe-group nucleosynthesis in the early Universe
Combining renewable and traditional energy solutions
Clusters of galaxies The ICM, mass measurements and statistical measures of clustering.
AGB POPULATION IN GALAXIES WHY? Up to 80% of the K-band luminosity in a 1 Gyr old simple stellar population comes from AGB stars High redshift galaxies.
Formation of Planets Lecture 43. Condensation Sequence Theoretical and astronomical evidence suggests inner nebulae get hot. We have high-T materials.
Organic Chemistry Introduction to organic chemistry Principles of carbon chemistry Principle of polymers Hydrocarbons Organic chemistry and biochemistry.
Planetary Nebulae as a Testground of Interstellar Molecular Chemistry Tatsuhiko Hasegawa.
Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth
Formation of Planets
AGB POPULATION IN GALAXIES
