Chapter 8 Formation of Planetary Systems Our Solar System and Beyond.
Protostars are difficult to observe because A. the protostar stage is very short. B. they are surrounded by cocoons of gas and dust. C. they radiate mainly.
Photochemistry Lecture 7 Photoionization and photoelectron spectroscopy.
© 2010 Pearson Education, Inc. Chapter 8 Formation of the Solar System.
This set of slides This set of slides starts the topic of stellar evolution, overview, protostars, main sequence… Units covered: 59, 60, 61.
Chapter 8 Formation of the Solar System. 8.1 The Search for Origins Our goals for learning: What properties of our solar system must a formation theory.
Units to cover 60-63. Homework 8 Unit 56 problems 6,7 Unit 59 problems 6, 8, 9 Unit 60 problems 6, 8, 11 Unit 61 problems 4, 7 Unit 62, problem 8.
Fabrication of a Superconducting Hot- Electron Bolometer Receiver with Micromachined Waveguide Components Aaron Datesman Bechtel Bettis Atomic Power Laboratory,
Units to cover: 70, 72,73,74, 75, 76, 78. Homework Unit 70, Problems 17, 19 Unit 72, Problem 18 Unit 73, Problem 18 Unit 75, Problems 12, 17, 18 19.
Where did the solar system come from? Astr 221 2015 NW Chs. 8&9 Also: Sun – Moon -Eclipses.
Lecture 32: The Origin of the Solar System
Chapter 6 Formation of Planetary Systems Our Solar System and Beyond.