8.2 Exploring the Sun Homework: page 340 # 2, 3, 5, 7, 9.
Solar Science Workshop 6/8/05 An Introduction to the Physics of Our Star: The Sun Distance from Earth –1 AU Travel time for Light to Earth –About 8 minutes.
ES 023 Planet Earth: Shaken and Stirred ES 123 The Dynamic Earth Quick review of last class Hertzsprung-Russell diagram (star classification) A tour of.
The Sun
LG (1). Understand basic principles of the sun’s structure and how it functions Success Criteria (SC) I can name the layers of the sun in order (or label.
© 2010 Pearson Education, Inc. 1. The Sun appears bright orange because of the extremely hot fires that are constantly burning carbon. TRUE or FALSE 2.
Review of last class Dimitri Mendeleev and the Periodic Table What is an isotope? Internal structure of the Sun Stars and nuclear fusion Stars: Element.
A105 Stars and Galaxies ROOFTOP TONIGHT AT 9 PM HAND IN HOMEWORK Exam coming on Nov. 2 Today’s APODAPOD.
The Sun Our Star Please press “1” to test your transmitter.
A105 Stars and Galaxies
© 2010 Pearson Education, Inc. Our goals for learning: Why was the Sun’s energy source a major mystery? Why does the Sun shine? What is the Sun’s.
The sun and our solar system Grade 9 Science Space Part 2.
