1.Prentice Hall EARTH SCIENCE Tarbuck Lutgens2. Chapter 25 Beyond OurSolar System 3. 25.1 Properties of Stars Star Color and Temperature •Color is a clue to a star’s…

Slide 1 Origin of Our Solar System Slide 2 TEK Objective 5: Earth in space and time. The student understands the solar nebular accretionary disk model. The student is expected…

Slide 1 Slide 2 Thursday May 2 nd Objective You will apply knowledge of Astronomy in order to review for unit test. Warm-up What is the big bang? What did it create? Slide…

The “Crab Nebula”: the most famous supernova remnant. distance  2000 pc diameter  3 pc Synchrotron Emission: relativistic electrons spiralling around magnetic field…

Design in the Cosmos Dr. Hugh Ross Reasons To Believe Who Discovered the Big Bang? A. Penzias & R. Wilson? Who Discovered the Big Bang? George Gamow? Who Discovered the…

Star birth occurs in a nebula. A star's initial mass determines the star’s temperature, luminosity, and diameter that ultimately decides which life stages and type…

Team L Supernovae Mark Blount Elizabeth Brooks Blaze Campbell Sonia Vazquez Yanet Zavala Goal To learn about stellar evolution theory To discover how elements spread across…

Quark Matter Under Extreme Conditions Quark Matter Under Extreme Conditions Neda Sadooghi Sharif University of Technology Tehran-Iran Munich-January 2011 1 1 Force Strength…

Star Life Cycles Dark Nebulas: Cold Clouds of gas and dust located in arms of galaxies. Gravity pulls gas and dust together to form protostar (no fusion). Young Protostars…