Astronomy 4.1 Energy formation and layers of the Sun - IT6230
2012 Again
Solar dynamo1
Objectives Explore the structure of the Sun. The Sun Describe the solar activity cycle and how the Sun affects Earth. Compare the different types of spectra.
1 Climate Change some astrophysical perspectives.
Our star, the Sun is a big ball of gas And it's 99 percent of our solar system's mass It's an average star in our Milky Way Warming the Earth every day.
CHAPTER 10: CHAPTER 10: The Sun – Our Favorite (and Ordinary) Star.
Exploring the Universe Chapter 26 26.1 Energy From the Sun.
Solar System Physics I Dr Martin Hendry 5 lectures, beginning Autumn 2007 Department of Physics and Astronomy Astronomy 1X Session 2007-08.
Our Sun – Physical Properties. 109 Earths would fit across the diameter of the sun!! Diameter: 1,400,000 km, 864,000 miles 4.5 light-seconds 1,300,000.
Quantum Phenomena II Question & Answer Session Quantum Phenomena II Question & Answer Session Using the handsets A. Check handset is turned on -- green.
