Life Cycle of Stars
Look familiar?
First step: Nebula
Equilibrium
Birth of A Star
Main Sequence
Red Giant
The hydrogen fuel runs out and the star has entered the old age stage. If the star wants to maintain equilibrium between gravity and gas pressure, it needs increased temperatures in the core to re-ignite fusion. The star is forced to burn helium in an effort to maintain stability. The core contracts the atoms that are packed together so they are even tighter than before. The outer shell has expanded in an effort to help heat from the core from escaping into space.
White Dwarf
Black Hole
Origin Of Elements
Hydrogen
Iron
Oxygen
Star light
Easy Bib
Works Cited
"Equilibrium and Statics." Equilibrium and Statics. Web. 24 Mar. 2015. <http://www.physicsclassroom.com/class/vectors/Lesson-3/Equilibrium-and-Statics>.
"Interstellar Medium." ScienceDaily. ScienceDaily. Web. 25 Mar. 2015. <http://www.sciencedaily.com/articles/i/interstellar_medium.htm>.
"The Life Cycle of Stars." The Life Cycle of Stars. Web. 24 Mar. 2015. <http://www2.hesston.edu/Physics/StarsAmy/starspaper.htm>.
"Stellar Evolution." Wikipedia. Wikimedia Foundation. Web. 10 Mar. 2015. <http://en.wikipedia.org/wiki/Stellar_evolution>.http://4.bp.blogspot.com/-rmYKjvJ7kbE/TuZRS5Mm9NI/AAAAAAAAABU/icY_7OgRr9Y/s1600/star_human.jpg
http://www.sidleach.com/m16.jpg
http://www.nessnet.eu/ness_logo_unequilibrium_light_7.jpg
http://www.wired.com/images_blogs/wiredscience/2011/12/hubbleheic1118a.jpg
http://www.for68.com/upload/image/200512su86402129331912150024200-0-1.jpg
http://img4.wikia.nocookie.net/__cb20141109025528/walkingdead/images/d/da/RedGiant.jpg
https://universodoppler.files.wordpress.com/2011/11/white_dwarf_by_i3a12c1.jpg
http://s.ngm.com/2014/03/black-holes/img/black-holes-opener-615.jpg
http://philosophyofreality.com/wp-content/uploads/2010/09/Doppler-redshift.jpg