Steller nucleosynthesis of carbon by thermonuclear fusion
PowerPoint slideshow describing how stars fuse hydrogen atoms into helium atoms, and how helium atoms fuse to form carbon atoms. Also covers the nebular theory for the origin of our solar system, and the concept of a pre-existing star that underwent a supernova to form the nebula from which our solar system condensed under the influence of static charges and then gravity. copy edited
File 49693 is a 8.1MB PowerPoint
Uploaded:
Aug11 16
Last Modified: 2016-08-11 18:02:35
https://serc.carleton.edu/download/files/49693/steller_nucleosynthesis_carbon.v7.ppt