Creation of the Chemical Elements. By Dr. Harold Williams of Montgomery College Planetarium http://montgomerycollege.edu/Departments/planet/. 17.3 Life as a High-Mass Star. Our goals for learning What are the life stages of a high-mass star?
Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.
By Dr. Harold Williams
of Montgomery College Planetarium
Iron is dead end for fusion because nuclear reactions involving iron do not release energy
(Fe has lowest mass per nuclear particle)
Higher abundances of elements with even numbers of protons
Iron builds up in core until degeneracy pressure can no longer resist gravity
Core then suddenly collapses, creating supernova explosion
Energy and neutrons released in supernova explosion enable elements heavier than iron to form, including Au and U