Stars are some of the most abundant and impressive things in the universe. Each galaxy contains hundreds of billions of stars, and there are trillions of galaxies out there. That equates to a whole lot of stars- some estimate 300 sextillion. But what makes stars so common, and why are they the way that they are? How do they form, and how do they live and die? Well, the answers to these questions lie within one of the most fascinating processes in astronomy, and today we're going to be examining that process, from their chaotic births to their cataclysmic deaths!

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SOURCES OF INFORMATION:

- Origins: Smith, Michael David (2004). The Origin of Stars. Imperial College Press. pp. 57–68. ISBN 978-1-86094-501-4.

- Star Evolution: "Stellar Evolution & Death". NASA Observatorium. Archived from the original on 2008-02-10. Retrieved 2006-06-08.

- Star Estimates: Borenstein, Seth (December 1, 2010). "Universe's Star Count Could Triple". CBS News. Retrieved 2011-07-14.

- Low Mass Stars: Richmond, Michael. "Late stages of evolution for low-mass stars". Rochester Institute of Technology. Retrieved 2006-08-04.

- Massive Stars: "The Evolution of Massive Stars and Type II Supernovae". Penn Stats College of Science. Retrieved 2016-01-05.

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