I've spent a lot of time lately discussing super massive stars, their explosive ending as supernova and shared a program for seeing their remenants, ie supernovae remnants.
Now we'll take a look at the opposite side of the coin. Here we discuss main sequence stars that are from 0.4 to 8 solar masses (stars similar to our own Sun) and discuss their lifecyle and how they end up as planetary nebula with white dwarf stars.
The video is long, and I share my notes that I have created on this from my Astronomy Class way back in college many, many years ago. I've tried to update it. Anyway, this is to prepare to share a Planetary Nebula Observing/Imaging Program.
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