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A spectrum, not two boxes
Mass exists on a continuum — this page shows two representative cases, but intermediate masses follow intermediate paths.
Every star begins the same way — a cloud of gas collapsing under its own gravity. What it becomes at the end depends almost entirely on one number: how much mass it started with.
Mass exists on a continuum — this page shows two representative cases, but intermediate masses follow intermediate paths.
A Sun-like star lives roughly 10 billion years; a very massive star can burn out in just a few million — thousands of times faster.
Event horizon, accretion disk and gravity well.
One possible ending for the most massive stars.
Zoom out from a single star to the whole observable universe.