Teach the Cast
Some of StarForge’s cast are still learning. When you teach them, YOU learn it best — catch what they get wrong, then quiz them.
Teach Brawn
You be the teacher — Brawn is still learning. Helping Brawn figure it out is the practice. (Only for you; nothing is saved.)
Teach the connections
Show how the star-life ideas connect
You've helped them one at a time. The real understanding is how the ideas CONNECT — teach that next.
Brawn (stellar mass at birth) × Pinch (stellar collapse — supernova / neutron star)
Two stars run out of fuel. Why does one Pinch into a supernova and the other just cool quietly?
Brawn then says: “Our Sun will supernova at the end of its life, like all stars.” — is that right?
The link: birth mass (Brawn) is the single dial that sets whether a star ends in a Pinch or fades gently.
How heavy it's born decides how it dies.
Glow (main-sequence star — steady hydrogen fusion) × Swell (red giant — expands and fuses helium)
A star fuses hydrogen calmly for billions of years, then suddenly balloons. What just changed inside it?
Glow then says: “A red giant is a totally different star from a main-sequence one — no connection.” — is that right?
The link: red giant is main-sequence's next stage — Swell begins when Glow's core fuel ends.
Burn the core, then balloon.
Capstone — trace a Sun-like star together
One star, three stages of life. Bring in the cast member for each.
A cloud of gas collapses and just ignites its first fusion. Who?
Who do you bring in?
Billions of years of steady hydrogen fusion. Who?
Who do you bring in?
Core hydrogen spent; the star balloons and fuses helium. Who?
Who do you bring in?
The synthesis: born, burning steady, then swelling — a star's stages are one continuous story set by its mass.
Ignite, burn, swell — the arc of a star.
Trace it in the star tools →
