๐Ÿ’ฅ Supernova
Stellar lifecycle & explosion
Phases
Progenitor Mass
Actions
Ejecta Elements
H/He
C/O
Si/S
Fe core
Shock
Stats
Phase
MS
Remnant
โ€”
Shock (Rโ˜‰)
0
Energy (ร—10โดโดฆ)
0
Main Sequence: Hydrogen fusion in the core balances gravity. A 20 Mโ˜‰ star burns for ~10 million years.