Timeline for Ways to make a star go supernova?
Current License: CC BY-SA 3.0
4 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Jul 16, 2023 at 8:54 | comment | added | Anders Sandberg | @blademan9999 - The inflow meets the massive radiation pressure from inside, slowing down or even nearly stopping. | |
| Jul 12, 2023 at 15:39 | comment | added | blademan9999 | What does "the inflow chokes" mean? | |
| Nov 1, 2017 at 8:40 | comment | added | userLTK | Nice answer. I imagine the iron inside a star, once the fusion stops would undergo the equivalent of chandrasekhar collapse, so you probably wouldn't need solar "Masses" of it, a bit over 1 solar mass should be close to enough but it would need a good bit of time to coalesce in the center and condense. How about adding a Neutron star? | |
| Oct 30, 2017 at 22:57 | history | answered | Anders Sandberg | CC BY-SA 3.0 |