Editing 1422: My Phone is Dying
Warning: You are not logged in. Your IP address will be publicly visible if you make any edits. If you log in or create an account, your edits will be attributed to your username, along with other benefits.
The edit can be undone.
Please check the comparison below to verify that this is what you want to do, and then save the changes below to finish undoing the edit.
| Latest revision | Your text | ||
| Line 8: | Line 8: | ||
==Explanation== | ==Explanation== | ||
| β | [[Beret Guy|Beret Guy's]] phone is about to "die". [[Cueball]] assumes this just means that the battery is running out and it needs to be recharged, but the phone in question appears to "die" in a way analogous to the {{w|Stellar_evolution|life and death}} of a star: expending its fuel while heating up and expanding before ultimately losing its outer layers and becoming a white dwarf or similar "lesser" star | + | [[Beret Guy|Beret Guy's]] phone is about to "die". [[Cueball]] assumes this just means that the battery is running out and it needs to be recharged, but the phone in question appears to "die" in a way analogous to the {{w|Stellar_evolution|life and death}} of a star: expending its fuel while heating up and expanding before ultimately losing its outer layers and becoming a white dwarf or similar "lesser" star. However, this is something phones usually don't do.{{Citation needed}} |
Stars constantly undergo fusion reactions. The pressure generated by these reactions counteracts gravity, preventing it from collapsing the star during its main lifespan. As the hydrogen mostly fuses into helium in the core, the core gradually becomes more dense and the region of fusion gradually moves away from the center. Then, the star grows in size, reaching the stage of a {{w|red giant}}. When most of the "fuel" for fusion has been consumed, gravity will collapse the star into a {{w|white dwarf}} while the outer layers are shed. For stars much more massive than the Sun, there will be a {{w|supernova}} explosion caused by a violent collapse, which is {{what if|73|very powerful}} (and leaves behind a {{w|neutron star}} or a {{w|black hole}}, depending on how much mass is left after the supernova). Stars with more hydrogen fuel tend to burn brighter and faster. Beret Guy's refusal of a charger is probably a reference to this. | Stars constantly undergo fusion reactions. The pressure generated by these reactions counteracts gravity, preventing it from collapsing the star during its main lifespan. As the hydrogen mostly fuses into helium in the core, the core gradually becomes more dense and the region of fusion gradually moves away from the center. Then, the star grows in size, reaching the stage of a {{w|red giant}}. When most of the "fuel" for fusion has been consumed, gravity will collapse the star into a {{w|white dwarf}} while the outer layers are shed. For stars much more massive than the Sun, there will be a {{w|supernova}} explosion caused by a violent collapse, which is {{what if|73|very powerful}} (and leaves behind a {{w|neutron star}} or a {{w|black hole}}, depending on how much mass is left after the supernova). Stars with more hydrogen fuel tend to burn brighter and faster. Beret Guy's refusal of a charger is probably a reference to this. | ||
