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May 3 at 19:28 comment added Chromatic Realms @KyleG honestly that's a great idea. Maybe I'll make it so instead of just exploding it drilled itself down into the crust and is still emitting radiation, circumventing the need for a natural cooling timeline. Just keepin' it molten 24/7. Love it.
Apr 27 at 22:16 comment added Kyle G @ChromaticRealms Certainly! Jupiter has a moon covered in volcanoes that might serve as a muse. Perhaps the warpcore has stuck around and is still emitting gravitational waves or something?
Apr 27 at 16:10 comment added Chromatic Realms @AlexP if the surface layer freezes but the innards of the mare are very hot and molten, what are the chances of localized volcanic/siesmic activity resulting in lava flows, fissures, and eruptions that could be visible? I know the Moon is not geologically active, but would a fresh molten mare with a thin crust be locally active in the aftermath?
Apr 27 at 16:08 comment added Chromatic Realms @KyleG thank you for being the first person to try and give an actual time estimate! :) I appreciate it! I think the radiation cooling would play a large role irl and my gut tells me it probably wouldn't be visible for long, since the heat gradient even in the "vacuum" of space is pretty extreme toward heat rapidly leaving warm bodies, but you're exactly right the purpose of this isn't to make this happen irl, it's to make it sound plausible. I WANT the Moon to have a glowing scar. If people read it and go "is that possible? Actually it might be, hmmmmm..." That's good enough for me :)
Apr 27 at 16:02 vote accept Chromatic Realms
Apr 26 at 21:48 comment added Kyle G Even adding a term for the radiant emissivity (assuming the mare/rock interface is about the same area as the mare/moon interface) doesn't really move the needle on the orders of magnitude involved here. Is this calculation exact? No. Is it enough to completely suspend any disbelief in a rather cool plotpoint? I think so but YMMV.
Apr 26 at 21:16 comment added AlexP On the contrary, I would expect that the topmost layer at the surface will freeze quite fast, exactly because radiative cooling. Yes, below it the rock may remain molten for a long time, but the question is about the surface layer.
Apr 26 at 21:11 comment added Kyle G Very true, like I said this is a pretty fast and loose calculation. Part of my simplification was to disregard any radiative cooling (since it will have a negligible effect compared to the "heatsink" of the moon), which means in my simple model the hottest portion will actually be at the surface of the moon. A better model would account for that, but then you're talking about heat gradients and black bodies etc. Since the simplified model spit out numbers MUCH larger than needed, I wouldn't worry too much about it myself, but you are welcome to do those calculations!
Apr 26 at 20:55 comment added AlexP Unfortunately, what counts is not the time needed for all the rock to cool down, but rather the time needed for the topmost layer of the rock to cool down. For example, the interior of the Earth is still molten, four and a half billion years after it was formed; but the thin crust is cold, and as a result Earth does not glow at all.
S Apr 26 at 20:39 review First answers
Apr 26 at 23:20
S Apr 26 at 20:39 history answered Kyle G CC BY-SA 4.0