Breadknife wrote:I know I've mentioned somewhere recently on a forum (this one, in this thread?) the possibility of a "Galactic Goldilocks Zone". Another thing that's not my idea, but looks like you have the same sort of one. Too close to glactic centre and allthat Cygnus X-1 thing and the radiation in amongst the mass of close-knit stars isn't good for (our kind of) life, and there's probably no stability of planets if you've got a dozen stars between an otherwise likely sun and its equivalent of our neighbouring Alpha Centauri, whizzing about like nobody's business and gravitationall ypurturbing all the debris.Grave_n_idle wrote:...it got me to thinking - we tend to think of our 'habitable zone' pretty much entirely in terms of distance from the sun, but our habitable zone may be much more specific than that. In fact, it pretty certainly is. [...]
Too far out and nebulae may just not have enough purturbation to recoallesce into the next generation of stars (or at least with not the right mix of matter).
Similar patterns perhaps within the core of spiral arms and definitely in the gaps between them, and obviously zones that aren't "stellar nurserys" are going to have to do with whatever stars and planets they got the last time their area was a stellar nursery (and deal with the slow death of the stars that are dying), at least until the next good nova stirs things up again.
And of course we're a spiral galaxy. Other types (already different ages from our own, with different suns also representing different points throughout the standard stellar evolution graph, and some apparently with hyperactive cores that might make the entire span of that galaxy uninhabitable to radiation-sensitive life1) will have their own problemaic/advantageous areas. Especially if the potential life would have been arising just about the time that the neighbouring galaxy in the cluster starts its deathly-slow 'collision' with your own, bringing in a hail of 'fast'-moving stars through one's neighbourhood. (Mostly them all missing, I presume, given how big space is, even compared to stars, but I bet it's spectacular when you get a direct collision, and even more so with a glancing hit, from the right angle...)
(But by the time we're talking about looking for life in other galaxies, I tend to go "Of course its there," (above-mentioned 'dead zones', possibly excepting), "but we'll probably never know of it, even if Humanity lasts faaaar beyond the lifetime of our own sun." The same may be true of life from the other side of the Milky Way, but at least if we compartmentalise our own galaxy into more and less likely areas to find life (as we know it!) we can get a good idea of how long we might have to wait (or, ourselves, travel, barring breakthrough shortcuts that would be a game-changed on every level) to meet the 'neighbours'.)
1 Or inhabitable to life that demands it? That couldn't have arisen in our neck of the woods because the conditions were too quiescent?
Sounds like we're on the same sort of wavelength, yes.
One thing I wanted to point out - I'd imagine that 'radiation-sensitive' is probably going to be a fairly common ingredient in the make-up of life, to some extent or another - because adaptability requires variation, and variation is favoured by mutation.


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