A Simulated Stable Planetary System with 416 Planets in the Habitable Zone
nautil.us
nautil.us
If I understand correctly, I think the author uses "stable" to just mean a _fixed point_. The fixed point must actually be unstable to just about every possible perturbation, which justifies the second statement; if the fixed point were actually "stable" (to perturbations) then it would occur relatively easily in nature.
As soon as one planet wanders a bit too far out of line it'll smack into others going the opposite direction and the debris will take out all the others inside of a few revolutions.
Interesting, but highly risky.
It's not going to stay math-stable for long, but it could stay engineering-stable for millions of years.
As, by-the-by, how important are "habitable zones" to the Drake equation these days?
We have an abundance of earth-life adapted to almost any temperature conditions commonly found on earth. Doesn't this imply that the total viable is wider than what we find here?
How cold could a planet be and still have chemosynthesis?
The mass increase would be a rounding error. The Sun is more than 300,000 times more massive than the Earth. It'd be a time for somewhat spectacular fireworks and the life of the star would be somewhat shortened (by the addition of some heavy elements) but, apart from that, nobody would be able to tell there was once a very large art installation around that star.
N = R × N(Earth) × F(Life) × F(Intelligence) × F(Communication) × L
The individual components are quite straightforward. What I don't get is that it seems like breaking one problem down into several more unknown problems none of which really help. In fact, it seems a harder to know the individual frequencies than it would be to actually find any single ET life. Even if we found life, we still wouldn't have a much of a clue of the frequencies (unless, I suppose, the ET life had mapped or sampled the universe and shared that knowledge with us or gave us FTL tech -- one can dream!).
Other discussions have focused around approximation of the # of habitable planets, which makes total sense.
I guess my question is what knowledge or insight would enable us to estimate the frequency of life occurring?
Maybe I'm overthinking this, but I see the problem as akin to someone giving me an uncountably large number of boxes with each having a some chance between zero or more of them containing a treasure of immeasurable value. The value of the treasure approaches infinity, so even a near 0 chance of its existence means that it has a positive ROI. In that vein, it doesn't really matter what the odds are of finding life, it is a justifiable expenditure that will statistically pay for itself.
Unless the formula can take down to actually zero the odds of their being discoverable life it doesn't change the calculation. That is, whether the odds are 1e-1000% or 99% we should expend basically the same amount of resources to find it.
It could also tell us what the consequences will be of actually making big discoveries like managing to recreate life from scratch in the lab, find it on Mars, or find life on earth opposite chirality indicating independent orign. If we do (or can't!) find those things, how much will that help us predict that we find other civilizations in the galaxy?
I don't think the infinite value argument really works. Finding aliens isn't worth sacrificing everything else for if it's extremely unlikely to succeed. We could just carry on without knowing.
Like, how big and hot it is?
I could imagine it always has the same "width" but I could imagine that the zone of a rather big and hot star has a much higher circumference and would allow for more planets.
Also, if the planets are in the same plane, wont they eclipse every now and then?
Time to watch Firefly again!
It's amazing to think how far a civilization would have to advance to go from "simulated" to "built" for something like this.