It's more fun than that, really: the thin disk is embedded in the thick disk is embedded in the halo. So there are quite a few nearby stars from both systems - the three are distinguished primarily by dynamical properties,although once you start sorting them the other differences really do stand out. So there are a few stars that _could_ be disk, from their orbits, that are classed as 'probable halo objects' due to age and metallicity and what-have-you.
However, you're right. If you look at the Kepler field, for example, you'll see that it's just above the galactic disk where it catches a large thin-disk sample but relatively faint objects aren't lost against the essentially unresolvable mass of stars. There will still be plenty of stars from the other groups in the field, though, so they are being sampled already.
BTW, if I were trying to hide from the Gbaba, I'd want to be as close to the galactic plane as possible on a line between them and the bulge - it doesn't matter how good your sensor tech is, if there are 17,000 stars per pixel in the line of sight you are _not_ going to see the one that's a bit off. Of course, it's a safe bet that the Gbaba know that too, so it's just as well that the bulge is big and figuring out _which_ line is very much a guessing game.
isaac_newton wrote:Louis R wrote:1. Those sorts of numbers are actually typical of Himself's style of space opera [I may have had some influence on the public discussion of the 'siphon effect' of Honorverse impeller drives when I and others posted calculations showing that each of 8th Fleet's ships would have had to fuse its entire mass in hydrogen to make the approach to Barnett on internal power. Probably not, of course, since he knows what we're like and would have realised the ammunition he was handing us with that description], which is one reason authors bury them in the bushes: avoids the accusations of implausibility from people who figure that if we can do it, it can't be done. You have to remember that _both_ sides have those power levels to play with, though, so it comes out pretty even in the end.
2. Not planetary-formation theory per se: while the very first stars to form in a galaxy would not have had any planets, because there wasn't yet anything to make them from - and do indeed seem to have formed by slightly different mechanisms for the same reason, it's thought that later generations formed in essentially the same way that we see in operation today. And planets appear to fall out the bottom of the blender almost automatically. However, the oldest of them have very low metallicities as a rule, which means that there wouldn't have been very _much_ material to make planets from and the planets that did form would be [this is my speculation, BTW] tiny and/or ice balls, rather like very large comets. The stars of the galactic halo are precisely those old, low-Z stars, meaning that the ones still shining are small very-late K or M dwarves with planets that are either warm and _very_ dry or dimly-lit and cold. Neither condition is as exclusive of life as some have assumed, but any life is going to be built around biochemistries that aren't as dependent on atoms heavier than iron - or between neon and iron, for that matter - as ours is. We won't be looking to settle, or even hide, out there because from our point of view there are _no_ resources to exploit. A methane-breather, of course, would probably think we're insanely picky

yet more cogent explanations - thanks

I guess that our planet hunters have not yet 'reached out' as far as the halo in their searches - I'm assuming that they are working from the nearest stars out...
On the energy levels - I guess it was more a gut feeling that the descriptions in OAR especially of the early days just didn't seem to tie up with the energy levels for planet moving - sort of like comparing the start of the Lensman series with the stuff at the end - if Himself will pardon the comparison!!
