Hotfoot wrote:Sure, you can see galaxies with the "naked eye", but galaxies are huge. We can see individual stars rather easily, but they're still considerably larger than a planet, and they're tossing out massive amounts of EM radiation. In comparison, how many planets can we see outside of our own solar system? By that, I mean how many planets do we have the ability to directly see with a purely optical telescope? None. The best we can do is say that, given the data we have, we can indirectly approximate the presence of a Jupiter-sized mass. Smaller planets like Earth are impossible given our current technology, and forget about moons and asteroids.
It's possible to detect the shadow of a planet when it's in front of another star, even with planets in other solar systems. It has been done !
And you don't need to see something within another solar system, all we need is a detection system with a few lightminutes range...
If you look for the engine trails even lighthours might be possible as a detection range.
With passive detection, if it's not emitting or reflecting anything, you can't see it. Closer to a star, things get easier, since the star acts as a massive active sensor in that it is constantly pinging everything nearby with all manner of energy. This does give you the best of both worlds, after a fashion, but limiting yourself to just the Optical range of the EM spectrum does seriously limit your ability to detect things even within the solar system.
EVERYTHING is emitting radiation at all times. It's called heat ( for example. Or just reflection of sunlight. An IR telescope would detect a ship easily, especially if it use some kind of nuclear engine...
The Hubble Telescope is a darn good piece of hardware, don't get me wrong, and it could see the carrier, but only provided that it knew where to look, first. Depending on how much and what kind of EM radiation the carrier is emitting/reflecting, it will be easier to get a bead on it. This can be made more difficult by increasing the distance between the carrier and the telescope, and altering the EM output of the carrier in both emissions and potentially reflections. It would be tricky, but it is possible. In any event, even with all the equipment we have, sometimes things slip past us. I remember a case a short while ago in which a rather sizable asteroid travelling at a considerable relative velocity to Earth (the exact numbers are very hazy, but I can always try to find them again), and it wasn't detected until it had already passed through Earth's orbit. It was marked as a "near miss", though in this case "near miss" has the same meaning as "rapid change" in geology.
Nasa has enough resources to monitor a fraction of the sky we see. It's no miracle that they missed the asteroid, it's just statistics.
A military would build more passive detection arrays to have a 100% coverage of the sky.
Now, if you're actively looking for something using a full array of passive sensors, especially near a star, chances are good you'll find it, so long as you know what you're looking for.
Just look for something hotter than the background, search for engine trails and active sensor signals.
Passive sensor systems get better when they become larger, so the defender/carrier/ect. will have an advantage compared to small crafts.