Regarding dark matter and dark energies, I find they are strangely similar to ye olde aether. In ways there must be superheavy exotic particles somewhere to make galaxies rotate "correctly" but in similar fashion most of the universe should be made of this stuff and yet we cannot find a single particle here. I recall we had this same thing in the beginning of the 1900s.
I've been thinking about it too, but in a bit different sense... Aether is actually closer to Higgs field, which supposedly is a quantum field filling every place... it is supposedly source of inertia, mass would interact through it using particle called "Higgs' boson" if I've understood if correctly, but it's just a hypothesis since there's no record of such particle. Dark matter, though, is more like when Wolfgang Pauli postulated that according to quantum mechanics, there should be this very difficult-to-observe particle released in nuclear reactions... which we know now as "neutrino". He based his postulate on undirect observations, just like the assumption of dark matter is made from galactic rotation.
More like 1900's is the fact that we tend to think we've got most things figured out, just like smost physicist tended to believe that klassical mechanics explained everything along with Maxwell's electrondynamics... there were small anomalies that were thought to be explained by further research but basically based on existing theories. Then came two gentlemen called Einstein and Planck and laid basis to quantum mechanics and theories of relativity. Applied to this day, we think that quantum electrodynamics, quantum chromodynamics and general relativity explain everything, when sufficiently improved... while in fact there could be some unexplained observation that is explained much better with some new ideas that possibly are much different from GR or quantum mechanics, but so that quantum mechanics and GR can be derived from them. But I digress, again...
So, about the rotation of galaxies... The problem seems to be that current gravity theories applied to galactic movements don't predict the movements accurately. Thus there are two possibilities.
1. The gravity model (general relativity) is wrong
2. The gravity model is right, which means that an indirect observation of
something, later named "dark matter" is made.
Option 1 is certainly possible, but the thing is that general theory of relativity is very accurate model of gravity, according to all field experiments - other than galactic movements, that is. That means that GR [general relativity] would be accurate only on "medium" scale and inaccurate on both quantum scale and galactic scale. Which leaves us wondering, why would it be so fricking accurate in between. It is a possibility, but it feels so unlikely that the more believable option is the existence of unknown and difficult to observe substance - dark matter.
Anyways, the experimentalist's insight is that if you can't measure it you can't really base any assumptions on it - and you can't really build much on top of it.
Empiristic science is based on observations. And observations of galactic rotation movement seem to suggest that there's literally more to galaxies than it looks. That is, assuming that GR is reasonably accurate theory of gravitation. Which assumption seems to be supported by multiple experiments. It's like this: you have two die. The maximum result of one throw is 12, minimum is 2. Statistically most common result would be seven. Now, you do an experiment a thousand times and look at the results, and none of the throws shows more then twelve or less than two, and the most commonly observed value will be seven. So, when two thousand die are cast at once, the results should be between 2000 and 12000, and most likely the result should be somewhere around 7000.
Now you look at distant place, where someone seemingly throws two thousand die onto a table at once and sends you the result of all the eyes counted together. And what is the most immediate assumption if the result happens to be more than 12,000?
This is kinda what the observations tell us about the galaxies... the analogy is not perfect, but will do for now. There are three chances here:
1. Someone is sending the wrong results (observations are misinterpreted) - unlikely, but possible.
2. The die used are different from the ones used in the experiments - equivalent to general relativity becoming unreliable at extreme distances. Possible, but why the hell would someone use differently eyed die when they only have six sides... It is possible, but makes no sense at all. Although that's what universe is like most of the time anyways.
3. There are invisible or hidden die in addition to the die that we see. If we assume that the die are similar (GR applies) and the results are correct (observations are not flawed), then this is the option that is preferable.
But since there seem to be people who are more familiar with the astronomical things, I have been wondering for some time how has the cosmic background radiation been measured and how uniform it turned out to be?
As to how it has been measured... the answer is, with microwave telescopes. The cosmic background radiation is, in general, similar in spectrum distribution of a very cold black body radiation - approximately 2.725 K - but the expansion of universe has stretched the infra-red radiation all the way to micro-wave radio spectrum. The temperature distribution of the background sky has small, really small differences above and below said 2.725 K radiation, so it's not uniform... Although the differences are (AFAIK) only about 1/100,000 compared to the average temperature... But those small differences in the beginning eventually ensured that the enthropy level of the universe was sufficient to last billions of years until thermal death.
The first satellite to research cosmic background radiation was named COBE (Cosmic Background Explorer) and it gave this kind of results:

The last and most accurate observations were made by WMAP (Wilkinson Microwave Anisotropy Probe), and it recorded fluctuations with much greater resolution and accuracy:

Again, the difference between coldest and hottest spots is exaggerated on the image. It's only fractions of a degree between the "hottest" and "coolest" place in the map.
In near future, the Planck Surveyor will hopefully improve the WMAP results further.

Long message again. Sorry about that. Hope you could get through it...
