This is the most frequently asked question by a long way on this forum!
Bear with me. It's quite a long story, and it is from something begun in December, called "The Bias Study".
One of the things Galaxy Zoo was trying to find out was whether or not a study of galaxies done by Michael Longo held true across a larger area of the Universe. He had surveyed well over 1000 spiral galaxies and there seemed to be more rotating anticlockwise than clockwise in his sample. (This is from our point of view. You might very correctly point out that from their other side they would be rotating clockwise. But it is still strange if more galaxies are rotating in any one direction than another. We wondered why it might be . . .)
Anyway, we found the same thing in our much larger sample. There seemed to be more anticlockwise than clockwise spirals in our sample, too. But we had to check one thing: was this human bias? To find out, zookeeper Kate designed a program to deliberately flip and rotate some images. For example, if a galaxy is really clockwise, we might see it as anti-clockwise in Galaxy Analysis, and click the anti-clockwise button.
Guess what we found? Well, if there really are more anti-clockwise galaxies in the Universe, the bias study should have found an excess of clockwise galaxies. In fact we found the opposite. People are still clicking anti-clockwise more often. The zookeepers have started to look for psychologists to work with to find out why this might be. It may have a deep psychological bearing, or it may simply be the web design layout. Who knows?
In any case, please always classify what you see in Galaxy Analysis, not what you see in the SDSS page.
Hope that helps.
Update: We're getting a lot of questions about black and white galaxies as well. In short, this was another test that was done at the same time - but it didn't show any interesting results so it didn't get talked about much. Again just classify what you see in Galaxy Analysis, and if you really want to see it in colour you can go to the SDSS pages.