What we're missing here is the sample size and distribution. Were the Aussie's involved in this much? Or are most of the galaxies only visible from the northern hemisphere?
The data comes from the Sloan digital sky survey.
The aim of which is to map out a quarter of the sky.
I quote from the SDSS web page:
QUOTE
The SDSS completed its first phase of operations — SDSS-I — in June, 2005. Over the course of five years, SDSS-I imaged more than 8,000 square degrees of the sky in five bandpasses, detecting nearly 200 million celestial objects, and it measured spectra of more than 675,000 galaxies, 90,000 quasars, and 185,000 stars. These data have supported studies ranging from asteroids and nearby stars to the large scale structure of the Universe.
So, the sample size used by the Galaxy Zoo, is 200,000,000. This includes (I believe) stars, galaxies, and the occasional satelite (As those are the possible classifications on the Galaxy Zoo website.
And this from the second phase of operations:
QUOTE (->
| QUOTE |
| The SDSS completed its first phase of operations — SDSS-I — in June, 2005. Over the course of five years, SDSS-I imaged more than 8,000 square degrees of the sky in five bandpasses, detecting nearly 200 million celestial objects, and it measured spectra of more than 675,000 galaxies, 90,000 quasars, and 185,000 stars. These data have supported studies ranging from asteroids and nearby stars to the large scale structure of the Universe. |
So, the sample size used by the Galaxy Zoo, is 200,000,000. This includes (I believe) stars, galaxies, and the occasional satelite (As those are the possible classifications on the Galaxy Zoo website.
And this from the second phase of operations:
DR6 includes images of roughly 287 million objects over 9,583 square degrees of the sky. The survey also includes 1.27 million spectra of stars, galaxies and quasars.
DR6 is the sixth public data release.
So, the problem is not small sample size, and the data is from above the plane of the ecliptic.
Here's the photometry coverage:

Here's the spectroscopy coverage:

These images are at the time of DR5.
Corvidae
25th October 2007 - 07:18 PM
Just looking at those coverage area's, unless it's a HUGE bias for one direction over another, I'd say wait until they have more galaxies cataloged.
The thing to remember is that a few thousand galaxies in our neighborhood is a statistical nothing in the scale of the galaxy. We still need a larger sample set to say the rotation direction is anything more than an odd fluke of chance.
There could very well be sets of hundreds or thousands of galaxies all rotating in uniform direction in discreet groups all over the universe. Of course if there are, then we'd have to come up with a theory to explain it. Galactic super groups don't seem to be capable of causing that type of effect.
Trippy
25th October 2007 - 07:28 PM
I'm not sure (off the top of my head) what sort of depth it represents, but here's a map of part of the survey:

It maps out to a redshift of 60,000 km/s.
Trippy
25th October 2007 - 09:06 PM
this from the galaxy zoo faq:
QUOTE
Q. Why record the rotation of the galaxy when it depends on your position? A different observer on the other side of the galaxy would observe it rotating the opposite way. And shouldn't they all be random?
A. Yes, they should be, but a recent investigation, involving many fewer galaxies, suggested that the odds of seeing a clockwise or an anticlockwise galaxy changed depending on where you look in the sky. If this is true, it suggests we're missing something about how the Universe is organised on large scales, and so we decided - with your help - to see if the effect is real. We are also interested in the correlation s between neighbouring galaxies, for example whether a close pair of galaxies rotate the same way, as this contains information about the way galaxies form and the large-scale forces acting on them. All observers would agree on such an observation.
I'm not able to find any exact figures yet, but as near as I can tell, the Bias seems to be statistically significant (from the comments that I have been able to find).
There is this paper from arxiv:
http://arxiv.org/abs/0707.3793 which has yet to be accepted (I think it has something to do with his proposed causes of bias) but he cites the significance as being 3.11 standard deviations (I think his sample size was in the hundreds of thousands).
The other thing that I can tell you is that as of August, 10,000,000 images had been classified - so we have a statistically significant result (I'm still looking for the data) possibly as great as 3 standard deviations, from a sample size of 10,000,000.
NeoNo.1
26th October 2007 - 01:39 AM
Well, this is all very interesting, but i see a big problem with determining Right handedness with left handedness since spacetime has no direction. In space, no matter what inertia point and momentum a system has, from its frame there is an up and a down a left and a right, but on the whole, we find there are actually no directions in spacetime. This is true, and no scientist will argue. Then...
Right handed momenta and left handed moments are equal and the same. No reference when the universe is concerned.
Trippy
26th October 2007 - 06:16 AM
QUOTE (NeoNo.1+Oct 26 2007, 02:39 PM)
Well, this is all very interesting, but i see a big problem with determining Right handedness with left handedness since spacetime has no direction. In space, no matter what inertia point and momentum a system has, from its frame there is an up and a down a left and a right, but on the whole, we find there are actually no directions in spacetime. This is true, and no scientist will argue. Then...
Right handed momenta and left handed moments are equal and the same. No reference when the universe is concerned.
Actually, you're wrong, there may or may not be a universal reference frame, but if you actually comprehended what I wrote, each time I referred to up and down, I did in fact specify a local reference frame (the galactic magnetic field) so this objection has no substance.
kaneda
26th October 2007 - 03:18 PM
Corvidae. As to a galactic black hole (or any black hole) and dark matter, BH's should scoop it all up when it comes close enough. Regardless of what particle DM is supposed to be made of, it is said to interact gravitationally so would not last long close to a black hole.
If DM forms large structures, I would think that as a central black hole absorbed one of them, that would cause another to fall into it's place which would also promptly be absorbed and so on till only a little DM was left in the outer reaches of the galaxy.
Nowtime
18th December 2007 - 08:01 PM
I think some brilliant minds have missed the point here. Trippy has provided the article reference - its shortcomings could be checked by anyone (as he painstakingly has shown).
To the extent that it has been verified, the discussion ( as I said, your minds are superb) could be a brainstorm of ideas as to its possible causes and implications.
There is unquestionably something wrong with the present 'analogy' of science which has non-directional space changing direction and universal time slowing down for certain objects, and where pairs of spinning particles, separated by kilometers, can make the spin of one change with respect to the other.
Incongruous events should be (evaluated, naturally) explored when even slightly possible, because that, in a blog where only the poorly self-confident look for esteem) is an opportunity to go beyond the limits usually imposed by the work place.
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