DasBastard wrote:
You are as blind as you are stupid... there is clearly a decimal point inbetween the 1 and the 3, and the units line up perfectly with those of its neighbours. Concession accepted.
And to further debunk your "poor scan made it 11" bullshit:

My, my, my... I find it very interesting that your posted images are at a resolution far greater than what we see in the original scan-job. For instance, the original scan doesn't give us the right side of the U in Miranda's U3, nor is there a decimal point between 1 and 3 ... indeed, the 3 isn't even complete.
Where did you get these? Or, did you simply make them yourself?
You said that 7000kg/m^3 was more than double the density of any known asteroid, I have proven you wrong with the densities of both Vespa and Loreley. Deal with it.
No, I said "almost twice", so mark Vesta off. Since you feel it necessary to use straw men against me, you might also consider marking 'honesty' out of your self-opinion.
Your contention fails on numerous counts: Vespa alone crushes your lame argument.
1. It is Vesta. Idiot.
2. Vesta crushes only your straw man version of my argument.
Loreley (as well as the aforementioned but DarkStar-anaethema logic and science) show that there are asteroids considerably more dense than 7000kg/m^3.
And where does he get that figure, hmm? There is no other data on Loreley's density or mass available, that I have found, and he didn't even get the spelling right. For all we know, he got the density from the same place he got his other weird ideas:
http://www.geocities.com/CapeCanaveral/ ... mePage.htm
All I'm suggesting is that it would behoove you to find something to confirm the Expanding Earth guy's story, because basing your entire argument off of a single data point in a shoddy scan-job from a weird guy's page is pretty weak.
You conspicuously left out any links to any article that puts a specific number (or even range) to the density of Kleopatra.
Well, then, let's just do it ourselves, shall we?
Kleopatra's shape: dogbone
http://www.jpl.nasa.gov/pictures/kleopatra/
Kleopatra's size: 217km x 94km (x 94km)
http://www2.jpl.nasa.gov/files/images/c ... a02454.txt
Kleopatra's mass: ~2e18kg (using solar mass of 1.99e30kg and rounding up)
http://aa.usno.navy.mil/hilton/asteroid_masses.htm
So, we know it is a dogbone and we know the maximum size of the bone. We can therefore find upper and lower limits on density by using the maximum and minimum radii of the bone, and solving for volume on the basis of a cylinder.
A 47,000 meter cylinder yields a density of 1,328 kg/m^3.
A 23,500 meter cylinder yields a density of 5,312 kg/m^3.
Given that this is a dogbone, the actual density will fall somewhere near the middle. The middle happens to be about 3,300 kg/m^3.
Well, well, lookie at that...
Oh, now you're just a damned liar. And here you keep trying to accuse me of such things. The article doesn't say that Kleopatra is like moon rock, he says it is like the moon's surface. He also says it is "porous and loosely consolidated," where loose consolidation is precisely how he describes a fragment-and-rubble pile idea of Kleopatra's origin in the paragraph above.
Nice job in evading the point; you have yet to provide any source which shows Kleopatra has a density anywhere near what you implicitly claim.
Oooooh, stinging.
Here's a succinct quote about the issue, but I've seen it all over the place. You really don't do your homework, do you?:
Ah, fallacy, your best friend. It is your burden to provide references for your claims, not mine.
It is your burden not to be a total idiot about the basic facts of what we are discussing.
Agglomerated objects will not disappear in a puff of smoke in a collision - they will immediately break into pieces along the weakest grain surfaces. For the asteroid to be completely obliterated by explosive disintegration (as was observed), an enormous quantity of elastic strain energy must be stored in the bulk prior to mechanical failure - porous objects (especially if they are ceramic) will break apart long before sufficient energy is stored. That quantity of energy can only be stored in an object that is not only non-porous, but virtually free of microvoids, cracks or alternate-phase particles.
I've noticed a very high "bullshit density" in what you say, but this is still an impressive amount of BS, even for you.
1. You confuse the "rubble pile" with "porous".
2. You then use "porous" exclusively.
3. You claim that the asteroid's disintegration could only have been due to elastic strain, ignoring the fact that a simple dirtball will dissociate quite nicely.
3a. Further, you fail to account for the volatiles (water ice or other frozen substances) present in asteroids (which, given your assumption that the muted gray asteroid is somehow reddish and therefore M-type (which means "solid hunk'o'metal" in your mind), is understandable... if wrong. This means that the violence of the collision event and heat involved could cause these volatiles to liquify or vaporize, which will add to the dissociation during the collision, depending on how much of the asteroid these volatiles represented.
Finally, take a look at this, and notice the behavior of the asteroids:
http://www.astro.umd.edu/~dcr/Research/rubble.html
Hmm... doesn't look like your story at all, does it?