S
scottb50
Guest
I still think it is more probable that the material in the asteroid belt is low in resources, basically rocks that didn't have enough mass to clump into planets. I doubt the metallic content is very high. I also question the Ort Cloud having a lot of hydrocarbons and water ice. Judging by what we have observed it may just be more debris, like the asteroid belt, but even lighter and various Elemental gasses. <br /><br />The only reason most people talk about water ice is comets and their composition and associating them with the Ort Cloud, rather than them being much more massive objects that had the momemtum when they were formed to reach orbits at that distance. In other words Comets y pass through the Ort Cloud region in their orbits of the Sun, but they are distinct objects unrelated to the Ort Cloud. Accumulation of water and hydrocarbons can occur anywhere in their orbits and can still be occuring, shedding material when near the Sun and accumulating it as they travel outbound and back towards the Sun.<br /><br />I can see Hydrogen, Oxygen, Carbon and other atoms existing that far from the Sun, but where is the energy required to chemically combine them coming from? Maybe the velocity of a Comet could trigger it. But maybe not.<br /><br />I still think the best chance of finding profitable asteroids is to look inward from Earth, and maybe outward a ways, but probably not even as far as Mars orbit. <br /><br />I've got the Phobos photo on my desk top now and it looks like a rock, I would think if there was a lot of various materials in it you would see streaks or variations on the surface. If this is a typical asteroid object captured by Mars gravity it doesn't look too promising. <div class="Discussion_UserSignature"> </div>