psksvp said:
What I am trying to guess is,
Let's not guess - how about we work it out, together?
with that much ice, there could be O2 produced as a result??
OK, so how does one get O
2 from H
2O? As berkeman said, somehow the energy of the collision dissociates the water into H and O, which somehow get separated sufficiently to prevent any significant recombination, right?
Well, there's no lack of energy to do the dissociation! I'd worry about the separation though - what could prevent all but a tiny fraction of the H and O from recombining?[qutoe]and about the orbit of Venus, what if the Venus's orbit get bigger after the collision, the gravitation field of Venus would effect the Earth??(My Guess would be the Earth's orbit get put out also).[/QUOTE]Again, let's not guess, let's do an OOM calculation!
"Venus's orbit get bigger" is pretty much the same as 'Venus gains angular momentum', or 'Venus gets some deltaV'. The best we could do would be if the impactor added as much deltaV to Venus as it could. How much would that be? Well, we have the mass of the impactor, the mass of Venus (we can look that up easily, right?), so all we need is the impactor's relative velocity. Let's assume it's directed in the best possible way (which is what? in the same direction as Venus is traveling in its orbit? opposite? orthogonal? something else??), and is as high as an incoming KBO could be (what I mean is, if you 'drop' an object, initially at rest wrt the Sun, from a distance of a typical KBO, how fast would it be going when it hit Venus?).
What are the equations that we need?