[X] My Assistant

[dvandorn]

It occurs to me that there are two rather obvious mechanisms that could be limiting the obvious signs of cratering on Titan. The one that seems to get all the discussion is weathering/resurfacing -- it's common to date planetary surfaces by crater counts, after all.

But Titan has another mechanism going that we here on Earth are all too familiar with -- atmospheric destruction of impactors. Titan not only has an atmosphere, it's something like 1.5B at the surface, so it's even denser than our atmosphere. Result: a lot of the impactors that would leave visible craters on other planetary bodies burn up in Titan's atmosphere.

Also, while some reports are saying that the radar has discovered the only two craters found on Titan, I seem to see craters of varying sizes and levels of degradation in both the radar images and the ISS images. Circular features that remind me strongly of craters, at any rate. Not very many of them, but they're there, I think. So, there ought to be a way to use crater counting, even on Titan.

So, I guess my question is: Is there a correction algorithm of some kind that can account for the winnowing of impactors by Titan's atmosphere? If so, can it be applied to help us use crater counting to determine surface ages? And, I guess more basically, what's the current thinking on how important atmospheric winnowing is in the lack of numerous Titanian craters?

-the other Doug