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Thank you for taking my question. I really appreciate that. I have studied the material in Occator and other craters. This instance seems to be unique in it's preservation/age and form. Can you point me to a similar one? How do you determine impact trigger probability? TY!
The last few @NASA_Dawn journals show pictures of material flowing down crater walls. Look here:https://dawn.jpl.nasa.gov/mission/journal.html …
I'm familiar. Which image(s) are you referring to exactly? To say material flows down walls of craters is different from explaining a 30+ mile avalanche spanning across the rugged terrain of a large impact crater. Wouldn't you say? We have analogs on Mars. How's it not similar?
I'm not sure if you studied the fourth image, but you might have missed just how massive this avalanche is. I don't think material being pulled by gravity has the energy to make this kind of avalanche. I think there are many other reasons to think it was impact-triggered as well.
So, let me get this straight: my explanation (the same as here) on Mars is a "viable contender" to @NASAAmes, however, @NASAJPL seems to think it isn't when applied to Ceres?
I still can't get any response from @NASA_Dawn. I don't know why this is so difficult.
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