Robert Maynard
Volunteer Moderator
The video is uploaded now: https://www.youtube.com/watch?v=gEtHu3AXw2Q
Wow they seriously posted the whole 7.5hr feed? How about a nice summary for those of us with a life?
David Braben answers for the first hour of the video.
On a related note, Ed read my question (YAY!), but I didn't write clearly enough and neither of them understood it (I'M NOT WORTHY!).
(I had tried to ask why the new terrain system introduced in 2.0 wasn't implemented on rocky, metal, or ice worlds if they have atmosphere) I'll try again for 2.2 I guess.
On a related note, Ed read my question (YAY!), but I didn't write clearly enough and neither of them understood it (I'M NOT WORTHY!).
(I had tried to ask why the new terrain system introduced in 2.0 wasn't implemented on rocky, metal, or ice worlds if they have atmosphere) I'll try again for 2.2 I guess.
Well obviously it's because they won't look the same if they have an atmosphere (and won't have nearly as much craters). Oxygen or other gases + winds tend to influence the way surfaces are formed. So basically you need a different terrain system for those planets.
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A written summary on the forum would be nice