granthutchison wrote:Hmm, your link doesn't bring anything up but an empty page, for me.
Hmm. Try right-clicking and saving the file that way. It's probably coming up empty because it's spending ages downloading the file - the link definitely works though
Am I right in thinking that in this situation the orbital distance does change slightly in order to preserve angular momentum, but because the orbital angular momentum is so much larger than the change in rotational angular momentum, the change in orbital distance is negligible? Or is something going in that preserves the orbital distance unchanged?
Well, OK - to clarify, it does change a bit, but it's a really really small change that isn't worth considering here
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Though of course, nowadays we have all these ideas of planets spiralling in and out through gas drag and other things, but I didn't consider that sort of thing in my thesis.