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Mar 8, 2019 at 6:47 answer added Dubukay timeline score: 1
Mar 8, 2019 at 2:08 history edited QuiGonJon CC BY-SA 4.0
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Mar 8, 2019 at 1:10 history edited QuiGonJon CC BY-SA 4.0
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Mar 8, 2019 at 0:44 comment added QuiGonJon I guess just imagine increasing Venus's rotational rate, but at what point would the wind currents divide into multiple Hadley cells. Except with earth like conditions and similar temperature conditions. I saw your previous answer, and in a lot of ways that would make my job easier lol, but I still threw this out here in case someone had an answer.
Mar 8, 2019 at 0:42 comment added QuiGonJon Ah, I'll have to go back and edit for clarity. The planet rotates on an axis in the same way Earth does, just much slower. Its not tidally locked, but it is rotating slow enough so that hot and cold "poles" slowly migrate along the equator. Essentially the day cycle is so long that the temperature differential creates one large Hadley cell of winds migrating from hot pole to cold pole, etc., as you would theoretically see in a tidally locked planet, and as we can observe on Venus.
Mar 7, 2019 at 7:54 comment added Dubukay Also, to clarify - your planet has one hot pole and one cold pole, as in it’s rotating on an axis that constantly points at the star? And the equator is medium temperature?
Mar 7, 2019 at 7:52 comment added Dubukay My answer here feels relevant, but that’s also the shameless self promotion talking
Mar 7, 2019 at 7:05 history edited QuiGonJon CC BY-SA 4.0
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S Mar 7, 2019 at 3:51 history suggested DrSheldon CC BY-SA 4.0
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Mar 7, 2019 at 3:31 review Suggested edits
S Mar 7, 2019 at 3:51
Mar 7, 2019 at 2:20 review First posts
Mar 7, 2019 at 3:31
Mar 7, 2019 at 2:16 history asked QuiGonJon CC BY-SA 4.0