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Jan 8, 2023 at 8:43 comment added longtry Here's my napkin calc. Assuming a long totality of 2mins, that translates to 50km of 'gain' for a person at the equator looking at sunrise/set. That corresponds to ~0.13% change in angle in apparent diameter. So at best, a totality will change to/from just a few tiny Bailey beads. Yet it could mean a 50-fold change in brightness!
Jan 7, 2023 at 17:08 comment added James K But even then the moon is moving transversely at over 2000 mph, I think the transverse motion always "wins"
Jan 7, 2023 at 16:50 comment added Greg Miller I think one case to consider is an observer viewing an eclipse at sunrise/sunset. At the equator, that person would be moving about 1000Mph towards or away from the moon. I think it's conceivable an observer could move from a distance of annularity to totality. I doubt there's an eclipse where this actually happens though.
Jan 7, 2023 at 16:36 history answered James K CC BY-SA 4.0