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Originally Posted by tomtom
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Does anyone know how fast the moon's shadow will move across the landscape at the beginning and end of totality? (And will the speeds be different?)
I remember the eclipse of 1976 in southeastern Australia and we saw the shadow moving out across the Pacific Ocean, but by golly that was quick! I wonder how fast next month's shadow will move ... in km/hr (out of theoretical interest) and in tenths of seconds from horizon to horizon (out of practical interest)?