- #1
Surayabay
- 15
- 5
Leavitt's Law allows us to determine how far stars are from us by calculating their variable magnitude of brightness. Please explain how it's possible then for us to see, with the 'natural eye', the distances from one star to another, from one point in the night sky to the opposite, that would take x-# of lightyears traveling at the 'SOL' to reach? (What process allows us to 'see lightyears of distance' with the natural eye?)