0 Members and 1 Guest are viewing this topic.
Before the development of the marine chronometer by Harrison et al the chief source of timekeeping for navigation was the passage of the Moon thru the star field.As Lee points out the eccentricity of the orbit causes a lot of problems and prediction tables had to be prepared so that adjustments could be made.When I suggested that large bodies made good time keepers I had in mind their rotational periods not of course their orbital time about other bodies.
It's the former: as I thought we'd already agreed, the second is defined by the "transition between the two hyperfine levels of the ground state of the caesium 133 atom" and most definitely not by the Earth's rotational and/or orbital periods (which are subject to stuff like earthquakes etc.).The Earth's rotational and orbital periods are defined in terms of the second.
GeezerNo the second was never defined with reference to the Earths orbital time it was defined with reference to the Earths rotational period relative to the distant stars.