Editing Talk:2682: Easy Or Hard
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I got 2.125*10^-17 m/s^2, or 3.18*10^-18 N, for the gravitational force/acceleration from the Eiffel Tower on a baseball on Fenway Park. Someone might want to check my calculations, though.--[[User:Account|Account]] ([[User talk:Account|talk]]) 23:42, 7 October 2022 (UTC) | I got 2.125*10^-17 m/s^2, or 3.18*10^-18 N, for the gravitational force/acceleration from the Eiffel Tower on a baseball on Fenway Park. Someone might want to check my calculations, though.--[[User:Account|Account]] ([[User talk:Account|talk]]) 23:42, 7 October 2022 (UTC) | ||
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: It occurred to me that the Boston to Paris gravity question might not be quite as easy as it seems, since the relevant distance would be not “as the crow flies,” but more “as the mega-gopher digs.” (I think?) [[User:Miamiclay|Miamiclay]] ([[User talk:Miamiclay|talk]]) 21:11, 9 October 2022 (UTC) | : It occurred to me that the Boston to Paris gravity question might not be quite as easy as it seems, since the relevant distance would be not “as the crow flies,” but more “as the mega-gopher digs.” (I think?) [[User:Miamiclay|Miamiclay]] ([[User talk:Miamiclay|talk]]) 21:11, 9 October 2022 (UTC) | ||
:: I already edited it away from the (implied) suggestion of Great Circle distance (as a trivial understanding of 'distance between', and probably what most searches for a value would turn up). But using latitude, longitude and radius (local, +altitude if you're into the detail) from a sufficiently accurate geophysical model (at least an oblate spheroid) as spherical coordinates leads quickly to true-ish straight-line length. And probably doesn't need to be sigbificantly further adjusted by the small dimple in spacetime that the Earth puts there, or even the fringe distortions of other tide-inducing (and therefore variable) gravitational bodies. | :: I already edited it away from the (implied) suggestion of Great Circle distance (as a trivial understanding of 'distance between', and probably what most searches for a value would turn up). But using latitude, longitude and radius (local, +altitude if you're into the detail) from a sufficiently accurate geophysical model (at least an oblate spheroid) as spherical coordinates leads quickly to true-ish straight-line length. And probably doesn't need to be sigbificantly further adjusted by the small dimple in spacetime that the Earth puts there, or even the fringe distortions of other tide-inducing (and therefore variable) gravitational bodies. | ||
