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We describe a rigorous construction, using matched asymptotic expansions,
which establishes under very general conditions that local terrestrial and
solar-system experiments will measure the effects of varying constants' of Nature occurring on cosmological scales to computable precision. In particular, constants’ driven by scalar fields will still be found to evolve in time when
observed within virialised structures like clusters, galaxies, and planetary
systems. This provides a justification for combining cosmological and
terrestrial constraints on the possible time variation of many assumed
`constants’ of Nature, including the fine structure constant and Newton’s
gravitation constant.

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