Astronomy spans an enormous hierarchy of physical scales: planets orbit stars, stars inhabit galaxies, galaxies gather into groups and clusters, and those systems trace filaments and voids in the cosmic web.
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The apparent size and brightness of an object depend on both its physical size and distance.
supportedSolar-system distances are measured with radar and spacecraft tracking; stellar distances use parallax and related methods; galaxy distances use calibrated luminosity relations and redshift-dependent cosmological models.