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AsteriaStar
Distance indicator · Secondary rung

Surface Brightness Fluctuations

A distance method that uses the graininess of a galaxy's light: because a nearer galaxy resolves into fewer, brighter patches of unresolved stars per pixel, the amount of pixel-to-pixel fluctuation measures distance. Best suited to smooth elliptical galaxies and the bulges of spirals.

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Sources

The primary and reference sources this topic draws on.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.