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New Solar Model Shows Sun Has 55% More Silver

Replacing simplified solar-atmosphere and atomic models with more realistic physics resolves a decades-old mismatch, leading to planned validation followed by tests on other stars.

Overview

  • The revised analysis published Monday, July 20, 2026, raises the Sun’s silver abundance by about 55%, bringing the solar value into close agreement with primitive meteorites.
  • The change comes from better modeling of the Sun’s outer layers and updated atomic data for silver, which together alter how ultraviolet absorption lines are interpreted.
  • Silver’s strongest spectral lines fall in the ultraviolet and are highly sensitive to atmospheric turbulence and how light affects atoms, which earlier simpler models did not fully capture.
  • The authors say the update is a model-driven correction rather than the result of new telescope observations and they list validation steps to check for biases from other elements.
  • If confirmed, the revision will affect the Sun’s role as a chemical reference for studies of stellar composition, planet formation, and where heavy elements like silver formed in the Milky Way.