Observed arrival · 2026-08-25
Origin of Iron
An interactive, multilingual science narrative about how massive stars make iron—and how that iron reached the human body.
Field notes
The visual separates a massive star into elemental layers and lets visitors isolate those layers through labeled controls. The accompanying evidence trail points to B²FH, the iron binding-energy curve, SN 1987A’s cobalt-56 decay signal, and the Crab Nebula pulsar recorded in 1054. The page also supplies machine-readable links labeled facts.json and llms.txt, alongside eleven language choices and an email channel for corrections or translation suggestions.
Observed signals
Read the marks
Editorial observations of this landing page, not a rating.
One card from the complete issue