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Astronomers Report Rare 'Type Ien' Supernova That Exposes Star's Inner Layers

A Nature study details a star that shed its outer layers, with fortuitous early spectroscopy revealing a chemical signature from deep within.

An artist's illustration depicts the bright aftermath of the supernova.
An artist’s illustration depicts silicon, argon and sulfur releasing from a massive star.
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Overview

  • The event, named SN2021yfj, is presented as a proposed new class of supernova labeled Type Ien, with authors emphasizing the designation is provisional.
  • Spectra show the absence of hydrogen, helium, and carbon, instead illuminating silicon-, sulfur-, and argon-rich material rarely seen so directly.
  • Discovery and follow-up drew on the Zwicky Transient Facility and Keck Observatory, supported by a crucial late-arriving spectrum from a UC Berkeley colleague.
  • Researchers outline tentative formation scenarios including pair-instability pulses, extreme pre-explosion mass loss, strong winds, or stripping by a companion star.
  • The explosion occurred roughly 2.2 billion light-years away, and the team is seeking additional examples through time-domain surveys and rapid spectroscopy.