Overview
- Astrophysicists now recognize black hole–star encounters as a viable trigger for supernovae, providing the strongest direct evidence of this mechanism
- The paper outlines two plausible scenarios: a >30-solar-mass star engulfing a stellar-mass black hole or a tidal disruption of the star by its black hole companion
- Detailed archival photometry identifies years of pre-explosion brightening and two concentric circumstellar shells whose interaction with the blast explains SN 2023zkd’s double-peaked light curve
- The LAISS AI system flagged SN 2023zkd as an outlier in ZTF data, enabling rapid multiwavelength observations that underpinned the comprehensive analysis
- Authors recommend systematic searches with next-generation facilities such as the Vera C. Rubin Observatory to discover more rare black hole–driven transients and refine stellar-evolution models