Overview
- Using the VLT’s FORS2 spectropolarimetry, researchers inferred an axisymmetric, elongated breakout rather than a simple spherical blast.
- SN 2024ggi erupted in the galaxy NGC 3621 about 22 million light-years away and originated from a red supergiant roughly 12–15 times the Sun’s mass.
- The olive-like geometry flattened as the ejecta encountered surrounding material, yet the explosion maintained a consistent axis of symmetry.
- The early-time dataset supports neutrino-driven initiation and constrains competing supernova models, though key mechanism details remain open.
- The findings, led by Yi Yang and published in Science Advances, highlight the value of rapid-response observations to build a broader sample of early supernovae.