Overview
- Researchers observed SN 2024ggi in galaxy NGC 3621 roughly 22 million light-years away during the fleeting breakout phase of its core-collapse supernova.
- FORS2 spectropolarimetry on the Very Large Telescope enabled reconstruction of the explosion’s geometry from the polarization of unresolved light.
- The initial blast exhibited a strongly axisymmetric, olive-like shape that later flattened as it encountered surrounding material while keeping the same symmetry axis.
- The results support asymmetric, neutrino-driven shock scenarios as leading explanations for how such explosions begin, though the data do not definitively settle the mechanism.
- A rapid target-of-opportunity request led by Yi Yang secured VLT observations 26 hours after discovery and about 29 hours after the shock first breached the star’s surface.