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Astronomers Capture First Ever Early Snapshot of Supernova Shock Wave Using ESO’s VLT

Astronomers Capture First-Ever Early Snapshot of Supernova Shock Wave Using ESO’s VLT

ESO’s Very Large Telescope captured an unprecedented early snapshot of supernova SN 2024ggi, revealing an elongated, olive-shaped shockwave just a day after discovery.

Written by Gadgets 360 Staff | Updated: 17 November 2025 23:15 IST

Astronomers Capture First-Ever Early Snapshot of Supernova Shock Wave Using ESO’s VLT

Photo Credit: ESO/L. Calçada

This artist’s impression shows a star going supernova.

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Highlights

VLT records rare shock-breakout supernova phase
SN 2024ggi shows an unexpected olive-shaped blast
Discovery reshapes models of star death

Astronomers using the European Southern Observatory's Very Large Telescope (VLT) captured a rare early view of a supernova's explosion, including the shape of its expanding shock wave. The star, SN 2024ggi, erupted in April 2024 in the galaxy NGC 3621 about 22 million light-years away. Observations just a day after discovery revealed that the blast was elongated – an olive-like shape rather than spherical. This first-of-its-kind snapshot provides new clues about how massive stars die.

Capturing the Explosion

According to media reports, the supernova was first detected on April 10, 2024, and the VLT began follow-up observations the next day. Using the FORS2 instrument for spectropolarimetry, astronomers measured the polarisation of the star's light. Although the supernova appeared as a point of light, its polarization pattern revealed details of the explosion's shape. This rapid spectropolarimetric snapshot captured the shock-breakout phase – the moment the explosion's blast wave punched through the star's surface – a phase normally too brief to study.

Astronomers Reveal Early Asymmetric Blast of a Supernova

Olive-Shaped Blast Surprises

According to the recent study published in Science Advances, analysis of the FORS2 data revealed that the early blast was indeed olive-shaped, flattening as it expanded while retaining the same axis of symmetry. This points to a global mechanism driving the explosion along that axis.

Interestingly, when the blast interacted later with older gas shed by the star, the explosion's axis seemed to shift-maybe because a companion star had affected the geometry. Already, these results rule out some models of supernovae and fill in details of others, sharpening the picture of how stars die.

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