Astronomers have captured a historic image of a massive star just 26 hours after it exploded, revealing the supernova's shape in unprecedented detail. The European Southern Observatory's Very Large Telescope in Chile pointed its cameras at the phenomenon, which was first detected in April this year.
The explosion is thought to be the result of a massive star running out of fuel, causing its core to collapse and surrounding shells of mass to fall inward before bouncing off and releasing an enormous amount of energy when it breaks through the surface. This event has been described as a "cosmic firework," with scientists eager to understand the underlying processes that drive these explosive events.
The supernova, known as SN 2024ggi, is located 22 million light-years away in the galaxy NGC 3621 and is thought to have originated from a red supergiant star with 12-15 times the mass of our sun. The team used a technique called spectropolarimetry to capture the supernova's geometry, which involves measuring the polarization of its light.
The resulting image shows that the initial blast was olive-shaped, with the material spreading outward and flattening as it interacted with surrounding matter. Despite being just one point in space, researchers were able to reconstruct the supernova's shape from this data, providing a unique insight into these cosmic events.
These findings have significant implications for our understanding of stellar evolution and the physical processes that lead to supernovas. According to Yi Yang, an astronomer at Tsinghua University, "the geometry of a supernova explosion provides fundamental information on stellar evolution and the physical processes leading to these cosmic fireworks." The discovery also challenges current supernova models, paving the way for further research into these powerful explosions.
The fact that scientists were able to capture this phenomenon in its earliest moments is a testament to the power of modern astronomy. By using advanced techniques such as spectropolarimetry, researchers can now gain a deeper understanding of these cosmic events and shed light on some of the biggest mysteries in the universe.
The explosion is thought to be the result of a massive star running out of fuel, causing its core to collapse and surrounding shells of mass to fall inward before bouncing off and releasing an enormous amount of energy when it breaks through the surface. This event has been described as a "cosmic firework," with scientists eager to understand the underlying processes that drive these explosive events.
The supernova, known as SN 2024ggi, is located 22 million light-years away in the galaxy NGC 3621 and is thought to have originated from a red supergiant star with 12-15 times the mass of our sun. The team used a technique called spectropolarimetry to capture the supernova's geometry, which involves measuring the polarization of its light.
The resulting image shows that the initial blast was olive-shaped, with the material spreading outward and flattening as it interacted with surrounding matter. Despite being just one point in space, researchers were able to reconstruct the supernova's shape from this data, providing a unique insight into these cosmic events.
These findings have significant implications for our understanding of stellar evolution and the physical processes that lead to supernovas. According to Yi Yang, an astronomer at Tsinghua University, "the geometry of a supernova explosion provides fundamental information on stellar evolution and the physical processes leading to these cosmic fireworks." The discovery also challenges current supernova models, paving the way for further research into these powerful explosions.
The fact that scientists were able to capture this phenomenon in its earliest moments is a testament to the power of modern astronomy. By using advanced techniques such as spectropolarimetry, researchers can now gain a deeper understanding of these cosmic events and shed light on some of the biggest mysteries in the universe.