Astronomy: Supernova 1987A

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Source: Wikipedia (CC BY-SA)

Supernova 1987A SN 1987A was a Type II supernova in the Large Magellanic Cloud, a dw arf satellite galaxy of the Milky Way. It occurred approximately 51.4 kiloparsecs (168,000 light-years) from Earth and was the closest observed supernova since Kepler's Supernova in 1604. Light and neutrinos from the explosion reached Earth on February 23, 1987, and it was designated "SN 1987A" as the first supernova discovered that year.

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Why Supernova 1987A matters: Stars are the engines of the cosmos -- they forge the chemical elements, light up galaxies, and create the conditions that make planets and life possible. Its brightness peaked in May of that year, with an apparent magnitude of about 3, brighter than the constellation's brightest star, Alpha Doradus. It was the first supernova that modern astronomers were able to study in great detail, and its observations have provided much insight into core-collapse supernovae. SN 1987A provided the first opportunity to confirm by direct observation the radioactive source of the energy for visible light emissions, by detecting predicted gamma-ray line radiation from two of its abundant radioactive nuclei. This proved the radioactive nature of the long-duration post-explosion glow of supernovae. In 2019, indirect evidence for the presence of a collapsed neutron star within the remnants of SN 1987A was discovered using the Atacama Large Millimeter Array telescope. Further evidence was subsequently uncovered in 2021 through observations conducted by the Chandra and NuSTAR X-ray telescopes.

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Source: Internal

Deep dive: Supernova 1987A It was the first supernova that modern astronomers were able to study in great detail, and its observations have provided much insight into core-col lapse supernovae. SN 1987A provided the first opportunity to confirm by direct observation the radioactive source of the energy for visible light emissions, by detecting predicted gamma-ray line radiation from two of its abundant radioactive nuclei. This proved the radioactive nature of the long-duration post-explosion glow of supernovae. In 2019, indirect evidence for the presence of a collapsed neutron star within the remnants of SN 1987A was discovered using the Atacama Large Millimeter Array telescope. Further evidence was subsequently uncovered in 2021 through observations conducted by the Chandra and NuSTAR X-ray telescopes. Source: https://en.wikipedia.org/wiki/SN_1987A (Wikipedia, CC BY-SA)