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Scientists Have Discovered A Neutron Star That Released As Much Energy As The Sun Produces In 100,000 Years

Scientists Discovered Variations In The Eruption Of A Neutron Star With The Same Amount Of Energy As The Sun

The Sun is the closest star to Earth, but scientists are still trying to grasp the Sun’s core, which often generates tremendous solar winds that threaten our planet. While such research is underway, an international team of scientists has attempted to investigate a neutron star formed when a giant star dies in a supernova and its core collapses, resulting in neutrons.

The research claims to have measured the oscillations in a magnetar — a type of neutron star thought to have an extraordinarily powerful magnetic field during its turbulent moments as a first. However, the scientists discovered that the magnetar was released in less than a tenth of a second.

“Even in an inactive state, magnetars can be one hundred thousand times more luminous than our Sun, but in the case of the flash that we have studied — the GRB2001415 — the energy that was released is equivalent to that which our Sun radiates in one hundred thousand years,” lead researcher Alberto J. Castro-Tirado, from the IAA-CSIC, a Spanish government institute, said in a statement.

According to the study, the tenth-of-a-second explosion was discovered on April 15, 2020, amid COVID-19. The flare was “detected by the Atmosphere–Space Interactions Monitor instrument aboard the International Space Station.” Scientists have been analyzing the data since then.

Magnetars are neutron stars with the most strong magnetic fields known. They can hold half a million times the mass of the Earth. So far, just 30 of these objects have been discovered.

This artist’s impression shows the magnetar in the very rich and young star cluster Westerlund 1. This remarkable cluster contains hundreds of very massive stars, some shining with a brilliance of almost one million suns. European astronomers have, for the first time, demonstrated that this magnetar — an unusual type of neutron star with an extremely strong magnetic field — probably was formed as part of a binary star system. The discovery of the magnetar’s former companion elsewhere in the cluster helps solve the mystery of how a star that started off so massive could become a magnetar rather than collapse into a black hole.

“These extremely high-frequency oscillations in the burst peak are a crucial component that will aid our understanding of magnetar giant flares,” the study added.

The findings were reported in the journal Nature.