“NASA’s Fermi telescope has detected gamma rays from a rare superluminous supernova, providing new clues about one of astronomy’s biggest mysteries. Credit: Shutterstock.” (ScitechDaily, NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before)
NASA’s Fermi telescope spotted a supernova. That has incredible brightness. There is suspicion that the powerhouse behind this hyper-powerful supernova is a magnetar. That beam sends a beam. That hits. The giant star. When a high-energy particle beam hits the star. That thing can cause a violent explosion. In some cases, there is suspicion that the neutrino or electron beam.
Or a fast radio burst (FRB) can cause a violent eruption. In the case of neutrino beams, the neutrino beam forms the energy pothole. Or a lower energy tunnel in the star’s plasma. That lower energy tunnel. Causes a situation where energy starts to fill it. In that case, the plasma falls into that tunnel. And then it forms a fusion reaction. The reaction is the same as in the massive plasma eruptions on the sun. They form in the lower energy point. And then plasma starts to pack in that point. That causes a violent eruption. In the cases. That magnetars send a beam through the giant star. That creates. The lower energy tunnel.
That goes through the entire star. In that case, the area where the plasma starts to pack is much larger. Than in the cases. Of the solar massive plasma eruptions. If the Earth is a straight line to the beam that this reaction sends. That makes. The energy that the eruption sends. Seems very powerful.
In the cases of the FRB, the beam causes interaction in the star’s core. The energy level rises. And that can blow the outer shell of the star away. In all cases, they form the asymmetry in energy levels. That causes a situation. Where plasma starts to pack. In those lower energy points. In both cases. The problem is this. The magnetar can send a beam through the star. But the point that starts the reaction is hidden. There is a possibility. That is when the temperature of the star’s core rises.
That thing sends massive neutrino or electron beams through the star. That makes the radiation look like the sea urchin. That causes an energy pack. To those lower energy points. The higher energy point in the star will not destroy it as easily as the lower energy point. The higher energy point will send the wave across the star. But. That wave spreads all over the star. The lower energy point. Or, tunnel packs the matter and energy into those points. And that causes fusion or the reflecting wave that travels across the star. In some models, when the energy production in the star ends.
The magnetic field starts to pack matter in the star’s magnetic poles. That forms a fusion reaction that sends the energy impulse straight to the star’s core. In that model, the fusion reactions at the star’s poles push the star into form. That looks like a balloon that was pressed from the top. This forms an energy asymmetry. That stretch gives energy space to move.
“This composite image shows two views of SN 2017egm, in visible light (inset) and gamma rays (background). The optical image shows the supernova — the brightest object in the scene — and its host galaxy on July 1, 2017. The background map shows a wide area of the sky surrounding the supernova’s position. Brighter colors indicate a greater statistical likelihood that gamma rays are associated with the explosion. The map includes gamma rays detected by Fermi’s Large Area Telescope from July 5, 2017, to October 25, 2017, or from 43 to 155 days after the supernova was discovered. Credit: Background, NASA/DOE/Fermi LAT Collaboration and Acero et. al. 2026; inset, NOT+ALFSOC/Bose et al. 2020” (ScitechDaily, NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before)
“The superluminous supernova SN 2017egm was discovered by the European Space Agency’s Gaia mission on May 23, 2017. It exploded in a massive barred spiral galaxy known as NGC 3191, shown on the left before the eruption. The image at right, taken on July 1, 2017, shows the supernova outshining the entire galaxy. Credit: Left, SDSS and PS1; right, NOT+ALFSOC/Bose et al. 2020. (ScitechDaily, NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before)
“This X-ray image shows extended emission around a source known as Swift J1834.9-0846, a rare ultra-magnetic neutron star called a magnetar. The glow arises from a cloud of fast-moving particles produced by the neutron star and corralled around it. Color indicates X-ray energies, with 2,000-3,000 electron volts (eV) in red, 3,000-4,500 eV in green, and 5,000 to 10,000 eV in blue. The image combines observations by the European Space Agency’s XMM-Newton spacecraft taken on March 16 and October 16, 2014.” (ScitechDaily, NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before)
“The Crab Nebula formed in a supernova explosion observed in 1054. At its heart lies an isolated neutron star, the crushed core of the original star. It spins about 30 times a second, sweeping a beam of radiation toward Earth with every rotation, lighthouse style, which classifies the neutron star as a pulsar. This rapid spin powers X-ray jets (elongated blue-white feature near center) and a high-speed outflow of electrons and other particles. The particles collect in a vast cloud-like structure called a pulsar wind nebula, which also forms around magnetars, the pulsar’s supermagnetized cousin. This emission gradually slows the neutron star’s spin. These images combine X-ray data from NASA’s Chandra X-ray Observatory (bluish white) and infrared data from NASA’s James Webb Space Telescope. Credit: X-ray, Chandra: NASA/CXC/SAO; Infrared, Webb: NASA/STScI; Image Processing: NASA/CXC/SAO/J. Major.”(ScitechDaily, NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before)
There is always. A small whirl in the points of the spin axle of the star’s core. That denser plasma point aims energy into the star’s core. The process is similar. As we will hit the apple. From both sides with nails. When those energy pikes hit together. They send a shockwave through the star. The symmetry of the energy waves is the thing. That determines whether the star resists that wave. If the energy that the star’s core sends through the star. It is a symmetrical ball. It matters ahead. That causes a fusion reaction ahead of that wave.
But if the wave is asymmetrical. Or, it looks like a plate or disk. That thing forms two whirls. Those whirls push matter. That injects energy into the star’s core. In symmetrical eruptions, the energy level must be higher than in asymmetrical eruptions. So that it destroys the star. In the cases of asymmetrical eruption, the eruption forms whirls. That causes energy impulses inside the star. Those energy impulses cross each other. They send a reflecting wave. And that forms entropy. That destroys the star.
That energy creates asymmetry in the energy fields. And those asymmetrical structures allow energy to move. In normal cases, the energy travels. Out from the star nicely. But that radical reaction causes whirls in the star. Those whirls pack matter in them. And that thing forms multiple energy points in the star. Those points send energy that breaks the gravity.
https://scitechdaily.com/nasas-fermi-telescope-caught-a-supernova-doing-something-never-seen-before/
