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NASA Kepler's space telescope recently withdrew its ability to capture thousands of exoplaneers for its reputation. But this year he presented the mysterious observation of the supernova.
Kepler's scientists offered an alternative to the supernova before, during and after the coming lights. This excellent data, when the scientists write, have deepened the mystery why this supernova type 1 shines brightly after the blow and the last explosion.
Scientists were first presented with a supernova 2018oh called the Super All Inclusive Sky Survey, which was released on February 4, 2018 through five telescopes around the world.
Fortunately, the UGC 478 supernova happened to be part of the galaxy-watching campaign of the Kepler space telescope. Scientists could combine sensitive data from Kepler with specialized observations of supernova colors using telescopes such as the Dark Energy Camera and the Pan-STARRS1 telescope.
It may be strange – why was the exoplanet hunter looking at the remote galaxy? Kepler unveils the images of the same place in the same survey and sees thousands of galaxies simultaneously. Additionally, the slight changes in the number of light given by the objects are sensitive, because it looks for clear lights that are on the planets passing through the farthest stars.
2018 and type 1 is a supernova, depending on what the light looks like. The modules show that these supernumbers, which come from a pair of stars, that is, a white dwarf, is a great deal before it starts to explode. This is still the fourth kind of supernova seen in a Kepler survey, and the closest and brightest is the most accurate data.
Many researchers recently released supernova cleansing tests. Both results, such as the "light curve" or the graph of the amount of light did not appear the same curve. Instead, he had an upward direct piece, where the supernovae had more hopes for more than five days before rising, it seemed to be happening in two different processes.
They emphasized that the supernova was lower than the others.
So what was the brilliance of the two sides of the supernova? There are several ideas. Maybe the lights came together with the nearby star, which offered the explosion fuel. Or maybe there was a helium shell on the surface of the white dwarf, and he gave more material ignition. Or maybe the radioactive nickel was mixed with the star, which signaled the signature. The observations with the X-ray telescope exploded the interactions with the star-shaped interactions.
We talked about a researcher, it would start too early for a response, and maybe it might be a drawback again. "The theory that people have to go back to books and have to build a model of different ways of early broadcasting," said Maximillian Stritzinger, a Danish physicist at Aarhus University, who has studied the colors given by these supernova types.
Supernova combines the list of difficult types to describe the type 1, according to studies. But it's still hope. Kepler has still seen more supernumbers, which scientists say will help them solve the mystery.
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