The Crab Nebula has been part of several studies by astronomers. It began back on February 22, 1971, when a sounding rocket took off carrying specialized sensors directed towards the Crab Nebula from Wallops Island, Virginia. Later on, Martin Weisskopf, an astronomer, suggested the creation of an Earth-orbiting satellite, equipped with advanced instruments to obtain more comprehensive data on the Crab Nebula and other enigmatic cosmic entities. This idea eventually emerged with NASA's Imaging X-ray Polarimetry Explorer (IXPE), which was launched on December 9, 2021.
Following over five decades since the sounding rocket trial, scientists have used IXPE to produce a comprehensive and intricate depiction of the Crab Nebula's magnetic field, revealing more about its inner mechanics than ever before. According to IXPE findings, the Crab Nebula's magnetic field structure bears a resemblance to the Vela Pulsar Wind Nebula, taking on a similar donut shape. However, scientists were taken aback to observe that in the Crab Nebula, patches of magnetic turbulence were more unevenly distributed and asymmetrical than anticipated.
The Crab Nebula is situated in the Taurus constellation, a staggering 6500 light-years distant from Earth, and was formed as a result of a supernova recorded in 1054. The aftermath of the explosion left behind a dense object known as the Crab Pulsar, which is about the size of Huntsville, Alabama, or the length of Manhattan, but possesses a mass equivalent to two Suns.
With the hope to understand the extreme environmental conditions of the Nebula, they used the polarization of X-rays emanating from the Crab Nebula, which emits a brilliant X-ray glow. The polarization of X-rays provides scientists with indications
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