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Most of the objects that NASA and other scientific organizations choose to study in space are incredibly old, but this is not the case of Kes 75. Located 19,000 years ago -Light of the Earth, Kes 75 is an ultra-dense star block become supernova. , and now scientists call it the youngest known pulsar of the Milky Way galaxy.
In a new message on its website, NASA explains how the pulsar was detected and displays a pretty stunning picture of its current appearance.
A pulsar is a neutron star that seems to pulse when it is observed. Neutron stars are the remains left after certain stars have turned into supernovae. These super-dense objects have really weird properties and often spin quickly, releasing energy as they spin. When the flow of radiation sweeps our position, the star seems to throb.
NASA's Chandra X-Ray observatory is very effective at detecting such objects. It follows the development of Kes 75 since 2000. After checking the star in 2000, 2006, 2009 and 2016, NASA was able to see how the pulsar has changed over time. The result is the image you see above.
In this composite image of Kes 75, the high-energy X-rays observed by Chandra are colored blue and highlight the pulsar nebula surrounding the pulsar, while the low-energy X-rays appear in purple and show the debris of the pulsar. Explosion, NASA explains
Late last week, NASA announced that its Chandra X-Ray observatory had broken down due to a system malfunction and that the safe mode of the spacecraft had been activated. Earlier this week, it was announced that the satellite was operational again, which is good news, especially when it is able to make discoveries like this one.
Image Source: X-Ray: NASA / CXC / NCSU / S. Reynolds; Optics: PanSTARRS
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