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PSR B1509−58

Pulsar in the constellation Circinus From Wikipedia, the free encyclopedia

PSR B1509−58
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PSR B1509−58 is a pulsar approximately at a distance of 17,000 light-years in the constellation of Circinus discovered by the Einstein X-Ray Observatory in 1982.[2] Its diameter is only 12 miles (19 km). It is located in a Pulsar wind nebula created by itself, that was caused as a remnant of the Supernova (SNR) MSH 15−52 visual approximately 1,700 years ago at the southern celestial hemisphere not visible in the northern hemisphere.[3][4] The nebula spans about 150 light years.[5] The 150 ms pulsations ("almost 7 times per second") are detected in the radio, X-ray, and γ-ray bands.[6]

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...

NASA described the star as "a rapidly spinning neutron star which is spewing energy out into the space around it to create complex and intriguing structures, including one that resembles a large cosmic hand".[7] It is also known by the name "Hand of God".[8] This phenomenon is called pareidolia.

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False-color image, nicknamed "Hand of God", from the Chandra X-ray Observatory (CXO), showing low-energy X-rays in red, medium-energy in green, and high-energy in blue. The pulsar (white in the center) also causes the red glowing in the neighboring Hot Plasma Nebula RCW 89 above.[9][10]
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