16K views · 511 reactions | This visualization features a...
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FacebookNASA's Hubble Space Telescope
16K views · 511 reactions | This visualization features a...
NASA's Hubble Space Telescope. . This visualization features a three-dimensional multiwavelength representation of the Crab Nebula, an iconic remnant of a star that was seen exploding in the year 1054 AD. This is a view looking into the heart of the nebula, home to its rapidly spinning crushed stellar core, called a pulsar. The torrential ...
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What’s a pulsar? Why does it pulse?
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On November 28, 1967, astronomers found the first pulsar. Space History Archives👉 https://space-com.visitlink.me/xsOjwW A pulsar is a super-dense star that rotates super fast. As the pulsar spins, it emits two beams of light in opposite directions. When astronomers look at a pulsar, it looks like a star that's flickering on and off at a steady, constant pace. The first pulsar was observed by Jocelyn Bell Burnell and Antony Hewish. They were looking at the constellation Vulpecula when they saw a
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A pulsar is a rapidly rotating neutron star that emits a radio beam the way a lighthouse emits a light beam. We receive a radio pulse for each rotation of the star. The period T of rotation is found by measuring the time between pulses. The pulsar in the Crab nebula has a period of rotation of T=0.033  s that is increasing at the rate of 1.26 ×10^-5  s / y. (a) What is the pulsar's angular acceleration α? (b) If αis constant, how many years from now will the pulsar stop rotating? (c) The pulsar
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