The Slowest spinning Pulsar - " Do Scientists really need to refresh their Death Line "
Pulsars are one of the most dense and the most strange objects present out there in the Cosmos. They are called as the Light-house of the Cosmos because they continuously emit a beam of electromagnetic radiation from their poles and rotates at a rate upto 716 times per second ( that's the fastest rate ) and they are so dense that a even a teaspoon of the material would weigh more than all of the fishes present on the Earth. Recently, the rate of the slowest spinning pulsar was 7.833 times per second and everyone thought that this would be the slowest among all.
But, now researchers have found a Pulsar rotating nearly at a rate of once every 23.5 seconds - nearly three times slower than the previous record holder. This Pulsar is located at some 14 million light-years away. This Pulsar is discovered by the team led by Chia Min Tan, a doctoral student from the University of Manchester. As part of the LOFAR ( Low Frequency Array ) tied-array all-sky survey, Tan and her colleagues searched the entire Northern sky and they found one in radio pulsar PSR J0250+5854.
The radiation emitted from the Pulsar can be observed if and only if the beam of emission is pointing towards the Earth. The first Pulsar was discovered on November 28, 1967 by Jacoelyn Bell Burnell and Antony Hewish. They observed pulses separated by 1.33 seconds that originated from a particular location in the sky.
The discovery was recognised by the award of the 1974 Nobel Prize in Physics, but despite the fact that Jacoelyn Bell Burnell was the first to observe the Pulsars, Bell was excluded from the recipients of the prize. But, finally after a long time, in 2018 Bell was awarded with the Special Breakthrough Prize and with the tittle - Women of the year 2018.
- What are Pulsars ?
Gravitational Collapse of Core |
- What made PSR J0250+5854 so slow ?
This discovery was completely unexpected. All the researches across the globe are still a bit shocked. This discovery challenges and informs our theories for how Pulsars shine.
Moving forward, the team will continue to analyse the data collected by the LOFAR survey, hoping to discover the new aspects of Pulsars and as far as PSR J0250+5854 is concerned, they plan to use ESA ( European Space Agency ) XMM-Newton space telescope to further study the object in greater detail. If the super-slow Pulsar is detected as the source of X-rays, then this will give important insights into its history and origin !
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