A composite image of the supernova 1E0102.2-7219 contains X-rays from Chandra (blue and purple), visible light data from VLT’s MUSE instrument (bright red), and additional data from Hubble (dark red and green). A neutron star, the ultra-dense core of a massive star that collapses and undergoes a supernova explosion, is found at its center. Photo courtesy of NASA.
When a massive star dies, first there is a supernova explosion. Then, what’s leftover becomes either a black hole or a neutron star.
That neutron star is the densest celestial body that astronomers can observe, with a mass about 1.4 times the size of the sun. However, there is still little known about these impressive objects.
Now, a Florida State University researcher has published a piece in Physical Review Letters arguing that new measurements related to the neutron skin of a lead nucleus may require scientists to rethink theories regarding the overall size of neutron stars.
In short, neutron stars may be larger than scientists previously predicted.
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