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Recent Podcast
A Tour of SDSS J103842.59+484917.7
A Tour of SDSS J103842.59+484917.7
One hundred years ago this month, Albert Einstein published his theory of general relativity, one of the most important scientific achievements in the last century. (2015-11-24)

47 Tucanae: The Mysterious Afterlife of Stellar Giants

Narrator (April Hobart, CXC): Neutron stars are the ultra-dense cores left behind after a massive star reaches the end of its life and explodes. The star's outer layers are blasted away in the explosion, but material at the centre of the star collapses in on itself. This forming a tightly packed ball of material and what we end up with is the densest (meaning 'most tightly packed') object known in the entire Universe outside of a black hole: a neutron star!

This new space picture shows a group of stars called a globular cluster. These are some of the oldest objects in space - almost as old as the Universe itself! This means many of the stars within have already lived their lives. The most massive have long since exploded, leaving behind several neutron stars.

Using a neutron star within this cluster, along with several others, astronomers have worked out the relationship between the stars' mass (how much material they have) and how big they are.

The new data shows that an average neutron star, with the same mass as around one and a half of our Sun's, would be around 12 km across. That's about the size of a town! With all this material packed down into such a small space, neutron stars are unbelievably dense objects. The pressure at their centers is over ten trillion trillion times the pressure required to form diamonds inside the Earth.

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