The Times Australia
The Times World News

.

What happens when matter is squashed to the brink of collapse? We weighed a neutron star to help NASA find out

  • Written by Daniel Reardon, Postdoctoral researcher in pulsar timing and gravitational waves, Swinburne University of Technology

Neutron stars are some of the most extreme objects in the universe. Formed from the collapsed cores of supergiant stars, they weigh more than our Sun and yet are compressed into a sphere the size of a city.

The dense cores of these exotic stars contain matter squashed into unique states that we can’t possibly replicate and study on Earth. That’s why NASA is on a mission to study neutron stars and learn about the physics that governs the matter inside them.

My colleagues and I have been helping them out. We used radio signals from a fast-spinning neutron star to measure its mass. This enabled scientists working with NASA data to measure the star’s radius, which in turn gave us the most precise information yet about the strange matter inside.

Read more: Explainer: what is a neutron star?[1]

What is inside a neutron star?

Matter in the core of neutron stars is even denser than the nucleus of an atom. As the densest stable form of matter in the universe, it is squashed to its limit and on the brink of collapse into a black hole. Understanding how matter behaves under these conditions is a key test of our theories of fundamental physics.

NASA’s Neutron star Interior Composition ExploreR (NICER) mission[2] is trying to solve the mysteries of this extreme matter.

NICER is an X-ray telescope on the International Space Station. It detects X-rays coming from hot spots on the surface of neutron stars where temperatures can reach millions of degrees.

Scientists model the timing and energies of these X-rays to map the hot spots and determine the mass and size of the neutron stars.

Knowing how the sizes of neutron stars relate to their masses will reveal the “equation of state” of the matter in their cores. This tells scientists how soft or hard – how “squeezeable” – the neutron star is, and therefore what it is made of.

A softer equation of state would suggest that neutrons in the core are breaking apart into an exotic soup of smaller particles. A harder equation of state might mean neutrons resist, leading to larger neutron stars.

The equation of state also dictates how and when neutron stars get ripped apart when they collide[3].

Solving the mystery with a neutron star neighbour

One of NICER’s primary targets is a neutron star called PSR J0437-4715, which is the nearest and brightest millisecond pulsar.

A pulsar[4] is a neutron star that emits beams of radio waves that we observe as a pulse every time the neutron star rotates.

This particular pulsar rotates 173 times per second (as fast as a blender). We have been observing it for almost 30 years with Murriyang[5], CSIRO’s Parkes radio telescope in New South Wales.

Murriyang, CSIRO’s Parkes radio telescope. CSIRO

The team working with NICER data faced a challenge for this pulsar. X-rays coming from a nearby galaxy made it hard to accurately model the hot spots on the neutron star’s surface.

Fortunately, we were able to use radio waves to find an independent measurement of the pulsar’s mass. Without this crucial information, the team would not have recovered the correct mass.

Weighing a neutron star is all about timing

To measure the neutron star’s mass, we rely on an effect described by Einstein’s theory of general relativity, called the Shapiro delay.

Massive and dense objects such as pulsars – and in this case its companion star, a white dwarf – warp space and time. The pulsar and this companion orbit one another once every 5.74 days. When pulses from the pulsar travel to us across the compressed spacetime surrounding the white dwarf, they are delayed by microseconds.

A white dwarf orbits a pulsar, warping spacetime and delaying radio pulses from the pulsar. Credit: Carl Knox / OzGrav.

Such microsecond delays are easy to measure with Murriyang from pulsars like PSR J0437-4715. This pulsar, and other millisecond pulsars like it, are observed regularly by the Parkes Pulsar Timing Array[6] project, which uses these pulsars to detect gravitational waves.

Read more: Using a detector the size of a galaxy, astronomers find strongest evidence yet for gravitational waves from supermassive black hole pairs[7]

Because PSR J0437-4715 is relatively close to us, its orbit appears to wobble slightly from our point of view as Earth moves around the Sun. This wobble gives us more details about the geometry of the orbit. We use this together with the Shapiro delay to find the masses of the white-dwarf companion and the pulsar.

The mass and size of PSR J0437-4715

We calculated[8] that the mass of this pulsar is typical of a neutron star, at 1.42 times the mass of our Sun. That’s important because the size of this pulsar should also be the size of a typical neutron star.

Scientists working with the NICER data were then able to determine the geometry of the X-ray hot spots and calculate that the neutron star’s radius is 11.4 kilometres[9]. These results give the most precise anchor point[10] yet found for the neutron star equation of state at intermediate densities.

Our new picture already rules out the softest and hardest neutron star equations of state. Scientists will continue to decode exactly what this means for the presence of exotic matter in the inner cores of neutron stars. Theories suggest this matter may include quarks that have escaped their normal homes[11] inside larger particles, or rare particles known as hyperons[12].

The millisecond pulsar PSR J0437-4715, on the left as seen from Earth and on the right as seen from its own equatorial plane. The purple-pink colour indicates the temperature of the hot spots at the poles. The hot magnetic poles are not exactly opposite each other. Because the star is so dense, the animations also show the effect of light bending caused by extreme gravity. NASA / Sharon Morsink / Devarshi Choudhury et al.

This new data adds to an emerging model of neutron star interiors that has also been informed by observations[13] of gravitational waves from colliding neutron stars and an associated explosion called a kilonova.

Murriyang has a long history of assisting with NASA missions, and was famously used as the primary receiver of footage for most of the Apollo 11 moonwalk[14]. Now, we have used this iconic telescope to “weigh in” on the physics of neutron star interiors, advancing our fundamental understanding of the universe.

References

  1. ^ Explainer: what is a neutron star? (theconversation.com)
  2. ^ Neutron star Interior Composition ExploreR (NICER) mission (science.nasa.gov)
  3. ^ collide (theconversation.com)
  4. ^ A pulsar (theconversation.com)
  5. ^ Murriyang (www.csiro.au)
  6. ^ Parkes Pulsar Timing Array (www.atnf.csiro.au)
  7. ^ Using a detector the size of a galaxy, astronomers find strongest evidence yet for gravitational waves from supermassive black hole pairs (theconversation.com)
  8. ^ We calculated (arxiv.org)
  9. ^ the neutron star’s radius is 11.4 kilometres (arxiv.org)
  10. ^ most precise anchor point (arxiv.org)
  11. ^ escaped their normal homes (www.nature.com)
  12. ^ hyperons (royalsocietypublishing.org)
  13. ^ observations (theconversation.com)
  14. ^ most of the Apollo 11 moonwalk (theconversation.com)

Read more https://theconversation.com/what-happens-when-matter-is-squashed-to-the-brink-of-collapse-we-weighed-a-neutron-star-to-help-nasa-find-out-229813

Times Magazine

Headless CMS in Digital Twins and 3D Product Experiences

Image by freepik As the metaverse becomes more advanced and accessible, it's clear that multiple sectors will use digital twins and 3D product experiences to visualize, connect, and streamline efforts better. A digital twin is a virtual replica of ...

The Decline of Hyper-Casual: How Mid-Core Mobile Games Took Over in 2025

In recent years, the mobile gaming landscape has undergone a significant transformation, with mid-core mobile games emerging as the dominant force in app stores by 2025. This shift is underpinned by changing user habits and evolving monetization tr...

Understanding ITIL 4 and PRINCE2 Project Management Synergy

Key Highlights ITIL 4 focuses on IT service management, emphasising continual improvement and value creation through modern digital transformation approaches. PRINCE2 project management supports systematic planning and execution of projects wit...

What AI Adoption Means for the Future of Workplace Risk Management

Image by freepik As industrial operations become more complex and fast-paced, the risks faced by workers and employers alike continue to grow. Traditional safety models—reliant on manual oversight, reactive investigations, and standardised checklist...

From Beach Bops to Alpine Anthems: Your Sonos Survival Guide for a Long Weekend Escape

Alright, fellow adventurers and relaxation enthusiasts! So, you've packed your bags, charged your devices, and mentally prepared for that glorious King's Birthday long weekend. But hold on, are you really ready? Because a true long weekend warrior kn...

Effective Commercial Pest Control Solutions for a Safer Workplace

Keeping a workplace clean, safe, and free from pests is essential for maintaining productivity, protecting employee health, and upholding a company's reputation. Pests pose health risks, can cause structural damage, and can lead to serious legal an...

The Times Features

Prefab’s Second Life: Why Australia’s Backyard Boom Needs a Circular Makeover

The humble granny flat is being reimagined not just as a fix for housing shortages, but as a cornerstone of circular, factory-built architecture. But are our systems ready to s...

Melbourne’s Burglary Boom: Break-Ins Surge Nearly 25%

Victorian homeowners are being warned to act now, as rising break-ins and falling arrest rates paint a worrying picture for suburban safety. Melbourne residents are facing an ...

Exploring the Curriculum at a Modern Junior School in Melbourne

Key Highlights The curriculum at junior schools emphasises whole-person development, catering to children’s physical, emotional, and intellectual needs. It ensures early year...

Distressed by all the bad news? Here’s how to stay informed but still look after yourself

If you’re feeling like the news is particularly bad at the moment, you’re not alone. But many of us can’t look away – and don’t want to. Engaging with news can help us make ...

The Role of Your GP in Creating a Chronic Disease Management Plan That Works

Living with a long-term condition, whether that is diabetes, asthma, arthritis or heart disease, means making hundreds of small decisions every day. You plan your diet against m...

Troubleshooting Flickering Lights: A Comprehensive Guide for Homeowners

Image by rawpixel.com on Freepik Effectively addressing flickering lights in your home is more than just a matter of convenience; it's a pivotal aspect of both home safety and en...