{"id":384506,"date":"2026-03-11T01:40:14","date_gmt":"2026-03-10T15:40:14","guid":{"rendered":"https:\/\/www.nasa.gov\/?p=971920"},"modified":"2026-03-11T01:40:14","modified_gmt":"2026-03-10T15:40:14","slug":"nasa-discovers-crash-of-extreme-stars-in-unexpected-site","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=384506","title":{"rendered":"NASA Discovers Crash of Extreme Stars in Unexpected Site"},"content":{"rendered":"
\n
\n
\n
\"These<\/a><\/figure>
\n
X-ray: NASA\/CXC\/Penn State Univ.\/S. Dichiara; IR: NASA\/ESA\/STScI; Illustration: ERC BHianca 2026 \/ Fortuna and Dichiara, CC BY-NC-SA 4.0; Image Processing: NASA\/CXC\/SAO\/P. Edmonds<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

A fleet of NASA missions has likely uncovered a collision between two ultradense stars in a tiny galaxy buried in a huge stream of gas. Astronomers have never seen this type of explosive event in an environment like this before \u2014 and it may help solve two outstanding cosmic mysteries. A paper describing these results published today in The Astrophysical Journal Letters<\/a>.<\/p>\n

Neutron stars are the cores left behind after a star much heavier than the Sun runs out of fuel, collapses on itself, and then explodes. They are small (only a dozen or so miles across) but slightly more massive than the Sun, making them amazingly dense. Astronomers consider them to be some of the most extreme objects in the universe.<\/p>\n

In recent years, astronomers have collected data on collisions, or mergers, of two neutron stars inside of moderately sized or large galaxies. This latest discovery, however, shows that a neutron star collision may take place inside a tiny galaxy.<\/p>\n

\u201cFinding a neutron star collision where we did is game changing,\u201d said Simone Dichiara of Penn State University, who led the study. \u201cIt may be the key to unlocking not one, but two important questions in astrophysics.\u201d<\/p>\n

The first puzzle this unprecedented location for a neutron star collision may explain may explain is the fact that gamma-ray bursts (GRBs), which can be produced by the collapse of two neutron stars, sometimes do not appear within the core of a galaxy, or any galaxy at all.The other question this result could address is how elements like gold and platinum have been found in stars located at large distances from the centers of galaxies.<\/p>\n

This neutron star collision is unexpectedly located in a tiny galaxy, about 4.7 billion light-years away, embedded within a stream of gas that stretches some 600,000 light-years long. (For context, our Milky Way galaxy is about 100,000 light-years across.) This stream was likely created when a group of galaxies collided hundreds of millions of years ago, stripping gas and dust from the galaxies and leaving it in intergalactic space.<\/p>\n

\u201cWe found a collision within a collision,\u201d said co-author Eleonora Troja of the University of Rome in Italy. \u201cThe galaxy collision triggered a wave of star formation that, over hundreds of millions of years, led to the birth and eventual collision of these neutron stars.\u201d<\/p>\n

To discover the event dubbed GRB 230906A, which occurred on 2023 September 6th, astronomers needed several NASA telescopes including the Chandra X-ray Observatory, Fermi Gamma-ray Space Telescope, Neil Gehrels Swift Observatory, and Hubble Space Telescope.<\/p>\n

Fermi discovered the neutron star collision by picking up the distinctive signal of a gamma-ray burst, or GRB, explosion. After using the InterPlanetary Network to derive a preliminary location for the Fermi source, astronomers then needed the sharp vision of Chandra, Swift, and Hubble to more precisely pinpoint the location of the object. NASA\u2019s missions are part of a growing, worldwide network that watches for these changes, to solve mysteries of how the universe works.<\/p>\n

\u201cChandra\u2019s pinpoint X-ray localization made this study possible,\u201d said co-author Brendan O\u2019Connor, a McWilliams Postdoctoral Fellow at Carnegie Mellon University. \u201cWithout it, we couldn\u2019t have tied the burst to any specific source. And once Chandra told us exactly where to look, Hubble\u2019s extraordinary sensitivity revealed the tiny, extremely faint galaxy at that position. We were only able to make this discovery after we put all the pieces together.\u201d<\/p>\n

This finding may explain why some GRBs do not appear to have host galaxies. This result implies that some host galaxies are too small and faint to be seen in most optical light images from ground-based observatories.<\/p>\n

The unusual location of GRB 230906A may also help explain how astronomers have spotted elements like gold and platinum in stars at relatively large distances from galaxies. Such stars are generally expected to be older and to have formed from gas that had less time to be enriched in heavy elements from supernova explosions.<\/p>\n

Through a chain of nuclear reactions, a collision between two neutron stars can produce heavy elements like gold and platinum, which astronomers witnessed in a well-documented collision seen in 2017 . Events like GRB 230906A could generate elements like these and spread them throughout the outskirts of galaxies, eventually appearing in future generations of stars.<\/p>\n

An alternative explanation for the explosion is that it is located in a much more distant galaxy that is behind the galaxy group. The team considers this to be a less likely explanation than the tiny galaxy idea.<\/p>\n

NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.<\/p>\n

To learn more about Chandra, visit:<\/p>\n

https:\/\/science.nasa.gov\/chandra<\/a><\/p>\n

Read more from NASA\u2019s Chandra X-ray Observatory<\/a><\/p>\n

Learn more about the Chandra X-ray Observatory and its mission here:<\/p>\n

https:\/\/www.nasa.gov\/chandra<\/a><\/p>\n

https:\/\/chandra.si.edu<\/a><\/p>\n

Visual Description<\/h2>\n

This release features two artist’s concepts and a composite image depicting two cosmic collisions that began hundreds of millions of years ago.<\/p>\n

At the center of the large artist’s concept is a brilliant glowing ball with a nearly white core, and golden orange outer layers. This brilliant ball represents the brightest galaxy in a collision between two groups of galaxies, which began hundreds of millions of years ago. Gas and dust from that collision were tossed into intergalactic space in long tidal streams. In the illustration, the tidal streams resemble swooping blue streaks shooting off the brilliant ball. Near the end of each swooping tidal stream is a glowing orange streak, or ellipse. These glowing shapes are smaller individual galaxies, some of which are revealed to have spiraling arms when examined closely.<\/p>\n

One of the tidal streams shoots toward our upper left, then begins to hook back down, passing two glowing orange galaxies along its path. Near the end of this tidal stream is a tiny galaxy and an X-ray source presented in the middle of a close-up insert. In the center of the composite insert, Hubble observations in orange reveal the tiny, faint galaxy buried in the tidal stream. A pool of neon blue haze shows X-rays detected by Chandra from the collision of two ultra-dense neutron stars.<\/p>\n

Astronomers believe that the tiny galaxy was born from gas and dust along the 600,000 light-year-long tidal stream, created by the initial collision of the galaxy groups. Over hundreds of millions of years, that material contributed to the birth of many stars within the tiny galaxy. Two of those stars collapsed into neutron stars, and ultimately collided, producing important elements like gold and platinum, and gravitational waves that rippled across space.<\/p>\n

The artist’s concept in the other insert shows a close-up view from the side of what the aftermath of a neutron star collision might look like. A burst of gamma rays was originally detected by viewing it down the barrel of the jet, which triggered follow-up X-ray observations with Chandra and other X-ray telescopes.<\/p>\n

News Media Contact<\/h2>\n

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu<\/a><\/p>\n

Joel Wallace
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
joel.w.wallace@nasa.gov<\/a><\/p>\n

\n
\n
\n
\n
\n
\n

Share<\/h2>\n<\/p><\/div>\n
\n