Colliding stars spill radioactive molecules into space

When two Sun-like stars collide, the result can be a spectacular explosion and the formation of an entirely new star. One such event was seen from Earth in 1670. It appeared to observers as a bright, red "new star."

Though initially visible with the naked eye, this burst of cosmic light quickly faded and now requires powerful telescopes to see the remains of this merger: a dim central star surrounded by a halo of glowing material flowing away from it.

Approximately 348 years after this event, an international team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) and the NOEMA (Northern Extended Millimeter Array) radio telescopes studied the remains of this explosive stellar merger - known as CK Vulpeculae (CK Vul) - and discovered the clear and convincing signature of a radioactive version of aluminum (26Al, an atom with 13 protons and 13 neutron) bound with atoms of fluorine, forming 26-aluminum monofluoride (26AlF).

This is the first molecule bearing an unstable radioisotope definitively detected outside of our solar system. Unstable isotopes have an excess of nuclear energy and eventually decay into a stable, less-radioactive form. In this case, the 26-aluminum (26Al) decays to 26-magnesium (26Mg).

"The first solid detection of this kind of radioactive molecule is an important milestone in our exploration of the cool molecular universe," said Tomasz Kaminski, an astronomer with the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., and lead author on a paper appearing in Nature Astronomy.

The researchers detected the unique spectral signature of these molecules in the debris surrounding CK Vul, which is approximately 2,000 light-years from Earth. As these molecules spin and tumble through space, they emit a distinctive fingerprint of millimeter-wavelength light, a process known as "rotational transition." Astronomers consider this the "gold standard" for molecular detections.

These characteristic molecular fingerprints are usually taken from laboratory experiments and then used to identify molecules in space. In the case of 26AlF, this method is not applicable because 26-aluminum is not present on Earth. Laboratory astrophysicists from the University of Kassel/Germany therefore used the fingerprint data of stable and abundant 27AlF molecules to derive accurate data for the rare 26AlF molecule.

"This method of extrapolation is based on the so-called Dunham approach," explained Alexander Breier from the Kassel team.

"It allows researchers to precisely calculate the rotational transitions of 26AlF with an accuracy far beyond the needs of astronomical observers."

The observation of this particular isotopologue provides fresh insights into the merger process that created CK Vul. It also demonstrates that the deep, dense inner layers of a star, where heavy elements and radioactive isotopes are forged, can be churned up and cast into space by stellar collisions.

"We are observing the guts of a star torn apart three centuries ago by a collision," observed Kaminski.

"How cool is that?"

The astronomers also determined that the two stars that merged were relatively low-mass, with one being a red giant star with a mass somewhere between 0.8 and 2.5 times that of our Sun.

"This first direct observation of this isotope in a stellar-like object is also important in the broader context of galactic chemical evolution," noted Kaminski.

"This is the first time an active producer of the radioactive nuclide 26Al has been directly observationally identified."

It has been known for decades that there is about three entire Suns' worth of 26Al spread across the Milky Way. But these observations, made at gamma-ray wavelengths, could only identify that the signal was there; they couldn't pinpoint individual sources and it was unclear how the isotopes got there.

With current estimates on the mass of 26Al in CK Vul (about a quarter the mass of Pluto) and the rare occurrence of mergers such as this, it seems rather unlikely that mergers are solely responsible for this galactic radioactive material, the astronomers conclude.

However, ALMA and NOEMA can only detect the amount of 26Al bound with fluorine. The actual mass of 26Al in CK Vul (in atomic form) may be much greater. It is also possible that other merger remnants may have far greater amounts. Astronomers may also have underestimated the current merger rates in the Milky Way.

"So this is not a closed issue and the role of mergers may be non-negligible," speculated Kaminski.

Research Report: "Astronomical Detection of a Radioactive Molecule 26AlF in a Remnant of an Ancient Explosion," T. Kaminski et al., 2018 July 30, Nature Astronomy

Related Links
National Radio Astronomy Observatory
Stellar Chemistry, The Universe And All Within It

Tweet

Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Monthly Supporter
$5+ Billed Monthly

paypal only

SpaceDaily Contributor
$5 Billed Once

credit card or paypal

Young galaxy's halo offers clues to its growth and evolution
Maunakea HI (SPX) Jul 25, 2018
A team of astronomers has discovered a new way to unlock the mysteries of how the first galaxies formed and evolved. In a study published in Astrophysical Journal Letters, lead author Dawn Erb of the University of Wisconsin-Milwaukee and her team - for the very first time - used new capabilities at W. M. Keck Observatory on Maunakea, Hawaii to examine Q2343-BX418, a small, young galaxy located about 10 billion light years away from Earth. This distant galaxy is an analog for younger galaxies ... read more