Stockholm university

IceCube neutrinos provide new view of a nearby galaxy

For the first time, an international team of scientists has found evidence of high-energy neutrino emission from a nearby galaxy. The galaxy, NGC 1068 (also known as Messier 77) is an active galaxy in the constellation Cetus and one of the most familiar and well-studied active galaxies. The results are published in Science.

IceCube neutrino detector at the South Pole. Photo: Martin Wolf, IceCube/NSF

The neutrinos were detected using the IceCube Neutrino Observatory, a massive neutrino telescope encompassing 1 billion tons of instrumented ice at depths of 1.5 to 2.5 kilometers below Antarctica's surface at the South Pole. Members of the IceCube Collaboration at Stockholm University and Uppsala University have been involved in the analysis of the data acquired during ten years of observations and in the interpretation of the results.

“This represents the slow and steady accumulation of a neutrino signal, until it has become the single brightest spot in the neutrino sky,” says Chad Finley, associate professor at Stockholm University and previously the coordinator for neutrino point-source searches in IceCube.  

In 2018, IceCube together with gamma-ray observatories identified the distant blazar galaxy TXS 0506+056 as a neutrino source after the detection of a very high-energy neutrino in coincidence with gamma-rays during the same period of time.  In contrast, the emission attributed to NGC 1068 consists of approximately 80 lower-energy neutrino events recorded by IceCube since it became fully operational in 2011.


Black hole millions of times more massive than our Sun

Chad Finley vid Sydpolen
Chad Finley at the South Pole. Poto: private

First spotted in 1780, NGC 1068 is located 47 million light-years away from us, and can be seen with large binoculars. Like our home galaxy the Milky Way, NGC 1068 is a barred spiral galaxy, with loosely wound arms and a relatively small central bulge. However, unlike the Milky Way, NGC 1068 is also an “active galaxy” where most radiation is not emitted by stars but by material falling into the black hole at its center. This black hole is millions of times more massive than our Sun and even more massive than the inactive black hole at the center of our galaxy.

“What is surprising about seeing NGC 1068 with neutrinos is that it has not been detectable with gamma rays in the same energy range, 1 to 10 tera-electron volts,” says Chad Finley.  Both neutrinos and gamma-rays are generally expected to be produced in the same processes, in cosmic ray interactions. “The lack of gamma rays suggests that the neutrinos are emerging from a dense region where the gamma rays get absorbed.”


Will improve understanding of environments around supermassive black hole

When a neutrino interacts with molecules in the clear Antarctic ice, it produces secondary particles that leave a trace of blue light as they travel through the IceCube detector.
When a neutrino interacts with molecules in the clear Antarctic ice, it produces secondary particles that leave a trace of blue light as they travel through the IceCube detector. Photo: Nicolle R. Fuller, IceCube/NSF

Unlike photons, neutrinos interact extremely weakly with matter, and can thus escape from extremely dense environments in the universe. NGC 1068 is not only an active galaxy, but is classified as a Seyfert II-type active galaxy, meaning that it is seen from Earth at an angle such that the central region where the black hole is located is hidden within a torus of dust that encircles it.

"Recent models of the black hole environments in these objects suggest that gas, dust, and radiation should block the gamma rays that would otherwise accompany the neutrinos," says Hans Niederhausen, a postdoctoral associate at Michigan State University and one of the main analyzers of the paper. "This neutrino detection from the core of NGC 1068 will improve our understanding of the environments around supermassive black holes."


Stockholm University and Uppsala University – two of the founding members for IceCube

The IceCube Collaboration presently consists of about 350 scientists at 58 institutions around the world.  IceCube counts Stockholm University and Uppsala University among its founding member institutions.

“These results are very encouraging for our planned improvements of IceCube,” says Professor Klas Hultqvist at Stockholm University, who was already engaged in the effort to develop neutrino astronomy during the predecessor experiment AMANDA and who helped to build IceCube. “It is deeply rewarding to see our efforts bear fruit.”

The IceCube Neutrino Observatory is supported by the US National Science Foundation, as well as the Swedish Research Council and national funding agencies of other member countries.


Facts on IceCube

The IceCube Neutrino Observatory is funded and operated primarily through an award from the National Science Foundation to the University of Wisconsin–Madison. The IceCube Collaboration, with over 350 scientists in 58 institutions from around the world, runs an extensive scientific program that has established the foundations of neutrino astronomy.

IceCube’s research efforts, including critical contributions to the detector operation, are funded by agencies in Australia, Belgium, Canada, Denmark, Germany, Italy, Japan, New Zealand, Republic of Korea, Sweden, Switzerland, Taiwan, the United Kingdom, and the United States. The IceCube EPSCoR Initiative (IEI) receives additional support through NSF-EPSCoR-2019597. IceCube construction was also funded with significant contributions from the National Fund for Scientific Research (FNRS & FWO) in Belgium; the Federal Ministry of Education and Research (BMBF) and the German Research Foundation (DFG) in Germany; the Knut and Alice Wallenberg Foundation, the Swedish Polar Research Secretariat, and the Swedish Research Council in Sweden; and the University of Wisconsin–Madison Research Fund in the U.S.

Artricle in Science: Evidence for neutrino emission from the nearby active galaxy NGC 1068, The IceCube Collaboration: R. Abbasi et al. DOI:10.1126/science.abg3395