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Date(s) - 05/03/2021
11:30 am - 1:00 pm


The microphone on stage against a background of auditorium


Astrophysicists in Germany and North America have published plans to build the world’s larg­est neutrino telescope on the sea floor off the coast of Canada. The Pacific Ocean Neutrino Experiment (P-ONE) is designed to snare very-high-energy neutrinos generated by extreme events from beyond our galaxy. Neutrino telescopes observe the Cerenkov radiation that is emitted when neutrinos passing through the Earth interact very occasionally with atomic nuclei resulting in the production of fast-moving secondary particles. Being uncharged and exceptionally inert, neutrinos can penetrate gas and dust as they travel through the universe, allowing astronomers in principle to identify the exceptionally energetic phenomena that generate them. Photons from such events, in contrast, are absorbed on their journey. We are now on the verge of opening up neutrino astronomy

The world’s largest neutrino tele­scope, known as IceCube, consists of dozens of strings of photomultiplier tubes suspended in holes drilled deep into the ice at the South Pole. Covering a volume of 1 km3, Ice­Cube made history in 2013 when it reported intercepting the first extra­galactic neutrinos. Four years later it then recorded an event that could be tied to a very distant, bright galactic nucleus known as a blazar, thanks to concurrent gamma-ray observations. According to P-ONE head, Elisa Resconi at the University of Munich, IceCube’s 2017 result strictly speak­ing only constitutes “evidence” for the blazar source. To really claim a discovery and pinpoint the origin of other cosmic neutrinos, she argues, requires the construction of addi­tional neutrino observatories as well as the extension of IceCube. “We are now on the verge of opening up neutrino astronomy,” she says, “but if we base this process on just one telescope it could take a really long time, perhaps decades.”

P-ONE will consist of seven groups of 10 detector strings creat­ing an instrument volume of about 3 km3. Being larger than IceCube, it will detect rarer, higher-energy neutrinos, and will be most sensi­tive at a few tens rather than a hand­ful of teraelectronvolts. It will also observe a different part of the sky, mainly capturing neutrinos from the southern hemisphere rather than the north. But there will be some over­lap between the two, says Resconi, potentially allowing independent observations of the same event.

The new facility will be located at a depth of about 2.6 km in the Cas­cadia Basin, some 200 km from the coast of British Columbia. As such, it will take advantage of pre-existing infrastructure – an 800 km-long loop of fibre-optic cable operated by the University of Victoria’s Ocean Net­works Canada that supplies power and ferries data to and from existing sea-floor instruments.  Having already confirmed that this site has the necessary optical prop­erties by sending down two initial strings of light emitters and sensors in 2018, the P-ONE collaboration are now planning to deploy a steel cable with addi­tional detectors to investigate the site – including spectrometers, lidars and a muon detector. The plan then, says Resconi, is to install the first part of the observatory – a ring containing seven 1 km-long strings – around the end of 2023. And if that succeeds, the researchers will then apply for the bulk of the $50–100m needed to complete the project, with personnel costs adding roughly $100m more. Resconi hopes that the full obser­vatory will be installed and taking data by the end of the decade. But she describes this timeline as “very ambitious”. In addition to delays caused by the ongoing COVID- 19 pandemic, she says it will be a challenge to ensure that the detec­tors work as planned – given the huge pressures and the presence of salt and sea creatures, which together make the seabed such a harsh environment.


Dr. Kate Moran

President & CEO, Ocean Networks Canada, Victoria




Dr Kathryn (Kate) Moran joined the University of Victoria in September 2011 as a Professor in the Faculty of Earth and Ocean Sciences and as Director of NEPTUNE Canada. In July 2012, she was promoted to the position of President & CEO, Ocean Networks Canada. Her previous appointment was Professor at the University of Rhode Island with a joint appointment in the Graduate School of Oceanography and the Department of Ocean Engineering. She also served as the Graduate School of Oceanography’s Associate Dean, Research and Administration. From 2009 to 2011, Moran was seconded to the White House Office of Science and Technology Policy where she served as an Assistant Director and focused on Arctic, polar, ocean, the Deepwater Horizon oil spill, and climate policy issues. Moran holds degrees from the University of Pittsburgh, the University of Rhode Island and Dalhousie University. Her research focuses on marine geotechnics and its application to the study of paleoceanography, tectonics and seafloor stability. She has authored more than 45 publications. Dr. Moran is a Fellow of the Canadian Society of Senior Engineers, FCSSE, among other honours.


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