Anomaly in the deep sea

Beryllium-10, a rare radioactive isotope produced by cosmic rays in the atmosphere, provides valuable insights into the Earth's geological history. A research team from the Helmholtz-Zentrum Dresden-Rossendorf (HZDR), in collaboration with the TUD Dresden University of Technology and the Australian National University (ANU), has discovered an unexpected accumulation of this isotope in samples taken from the Pacific seabed. Such an anomaly may be attributed to shifts in ocean currents or astrophysical events that occurred approximately 10 million years ago. The findings hold the potential to serve as a global time marker, representing a promising advancement in the dating of geological archives spanning millions of years. The team presents its results in the scientific journal Nature Communications (DOI: 10.1038/s41467-024-55662-4).

Radionuclides are types of atomic nuclei (isotopes) that decay into other elements over time. They are used to date archaeological and geological samples, with radiocarbon dating being one of the most well-known methods. In principle, radiocarbon dating is based on the fact that living organisms continuously absorb the radioactive isotope carbon-14 (¹⁴C) during their lifetime. Once an organism dies, the absorption ceases, and the ¹⁴C content starts to decrease through radioactive decay with a half-life of approximately 5,700 years. By comparing the ratio of unstable ¹⁴C to stable carbon-12 (¹²C), researchers can determine the date of the organism's death.

Archaeological finds, such as bones or remnants of wood, can be dated quite accurately in this way. “However, the radiocarbon method is limited to dating samples no more than 50,000 years old,” explains HZDR physicist Dr. Dominik Koll. “To date older samples, we need to use other isotopes, such as cosmogenic beryllium-10 (¹⁰Be).” This isotope is created when cosmic rays interact with oxygen and nitrogen in the upper atmosphere. It reaches the Earth through precipitation and can accumulate on the seabed. With a half-life of 1.4 million years, ¹⁰Be decays into boron, allowing geological dating that can extend back over 10 million years.

Conspicuous accumulation of beryllium

Some time ago, Koll's research group examined unique geological samples retrieved from the Pacific Ocean at a depth of several kilometers. The samples consisted of ferromanganese crusts, primarily composed of iron and manganese, which had formed slowly but steadily over millions of years. To date the samples, the team analyzed the ¹⁰Be content using a highly sensitive method – Accelerator Mass Spectrometry (AMS) at HZDR. In this process, the sample is chemically purified before undergoing analysis for trace isotopes. Individual atoms from the sample are accelerated by high voltage, deflected by magnets, and then registered by specialized detectors. This method allows for the precise identification of ¹⁰Be, distinguishing it from other beryllium isotopes as well as molecules and isotopes with the same mass, such as boron-10.

When the research group evaluated the collected data, they were in for a surprise. “At around 10 million years, we found almost twice as much ¹⁰Be as we had anticipated,” reports Koll. “We had stumbled upon a previously undiscovered anomaly.” To eliminate any possibility of contamination, the experts analyzed additional samples from the Pacific, which also exhibited the same anomaly. This consistency allows the team to conclude that it is indeed a real phenomenon.

Ocean currents, stellar explosion or interstellar collision?

But how did such a striking increase in concentration come about 10 million years ago? Koll, who completed his doctorate at the TU Dresden and the ANU, proposes two possible explanations. One is related to the ocean circulation near Antarctica, which is thought to have changed drastically 10 to 12 million years ago. “This could have caused ¹⁰Be to be unevenly distributed across the Earth for a period of time due to the altered ocean currents,” explains the physicist. ”As a result, ¹⁰Be could have become particularly concentrated in the Pacific Ocean.”

The second hypothesis is astrophysical in nature. It suggests that the after-effects of a near-Earth supernova could have caused cosmic radiation to become temporarily more intense 10 million years ago. Alternatively, the Earth might have temporarily lost its protective solar shield – the heliosphere – due to a collision with a dense interstellar cloud, making it more vulnerable to cosmic radiation. ”Only new measurements can indicate whether the beryllium anomaly was caused by changes in ocean currents or has astrophysical reasons,” says Koll. ”That is why we plan to analyze more samples in the future and hope that other research groups will do the same.” If the anomaly were found all over the globe, the astrophysics hypothesis would be supported. On the other hand, if it were detected only in specific regions, the explanation involving altered ocean currents would be considered more plausible.

The anomaly could be extremely useful for geological beryllium dating. When comparing different archives for dating, one fundamental problem arises. Common time markers must be identified in all data sets so they can be properly synchronized with each other. Dominik Koll explains, “For periods spanning millions of years, such cosmogenic time markers do not yet exist. However, this beryllium anomaly has the potential to serve as such a marker.”

Publication:
D. Koll, J. Lachner, S. Beutner, S. Fichter, S. Merchel, G. Rugel, Z. Slavkovská, C. Vivo-Vilches, S. Winkler, A. Wallner: A cosmogenic 10Be anomaly during the late Miocene as independent time marker for marine archives, in Nature Communications, 2025 (DOI: 10.1038/s41467-024-55662-4)

Further information:
Dr. Dominik Koll | Institute of Ion Beam Physics and Materials Research at HZDR
Phone: +49 351 260 3804 | Email: d.koll@hzdr.de

Media contact:
Simon Schmitt | Head
Communications and Media Relations at HZDR
Phone: +49 351 260 3400 | Mobile: +49 175 874 2865 | Email: s.schmitt@hzdr.de

The Helmholtz-Zentrum Dresden-Rossendorf (HZDR) performs – as an independent German research center – research in the fields of energy, health, and matter. We focus on answering the following questions:

• How can energy and resources be utilized in an efficient, safe, and sustainable way?
• How can malignant tumors be more precisely visualized, characterized, and more effectively treated?
• How do matter and materials behave under the influence of strong fields and in smallest dimensions?

To help answer these research questions, HZDR operates large-scale facilities, which are also used by visiting researchers: the Ion Beam Center, the Dresden High Magnetic Field Laboratory and the ELBE Center for High-Power Radiation Sources.
HZDR is a member of the Helmholtz Association and has six sites (Dresden, Freiberg, Görlitz, Grenoble, Leipzig, Schenefeld near Hamburg) with almost 1,500 members of staff, of whom about 680 are scientists, including 200 Ph.D. candidates.