Ocean sediments reveal nearby supernovae mystery

A mystery surrounding the space around our solar system is unfolding thanks to evidence of  supernovae found in deep-sea sediments.

Professor Anton Wallner, a nuclear physicist at ANU Research School of Physics, led the study which shows the Earth has been travelling for the last 33,000 years through a cloud of faintly radioactive dust.

“These clouds could be remnants of previous supernova explosions, a powerful and super bright explosion of a star” Professor Wallner said.

The findings are published in the journal PNAS.

Professor Wallner conducted the research at the ANU Heavy Ion Accelerator Facility (HIAF). He also holds joint positions at the Helmholtz-Zentrum Dresden-Rossendorf (HZDR) and Technical University Dresden (TUD) in Germany.

The team included researchers from ANU, the Australian Nuclear Science and Technology Organization, HZDR, the University of Vienna and the TU Berlin . They searched through several deep-sea sediments from two different locations that date back 33,000 years using the extreme sensitivity of HIAF’s mass spectrometer. They found clear traces of the isotope iron-60, which is formed when stars die in supernova explosions.

Iron-60 is radioactive and completely decays away within 15 million years, which means any iron-60 found on the earth must have been formed much later than the rest of the 4.6-billion-year old earth and arrived here from nearby supernovae before settling on the ocean floor.

Professor Wallner previously found traces of iron-60 at about 2.6 million years ago, and possibly another at around 6 million years ago, suggesting earth had travelled through fallout clouds from nearby supernovae.

For the last few thousand years the solar system has been moving through a denser cloud of gas and dust, known as the local interstellar cloud, (LIC), whose origins are unclear. If this cloud had originated during the past few million years from a supernova, it would contain iron-60, and so the team decided to search more recent sediment to find out.

Sure enough, there was iron-60 in the sediment at extremely low levels - equating to radioactivity levels in space far below the Earth’s natural background levels - and the distribution of the iron-60 matched earth’s recent travel through the local interstellar cloud. But the iron-60 extended further back and was spread throughout the entire 33,000 year measurement period.

The lack of correlation with the solar system’s time in the current local interstellar cloud seems to pose more questions than it answers. Firstly, if the cloud was not formed by a supernova, where did it come from? And secondly, why is there iron-60 so evenly spread throughout space?

“There are recent papers that suggest iron-60 trapped in dust particles might bounce around in the interstellar medium,” said Professor Wallner.

“So the iron-60 could originate from even older supernovae explosions, and what we measure is some kind of echo.

“More data are required to resolve these details,” he said.

» read more

Contact

Dr Anton Wallner
E: anton.wallner@anu.edu.au
T: (02)61252074

Updated:  15 January 2019/ Responsible Officer:  Director, RSPhys/ Page Contact:  Physics Webmaster