25-million-year-old galactic dust provides insight into supernovae

Australian National University Press Release

During the 226 million years it takes for the Sun to make one orbit of the Milky Way, small amounts of heavy elements — including plutoniun-244 — from supernovae explosions fall on the Earth accumulating in deep ocean sediments. This is a false colour image of supernova remnant Cassiopeia A using observations from both the Hubble and Spitzer telescopes as well as the Chandra X-ray Observatory (cropped). Image credit: NASA/JPL-Caltech
During the 226 million years it takes for the Sun to make one orbit of the Milky Way, measurable amounts of heavy elements from supernovae explosions — including plutoniun-244 — fall on the Earth, accumulating in deep ocean sediments. This is a false colour image of supernova remnant Cassiopeia A using observations from both the Hubble and Spitzer telescopes as well as the Chandra X-ray Observatory (cropped). Image credit: NASA/JPL-Caltech
Scientists plumbing the depths of the ocean have made a surprise finding that could change the way we understand supernovae, exploding stars way beyond our Solar System. They have analysed extraterrestrial dust thought to be from supernovae, that has settled on ocean floors to determine the amount of heavy elements created by the massive explosions.

“Small amounts of debris from these distant explosions fall on the Earth as it travels through the galaxy,” said lead researcher Dr Anton Wallner, from the Research School of Physics and Engineering. “We’ve analysed galactic dust from the last 25 million years that has settled on the ocean and found there is much less of the heavy elements such as plutonium and uranium than we expected.”

The findings are at odds with current theories of supernovae, in which some of the materials essential for human life, such as iron, potassium and iodine are created and distributed throughout space. Supernovae also create lead, silver and gold, and heavier radioactive elements such as uranium and plutonium.

Dr Anton Wallner in the Nuclear Physics Department at Australian National University. Image credit: Stuart Hay, ANU
Dr Anton Wallner in the Nuclear Physics Department at Australian National University. Image credit: Stuart Hay, ANU
Dr Wallner’s team studied plutonium-244 which serves as a radioactive clock by the nature of its radioactive decay, with a half-life of 81 million years. “Any plutonium-244 that existed when the Earth formed from intergalactic gas and dust over four billion years ago has long since decayed,” Dr Wallner said. “So any plutonium-244 that we find on Earth must have been created in explosive events that have occurred more recently, in the last few hundred million years.”

The team analysed a 10 centimetre-thick sample of the Earth’s crust, representing 25 million years of accretion, as well as deep-sea sediments collected from a very stable area at the bottom of the Pacific Ocean.

“We found 100 times less plutonium-244 than we expected,” Dr Wallner said. “It seems that these heaviest elements may not be formed in standard supernovae after all. It may require rarer and more explosive events such as the merging of two neutron stars to make them.”

The fact that these heavy elements like plutonium were present, and uranium and thorium are still present on Earth suggests that such an explosive event must have happened close to the Earth around the time it formed, said Dr Wallner. “Radioactive elements in our planet such as uranium and thorium provide much of the heat that drives continental movement, perhaps other planets don’t have the same heat engine inside them,” he said.