Synopsis

# Seeking Stardust in the Snow

Physics 12, s93
Iron-60 found in fresh Antarctic snow was forged in nearby supernovae and could help deduce the structure and origin of interstellar dust clouds.

Sometime in the last 20 million years, one or more stars in the solar neighborhood went supernova, producing clouds of gas and dust enriched with radioisotopes. As the Solar System passes through such a cloud, some of this dust falls onto Earth’s surface, where, under certain conditions, detectable concentrations can accumulate. This is the case far inland in Antarctica, where Dominik Koll, of the Technical University of Munich, and colleagues discovered evidence of interstellar dust in the form of a rare isotope, iron-60 ( ${}^{60}$Fe). The finding could help pin down the source of the dust more precisely and reveal the history of the Solar System’s interactions with its interstellar environment.

Koll and colleagues collected 500 kg of snow that was less than 20 years old, melted it, and filtered out the solids. The researchers incinerated the residues and used a mass spectrometer to measure the presence of ${}^{60}$Fe and manganese-53 ( ${}^{53}$Mn). The latter isotope is produced with ${}^{60}$Fe when cosmic rays strike interplanetary dust. But the researchers found much more ${}^{60}$Fe compared to ${}^{53}$Mn than would be expected from this “local” source. The team also calculated the possibility that ${}^{60}$Fe from nuclear weapons and power plants had contaminated the snow, but they determined that the presence of artificially produced isotopes should be negligible. The most likely source, they say, is interstellar dust, which is enriched by ${}^{60}$Fe from supernovae.

The calculated ${}^{60}$Fe influx matches that deduced for other interstellar-dust deposits found in ocean sediments and lunar soil. Testing for a wider range of radioisotopes in older ice cores could tell researchers when and where the supernovae occurred and when the Solar System entered the local interstellar cloud.

This research is published in Physical Review Letters.

–Marric Stephens

Marric Stephens is a freelance science writer based in Bristol, UK.

## Related Articles

Superconductivity

### The Tiniest Superfluid Circuit in Nature

A new analysis of heavy-ion collision experiments uncovers evidence that two colliding nuclei behave like a Josephson junction—a device in which Cooper pairs tunnel through a barrier between two superfluids. Read More »

Nuclear Physics

### Distorting Nuclear Mirror

Two “mirror” nuclei, in which the numbers of neutrons and protons are interchanged, have markedly different shapes—a finding that defies current nuclear theories. Read More »

Geophysics

### Iceberg Shape Affects Melting

Experiments with large ice cubes show that the melting rate depends on the shape, an effect that climate modelers may need to consider. Read More »