Title(s): (1) Recent near-Earth supernovae probed by global deposition of interstellar radioactive iron-60 / (2) The locations of recent supernovae near the Sun from modelling iron-60 transport
Authors: (1) Wallner et al. / (2) Breitschwerdt et al.
First Author’s Institution(s): (1) Australian National University, Canberra, Australia / (2) Berlin Institute of Technology, Berlin, Germany
Status: (1) & (2) Published in Nature,
Stellar party all around us
The Solar neighbourhood is not a quiet and lonely place. Instead, a cosmic orchestra of perpetual (think cosmic timescales) supernova explosions is taking place and infecting space with their ejecta. Evidence of this can be seen locally on Earth by inspecting the abundances of iron-60, a radioactive isotope of iron with a half-life time of ~2.6 million years, in the deep-sea crust of the ocean, which was done by Wallner and co-workers in a recent publication. The global distribution of iron-60 coming from space might be a source of error here, as its is mainly injected via large dust grains. Read more about how to derive directional information of these grains from their interaction with the atmosphere in a bite on Monday!
The researchers of study (1) analysed the deposition in time of this very short-lived isotope (in comparison with isotopes which live for billions of years like some Uranium nuclides) and found that inbetween 1.5–3.2 million years and 6.5–8.7 million years ago iron-60 concentration rapidly increased. As this isotope has to come from the explosion(s) of massive stars (in a so-called core-collapse supernova) the increase in the abundance of it in the sea floor tells us that there had to be a close-by supernova at that time. Their measurements are shown in Figure 1.
Fig 1. Incorporation of iron-60 into the sea floor over the last ten million years. Focusing on the red shaded areas, which give the iron-60 abundances in the sea crust over time, you can see two clear peaks in the incorporation at ~3 and ~7.5 million years ago. The black stars are data points of the rate of sea floor sediment deposition. Source: Wallner+ (2016)
Connection to the outside
Fig 2. Computer simulations of the Local Bubble with the location of the Sun indicated with a white star. Source: Nature News, Adrian L. Melott
From these measurements we can directly link to what is already known from astrophysics. The Earth (and the Solar System) are embedded in a diffuse medium, which is called the ‘Local Bubble’. When supernovae explode they eject their outer shells into the surrounding and ‘pollute’ it with heavier elements. These ejecta are usually quite fast; they can travel ~100 parsec (~300 light years) in several 100,000 years and can therefore reach far-away locations in space which are not directly connected to their immediate surrounding. By analysing the spectrum of the interstellar medium (the gas and dust which lurks around seemingly everywhere) astronomers found that there is a huge bubble of material which was once ejected from several supernovae. You can imagine the dimensions from Figure 2.
Tracing the origin
Fig 3. Deposition of iron-60 on Earth. Top: Model results of the deposition of iron-60 from two computational models, with a “homogenuous” and “inhomogenuous” interstellar background medium. Bottom: Measurements of iron-60 deposition (dots) vs. the two models from above. The models produce peaks of varying intensity and both fit the increased deposition rates acceptable. Source: Breitschwerdt+ (2016)
But we don’t need to stop there. Using analytical calculations and computer simulations Breitschwerdt and colleagues (study 2) tried to relate the origin of the supernovae to stars which are now located in the Scorpius-Centaurus association (this apod gives you an orientation in our local neighbourhood). They tried to model the explosions and the likely pathways of the ejecta fronts and fitted the actual abundances on the sea floor to distinct supernovae (Figure 3).
The findings fit best to the detonations of two supernovae, which are called “SN 14” and “SN 15”. The overlapping explosion ejecta reach Earth together with the relicts of older explosions and form the local bubble. Different density shock fronts in the bubble transport the iron-60 to Earth via dust grains which are layered to the sea floor.
Did the supernovae affect our ancestors?
2 million years is not a huge amount in evolutionary and geological timescales. Therefore, you could speculate that such a devastating event in our close proximity affected the Earth and its biosphere in one or the other way. The explosion was definitely very bright in the sky and increased the flux of cosmic rays on Earth significantly. Luckily it was probably not in the ‘kill distance’ of ~8 parsecs, which would have wiped out life on Earth in a mass-extinction event – otherwise I would probably not type in these words. On the other hand, at roughly that time geologists measure a global decrease in temperature, which initiated the last ice age (called the ‘Pleistocene epoch’) and the cosmic ray flux was potentially high enough to do weird things to our climate. Could these supernova have influenced biological evolution and therefore human evolution by affecting global temperatures? Because of huge errors in these extrapolations this is pretty speculative to date, but with refined measurements we could disentangle lots of enigmatic connections like this.
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