Time resolved 2 million year old supernova activity discovered in Earth's microfossil record
arXiv:1710.09573 · doi:10.1073/pnas.1601040113
Abstract
Massive stars, which terminate their evolution as core collapse supernovae, are theoretically predicted to eject more than 1E-5 solar masses of the radioisotope 60Fe. If such an event occurs sufficiently close to our solar system, traces of the supernova debris could be deposited on Earth. Herein, we report a time resolved 60Fe signal residing, at least partially, in a biogenic reservoir. Using accelerator mass spectrometry, this signal was found through the direct detection of live 60Fe atoms contained within secondary iron oxides, among which are magnetofossils, the fossilized chains of magnetite crystals produced by magnetotactic bacteria. The magnetofossils were chemically extracted from two Pacific Ocean sediment drill cores. Our results show that the 60Fe signal onset occurs around 2.6 Ma to 2.8 Ma, near the lower Pleistocene boundary, terminates around 1.7 Ma, and peaks at about 2.2 Ma.
arXiv commentFigures from the Supplementary Information are not included due to file size restrictions. Download the, now open access, original article for those details (see doi)
References in corpus (12)
- A Unified Approach to the Classical Statistical Analysis of Small Signals
- The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
- Rapid formation of large dust grains in the luminous supernova SN 2010jl
- Evaluation of three methods for calculating statistical significance when incorporating a systematic uncertainty into a test of the background-only hypothesis for a Poisson process
- The origin of the Local Bubble
- SPI observations of the diffuse 60Fe emission in the Galaxy
- Evidence for Nearby Supernova Explosions
- Signatures of a two million year old supernova in the spectra of cosmic ray protons, antiprotons and positrons
- Search for supernova-produced 60Fe in a marine sediment
- Radioactive Iron Rain: Transporting Fe in Supernova Dust to the Ocean Floor
- Discovery Prospects for a Supernova Signature of Biogenic Origin
- AMS measurements of cosmogenic and supernova-ejected radionuclides in deep-sea sediment cores
Cited by in corpus (40)
- Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
- Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
- Radioactive nuclei from cosmochronology to habitability
- Magnetorotational supernovae: A nucleosynthetic analysis of sophisticated 3D models
- A supernova at 50 pc: Effects on the Earth's atmosphere and biota
- A discovery of a low-energy excess in cosmic-ray iron: an evidence of the past supernova activity in the Local Bubble
- Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. I. 60Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous ISM
- Magnetic Imprisonment of Dusty Pinballs by a Supernova Remnant
- Exploring the link between star and planet formation with Ariel
- The TeV Cosmic Ray Bump: a Message from Epsilon Indi or Epsilon Eridani Star?
- Cosmic nucleosynthesis: a multi-messenger challenge
- r-Process Radioisotopes from Near-Earth Supernovae and Kilonovae
- Activity measurement of 60Fe through the decay of 60mCo and confirmation of its half-life
- Heliospheric Compression due to Recent Nearby Supernova Explosions
- Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. II. Advanced modeling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernovae in the solar neighborhood
- Photobiological effects at Earth's surface following a 50 pc Supernova
- From cosmic explosions to terrestrial fires?
- Paleo-Detectors for Galactic Supernova Neutrinos
- Terrestrial Effects of Nearby Supernovae: Updated Modeling
- Supernova Dust Evolution Probed by Deep-sea 60Fe Time History
- A Way Out of the Bubble Trouble? - Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth
- X-Ray Luminous Supernovae: Threats to Terrestrial Biospheres
- Stellar encounters with giant molecular clouds
- The Fe(n, γ)Fe Cross Section from the Surrogate Ratio Method and Its Effect on the Fe Nucleosynthesis
- Enhanced production of 60Fe in massive stars
- Proposed Lunar Measurements of -Process Radioisotopes to Distinguish Origin of Deep-sea 244Pu
- Terrestrial effects of moderately nearby supernovae
- Formation and evolution of the local interstellar environment: combined constraints from nucleosynthetic and X-ray data
- Ozone depletion-induced climate change following a 50 pc supernova
- Recent progress on interstellar radionuclides on Earth and the Moon
- A possible role for stochastic radiation events in the systematic disparity between molecular and fossil dates
- The New Astronomical Frontier of Interstellar Objects
- Impacts of Dust Grains Accelerated by Supernovae on the Moon
- Direct measurements of cosmic rays and their possible interpretations
- The Link Between the Local Bubble and Radioisotopic Signatures on Earth
- Nearby Supernova and Cloud Crossing Effects on the Orbits of Small Bodies in the Solar System
- Nuclear astrophysics
- Cosmic Radioactivity and Galactic Chemical Evolution
- CO Structures with Narrow Lines in Nearby Quiescent Regions
- Simulations of Fe entrained in ejecta from a near-Earth supernova: Effects of observer motion