TY - JOUR
T1 - Time-resolved 2-million-year-old supernova activity discovered in Earth's microfossil record
AU - Ludwig, Peter
AU - Bishop, Shawn
AU - Eglib, Ramon
AU - Chernenko, Valentyna
AU - Deneva, Boyana
AU - Faestermann, Thomas
AU - Famulok, Nicolai
AU - Fimiani, Leticia
AU - Gómez-Guzmán, José Manuel
AU - Hain, Karin
AU - Korschinek, Gunther
AU - Hanzlik, Marianne
AU - Merchel, Silke
AU - Rugel, Georg
N1 - Funding Information:
The search for Fe supernova signatures is supported by the German Research Foundation (DFG), Grant DFG-Bi1492/1-1, and by the DFG Cluster of Excellence Origin and Structure of the Universe (www.universe-cluster.de).
PY - 2016/8/16
Y1 - 2016/8/16
N2 - Massive stars (M≳10 M⊙), which terminate their evolution as corecollapse supernovae, are theoretically predicted to eject >10-5M⊙ of the radioisotope 60Fe (half-life 2.61 Ma). 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 magnetofossilswere 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.
AB - Massive stars (M≳10 M⊙), which terminate their evolution as corecollapse supernovae, are theoretically predicted to eject >10-5M⊙ of the radioisotope 60Fe (half-life 2.61 Ma). 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 magnetofossilswere 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.
KW - Accelerator mass spectrometry
KW - Magnetofossils
KW - Supernova
UR - http://www.scopus.com/inward/record.url?scp=84982161931&partnerID=8YFLogxK
U2 - 10.1073/pnas.1601040113
DO - 10.1073/pnas.1601040113
M3 - Article
C2 - 27503888
AN - SCOPUS:84982161931
SN - 0027-8424
VL - 113
SP - 9232
EP - 9237
JO - Proceedings of the National Academy of Sciences of the United States of America
JF - Proceedings of the National Academy of Sciences of the United States of America
IS - 33
ER -