AMS measurements of cosmogenic and supernova-ejected radionuclides in deep-sea sediment cores
arXiv:1311.3481 · doi:10.1051/epjconf/20136303003
Abstract
Samples of two deep-sea sediment cores from the Indian Ocean are analyzed with accelerator mass spectrometry (AMS) to search for traces of recent supernova activity around 2 Myr ago. Here, long-lived radionuclides, which are synthesized in massive stars and ejected in supernova explosions, namely 26Al, 53Mn and 60Fe, are extracted from the sediment samples. The cosmogenic isotope 10Be, which is mainly produced in the Earths atmosphere, is analyzed for dating purposes of the marine sediment cores. The first AMS measurement results for 10Be and 26Al are presented, which represent for the first time a detailed study in the time period of 1.7-3.1 Myr with high time resolution. Our first results do not support a significant extraterrestrial signal of 26Al above terrestrial background. However, there is evidence that, like 10Be, 26Al might be a valuable isotope for dating of deep-sea sediment cores for the past few million years.
5 pages, 2 figures, Proceedings of the Heavy Ion Accelerator Symposium on Fundamental and Applied Science, 2013, will be published by the EPJ Web of conferences
References in corpus (4)
- The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
- The search for the origin of the Local Bubble redivivus
- Search for supernova-produced 60Fe in a marine sediment
- The Search for Supernova-produced Radionuclides in Terrestrial Deep-sea Archives
Cited by in corpus (6)
- Time resolved 2 million year old supernova activity discovered in Earth's microfossil record
- Astrophysical Shrapnel: Discriminating Among Near-Earth Stellar Explosion Sources of Live Radioactive Isotopes
- Radioactive Iron Rain: Transporting Fe in Supernova Dust to the Ocean Floor
- 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
- The Link Between the Local Bubble and Radioisotopic Signatures on Earth