Supernova footprint on the doorstep: 60Fe, 53Mn, and other possible correlations
Dr. Gunther Korschinek (Physik Department E15, TU München)
Datum: 09.01.2020 16:00 Uhr – 17:00 Uhr
Ort: Am Coulombwall 1, Garching
Lecture Hall (ground floor)
In our Galaxy, around 1 to 2 supernovae (SN) explode over the course of 100 years. Such a titanic event happened during the last 10 Million years close to our solar system, so to speak on our doorstep. The ejected debris has entered our solar system, and a fraction lodged on our Earth and on the Moon. Clear signals are long-living radioisotopes, which do not exist naturally or at low amounts on Earth; such as 60Fe (T1/2 = 2.6 Ma).
After a short summary of measurement results of 60Fe, performed at TU Munich and ANU (Canberra), I will present first indications of another supernova-formed radioisotope in deep-sea crusts, 53Mn (T1/2 = 3.7 Ma).
The so-called local fluff (local interstellar cloud), presently imbedding the solar system, could originate from these close-by SNe, hence should comprise 60Fe that enters the solar system now. Search in 500 kg snow from the Antarctica reveals a signal of 60Fe that supports a recent SN origin of the local fluff. The time slot where we found 60Fe deposition in crusts and sediments coincides with a drop in Earth's temperature, that happened between 2 or 3 Million years before now and it enforced glaciations on the Earth. These glaciations are considered the cause of the evolution and development of mankind. Possible correlations will be discussed.