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        STELLAR CHEMISTRY
        Stellar explosion in Earth's proximity
        by Staff Writers
        Munich, Germany (SPX) Oct 01, 2020

        This manganese crust started to grow about 20 million years ago. It grew layer by layer until it was retrieved a few years ago and analyzed in the Maier-Leibnitz-Laboratory at the Technical University of Munich. In layers that are around 2.5 million years old, the researchers found iron-60 and elevated levels of manganese-53. Their occurrence is evidence of a near-Earth supernova 2.5 million years ago.

        When the brightness of the star Betelgeuse dropped dramatically a few months ago, some observers suspected an impending supernova - a stellar explosion that could also cause damage on Earth. While Betelgeuse has returned to normal, physicists from the Technical University of Munich (TUM) have found evidence of a supernova that exploded near the Earth around 2.5 million years ago.

        The life of stars with a mass more than ten times that of our sun ends in a supernova, a colossal stellar explosion. This explosion leads to the formation of iron, manganese and other heavy elements.

        In layers of a manganese crust that are around two and a half million years old a research team led by physicists from the Technical University of Munich has now confirmed the existence of both iron-60 and manganese-53.

        "The increased concentrations of manganese-53 can be taken as the "smoking gun" - the ultimate proof that this supernova really did take place," says first author Dr. Gunther Korschinek.

        While a very close supernova could inflict massive harm to life on Earth, this one was far enough away. It only caused a boost in cosmic rays over several thousand years. "However, this can lead to increased cloud formation," says co-author Dr. Thomas Faestermann. "Perhaps there is a link to the Pleistocene epoch, the period of the Ice Ages, which began 2.6 million years ago."

        Ultra-trace analysis
        Typically, manganese occurs on earth as manganese-55. Manganese-53, on the other hand, usually stems from cosmic dust, like that found in the asteroid belt of our solar system. This dust rains down onto the earth continuously; but only rarely do we perceive larger specks of dust that glow as meteorites.

        New sediment layers that accumulate year for year on the sea floor preserve the distribution of the elements in manganese crusts and sediment samples. Using accelerator mass spectrometry, the team of scientists has now detected both iron-60 and increased levels of manganese-53 in layers that were deposited about two and a half million years ago.

        "This is investigative ultra-trace analysis," says Korschinek. "We are talking about merely a few atoms here. But accelerator mass spectrometry is so sensitive that it even allows us to calculate from our measurements that the star that exploded must have had around 11 to 25 times the size of the sun."

        The researchers were also able to determine the half-life of manganese-53 from comparisons to other nuclides and the age of the samples. The result: 3.7 million years. To date, there has only been a single measurement to this end worldwide.

        Research Report: Supernova-Produced 53Mn on Earth


        Related Links
        Technical University of Munich
        Stellar Chemistry, The Universe And All Within It


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        STELLAR CHEMISTRY
        Scientists precisely measure total amount of matter in the universe
        Riverside CA (SPX) Sep 29, 2020
        A top goal in cosmology is to precisely measure the total amount of matter in the universe, a daunting exercise for even the most mathematically proficient. A team led by scientists at the University of California, Riverside, has now done just that. Reporting in the Astrophysical Journal, the team determined that matter makes up 31% of the total amount of matter and energy in the universe, with the remainder consisting of dark energy. "To put that amount of matter in context, if all the matt ... read more

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