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|    EARTH    |    Uhh, that 3rd rock from the sun?    |    8,931 messages    |
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|    ScienceDaily to All    |
|    New models shed light on life's origin    |
|    10 Feb 23 21:30:38    |
      MSGID: 1:317/3 63e719f3       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        New models shed light on life's origin         The research reveals clues about the physical and chemical       characteristics of Earth when life is thought to have emerged.                Date:        February 10, 2023        Source:        University of Rochester        Summary:        Researchers from the University of Rochester and the University        of Colorado Boulder used experiments and zircon chemistry to build        more accurate computer models of fluids that act as pathways from        inner Earth to Earth's surface. The models allow researchers to        simulate what metals may have been transported to Earth's surface        when life first emerged, about four billion years ago. The research        has important implications not only for discovering the origins        of life but also in the search for life on other planets.                      Facebook Twitter Pinterest LinkedIN Email       FULL STORY       ==========================================================================       The first signs of life emerged on Earth in the form of microbes about       four billion years ago. While scientists are still determining exactly       when and how these microbes appeared, it's clear that the emergence       of life is intricately intertwined with the chemical and physical       characteristics of early Earth.                     ==========================================================================       "It is reasonable to suspect that life could have started differently       -- or not at all -- if the early chemical characteristics of our planet       were different," says Dustin Trail, an associate professor of earth and       environmental sciences at the University of Rochester.              But what was Earth like billions of years ago, and what characteristics       may have helped life to form? In a paper published in Science, Trail       and Thomas McCollom, a research associate at the University of Colorado       Boulder, reveal key information in the quest to find out. The research       has important implications not only for discovering the origins of life       but also in the search for life on other planets.              "We are now at an exciting time in which humankind is searching for       life on other planets and moons, as well as in other planetary systems,"       Trail says.              "But we still do not know how -- or even when, really -- life started on       our own planet. Research like ours helps identify specific conditions and       chemical pathways that could have supported the emergence of life, work       which is certain to factor prominently into the search for life outside of       our planet." The importance of metals in the emergence of life Research       into life and its origins typically involves a variety of disciplines       including genomics, the study of genes and their functions; proteomics,       the study of proteins; and an emerging field called metallomics, which       explores the important role of metals in performing cellular functions. As       life evolved, the need for certain metals changed, but Trail and McCollom       wanted to determine what metals may have been available when microbes       first appeared billions of years ago.              "When hypotheses are proposed for different origin-of-life scenarios,       scientists have generally assumed all metals were available because there       weren't studies that provided geologically robust constraints on metal       concentrations of fluids for the earliest times of Earth's history,"       Trail says.              To address this shortcoming, Trail and McCollom studied the composition       and characteristics of fluids in the lithosphere -- the outer layer       of Earth that includes the crust and upper mantle -- billions of years       ago. These lithospheric fluids are key pathways to transport dissolved       parts of rocks and minerals between Earth's interior and hydrothermal       pools in its exterior where microbial life could have formed. While       researchers cannot directly measure the metals that existed billions of       years ago, by determining the properties of the fluids, they can infer       what metals -- and the concentrations of the metals - - could feasibly       have been transported between Earth's interior and exterior during the       time when life emerged on the planet.              Clues in billion-year-old minerals Billion-year-old rocks and minerals       are often the only direct sources of information about Earth's earliest       history. That's because the rocks and minerals lock in information about       the composition of Earth at the time they are formed.              The researchers conducted high-pressure, high-temperature experiments and       applied these results to early-Earth zircons, a robust type of mineral       collected at sites in Western Australia, to determine the oxygen pressure,       chlorine content, and temperature of lithospheric fluids billions of       years ago.              They then input this information into computer models. The models allowed       them to simulate the properties of the lithospheric fluids, and, in turn,       simulate which metals could have travelled through the fluids to reach       hydrothermal pools at Earth's surface.              Understanding how life originated The researchers were surprised by       what the model simulations indicated. Many origin-of-life researchers,       for instance, consider copper a likely component in the chemistry that       could have led to life. But Trail and McCollom did not find evidence that       copper would have been abundant under the constraints in their analysis.              One metal they did test that may have been available in high       concentrations was manganese. While it is rarely considered in       origin-of-life scenarios, today manganese helps the body form bones and       assists enzymes in breaking down carbohydrates and cholesterol.              "Our research shows that metals like manganese may function as important       links between the 'solid' Earth and emerging biological systems at       Earth's surface," Trail says.              Trail says the research will help scientists studying the origin of life       to input more concrete data into their experiments and models.              "Experiments designed with this information in mind will result in a       better understanding of how life originated."        * RELATED_TOPICS        o Health_&_Medicine        # Healthy_Aging # Alternative_Medicine        # Patient_Education_and_Counseling #        Dietary_Supplements_and_Minerals # Medical_Topics #        Nutrition # Vitamin # Pregnancy_and_Childbirth        * RELATED_TERMS        o Longevity o Microorganism o Atmospheric_dispersion_modeling        o Computational_neuroscience o Stem_cell_treatments o Suicide        o Air_pollution o Bioethics              ==========================================================================       Story Source: Materials provided by University_of_Rochester. Original       written by Lindsey Valich. Note: Content may be edited for style and       length.                     ==========================================================================       Journal Reference:        1. Dustin Trail and Thomas M. McCollom. Relatively oxidized fluids fed        Earth's earliest hydrothermal systems. Science, 2023 DOI: 10.1126/        science.adc8751       ==========================================================================              Link to news story:       https://www.sciencedaily.com/releases/2023/02/230210185150.htm              --- up 49 weeks, 4 days, 10 hours, 50 minutes        * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! (1:317/3)       SEEN-BY: 15/0 106/201 114/705 123/120 153/7715 226/30 227/114 229/110       SEEN-BY: 229/111 112 113 114 307 317 400 426 428 470 664 700 292/854       SEEN-BY: 298/25 305/3 317/3 320/219 396/45       PATH: 317/3 229/426           |
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