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|    ScienceDaily to All    |
|    Two meteorites are providing a detailed     |
|    27 Mar 23 22:30:20    |
      MSGID: 1:317/3 64226d71       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        Two meteorites are providing a detailed look into outer space                Date:        March 27, 2023        Source:        American Chemical Society        Summary:        If you've ever seen a shooting star, you might have seen a meteor        on its way to Earth. Those that land here can be used to peek back        in time, into the far corners of outer space or at the earliest        building blocks of life. Scientists have conducted some of the most        detailed analyses yet on the organic material of two meteorites.                      Facebook Twitter Pinterest LinkedIN Email       FULL STORY       ==========================================================================       If you've ever seen a shooting star, you might have actually seen a       meteor on its way to Earth. Those that land here are called meteorites       and can be used to peek back in time, into the far corners of outer space       or at the earliest building blocks of life. Today, scientists report       some of the most detailed analyses yet of the organic material of two       meteorites. They've identified tens of thousands of molecular "puzzle       pieces," including a larger amount of oxygen atoms than they had expected.                     ==========================================================================       The researchers will present their results at the spring meeting of the       American Chemical Society (ACS).              Previously, the team led by Alan Marshall, Ph.D., investigated complex       mixtures of organic materials found on Earth, including petroleum. But       now, they are turning their attention toward the skies -- or the things       that have fallen from them. Their ultra-high resolution mass spectrometry       (MS) technique is starting to reveal new information about the universe       and could ultimately provide a window into the origin of life itself.              "This analysis gives us an idea of what's out there, what we're going to       run into as we move forward as a 'spacefaring' species," says Joseph       Frye-Jones, a graduate student who is presenting the work at the       meeting. Both Marshall and Frye-Jones are at Florida State University       and the National High Magnetic Field Laboratory.              Thousands of meteorites fall to Earth every year, but only a rare few are       "carbonaceous chondrites," the category of space rock that contains the       most organic, or carbon-containing, material. One of the most famous is       the "Murchison" meteorite, which fell in Australia in 1969 and has been       studied extensively since. A newer entry is the relatively unexplored       "Aguas Zarcas," which fell in Costa Rica in 2019, bursting through       back porches and even a doghouse as its pieces fell to the ground. By       understanding the organic makeup of these meteorites, researchers can       obtain information about where and when the rocks formed, and what they       ran into on their journey through space.              To make sense of the complicated jumble of molecules on the meteorites,       the scientists turned to MS. This technique blasts a sample apart into       tiny particles, then basically reports the mass of each one, represented       as a peak.              By analyzing the collection of peaks, or the spectrum, scientists can       learn what was in the original sample. But in many cases, the resolution       of the spectrum is only good enough to confirm the presence of a compound       that was already presumed to be there, rather than providing information       about unknown components.              This is where Fourier-transform ion cyclotron resonance (FT-ICR)       MS comes in, which is also known as "ultra-high resolution" MS. It       can analyze incredibly complex mixtures with very high levels of       resolution and accuracy. It's especially well suited for analyzing       mixtures, like petroleum, or the complex organic material extracted       from a meteorite. "With this instrument, we really have the resolution       to look at everything in many kinds of samples," says Frye- Jones.              The researchers extracted the organic material from samples of both the       Murchison and Aguas Zarcas meteorites, then analyzed it with ultra-high       resolution MS. Rather than analyzing only one specific class of molecules       at a time, such as amino acids, they chose to look at all soluble organic       material at once. This provided the team with more than 30,000 peaks for       each meteorite to analyze, and over 60% of them could be given a unique       molecular formula.              Frye-Jones says these results represent the first analysis of this type       on the Aguas Zarcas meteorite, and the highest-resolution analysis on       the Murchison one. In fact, this team identified nearly twice as many       molecular formulas as previously reported for the older meteorite.              Once determined, the data were sorted into unique groups based on       various characteristics, such as whether they included oxygen or sulfur,       or whether they potentially contained a ring structure or double       bonds. They were surprised to find a large amount of oxygen content       among the compounds. "You don't think of oxygen-containing organics as       being a big part of meteorites," explained Marshall.              The researchers will next turn their attention to two far more precious       samples: a few grams of lunar dust from the Apollo 12 and 14 missions of       1969 and 1971, respectively. These samples predate Marshall's invention       of FT-ICR MS in the early 1970s. Instrumentation has come a long way       in the decades since and is now perfectly poised to analyze these       powders. The team will soon compare their results from the meteorite       analyses to the data they obtain from the lunar samples, hoping to learn       more information about where the moon's surface came from. "Was it from       meteorites? Solar radiation? We should be able to soon shed some light       on that," says Marshall.              The researchers acknowledge funding from the National Science Foundation       Division of Chemistry and the State of Florida. They thank the Chicago       Field Museum Robert A Pritzker Center for Meteoritics and Polar Studies       and the Arizona State University Buseck Center of Meteorite Studies for       the meteorite samples.               * RELATED_TOPICS        o Space_&_Time        # Asteroids,_Comets_and_Meteors # Solar_Flare #        Space_Missions # NASA # Space_Exploration # Moon #        Sun # Solar_System        * RELATED_TERMS        o Meteor o Meteorite o Outer_space o Space_observatory        o Space_elevator o Spitzer_space_telescope o Venus o        Extraterrestrial_life              ==========================================================================       Story Source: Materials provided by American_Chemical_Society. Note:       Content may be edited for style and length.                     ==========================================================================                     Link to news story:       https://www.sciencedaily.com/releases/2023/03/230327114908.htm              --- up 1 year, 4 weeks, 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: 229/111 112 113 307 317 400 426 428 470 664 700 292/854 298/25       SEEN-BY: 305/3 317/3 320/219 396/45       PATH: 317/3 229/426           |
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