Origin of dust dunes on Saturn's moon Titan, their chemical composition unraveled

Scientists have found the chemical composition of organic dust dunes present on Saturn’s moon Titan — an advance that sheds more light on the mechanism by which carbon-based structures form in extremely cold environments in space. The researchers, including those from the University of Hawaii (UH) at Manoa in the US, examined remote sensing data from NASA’s Cassini-Huygens mission to Titan — the only body in our solar system, besides the Earth, with a solid surface, lakes, and a thick atmosphere with a pressure of about 1.5 atmosphere at surface level. The images from the mission exposed the existence of vast longitudinal dunes on Titan’s surface across its equatorial deserts reaching heights of up to 100 meters, the study, published in Science Advances_,_ noted. Earlier imaging studies revealed that Titan’s dunes contained dark organic chemicals, compared to the dunes on the Earth that are made of silicates or a large class of other minerals. [caption id=“attachment_7527681” align=“alignnone” width=“1280”] Cassini spacecraft catches a glimpse of bright sunlight reflecting off the hydrocarbon seas of Saturn’s large moon Titan. Image: NASA[/caption] The researchers exposed acetylene ice — a chemical that is used on Earth in welding torches and exists at Titan’s cold equatorial regions — to radiation similar to high-energy galactic cosmic rays. They subjected the acetylene ice to a chemical reaction process that formed more complex organic molecules like benzene and naphthalene — a compound that is found in mothballs. These chemical processes, the researchers said, also happen in the interstellar medium — the space between stars — on hydrocarbon-rich layers of interstellar nanoparticles. “Titan’s dunes represent the dominating surface sink of carbon in Titan’s organic chemistry,” said Matthew Abplanalp, co-author of the study from UH. Abplanalp said that unraveling the origin and chemical pathways behind the dune material was vital not only to understand Titan’s chemical evolution but also to grasp how similar the chemistries on Titan and on the Earth might have been before life emerged on our planet 3.5 million years ago. “These processes eventually furnish the molecular building blocks not only for Titan’s organic dunes but also for organics on airless bodies in general such as on Kuiper Belt Objects like dwarf planet Makemake,” said co-author Ralf I Kaiser from UH. [caption id=“attachment_3913163” align=“alignnone” width=“640”] Methane clouds streaking across the hazy atmosphere on Titan. Image: NASA.[/caption] According to Kaiser, the discovery of low-temperature synthesis of complex organic compounds from acetylene ice represented a fundamental shift from currently accepted beliefs that such compounds only formed in the gas phase at elevated temperatures, such as in combustion processes. The researchers said that the findings of their study has unprecedented implications for the next space mission to Titan. “Overall, this study advances our understanding of the complex organics and fundamental chemical processing of simple molecules in deep space and provides a scientifically sound and proven mechanism of formation of aromatic structures in extreme environments in low-temperature ices,” Kaiser said. According to the researchers, since Titan is nitrogen-rich, the incorporation of the element in these complex organic molecules may also lead to carbon-nitrogen groups in molecules that play a vital role in contemporary biochemistry such as in DNA and RNA-based nitrogen-bases.