One-third of Mars' surface has shallow-buried HO, but it is currently too cold for use by life. Proposals to warm Mars using greenhouse gases require a large mass of ingredients that are rare on Mars' surface. However, we show here that artificial aerosols made from materials that are readily available at Mars-for example, conductive nanorods that are ~9 micrometers long-could warm Mars >5 × 10 time smore effectively than the best gases. Such nanoparticles forward-scatter sunlight and efficiently block upwelling thermal infrared. Like the natural dust of Mars, they are swept high into Mars' atmosphere, allowing delivery from the near-surface. For a 10-year particle lifetime, two climate models indicate that sustained release at 30 liters per second would globally warm Mars by ≳30 kelvin and start to melt the ice. Therefore, if nanoparticles can be made at scale on (or delivered to) Mars, then the barrier to warming of Mars appears to be less high than previously thought.
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http://dx.doi.org/10.1126/sciadv.adn4650 | DOI Listing |
Sci Adv
August 2024
Department of Electrical and Computer Engineering, Northwestern University, Evanston, IL, USA.
One-third of Mars' surface has shallow-buried HO, but it is currently too cold for use by life. Proposals to warm Mars using greenhouse gases require a large mass of ingredients that are rare on Mars' surface. However, we show here that artificial aerosols made from materials that are readily available at Mars-for example, conductive nanorods that are ~9 micrometers long-could warm Mars >5 × 10 time smore effectively than the best gases.
View Article and Find Full Text PDFAstrobiology
July 2024
Department of Earth and Environmental Sciences, Rutgers University, Newark, New Jersey, USA.
Jotun springs in Svalbard, Norway, is a rare warm environment in the Arctic that actively forms travertine. In this study, we assessed the microbial ecology of Jotun's active (aquatic) spring and dry spring transects. We evaluated the microbial preservation potential and mode, as well as the astrobiological relevance of the travertines to marginal carbonates mapped at Jezero Crater on Mars (the Mars 2020 landing site).
View Article and Find Full Text PDFSci Rep
October 2023
Centro de Astrobiología (CSIC-INTA), Madrid, Spain.
This investigation documents that the Rugged Terrain Unit, the Stimson formation, and the Greenheugh sandstone were deposited in a 1200 m-deep lake that formed after the emergence of Mt. Sharp in Gale crater, Mars, nearly 4 billion years ago. In fact, the Curiosity rover traversed on a surface that once was the bottom of this lake and systematically examined the strata that were deposited in its deepest waters on the crater floor to layers that formed along its shoreline on Mt.
View Article and Find Full Text PDFMicroorganisms
February 2023
Blue Marble Space Institute of Science, Seattle, WA 98104, USA.
Ultraviolet (UV) radiation responses of extremophilic and archaeal microorganisms are of interest from evolutionary, physiological, and astrobiological perspectives. Previous studies determined that the halophilic archaeon, sp. NRC-1, which survives in multiple extremes, is highly tolerant of UV radiation.
View Article and Find Full Text PDFMicroorganisms
December 2022
Exobiology Group, CNRS-Centre de Biophysique Moléculaire, Rue Charles Sadron, CEDEX 2, 45071 Orléans, France.
New detections of thermophiles in psychrobiotic (i.e., bearing cold-tolerant life forms) marine and terrestrial habitats including Arctic marine sediments, Antarctic accretion ice, permafrost, and elsewhere are continually being reported.
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