NASA: National Aeronautics and Space Administration

  1. Content with the tag: “oxygen

  2. A search for primordial water from deep in the Earth's mantle

    ROADMAP OBJECTIVES: 1.1, 4.1

    A Self-Perpetuating Catalyst for the Production of Organics in Protostellar Nebulae

    ROADMAP OBJECTIVES: 1.1, 3.1

    Acquisition and Installation of a new Cameca ims 1280 ion microprobe

    ROADMAP OBJECTIVES:

    Advancing Techniques for in situ Analysis of Complex Organics

    ROADMAP OBJECTIVES: 2.1, 2.2, 3.1, 3.2, 7.1

    Application of U-tube and fiber-optic distributed temperature sensor to characterize the chemical and physical properties of a deep permafrost and sub-permafrost environment at High Lake, Nunavut, Canada.

    ROADMAP OBJECTIVES: 2.1, 5.2, 5.3, 7.1

    Astrobiology Sample Analysis Program (ASAP)

    ROADMAP OBJECTIVES:

    Biological potential of Mars

    ROADMAP OBJECTIVES: 2.1, 3.1

    Biosignatures in chemosynthetic and photosynthetic systems

    ROADMAP OBJECTIVES: 2.1, 4.1, 5.1, 5.2, 6.1, 7.1, 7.2

    Breakdown of methane due to electric discharge: A Laboratory Investigation with Relevance to Mars

    ROADMAP OBJECTIVES: 2.1

    Chemical Models of Nebular Processes

    ROADMAP OBJECTIVES: 1.1

    Composition of Parent Volatiles in Comets: Oxidized Carbon

    ROADMAP OBJECTIVES:

    Current Status and Future Bioastronomy with the Large Millimeter Telescope

    ROADMAP OBJECTIVES: 3.1

    Early Metabolic Pathways

    ROADMAP OBJECTIVES: 2, 3

    Early Metabolic Pathways

    ROADMAP OBJECTIVES: 3.2, 3.4

    Fingerprinting Late Additions to the Earth and Moon via the Study of Highly Siderophile Elements in Lunar Impact Melt Rocks

    ROADMAP OBJECTIVES: 1.1

    Formation and Detection of Hot-Earth Objects in Systems with Close-in Jupiters

    ROADMAP OBJECTIVES: 1.1, 1.2

    Formation of Planetesimals in a Dynamically Evolving Nebula

    ROADMAP OBJECTIVES: 1.1

    Genes that regulate photosymbiotic relationships

    ROADMAP OBJECTIVES: 2

    Habitable Planets

    ROADMAP OBJECTIVES: 1.1, 1.2, 2.1, 4.3

    Icelandic subglacial lakes

    ROADMAP OBJECTIVES: 2.1, 4.1, 5.3, 6.2

    Interplanetary Pioneers

    ROADMAP OBJECTIVES: 5.3, 6.2

    Microbial Communities and Activities in the Deep Marine Subsurface

    ROADMAP OBJECTIVES: 5.1, 5.3, 6.1, 6.2

    Modeling grain surface reaction pathways for large organic molecules

    ROADMAP OBJECTIVES: 3.1

    Organic and Inorganic Acids from Ion-irradiated Ices

    ROADMAP OBJECTIVES: 2.2, 3.1, 7.1

    Origin and Evolution of Organics

    ROADMAP OBJECTIVES: 1.1, 2.1, 3.1

    Origin and Evolution of Organics in Planetary Systems

    ROADMAP OBJECTIVES: 1.1, 3.1, 3.2

    Origin of Irregular Satellites

    ROADMAP OBJECTIVES: 1.1

    Prebiotic Organics from Space

    ROADMAP OBJECTIVES: 1.1, 2.1, 2.2, 3.1, 3.4, 4.3, 7.1, 7.2

    Protist diversity in extreme environments

    ROADMAP OBJECTIVES: 6, 7

    Recovery of comet 85P/Boethin for the Deep Impact Extended Mission

    ROADMAP OBJECTIVES: 2.2

    Research Activities in the Astrobiology Analytical Laboratory

    ROADMAP OBJECTIVES: 1.1, 2.1, 2.2, 3.1, 7.1

    Sediment-buried basement deep biosphere

    ROADMAP OBJECTIVES: 1.1, 3.3, 4.1, 5.1, 5.2, 5.3, 6.1, 6.2

    Societal and Philosophical Aspects of Astrobiology

    ROADMAP OBJECTIVES: 18

    Studies in Planetary Formation and Evolution

    ROADMAP OBJECTIVES: 11, 12, 8, 9

    Studies of Organic Matter and Water in Meteorites

    ROADMAP OBJECTIVES: 1, 11, 8, 9

    The Main Belt distribution of basaltic asteroids

    ROADMAP OBJECTIVES: 2.2

    THE VYSOS PROJECT

    ROADMAP OBJECTIVES: 1.2

    Ultra-violet processing of ices in the Rosette Nebula

    ROADMAP OBJECTIVES: 3.1

    Understanding the Microbial Ecology of Geologically-based Chemolithoautotrophic Communities

    ROADMAP OBJECTIVES: 2.1, 4.1
  3. Greening the Earth


    carbonatesLate Precambrian carbonate outcropping is visable at the south end of Death Valley, California. Carbon isotopes in these layers bear evidence of the first extensive greening of the Earth
    One of the most dramatic and seemingly inexplicable events in the history of Earth’s biosphere occurred roughly 540 million years ago when multi-cellular life exploded all over the planet. This large-scale diversification of life is known as the ‘Cambrian explosion’ and lead to the variety of organisms we see on Earth today. Scientists have often attributed the Cambrian explosion to significant geologic or climatic changes on our planet, but new NASA-sponsored research may have a better explanation.

    Rather than catastrophic disruptions in Earth’s climate, a new study indicates that the Cambrian explosion may have been caused by more...


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    Source: [Nature]

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  4. Rock Bands Spin an Oxygen Record


    The rise of oxygen on early Earth may have been caused by a microbial changing of the guard between methane-producers and oxygen-producers. This swap may have been initiated by a drop in the ocean’s nickel abundance. Continuing studies of the world’s largest iron ore deposits could cement the case.

    Source: [Astrobiology Magazine]

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  5. Evidence for the Great Oxidation Event Challenged


    The timing of the rise of oxygen in Earth’s atmosphere is a key question in astrobiology. It is coupled not only to the question of when organisms capable of oxygenic photosynthesis first evolved on Earth, but also what signs of life might be found on young Earth-like planets around other stars.

    Members of NAI’s Penn State and Carnegie Institution of Washington Teams report in the current issue of Science that certain sulfur isotopes found in many sedimentary rocks older than 2.4 billion years may not be the result of photochemical reactions in an oxygen-free atmosphere as previously thought....

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  6. Early Oxygen



    Cores retrieved from layers of deep-sea rocks that are 3.46 billion years old suggest that oceans contained abundant oxygen and that the atmosphere of the Earth was as rich in oxygen as it is today. The cores were obtained in northwestern Western Australia, and contain evidence that the deep ocean 3.46 billion years ago was so rich in oxygen that oxygen-producing organisms must have been actively producing it. This means that oxygen-producing organisms like cyanobacteria were present much earlier in Earth’s history than previously believed.

    Source: [Astrobiology Magazine]

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  7. Oxygen in Earth's Early Atmosphere


    Researchers from NAI’s Carnegie Institution of Washington Team have a paper in this week’s Nature describing evidence that Earth’s Mesoarchean atmosphere (3.2 and 2.8 Gya) possessed very low amounts oxygen. These findings contrast with prior claims that Earth’s atmosphere underwent its first rise in oxygen during the Mesoarchean, and indicate that oxygen first rose above parts per million levels sometime between 2.45 and 2.4 billion years ago.

    Source: [Link]

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  8. Oxygen in Earth's Atmosphere Before Great Oxidation Event


    NAI’s Astrobiology Drilling Program supported researchers in 2004 to obtain subsurface core samples from the Hamersley Basin in Western Australia. Those samples, representing the time just before the Great Oxidation Event, have been analyzed, and two research papers detailing the results (Anbar, et al. and Kaufman, et al.) appear in September 28, 2007 issue of Science. Both groups found unexpected, correlated changes that reveal the presence of small but significant amounts of O2 in the environment 2.5 billion years ago, ~50-100 milion years before the Great Oxidation Event, and a shift from lower O2 abundance prior to that time.

    Source: [Link]

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  9. Subaerial Volcanoes Shift Oxygen Levels on Early Earth


    Biomarkers in rocks prior to the rise in Earth’s atmospheric oxygen 2.5 billion years ago show cyanobacteria released oxygen at the same levels as today. What was happening to that oxygen? A new paper in this week’s Nature from NAI’s Penn State Team proposes that the rise of atmospheric oxygen occurred because the predominant sink for oxygen—enhanced submarine volcanism—was abruptly and permanently diminished during the Archaean–Proterozoic transition by a shift from predominantly submarine volcanism to a mix of subaerial and submarine volcanism.

    Source: [Link]

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  10. Biogeochemistry and Oxygenic Photosynthesis


    Researchers from NAI’s University of Colorado, Boulder Team recently reported in Earth and Planetary Science Letters their new biogeochemical model relating to the Great Oxidation Event. With ion microprobe data for individual sulfides from water-lain sedimentary units in the 2.45–2.22 Ga Huronian Supergroup, the team proposes a new model where enhanced weathering rates during interglacial thawing stimulated blooms of oxygenic photosynthesis, the demise of methane, and ultimately the irreversible rise in atmospheric oxygen between the first and second Huronian glaciations. The paper’s lead author was also the recipient of an NAI Research Scholarship in 2004.

    Source: [Link]

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  11. Oxygen and Life in the Precambrian


    The December 2006 issue of Geobiology is a collection of papers focusing on the history of Earth’s biogeochemistry, from the earliest sedimentary rocks in Greenland to the late Proterozoic. The rise of atmospheric oxygen provides a thematic link. The papers in this issue, edited by David Catling and Roger Buick of NAI’s University of Washington Alumni Team, grew out of a session of the Earth System Processes 2 conference in Calgary, Canada, 8–11 August 2005, sponsored by the NAI.

    Source: [Link]

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  12. Romer's Gap Confirmed


    Peter Ward from NAI’s Alumni Team at the University of Washington and his collaborators have a new paper out in PNAS this week providing supportive evidence for Romer’s Gap. Their results link this gap in vertebrate terrestrialization with a low atmospheric oxygen interval. This paper supports Ward’s new book on the evolution of effective respiratory systems, entitled “Out of Thin Air.”

    Source: [Link]

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  13. Further Studies on the Rise of Atmospheric Oxygen


    Lee Kump of NAI’s Pennsylvania State University Lead Team is co-author on a new paper in GSA Today examining the rise of atmospheric oxygen at the Archean-Proterozoic transition, 2.5-2.0 billion years ago. The team of international researchers studied sedimentary and volcanic rocks from the Fennoscandian Shield, which provides a fairly complete record of the hallmark events of that transition.

    Source: [Link]

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  14. More on the Rise of Earth's Oxygen Levels


    A new paper in Earth and Planetary Science Letters from NAI’s Carnegie Institution of Washington Lead Team and NAI’s International Partner, the Australian Centre for Astrobiology, explores environmental changes during the rise of atmospheric oxygen and the relationship between tectonics, atmospheric oxygen, and climatic changes.

    Source: [Link]

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