NASA: National Aeronautics and Space Administration

  1. Content with the tag: “saturn

  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. Salt Discovered in Saturn's Outermost Ring


    For the first time, scientists working on NASA’s Cassini mission have detected sodium salts in ice grains of Saturn’s outermost ring. Detecting salty ice indicates that Saturn’s moon Enceladus, which primarily replenishes the ring with material from discharging jets, could harbor a reservoir of liquid water — perhaps an ocean — beneath its surface.

    Cassini discovered the water-ice jets in 2005 on Enceladus. These jets expel tiny ice grains and vapor, some of which escape the moon’s gravity and form Saturn’s outermost ring. Cassini’s cosmic dust analyzer has examined the composition of those grains and found salt within...

    Read More

    Source: [NASA Press Release]

    Tags , , ,
    Comments 1
  4. The Ions and Isoptopes of Enceladus


    Cassini will fly within 16 miles of Enceladus’ surface to measure molecules in the Saturnian moon’s environment. The data will provide insight into the early history of the solar system.

    Source: [Astrobiology Magazine]

    Tags , ,
    Comments 1
  5. Ocean on Enceladus May Be Short-Lived


    Three years ago, surprising evidence came out for an ocean underneath the surface of Saturn’s moon Enceladus. But a new report indicates just how hard it may be to keep water from freezing on this tiny moon.

    Read More

    Source: [Astrobiology Magazine]

    Tags , ,
    Comments No comments yet, you could be the first.
  6. Organics Erupting from Enceladus


    NASA’s Cassini spacecraft “tasted” and sampled a surprising organic brew erupting in geyser-like fashion from Saturn’s moon Enceladus during a close flyby on March 12. Scientists are amazed that this tiny moon is so active, “hot,” and brimming with water vapor and organic chemicals.

    Tags , ,
    Comments No comments yet, you could be the first.
  7. Explore Enceladus...Online!


    This new web interactive from NASA’s Cassini mission features dazzling new imagery of Saturn’s moon Enceladus. It details the discovery of the plumes of ice particles and water vapor erupting from the surface and extending hundreds of kilometers into space. These plumes have put Enceladus on the map as an object of astrobiological study; the Cassini spacecraft just completed a specialized fly-through to get a closer look.

    Tags , ,
    Comments No comments yet, you could be the first.
  8. Signs of Ocean Beneath Titan's Crust?


    NASA’s Cassini spacecraft has discovered evidence that points to the existence of an underground ocean of water and ammonia on Saturn’s moon Titan. The Cassini science team detail their findings in this week’s Science, explaining that radar mapping of Titan revealed a shift in landmarks on the moon’s surface of up to 30 kilometers between October 2004 and May 2007. The best explanation, they say, is an underground ocean that disconnects Titan’s icy crust from its rocky interior.

    Tags , , , , ,
    Comments No comments yet, you could be the first.
  9. Cassini Flies Through Watery Plumes of Enceladus


    Enceladus

    NASA’s Cassini spacecraft performed a daring flyby of Saturn’s moon Enceladus on Wed., March 12, flying about 15 kilometers per second (32,000 mph) through icy water geyser-like jets. The spacecraft snatched up precious samples that might point to a water ocean or organics inside the little moon.

    Read More

    Tags , , , , ,
    Comments No comments yet, you could be the first.
  10. Hydrocarbons on Saturn's Moon Hyperion


    NASA’s Cassini spacecraft has revealed for the first time surface details of Saturn’s moon Hyperion, including cup-like craters filled with hydrocarbons that may indicate more widespread presence in our solar system of basic chemicals necessary for life.

    Source: [Link]

    Tags , , , ,
    Comments Commenting has been closed.
  11. Earth's Future Glimpsed on Titan


    The enigmatic Saturnian moon Titan is still yielding surprising new details years after scientists first pierced its thick haze veil. The vision now emerging of Saturn’s largest moon, with its giant dunes and oceanless surface, is perhaps a glimpse of Earth’s desert future. Space.com has the story…

    Source: [Link]

    Tags , ,
    Comments Commenting has been closed.
  12. NASA's Cassini Spacecraft Images Seas on Titan


    Instruments on NASA’s Cassini spacecraft have found evidence for seas, likely filled with liquid methane or ethane, in the high northern latitudes of Saturn’s moon Titan. One such feature is larger than any of the Great Lakes of North America and is about the same size as several seas on Earth.

    Source: [Link]

    Tags , , , ,
    Comments Commenting has been closed.
  13. A Deeper Look into the Watery Plumes of Enceladus


    NASA astrobiologists are hard at work examining the nature of the plumes of water vapor recently discovered on Saturn’s moon Enceladus. If a new geological theory about the plumes, published in this week’s Nature, proves to be correct, it would preclude the existence of a subsurface ocean on the moon. The theory is testable with existing data from NASA’s Cassini mission…

    Source: [Link]

    Tags , , ,
    Comments Commenting has been closed.
  14. Titanic Moon: Orange Soup from Saturnian Turn


    Researchers for the NASA Astrobiology Institute and Penn State have recently developed a new method that has improved our understanding of Titan’s atmospheric chemistry.

    Read More

    Tags , ,
    Comments Commenting has been closed.
Tags