Astrobiology: Life in the Universe

NASA Astrobiology Institute (NAI)


  1. Virtual Planetary Laboratory (JPL/CalTech)

    PI Victoria Meadows
    Members 0 (Inactive)
    Active Dates 7/2001 - 6/2006
    Team Website http://vpl.ipac.caltech.edu/

    Executive Summary

    Untitled

    Project Reports

    A 1-D Climate Model for Extrasolar Terrestrial Planets

    ROADMAP OBJECTIVES: 1, 1, 7

    Characterization of Terrestrial Planets From Disk-Averaged Spectra: Earths Around Other Stars

    ROADMAP OBJECTIVES: 1, 4, 7

    Characterization of Terrestrial Planets From Disk-Averaged Spectra: Spatially and Spectrally Resolved Planetary Models

    ROADMAP OBJECTIVES: 1, 7

    Database of Molecular Spectroscopy to Support Extrasolar Planet Modeling

    ROADMAP OBJECTIVES: 1, 7

    Database of Stellar Spectra to Support Extrasolar Planet Modeling

    ROADMAP OBJECTIVES: 1, 4, 6, 7

    Exploring Conditions for Habitability in our Solar System

    ROADMAP OBJECTIVES: 2, 2, 4, 6, 7

    Extrasolar Planet Detection and Characterization

    ROADMAP OBJECTIVES: 1, 7

    Model Synthesis and Architecture

    ROADMAP OBJECTIVES: 1, 1, 4, 4, 7

    Modeling Terrestrial Planet Formation and Composition

    ROADMAP OBJECTIVES: 1, 1, 3

    Searching for Life on Mars: Interpretation of Remote-sensing Observations of Methane

    ROADMAP OBJECTIVES: 2, 7

    The Abiotic Planetary Model: The Upper and Lower Boundary Condition on the Atmosphere

    ROADMAP OBJECTIVES: 1, 4, 7

    The Astrophysical Environment and Planetary and Lunar Habitability

    ROADMAP OBJECTIVES: 2, 4, 6, 6

    The Generalized Terrestrial Planet Photochemical Model

    ROADMAP OBJECTIVES: 1, 7

    The Virtual Planetary Laboratory - The Life Modules

    ROADMAP OBJECTIVES: 4, 4, 5, 6, 6, 7, 7

    Understanding the Earth's Early Environment

    ROADMAP OBJECTIVES: 1, 4, 7

    EPO Reports

    no reports submitted

    Project Reports

    Organized by Astrobiology Roadmap Objective

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  • 1 Determine whether the atmosphere of the early Earth, hydrothermal or exogenous matter were significant sources of organic matter.
  • 2 Develop and test plausible pathways by which ancient counterparts of membrane systems, proteins and nucleic acid were synthesized from simpler precursors and assembled into protocells.
  • 3 Replicating, catalytic systems capable of evolution, and construct laboratory models of metabolism in primitive living systems.
  • 4 Expand and interpret the genomic database of a select group of key microorganisms in order to reveal the history and dynamics of evolution.
  • 5 Describe the sequences of causes and effects associated with the development of Earth's early biosphere and the global environment.
  • 6 Define how ecophysiological processes structure microbial communities, influence their adaptation and evolution, and affect their detection on other planets.
  • 7 Identify the environmental limits for by examining biological adaptations to extremes in environmental conditions.

  • Change search results by adding or removing a team:

  • Carnegie Institution of Washington
  • Indiana University, Bloomington
  • Marine Biological Laboratory
  • Michigan State University
  • NASA Ames Research Center
  • NASA Goddard Space Flight Center
  • Pennsylvania State University
  • SETI Institute
  • University of Arizona
  • University of California, Berkeley
  • University of California, Los Angeles
  • University of Colorado, Boulder
  • University of Hawaii
  • University of Washington
  • Virtual Planetary Laboratory (JPL/CalTech) [x]