Notice: This is an archived and unmaintained page. For current information, please browse

2001 Annual Science Report

NASA Ames Research Center Reporting  |  JUL 2000 – JUN 2001

Life Beyond the Planet of Origin

4 Institutions
3 Teams
0 Publications
0 Field Sites
Field Sites

Project Progress

Life Beyond the Planet of Origin (dm)

Progress during the first part of this project began September 1, 2000. Several team members have isolated halophiles from nature, and testing has begun to determine radiation resistance, as part opf a study to evaluate linkages between mechaisms of resistence to salt and to ionizing radiation. A new study has begun on the DNA damage resistance of Dunaliella salina, an extremely halophilic eukaryotic alga. We have explored new techniques to assess damage resistance, and ways to measure gene activation upon rehydration of yeast.

Previous experiments have shown that halophytic organisms isolated from salterns and intertidal environments can survive a two-week exposure to the space environment. Using the space simulation facility at the DLR in Cologne, Germany, we have completed a series of ground simulation experiments using a halophytic cyanobacterium from the genus Synechococcus spp. We have exposed this organism to vacuum desiccation and ultraviolet (UV) radiation. These experiments reveal that these organisms can survive exposure to UV radiation and vacuum desiccation for at least six months and probably longer.

    Lynn Rothschild
    Project Investigator

    Rocco Mancinelli

    Gerda Horneck

    Jeff Johansen

    Antonio Lazcano

    Petra Rettberg

    Peter Schultz

    Stephen Smerdon

    Ray Wolstencraft

    David Wynn-Williams

    Oliver de Peyer

    Kimberly Warren-Rhodes

    Richard Weinstein

    Lourdes Sanchez
    Doctoral Student

    Kevin Kelly
    Graduate Student

    Peter Pilewskie
    Unspecified Role

    Objective 5.0
    Describe the sequences of causes and effects associated with the development of Earth's early biosphere and the global environment.

    Objective 6.0
    Define how ecophysiological processes structure microbial communities, influence their adaptation and evolution, and affect their detection on other planets.

    Objective 7.0
    Identify the environmental limits for life by examining biological adaptations to extremes in environmental conditions.

    Objective 8.0
    Search for evidence of ancient climates, extinct life and potential habitats for extant life on Mars.

    Objective 10.0
    Understand the natural processes by which life can migrate from one world to another. Are we alone in the Universe?

    Objective 12.0
    Define climatological and geological effects upon the limits of habitable zones around the Sun and other stars to help define the frequency of habitable planets in the universe.

    Objective 14.0
    Determine the resilience of local and global ecosystems through their response to natural and human-induced disturbances.

    Objective 15.0
    Model the future habitability of Earth by examining the interactions between the biosphere and the chemistry and radiation balance of the atmosphere.

    Objective 16.0
    Understand the human-directed processes by which life can migrate from one world to another.

    Objective 17.0
    Refine planetary protection guidelines and develop protection technology for human and robotic missions.