2009 Annual Science Report

Carnegie Institution of Washington Reporting  |  JUL 2008 – AUG 2009

Executive Summary

The NASA Astrobiology Institute team led by the Carnegie Institution of Washington is dedicated to the study of the extrasolar planets, solar system formation, organic rich primitive planetary bodies, deep sequestration of CHON volatiles in terrestrial planets, prebiotic molecular synthesis through geocatalysis, and the connection between planetary evolution the emergence, and sustenance of biology – processes central to the missions of the NAI. Our program attempts to integrate the sweeping narrative of life’s history through a combination of bottom-up and top-down studies. On the one hand, we study processes related to chemical and physical evolution in plausible prebiotic environments – circumstellar disks, extrasolar planetary systems and the primitive Earth. Complementary to these bottom-up investigations of life’s origin, we will continue our field and experimental top-down efforts to document the nature of microbial life at extreme conditions, as well as the characterization of organic matter in ... Continue reading.

Field Sites
26 Institutions
7 Project Reports
168 Publications
5 Field Sites

Project Reports

  • Project 6: Application of Laboratory Experimentation to Flight Instrument Testing

    The Arctic Mars Analogue Svalbard Expedition (AMASE) tests instruments, procedures and protocols to answer critical science questions on Mars. NAI sponsored researchers undertake science tasks alongside scientists developing instruments for Mars missions (MSL and ExoMars).

  • Project 4: Geochemical Steps Leading to the Origins of Life

    The project titled “Geochemical Steps Leading to the Origins of Life” sets a out a research object focusing on exploring the natural intersection of abiological organic chemistry and the mineral world. Assuming that life emerged on Earth as a consequence of natural, geochemical, processes. We ask what did the organic landscape look like before life, how did organic-mineral surface interactions affect this landscape, and can we identify any connections between this abiotic organic Earth and the subsequent emergence of life.

  • Project 3: The Origin, Evolution, and Volatile Inventories of Terrestrial Planets

    The origin and Sustenance of life on Earth strongly depends on the fact that volatile elements H-C-O-N where retained in sufficient abundance to sustain an ocean-atmosphere. The research in this project involves studies of how terrestrial planets form, why differences exist among the terrestrial planets, how volatiles behave deep within the Earth, and how volatiles and life influence the large and small scale composition of the near surface Earth.

    ROADMAP OBJECTIVES: 1.1 3.1 4.1
  • Project 2: Origin and Evolution of Organic Matter in the Solar System

    Through telescopic observations of remote objects, we are learning about the distribution of organic matter in the outer Solar System and how it is thermally processed, as well as about dynamic processes that .could have delivered such organic-rich material to be incorporated into terrestrial planets. Extraterrestrial samples like primitive meteorites and interplanetary dust particles contain significant amounts of carbonaceous material and were likely a source of organic matter to the early Earth. By using a wide variety of advanced techniques to study organic matter in meteorites and other extraterrestrial samples, we are trying to learn how and where it formed, and how it has been modified during 4.5 billion years of solar system evolution. We also perform laboratory experiments to simulate formation of complex organic matter and how it is modified on planetary surfaces. Finally we are studying biological contamination of meteorites once they have landed on Earth to learn how this can affect studies of the indigenous non-biological organic matter.

    ROADMAP OBJECTIVES: 2.2 3.1 7.1
  • Project 1: Looking Outward: Studies of the Physical and Chemical Evolution of Planetary Systems

    We study the origin of life through a wide variety of approaches, beginning here with theoretical investigations of protoplanetary disks, the environments in which simple organic molecules first appeared and were concentrated in planetary bodies. We also study the survival of this organic matter during subsequent evolution through observations of circumstellar disks around both young and mature stars, extrasolar planetary systems, and small bodies in our Solar System, and through detailed models of planetary system formation.

    ROADMAP OBJECTIVES: 1.1 1.2 2.2 3.1
  • NAI ORAU Post Doc Report: CIW-NAI
    ROADMAP OBJECTIVES: 3.1 3.2 7.1
  • Project 5: Geological-Biological Interactions

    This project focuses on a wide range of questions spanning understanding microbial diversity in extreme environments to the identification of biosignatures in modern and ancient rocks. In terms of environments, research in this project focuses on research at deep sea hydrothermal vents, desert sulfate deposits, arctic hydrothermal fields, as well as Paleoproterozoic terrains of Australia, Canada, and India. By learning more how life adapts to extreme environments on Earth, we hope to gain a better understanding of the limits of life on other worlds. By understanding better the signature of life recorded in ancient rocks, we hope to better refine our search stategies for the presence of life on other worlds.

    ROADMAP OBJECTIVES: 4.1 5.1 6.1 6.2 7.1