2005 Annual Science Report
University of Hawaii, Manoa Reporting | JUL 2004 – JUN 2005
Executive Summary
Water is the medium in which the chemistry of all life on Earth takes place. Water is the habitat in which life first emerged and in which all of it still thrives. Water has modified Earth’s geology and climate to a degree that has allowed life to persist to the present epoch. We propose to create a research and education framework that links the biological, chemical, geological, and astronomical sciences to better understand the origin, history, distribution, and role of water as it relates to life in the universe. We focus on scenarios involving the sources and distribution of water in planetary systems and the delivery and incorporation of water into rocky planets that orbit within stellar habitable zones. Our framework connects research on major aspects of planetary water — in effect we aim to understand the terms of a “watery Drake equation”. Sub-themes of ... Continue reading.
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Karen Meech
NAI, ASTEP, ASTID, Exobiology -
TEAM Active Dates:
11/2003 - 10/2008 CAN 3 -
Members:
61 (See All) - Visit Team Page
Project Reports
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The Aqueous Environment of the Emergence of Complex Life
We have started a new initiative to study key steps in the evolution of complex life and the potential relationship to aqueous conditions (oxygen, ion concentrations, etc.) at the time of those events. We are studying two “model” systems.
ROADMAP OBJECTIVES: 4.2 -
Integrated Characterization of Microbial Communities Associated With Aquatic Redox Gradients
Our investigations of oxic-anoxic transitions are focused on understanding the synergy between geochemical processes and microbial community and metabolic diversity. These studies not only further our understanding of geochemical cycles that have shaped the evolution of Earth but also have the potential to contribute to flight-related missions through the development of in situ measurement technologies.
ROADMAP OBJECTIVES: 5.1 5.2 5.3 6.1 -
A Proteomic View of Adaptations to Extreme Environments
Over the past two decades, molecular biology techniques have ushered in a paradigm shift in environmental microbiology. Thriving microbial communities have been discovered inhabiting physical and chemical regimes once assumed limiting to life. These “novel” environments are collectively known as “extreme” environments and the organisms that inhabit them “extremeophiles”.
ROADMAP OBJECTIVES: 5.1 5.3 -
Subseafloor Basement (Basalt) Biosphere Studies
This project involves studies of the deep subseafloor basement biosphere. We are utilizing Ocean Drilling Program borehole (CORK) observatories to access the fluids that circulate through the ocean basin wide environment, where temperatures (2-100°C) and chemistry are conducive to a very broad range of aerobic and anaerobic and heterotrophic and chemolithotrophic metabolisms and survival strategies.
ROADMAP OBJECTIVES: 5.3 6.1 7.1 7.2 -
Icelandic Subglacial Volcanic Habitats
Successful field test of drill in June 2005. We expect drill to be fully operational for planned June 2006 expedition.
ROADMAP OBJECTIVES: 2.1 2.2 5.3 6.2 7.1 -
Lava Tube Microbiology
The extreme nature of the surface environments on Mars appear to exclude extant biological habitation.
ROADMAP OBJECTIVES: 5.1 5.2 6.2 -
Deep Impact Target Characterization
The Deep Impact mission is the first planetary mission to carry out direct experimentation on a cometary body by delivering a 360-kg impactor to comet 9P/Tempel 1 at 10.2 km/s on UT July 4, 2005. UHNAI team members were closely involved in the world-wide effort of ground- and Earth-orbital observations to characterize the target nucleus pre-impact and to observe throughout the period of Encounter
ROADMAP OBJECTIVES: 2.2 3.1 -
Origin of Irregular Satellites
ROADMAP OBJECTIVES: 2.2 -
The Lowell Telescope Scheduler
ROADMAP OBJECTIVES: None Selected -
AFAR: Adaptive Framework for Astrobiology Research
ROADMAP OBJECTIVES: None Selected -
The Evolution of Intelligence Under Environmental Change
ROADMAP OBJECTIVES: 4.2 6.2 7.2 -
Astrobiology Winter School
ROADMAP OBJECTIVES: 2.2 3.1 6.1 7.1 -
Analysis Software for in Situ Voltammetry
ROADMAP OBJECTIVES: 5.3 6.1 -
Analysis of Fine Scale Genetic Divergence in Oceanic Microbial Communities
The marine environment comprises the largest contiguous “surface” habitat on Earth, but it is far from a continuous, homogenous environment.
ROADMAP OBJECTIVES: 5.1 5.2 -
Formation of Astrobiologically Important Molecules in Water-Rich Environments
Our goal ultimate goal is to investigate the formation of biological molecules in water-rich environments. Water ice serves as the energy-transfer medium and active participant in a variety of radiation-driven chemistry reactions thought to be important in either the interstellar medium or the primordial solar nebula.
ROADMAP OBJECTIVES: 3.1 3.2 -
Cometary Water and Volatile Abundances
any comets have been observed to have activity at large heliocentric distances on their inbound orbital legs at distances too far from the sun to be caused by sublimation of pure water ice.
ROADMAP OBJECTIVES: 2.2 3.1 -
Analysis Tools for a Proteomic View of Adaptations to Extreme Environments
ROADMAP OBJECTIVES: 5.3 -
Young Low Mass Stars
ROADMAP OBJECTIVES: 1.2 -
Serpentinization, Abiogenic Methane, and Extremophilic Archaea Within the Seafloor
ROADMAP OBJECTIVES: 5.2 5.3 -
Formation of Planetesimals in a Dynamically Evolving Nebula
Work on the dynamics of dust grains in the neighborhood of density-enhanced structures in a planet-forming nebula has been continuing. In particular, a new project on the dynamics and coagulations of dust particles in a dynamically evolving nebula has been launched. In such and environment, the physical properties of the nebula, such as its temperature and pressure, constantly vary.
ROADMAP OBJECTIVES: 1.1 -
Ice in Sublimation Environments
Ice exists in sublimation environments on many planetary surfaces, including Mars, Antarctica, and possibly the polar regions of the Moon. Schorghofer and Edgett (2005) studied observations of seasonal ice at unusually low latitudes on Mars, where it exists on cold pole-facing slopes (Figure 1).
ROADMAP OBJECTIVES: 2.1 -
Habitability and Water Delivery in Binary-Planetary Systems
Study of habitability and water-delivery in binary star systems requires an expansive study of the dynamical evolution of these systems. While habitability requires identifying regions within the habitable zone of the system where a life-harboring planet (such as an Earth-size body) can have a long-term stable orbit, water-delivery requires identifying regions where water-carrying objects such as comets, and water-rich planetesimals and protoplanets, can be unstable.
ROADMAP OBJECTIVES: 1.1 -
Rapid Response to Remotely Detected Potential Seafloor Eruption
ROADMAP OBJECTIVES: 5.3 -
Aqueous Alteration on Mars
This project focuses on using our understanding of aqueous alteration from terrestrial laboratory experiments and field observations to try to place limits on the duration of aqueous alteration events on Mars. We are working on several aspects of this. We describe the most mature one here (to be submitted for publication in August, 2005).
ROADMAP OBJECTIVES: 2.1 -
Chondritic Meteorites as Records of Aqueous Activity on Asteroidal Parent Bodies
ROADMAP OBJECTIVES: 2.2 3.1 -
Kuiper Belt Orbital Studies
ROADMAP OBJECTIVES: 1.1 2.2 -
Miniature Mass Spectrometer Development
NAI support has contributed to the development of a center for mass spectrometer development at UH, with systems under development for chemical measurements using electron impact (for gases), electrospray (liquids), laser ablation resonance ionization (isotope and elemental abundance in solids), and secondary ionization (a standard for geochemical assays).
ROADMAP OBJECTIVES: 2.1 7.1 -
Searching for Water and Organic Material in the Outer Solar System
ROADMAP OBJECTIVES: 2.2
Publications
- There are no publications for this team in the 2005 annual report.
2005 Teams
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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, Manoa
University of Rhode Island
University of Washington
Virtual Planetary Laboratory (JPL/CalTech)