
"If the Fe is the heaviest element "produced"/fusioned in a star. How are "produced" the others, which are heavier than Fe?"
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University of California, Berkeley
Executive Summary
Berkeley Executive Summary
Project Reports
Landforms made by groundwater discharge on Mars and Earth
ROADMAP OBJECTIVES: 1Characterization of Aqueous Processes on Mars Through Spectral Remote Sensing
ROADMAP OBJECTIVES: 2Climate, Habitability, and the Atmosphere on early Mars
ROADMAP OBJECTIVES: 1, 1, 3, 6, 7, 7Early oceans on Mars
ROADMAP OBJECTIVES: 1, 2Earthbound microbial and geological robotic based observations for Mars
ROADMAP OBJECTIVES: 2, 2, 5, 5Evolution of the interior and its consequences for water on Mars
ROADMAP OBJECTIVES: 1, 2Iron and sulfur-based biospheres and their biosignatures
ROADMAP OBJECTIVES: 4, 6, 7, 7Isotopic fingerprints of past life and surface conditions on Mars
ROADMAP OBJECTIVES: 1, 2, 7EPO Reports
Improving Science Literacy Through the Use of BioMARS E/PO Instructional Materials
Project Reports
Organized by Astrobiology Roadmap Objective
- Objective 1: Determine whether the atmosphere of the early Earth, hydrothermal or exogenous matter were significant sources of organic matter. (6 reports)
- Objective 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. (6 reports)
- Objective 3: Replicating, catalytic systems capable of evolution, and construct laboratory models of metabolism in primitive living systems. (1 reports)
- Objective 4: Expand and interpret the genomic database of a select group of key microorganisms in order to reveal the history and dynamics of evolution. (1 reports)
- Objective 5: Describe the sequences of causes and effects associated with the development of Earth's early biosphere and the global environment. (2 reports)
- Objective 6: Define how ecophysiological processes structure microbial communities, influence their adaptation and evolution, and affect their detection on other planets. (2 reports)
- Objective 7: Identify the environmental limits for by examining biological adaptations to extremes in environmental conditions. (5 reports)
Goal 1: Understand the nature and distribution of habitable environments in the Universe
Goal 2: Explore for past or present habitable environments, prebiotic chemistry and signs of life elsewhere in our Solar System
Goal 3: Understand how life originates from cosmic and planetary precursors
Goal 4: Understand how past life on Earth interacted with its changing planetary and Solar System environment
Goal 5: Understand the evolutionary mechanisms and environmental limits of life
Goal 6: Understand the principles that will shape the future of life, both on Earth and beyond
Goal 7: Determine how to recognize signatures of life on other worlds and on early Earth
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