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Exploring Ocean Worlds: The Search for Life and Interesting Chemistry Throughout the Solar System
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Exoplanet and Excellence NASA's Search for Life in our Galaxy
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Biosignatures, Electrophoresis, and the Search for Life Beyond Earth
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The Search for Life and Habitable Worlds at NASA – Past, Present, and Future
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Enhancing the Sensitivity of Redox Detection in Search-for-Life Missions Using Chemical Vapor Deposition (CVD) Graphene Electrodes
The primary objective for this effort is to fabricate and characterize redox-active molecules using CVD graphene as working electrodes using standard "on-chip" lithographic techniques. We then plan to move away from “on-chip” graphene electrodes and study methods for CVD graphene transfer that can also accommodate in-space manufacturing (ISM), enabling the use of this technology for crewed mission operations of the future.
Rethinking CO Antibiosignatures in the Search for Life Beyond the Solar System
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Trace Element Concentrations Associated with Mid-Paleozoic Microfossils as Biosignatures to Aid in the Search for Life
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Habitability Considerations for Searching for Martian Life in Ground Ice
Introduction: The search for extant life on Marshas not been addressed since Viking, but the 2020 Decadal Survey judged it high priority. Missions proposed to search for extant life on Mars plan to sample ground ice, but the location and thermal properties of Martian ground ice change over time so such missions must consider its current and historical presence as well as its history of habitable conditions.
THE SEARCH FOR EXTRATERRESTRIAL LIFE
Detectors and techniques used in search for extraterrestrial life
"Nano" Scale Biosignatures and the Search for Extraterrestrial Life
A critical step in the search for remnants of potential life forms on other planets lies in our ability to recognize indigenous fragments of ancient microbes preserved in some of Earth's oldest rocks. To this end, we are building a database of nano-scale chemical and morphological characteristics of some of Earth's oldest organic microfossils. We are primarily using the new technology of Nano-Secondary ion mass spectrometry (NanoSIMS) which provides in-situ, nano-scale elemental analysis of trace quantities of organic residues. The initial step was to characterize element composition of well-preserved, organic microfossils from the late Proterozoic (0.8 Ga) Bitter Springs Formation of Australia. Results from that work provide morphologic detail and nitrogen/carbon ratios that appear to reflect the well-established biological origin of these 0.8 Ga fossils.
Analysis of methods for growth detection in the search for extraterrestrial life.
Microorganisms growth detection methods analyzed in search for extraterrestrial life
On the search for extant life on Mars
Proposals for continuing the search for extant life on Mars are primarily predicated on the assumption that specialized environmental niches that could support a biota may exist on the planet. Before attempting any critical tests for extant organisms, either in situ or on returned samples, it is imperative to determine whether any such sites actually exist. If, through remote sensing and landed instrumentation, sites of potential biological interest are discovered and characterized, biological tests can then more effectively be planned to elicit the presence of organisms that are adapted to living in these particular environments.
The Search for Extant Life on Mars: A Human Exploration Objective
A search for evidence of extant life on Mars should be conducted prior to and as part of human exploration missions. Potentially habitable environments for modern life occur on Mars. Despite a vigorous campaign of exploration of the surface over the last 3 decades, no mission has attempted to search for signatures of extant life since the Viking landers in 1976. Finding an example of extant life beyond Earth would be one of the greatest scientific discoveries of all time. This is especially important because (once discovered) the biochemistry and metabolism of the life form can be studied. Earth and Mars exchange materials over geologic time because impacts eject rock and crustal materials into space that are eventually deposited on other planets and moons [1]. Therefore, Earth and Mars could share life with a common origin and similar biochemistry; if this is the case, life on Mars likely experienced billions of years of evolution in isolation from Earth. Alternatively, Mars may host a distinct genesis of life which could be evident from its different biochemistry. Either discovery would change our understanding of life in the solar system and beyond. The Mars 2020/Perseverance sample collection mission is not optimized for finding extant life because the site for sample collection, Jezero Crater, was chosen for its ancient habitability and likelihood to host fossil evidence of life. Furthermore, the samples collected will not be returned for at least a decade. Within that period, technology development for human exploration will likely be underway and it is possible that humans will land on Mars without an updated knowledge of extant life on Mars, which may pose a risk both to those mission crews and to Earth when they return. Thus, it is important to perform a search for extant life on Mars prior to humans landing at a site where life may persist. Salts and shallow ground ice are particularly important environments to evaluate for extant life prior to human missions because they may be encountered and interacted with by human crews.
In the search for extraterrestrial life
The study of stellar, planetary and galactic evolution leads to the conclusion that the phenomenon of life must be coursing through the universe. It is estimated, by means of telescopic sampling, that there are billions of stars capable of having those photochemical reactions necessary for the origin of life. One approach in the search for other life would be to deploy men and instruments in spacecraft. Radio contact with other civilizations is another approach. Finally, the question might be approached by considering life as an inevitable consequence of the evolution of matter. A survey of Martian characteristics shows the possibility of life there to be dubious. The possibility of life in other parts of the galaxy is supported by a fundamental conclusion of living matter that all organisms have a common chemical ancestry. The experiment of Urey and Miller, wherein four amino acids were obtained by subjecting a mixture of methane, ammonia, and water to an electric arc, is believed to duplicate the initial organic syntheses which led to the emergence of life on earth.
The Polar Regions and the Search for Evidence of Life on Mars
The search for life on Mars and evidence for past life connects to polar exploration in two important ways. First the polar regions on Mars are sites of possible liquid water today, and hence possible locations for extant life. Secondly, ancient permafrost may preserve evidence of the nature of martian life.
The Icebreaker Life Mission to Mars: A Search for Biomolecular Evidence of Recent Life
The Icebreaker mission is the first mission to search for life signatures on Mars using biomolecular methods. Icebreaker lands in the ice-rich mid-latitudes of Mars and drills and collects samples down to at least 1 m depth to 1) search for molecular signatures of life and 2) assess the habitability of the icy regolith in the context of recent orbital cycles. Icebreaker is a NASA Discovery-class mission.
Field Simulation of a Drilling Mission to Mars to Search for Subsurface Life
The discovery of near surface ground ice by the Mars Odyssey mission and the abundant evidence for recent Gulley features observed by the Mars Global Surveyor mission support longstanding theoretical arguments for subsurface liquid water on Mars. Thus, implementing the Mars program goal to search for life points to drilling on Mars to reach liquid water, collecting samples and analyzing them with instrumentation to detect in situ organisms and biomarker compounds. Searching for life in the subsurface of Mars will require drilling, sample extraction and handling, and new technologies to find and identify biomarker compounds and search for living organisms. In spite of its obvious advantages, robotic drilling for Mars exploration is in its technological infancy and has yet to be demonstrated in even a terrestrial field environment.