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2008
In the mid-60’s NASA was developing instruments for the Viking spacecraft to detect life on Mars. To assist in this effort, NASA consulted James Lovelock, an iconoclastic British atmospheric chemist. Lovelock wondered: Can the existence of life be recognized from knowledge of the chemical composition of a planet’s atmosphere? What would the Earth be like now, if life had never evolved on it? Would there be oxygen in the air? Would the surface temperature be hot like Venus, or cold like Mars? He came to the conclusion that a spacecraft didn’t need to be sent to Mars. All one needed was a determination of the composition of the Martian atmosphere to see if it were in chemical equilibrium. This was done, and to the accuracy of the measurements, unlike the Earth’s atmosphere, the martian atmosphere was in chemical equilibrium. He concluded that Mars was dead (see Krasnopolsky et. al. 2004 and Formisano et. al. 2004 for a possibly low-level methane exception to this conclusion). However,...
The possible existence of life on Mars is now gaining credence. Evidence consistent with or supporting the presence of extant microbial life, as reported by a life detection experiment on the Viking Mission in 1976, has been rapidly accumulating from spacecraft orbital and lander operations, and from terrestrial observations. Vast oceans of frozen water near the planet's surface are being discovered, with strong indications of recent or present liquid flows, and theory and laboratory experiment have demonstrated that liquid water should exist on the surface of Mars. The biosphere on Earth has been extended into extreme environments until recently thought inimical to life. Places void of life have become rare. No life requirement has been found lacking on Mars. It is possible that, by the time of this 50th Anniversary SPIE Meeting, the paradigm shift accepting life beyond the Earth may have been made. Mankind will then emerge from its ancient fear of loneliness into a new fear of anticipation of what that still unidentified life might portend.
Journal of the History of Biology, 2005
George Beadle, a farm boy from Wahoo, Nebraska (pop. 3500) who won a Nobel Prize in 1958, was a key figure in the transition from classical to biochemical and molecular genetics. Plainspoken and unpretentious, he was disinclined to self-advertisement, and his career has been obscured, at least to younger scientists if not to historians of genetics, by the dazzle of DNA celebrity. Paul Berg and Maxine Singer, both distinguished senior scientists, aim to restore him to life in part to acquaint younger scientists with their forebears, not only Beadle but also his generation of geneticists. They have succeeded handsomely in this deeply researched and lucidly written biography, a work that historians as well as scientists will find informative and compelling. Beadle, the product of a prosperous if paternally stern household, escaped in 1922 to the University of Nebraska College of Agriculture, in Lincoln. In 1927 he went for doctoral training to Cornell, where he quickly hooked up with the corn geneticist Rollins A. Emerson, a former Nebraska faculty member who had established ''a Lincolnto-Ithaca [recruitment] tradition,'' Berg and Singer note (p. 25). Awarded his Ph.D. in 1930 for a dissertation on the cytogenetics of corn, he joined Thomas Hunt Morgan's Drosophila group at the California Institute of Technology as a postdoctoral fellow, where he gave up corn research for the cytogenetics of fruit flies. Beadle soon became interested in the relationship between genetics and development, a problem that awaited an experimental approach. To the end of devising one, he embarked in 1934 on a transatlantic collaboration with the Russian-French geneticist Boris Ephrussi. Berg and Singer authoritatively narrate how the two scientists learned by transplanting eye buds from one larva into the abdomens of others that single genes participate in the metabolic steps that produce brown eye pigment. They also show how in 1940-1941 Beadle, now a professor at
Gaia and Philosophy international symposium, 2022
Gaia now confronts us with states of operation and response that threaten long-term habitability for many species. Authored by a strong team of accomplished scholars—astrophysicist Adam Frank, planetary scientist David Grinspoon, and astrobiologist Sara Walker—the recent article “Intelligence as a Planetary Scale Process” probes ideas concerning a viable planetary integration of the technosphere with the biosphere. However, the concept of intelligence comes up short in their efforts to integrate planetary biology and technological society. In short, their description of planetary intelligence wavers between a control regime and an autonomous process. The conceptual strains of “Intelligence as a Planetary Scale Process” indicate that the preferable, properly Gaian formulation is planetary cognition, a theoretical framing that embeds the technosphere within its biospheric conditions of possibility.
Astrobiology
While it is anticipated that future human missions to Mars will increase the amount of biological and organic contamination that might be distributed on that planet, robotic missions continue to grow in capability and complexity, requiring precautions to be taken now to protect Mars, and particularly areas of Mars that might be Special Regions. Such precautionary cleanliness requirements for spacecraft have evolved over the course of the space age, as we have learned more about planetary environments, and are the subject of regular deliberations and decisions sponsored by the Committee on Space Research (COSPAR). COSPAR's planetary protection policy is maintained as an international consensus standard for spacecraft cleanliness that is recognized by the United Nations Committee on the Peaceful Uses of Outer Space. In response to the paper presented in this issue by Fairén et al. (2017), we examine both their concept of evidence for possible life on Mars and their logic in recommending that spacecraft cleanliness requirements be relaxed to access Special Regions ''before it is too late.'' We find that there are shortcomings in their plans to look for evidence of life on Mars, that they do not support their contention that appropriate levels of spacecraft cleanliness are unaffordable, that there are major risks in assuming martian life could be identified by nucleic acid sequence comparison (especially if those sequences are obtained from a Special Region contaminated with Earth life), and that the authors do not justify their contention that exploration with dirty robots, now, is preferable to the possibility that later contamination will be spread by human exploration. We also note that the potential effects of contaminating resources and environments essential to future human occupants of Mars are both significant and not addressed by Fairén et al. (2017).
July 30, 2006 was the 30 th anniversary of the Viking Mission's first Labeled Release (LR) life detection experiment on Mars. The strong response, together with supporting results from eight additional LR tests of Martian soil, established the presence of an active agent that was inhibited by heating. The data satisfied the pre-mission criteria for the detection of living microorganisms. However, the scientific community reacted cautiously, generally concluding that the activity in the soil was caused by chemistry or physics.
Humanity is waiting and is preparing for the future of a human Mars colony. Beside technological issues there are also many complicated evolutionary, psychological and ethical challenges. Here it will be discussed what the first humans on Mars will find under intensive selective pressure. How will this pressure affect the human evolution, especially the brain and psyche evolution? Humans will find for the first time in the human history in new situation when they will be dependent on supplies from Earth. Here it will be suggested to artificially accelerate biological evolution on Earth to prepare for future Mars colonizers.
JBIS, 1993
The outcome of terraforming on Mars is examined by considering the function of its biosphere. By borrowing a life-support model of the Earth's biosphere, scenarios of ecopoiesis and full terraforming are contrasted in terms of their energy flow and matter cycling. It is argued that Martian colonists are unlikely to be satisfied with the services provided by the anaerobic biosphere produced by ecopoiesis and that full terraforming will be the specific goal of planetary engineering. The distance of Mars from the sun and its probable lack of a closed rock cycle will require small scale, conscious intervention in biogeochemical cycles to maintain the habitability of the planet. Vernadsky's concept of the noosphere (an envelope of mind) will thus have more relevance to Mars as an abode of life than Lovelock's Gaia hypothesis.
2014
This paper examines the age old question of the basis of moral value in a the new context of astrobiology, which offers a fresh perspective. The goal is to offer the broad outline of a general theory of moral value that can accommodate the diversity of living entities we are likely to encounter beyond the confines of Earth. It begins with ratiocentrism, the view that the possession of reason is the primary means by which we differentiate entities having moral value in and of themselves from those having moral value merely by virtue of the uses to which they can be put. I extend this basic position by arguing that reason, sociality and culture tend to arise in evolution as a co-evolutionary “package deal.” Because of this, it’s really the sociality-reason-culture triad (SRCT) which should be the criterion for intrinsic moral value, not reason alone. Interestingly, if the SRCT linkage is sufficiently strong, it follows that this sort of moral valuation would be shared by any non-human entities capable of reflection on the nature of such things, granting it a curious kind of objectivity. Then I suggest that the unfolding of complexity produced by SRCT species may be the best means to realize the manifest destiny (or manifest complexity) of all life, which may provide an ultimate, metaphysical foundation for ethical value. Finally, I outline how this new theory can be applied to different types of entities that we may encounter beyond Earth.
In 1972, James Lovelock and Lynn Margulis began collaborating on the Gaia hypothesis. They suggested that over geological time, life on Earth has had a major role in both producing and regulating its own environment. Gaia is now an ecological and environmental worldview underpinning vital scientific and cultural debates over environmental issues. Their ideas have transformed the Earth and life sciences, as well as contemporary conceptions of nature. Their correspondence describes these crucial developments from the inside, showing how their partnership proved decisive for the development of the Gaia hypothesis. Clarke and Dutreuil provide historical background and explain the concepts and references introduced throughout the Lovelock-Margulis correspondence, while highlighting the major landmarks of their collaboration within the sequence of almost 300 letters written between 1970 and 2007. This book will be of interest to researchers in ecology, history of science, environmental hi...
A method is proposed to resolve the long-running issue of life on Mars. Based on the legacy of the Viking Mission Labeled Release (LR) experiment, the method exploits the sensitivity of C respirometry. In 1976, the LR obtained positive responses at Viking 1 and 2 sites on Mars, but, for a variety of posited reasons, the consensus favored chemical or physical agents in the Martian surface material, not life. Since Viking, no life detection experiment has been sent to Mars. New information about the Martian environment and the discoveries of extremeophiles on Earth have re-energized interest in the possibility of living microorganisms on the red planet. The new method, the "Chiral LR" (CLR), combines the LR with the chiral specificities displayed by living organisms. The isomers of C-labeled chiral substrates are separately injected onto soil samples, which are then monitored for the evolution of gas. Small self-sustaining probes are launched from the spacecraft in a manner protecting the original sterility of the probes. A strong preference for one chiral isomer over its sister in an on-going reaction with the soil is evidence of life. The new feature herein presented adds multiple controls to augment that supplied by a nonresponding chiral isomer. The added controls increase the reliability of the overall result to the point where an abiotic agent is difficult to propose. The results may solve the life-on-Mars issue, and may, also, usher in a new era of comparative biology. 14 14
The primary focus of NASA"s Mars and other planetary exploration programs, such as Titan, Enceladus, and Europa, "is to determine if life is or was present." The author suggests that NASA"s stated primary focus should, therefore, include a re-examination of the data from the 1976 Viking Mission Labeled Release (LR) life detection experiment. That experiment obtained repetitive strong positive signals supported by a variety of controls, altogether signifying the detection of microbial metabolism in the top few centimeters of the surface of Mars. The data fall well within those obtained from hundreds of terrestrial LR tests of soils and microbial cultures that made up the response library assembled for the Viking LR experiment. No physico-chemical theory or experiment of the many attempted over the years has duplicated or explained away the Viking LR results as indicative of life. Together with pertinent findings on Mars and Earth since Viking, the possibility of microbial life on Mars has become a singular scientific issue warranting the herein requested reexamination of the Viking LR data.
Astrobiology, 2015
The search for traces of life is one of the principal objectives of Mars exploration. Central to this objective is the concept of habitability, the set of conditions that allows the appearance of life and successful establishment of microorganisms in any one location. While environmental conditions may have been conducive to the appearance of life early in martian history, habitable conditions were always heterogeneous on a spatial scale and in a geological time frame. This "punctuated" scenario of habitability would have had important consequences for the evolution of martian life, as well as for the presence and preservation of traces of life at a specific landing site. We hypothesize that, given the lack of long-term, continuous habitability, if martian life developed, it was (and may still be) chemotrophic and anaerobic. Obtaining nutrition from the same kinds of sources as early terrestrial chemotrophic life and living in the same kinds of environments, the fossilized...
After 21 years of study, a case was made (1) that the 1976 Viking Labeled Release (LR) experiment detected microbial life in the Martian soil. However, two key factors prevent general acceptance of that conclusion. They are the failure of the Viking Gas Chromatograph Mass Spectrometer (GCMS) to find organic matter in the Martian soil; and the presumed inability of the Martian environment to support liquid water. Further examination of these often cited factors shows they do not prohibit a biological interpretation of the Mars LR results.
BIO-Complexity, 2013
Here I review the claim that the order of nature is uniquely suitable for life as it exists on earth (Terran life), and specifically for living beings similar to modern humans. I reassess Henderson's claim from The Fitness of the Environment that the ensemble of core biochemicals that make up Terran life possess a unique synergistic fitness for the assembly of the complex chemical systems characteristic of life. I show that Henderson's analysis is still remarkably consistent with the facts one century after it was written. It is still widely accepted even among researchers in astrobiology. I also review the evidence for believing that many of the properties of the same core set of biochemicals are specifically fit for the physiology of complex terrestrial beings resembling modern humans. I show that none of the recent advances in the field of extremophile biology, alternative biochemistries, or recent allusions to apparent defects in the fitness of nature for Terran life significantly undermine the core argument, that nature is peculiarly fit for carbon-based Terran life, and especially for the physiology of complex terrestrial beings resembling modern humans.
Ariel: A Review of International English Literature, 2002
"Esrth, l;ife, space: the social construction of the biosphere and its expansion into the solar system, and beyond, 2020
Earth, life, space: the social construction of the biosphere and its expansion into the solar system, and beyond This chapter will explore whether and how the scientific search for evidence of extraterrestrial life, in the solar system and beyond, has affected our conception of the terrestrial biosphere – and vice versa – and extended the idea of “biosphere” into outer space. From my biased perspective, as a long-time member of the astrobiology community, I’m convinced that, of course, the search for life elsewhere has affected the way we think about our home planet. This essay will consider the ways in which this has occurred. While it will not ignore the contributions of space-based Earth observations and human space flight to a change in conceptions of our biosphere, it will focus on the contributions of exobiology and astrobiology, focusing on the search for extraterrestrial life and, to some extent, the search for potentially habitable extrasolar planets (exoplanets).
Journal of Evolutionary Biology, 1993
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