Terraforming Mars the Role of Pioneer Organisms and the Possibility of a Biologically Driven Nitrogen Cycle
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The Terminal Oxidases of Paracoccus Denitrificans Gier, Jan-Willem L
University of Groningen The terminal oxidases of Paracoccus denitrificans Gier, Jan-Willem L. de; Lübben, Mathias; Reijnders, Willem N.M.; Tipker, Corinne A.; Slotboom, Dirk-Jan; Spanning, Rob J.M. van; Stouthamer, Adriaan H.; Oost, John van der Published in: Molecular Microbiology IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 1994 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Gier, J-W. L. D., Lübben, M., Reijnders, W. N. M., Tipker, C. A., Slotboom, D-J., Spanning, R. J. M. V., Stouthamer, A. H., & Oost, J. V. D. (1994). The terminal oxidases of Paracoccus denitrificans. Molecular Microbiology, 13(2), 183-196. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). The publication may also be distributed here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne” license. More information can be found on the University of Groningen website: https://www.rug.nl/library/open-access/self-archiving-pure/taverne- amendment. Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. -
A Theory of Mars Introduction Over the Last 10 Years Or So I Have Been
A Theory of Mars Introduction Over the last 10 years or so I have been researching the idea there might be alien artifacts on Mars. Over this time there have been many interesting discoveries by myself and others, and some candidate artifacts have been found to be likely natural. So far proof remains elusive but some evidence has grown stronger. As more and more of these candidate artifacts have been found, similarities have begun to emerge, pointing at a more plausible theory for their origin. So in this paper I am explaining this theory, with the caveat that nothing is proven at this stage. If more candidate artifacts are found and they also support this theory then this will be additional evidence for artificiality. The reason is formations of randomly appearing similar to artifacts should also randomly seem to fit in with many different contradictory theories. To explain this theory I will need to start at the beginning of this story, which is likely to be at least several hundred million years and possibly over a billion years ago. So these artifacts, if they exist at all, are likely to be incredibly old and only have survived because erosion on Mars is very small. The main reason for this is the near vacuum on Mars prevents most erosion because most of the atmosphere is frozen at the poles. This subject then is far removed from such things as UFOs or Von Daniken like theories of extra terrestrials visiting us today. By contrast any evidence of visitation from so long ago is likely to be archeological with little more than ruins to be found. -
Methane Production on Rock and Soil Substrates by Methanogens: Implications for Life on Mars
Bioastronomy 2007: Molecules, Microbes, and Extraterrestrial Life ASP Conference Series, Vol. 420, 2009 K. J. Meech, J. V. Keane, M. J. Mumma, J. L. Siefert, and D. J. Werthimer, eds. Methane Production on Rock and Soil Substrates by Methanogens: Implications for Life on Mars H. A. Kozup and T. A. Kral 1West Virginia University, WV 26505 2Arkansas Center for Space and Planetary Sciences, University of Arkansas, Fayetteville 72701 Abstract. In order to understand the methanogens as models for possible life on Mars, and some of the factors likely to be important in determining their abundance and distribution, we have measured their ability to produce methane on a few types of inorganic rock and soil substrates. Since organic ma- terials have not been detected in measurable quantities at the surface of Mars, there is no reason to believe that they would exist in the subsurface. Samples of three methanogens (Methanosarcina barkeri, Methanobacterium formicicum, and Methanothermobacter wolfeii) were placed on four substrates (sand, gravel, basalt, and a Mars soil simulant, JSC Mars-1) and methane production mea- sured. Glass beads were used as a control substrate. As in earlier experiments with JSC Mars-1 soil simulant, a crushed volcanic tephra, methane was pro- duced by all three methanogens when placed on the substrates, sand and gravel. None produced methane on basalt in these experiments, a mineral common in Martian soil. While these substrates do not represent the full range of materials likely to be present on the surface of Mars, the present results suggest that while some surface materials on Mars may not support this type of organism, others might. -
The Mystery of Methane on Mars and Titan
The Mystery of Methane on Mars & Titan By Sushil K. Atreya MARS has long been thought of as a possible abode of life. The discovery of methane in its atmosphere has rekindled those visions. The visible face of Mars looks nearly static, apart from a few wispy clouds (white). But the methane hints at a beehive of biological or geochemical activity underground. Of all the planets in the solar system other than Earth, own way, revealing either that we are not alone in the universe Mars has arguably the greatest potential for life, either extinct or that both Mars and Titan harbor large underground bodies or extant. It resembles Earth in so many ways: its formation of water together with unexpected levels of geochemical activ- process, its early climate history, its reservoirs of water, its vol- ity. Understanding the origin and fate of methane on these bod- canoes and other geologic processes. Microorganisms would fit ies will provide crucial clues to the processes that shape the right in. Another planetary body, Saturn’s largest moon Titan, formation, evolution and habitability of terrestrial worlds in also routinely comes up in discussions of extraterrestrial biology. this solar system and possibly in others. In its primordial past, Titan possessed conditions conducive to Methane (CH4) is abundant on the giant planets—Jupiter, the formation of molecular precursors of life, and some scientists Saturn, Uranus and Neptune—where it was the product of chem- believe it may have been alive then and might even be alive now. ical processing of primordial solar nebula material. On Earth, To add intrigue to these possibilities, astronomers studying though, methane is special. -
Histone Variants in Archaea and the Evolution of Combinatorial Chromatin Complexity
Histone variants in archaea and the evolution of combinatorial chromatin complexity Kathryn M. Stevensa,b, Jacob B. Swadlinga,b, Antoine Hochera,b, Corinna Bangc,d, Simonetta Gribaldoe, Ruth A. Schmitzc, and Tobias Warneckea,b,1 aMolecular Systems Group, Quantitative Biology Section, Medical Research Council London Institute of Medical Sciences, London W12 0NN, United Kingdom; bInstitute of Clinical Sciences, Faculty of Medicine, Imperial College London, London W12 0NN, United Kingdom; cInstitute for General Microbiology, University of Kiel, 24118 Kiel, Germany; dInstitute of Clinical Molecular Biology, University of Kiel, 24105 Kiel, Germany; and eDepartment of Microbiology, Unit “Evolutionary Biology of the Microbial Cell,” Institut Pasteur, 75015 Paris, France Edited by W. Ford Doolittle, Dalhousie University, Halifax, NS, Canada, and approved October 28, 2020 (received for review April 14, 2020) Nucleosomes in eukaryotes act as platforms for the dynamic inte- additional histone dimers can be taggedontothistetramertoyield gration of epigenetic information. Posttranslational modifications oligomers of increasing length that wrap correspondingly more DNA are reversibly added or removed and core histones exchanged for (3, 6–9). Almost all archaeal histones lack tails and PTMs have yet to paralogous variants, in concert with changing demands on tran- be reported. Many archaea do, however, encode multiple histone scription and genome accessibility. Histones are also common in paralogs (8, 10) that can flexibly homo- and heterodimerize in -
An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger Depauw University
DePauw University Scholarly and Creative Work from DePauw University Student research Student Work 2015 An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger DePauw University Follow this and additional works at: http://scholarship.depauw.edu/studentresearch Part of the Economics Commons, and the The unS and the Solar System Commons Recommended Citation Knappenberger, Clayton, "An Economic Analysis of Mars Exploration and Colonization" (2015). Student research. Paper 28. This Thesis is brought to you for free and open access by the Student Work at Scholarly and Creative Work from DePauw University. It has been accepted for inclusion in Student research by an authorized administrator of Scholarly and Creative Work from DePauw University. For more information, please contact [email protected]. An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger 2015 Sponsored by: Dr. Villinski Committee: Dr. Barreto and Dr. Brown Contents I. Why colonize Mars? ............................................................................................................................ 2 II. Can We Colonize Mars? .................................................................................................................... 11 III. What would it look like? ............................................................................................................... 16 A. National Program ......................................................................................................................... -
Life-Centered Ethics and the Human Future in Space Michael Noah Mautner Virginia Commonwealth University, [email protected]
Virginia Commonwealth University VCU Scholars Compass Chemistry Publications Dept. of Chemistry 2009 Life-Centered Ethics and the Human Future in Space Michael Noah Mautner Virginia Commonwealth University, [email protected] Follow this and additional works at: http://scholarscompass.vcu.edu/chem_pubs Part of the Biology Commons, Ecology and Evolutionary Biology Commons, and the Social and Behavioral Sciences Commons © 2008 The Author. Journal compilation © 2008 Blackwell Publishing Ltd. Downloaded from http://scholarscompass.vcu.edu/chem_pubs/77 This Article is brought to you for free and open access by the Dept. of Chemistry at VCU Scholars Compass. It has been accepted for inclusion in Chemistry Publications by an authorized administrator of VCU Scholars Compass. For more information, please contact [email protected]. Bioethics ISSN 0269-9702 (print); 1467-8519 (online) doi:10.1111/j.1467-8519.2008.00688.x Volume 23 Number 8 2009 pp 433–440 ARTICLES LIFE-CENTERED ETHICS, AND THE HUMAN FUTURE IN SPACE MICHAEL N. MAUTNER Keywords bioethics, ABSTRACT life-centered ethics, In the future, human destiny may depend on our ethics. In particular, biotic ethics, biotechnology and expansion in space can transform life, raising profound panbiotic ethics, questions. Guidance may be found in Life-centered ethics, as biotic ethics genetic engineering, that value the basic patterns of organic gene/protein life, and as panbiotic biophilia, ethics that always seek to expand life. These life-centered principles can be life in space, based on scientific insights into the unique place of life in nature, and the astroethics biological unity of all life. Belonging to life then implies a human purpose: to safeguard and propagate life. -
Environmental Philosophy and the Ethics of Terraforming Mars
ENVIRONMENTAL PHILOSOPHY AND THE ETHICS OF TERRAFORMING MARS: ADDING THE VOICES OF ENVIRONMENTAL JUSTICE AND ECOFEMINISM TO THE ONGOING DEBATE Robert Heath French Thesis Prepared for the Degree of MASTER OF ARTS UNIVERSITY OF NORTH TEXAS August 2013 APPROVED: Robert Figueroa, Committee Chair Eugene Hargrove, Committee Member Adam Briggle, Committee Member Patricia Glazebrook, Chair of the Department of Philosophy and Religion Studies Mark Wardell, Dean of the Toulouse Graduate School French, Robert Heath. Environmental Philosophy and the Ethics of Terraforming Mars: Adding the Voices of Environmental Justice and Ecofeminism to the Ongoing Debate. Master of Arts (Philosophy), August 2013, 133 pp., 1 table, bibliography, 78 titles. Questions concerning the ethics of terraforming Mars have received some attention from both philosophers and scientists during recent decades. A variety of theoretical approaches have been supplied by a number of authors, however research pursuant to this thesis has indicated at least two major blindspots in the published literature on the topic. First, a broad category of human considerations involving risks, dangers, and social, political, and economic inequalities that would likely be associated with efforts to terraform Mars have been woefully overlooked in the published literature to date. I attempt to rectify that oversight by employing the interpretive lens of environmental justice to address questions of environmental colonialism, equality in terms of political participation and inclusion in decision making structures, risks associated with technological progressivism, and responses to anthropogenic climate change. Only by including the historically marginalized and politically disenfranchised “voices,” of both humans and nonhumans, can any future plan to terraform Mars be deemed ethical, moral or just according to the framework provided by environmental justice. -
APP201895 APP201895__Appli
APPLICATION FORM DETERMINATION Determine if an organism is a new organism under the Hazardous Substances and New Organisms Act 1996 Send by post to: Environmental Protection Authority, Private Bag 63002, Wellington 6140 OR email to: [email protected] Application number APP201895 Applicant Neil Pritchard Key contact NPN Ltd www.epa.govt.nz 2 Application to determine if an organism is a new organism Important This application form is used to determine if an organism is a new organism. If you need help to complete this form, please look at our website (www.epa.govt.nz) or email us at [email protected]. This application form will be made publicly available so any confidential information must be collated in a separate labelled appendix. The fee for this application can be found on our website at www.epa.govt.nz. This form was approved on 1 May 2012. May 2012 EPA0159 3 Application to determine if an organism is a new organism 1. Information about the new organism What is the name of the new organism? Briefly describe the biology of the organism. Is it a genetically modified organism? Pseudomonas monteilii Kingdom: Bacteria Phylum: Proteobacteria Class: Gamma Proteobacteria Order: Pseudomonadales Family: Pseudomonadaceae Genus: Pseudomonas Species: Pseudomonas monteilii Elomari et al., 1997 Binomial name: Pseudomonas monteilii Elomari et al., 1997. Pseudomonas monteilii is a Gram-negative, rod- shaped, motile bacterium isolated from human bronchial aspirate (Elomari et al 1997). They are incapable of liquefing gelatin. They grow at 10°C but not at 41°C, produce fluorescent pigments, catalase, and cytochrome oxidase, and possesse the arginine dihydrolase system. -
What Would Happen to Our Globes on the Globe of Mars?
FEATURE Globes in space: What would happen to our globes on the globe of Mars? BY KATHERINE MCVEIGH AND TOMAS BURKE Many films have been made regarding life on alternative planets. With the Mars One mission approaching in 2023, there are high expectations regarding future interplanetary travel. The authors provide an ophthalmology perspective on what could happen to our eyes if exposed to the atmosphere of Mars. n 1990, Arnold Schwarzenegger starred in Total Recall [1], a film where he finds himself on Mars. Damage to his Ispacesuit and subsequent exposure to the environment on Mars results in excessive bodily swelling, along with extensive proptosis whereby the globes extend anteriorly beyond the eyelids as his optic nerves are undoubtedly stretched to their maximal capacity. From an ophthalmological perspective, the interpretation of the impact of atmospheric exposure is intriguing. With the anticipated Mars One mission launch in 2023 aiming to establish a habitable settlement in a hostile environment, we ask if what happened is an accurate depiction of what could be expected to happen to us and our ophthalmic globes on that other globe? The atmosphere on Mars has an O2 level of 0.13% and CO2 level of 95%, and is very Armstrong limit, meaning that exposure to thin, approximately 1% of that on Earth at Tense oedematous soft tissue swelling of sea level [2]. This is believed to be a result the environment would result in a prompt the lids will then make it challenging to of the loss of the magnetosphere four and severe dehydration from the mucosal open the lids. -
TIME Space Newsletter September 10, 2019
TIME Space Newsletter September 10, 2019 Dear readers, Not a lot of people would want to go back to the Paleocene Epoch. For one thing, the dinosaurs were only beginning to die out, and while they'd be nifty to see, they were murder on mammals. It would be a good 65 million years before humans got a literal toe-hold on the world. The Eocene wouldn't be much better. It was around that time that what is now the Indian subcontinent crashed into Asia, and while all that produced some lovely mountains, there was a lot of slo-mo violence of clashing plates before things settled down. As far as epochs go, the Holocene is everyone's favorite. It started close to 12,000 years ago, as the last Ice Age was ending, and produced the conditions that allowed all the species we love best—ourselves, and charismatic megafauna like the bald eagle, the panda and the tiger—to thrive. From humanity's perspective, it would be perfectly fine if the Holocene went on forever. But it won't. It's ending now—it may have already ended in the 1950s, according to some scientists—to be replaced by the Anthropocene. The name says it all: it's an epoch in which one species—ours, anthro—became the leading driver of the state of the planet, more powerful, at least in the short-term, than the larger forces of geology, meteorology, even biology. We have, of course, abused that power, fouling the air, annihilating species, wiping out forests and distorting the climate. -
Methanobacterium Paludis Sp. Nov. and a Novel Strain of Methanobacterium Lacus Isolated from Northern Peatlands
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by The University of North Carolina at Greensboro Archived version from NCDOCKS Institutional Repository http://libres.uncg.edu/ir/asu/ Methanobacterium Paludis Sp. Nov. And A Novel Strain Of Methanobacterium Lacus Isolated From Northern Peatlands By: Suzanna L. Brauer, Hinsby Cadillo-Quiroz, Noah Goodson, Joseph B. Yavitt & Stephen H. Zinder Abstract Two mesophilic, hydrogenotrophic methanogens, designated strains SWAN1T and AL-21, were isolated from two contrasting peatlands: a near circumneutral temperate minerotrophic fen in New York State, USA, and an acidic boreal poor fen site in Alaska, USA, respectively. Cells of the two strains were rod-shaped, non- motile, stained Gram-negative and resisted lysis with 0.1 % SDS. Cell size was 0.6 1.5–2.8 mm for strain SWAN1T and 0.45–0.85 1.5–35 mm for strain AL-21. The strains used H2/CO2 but not formate or other substrates for methanogenesis, grew optimally around 32–37 6C, and their growth spanned through a slightly low to neutral pH range (4.7–7.1). Strain AL-21 grew optimally closer to neutrality at pH 6.2, whereas strain SWAN1T showed a lower optimal pH at 5.4–5.7. The two strains were sensitive to NaCl with a maximal tolerance at 160 mM for strain SWAN1T and 50 mM for strain AL-21. Na2S was toxic at very low concentrations (0.01–0.8 mM), resulting in growth inhibition above these values. The DNA G+C content of the genomes was 35.7 mol% for strain SWAN1T and 35.8 mol% for strain AL-21.