ASTROBIOLOGY: the Study of the Living Universe
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Building Blocks That Fall from the Sky
Building blocks that fall from the sky How did life on Earth begin? Scientists from the “Heidelberg Initiative for the Origin of Life” have set about answering this truly existential question. Indeed, they are going one step further and examining the conditions under which life can emerge. The initiative was founded by Thomas Henning, Director at the Max Planck Institute for Astronomy in Heidelberg, and brings together researchers from chemistry, physics and the geological and biological sciences. 18 MaxPlanckResearch 3 | 18 FOCUS_The Origin of Life TEXT THOMAS BUEHRKE he great questions of our exis- However, recent developments are The initiative was triggered by the dis- tence are the ones that fasci- forcing researchers to break down this covery of an ever greater number of nate us the most: how did the specialization and combine different rocky planets orbiting around stars oth- universe evolve, and how did disciplines. “That’s what we’re trying er than the Sun. “We now know that Earth form and life begin? to do with the Heidelberg Initiative terrestrial planets of this kind are more DoesT life exist anywhere else, or are we for the Origins of Life, which was commonplace than the Jupiter-like gas alone in the vastness of space? By ap- founded three years ago,” says Thom- giants we identified initially,” says Hen- proaching these puzzles from various as Henning. HIFOL, as the initiative’s ning. Accordingly, our Milky Way alone angles, scientists can answer different as- name is abbreviated, not only incor- is home to billions of rocky planets, pects of this question. -
Prebiological Evolution and the Metabolic Origins of Life
Prebiological Evolution and the Andrew J. Pratt* Metabolic Origins of Life University of Canterbury Keywords Abiogenesis, origin of life, metabolism, hydrothermal, iron Abstract The chemoton model of cells posits three subsystems: metabolism, compartmentalization, and information. A specific model for the prebiological evolution of a reproducing system with rudimentary versions of these three interdependent subsystems is presented. This is based on the initial emergence and reproduction of autocatalytic networks in hydrothermal microcompartments containing iron sulfide. The driving force for life was catalysis of the dissipation of the intrinsic redox gradient of the planet. The codependence of life on iron and phosphate provides chemical constraints on the ordering of prebiological evolution. The initial protometabolism was based on positive feedback loops associated with in situ carbon fixation in which the initial protometabolites modified the catalytic capacity and mobility of metal-based catalysts, especially iron-sulfur centers. A number of selection mechanisms, including catalytic efficiency and specificity, hydrolytic stability, and selective solubilization, are proposed as key determinants for autocatalytic reproduction exploited in protometabolic evolution. This evolutionary process led from autocatalytic networks within preexisting compartments to discrete, reproducing, mobile vesicular protocells with the capacity to use soluble sugar phosphates and hence the opportunity to develop nucleic acids. Fidelity of information transfer in the reproduction of these increasingly complex autocatalytic networks is a key selection pressure in prebiological evolution that eventually leads to the selection of nucleic acids as a digital information subsystem and hence the emergence of fully functional chemotons capable of Darwinian evolution. 1 Introduction: Chemoton Subsystems and Evolutionary Pathways Living cells are autocatalytic entities that harness redox energy via the selective catalysis of biochemical transformations. -
The 29Th Annual Meeting the 29Th Annual Meeting of the Society Took Place on April 17Th, 2016 Program and Abstracts Program
The 29th annual meeting The 29th annual meeting of the society took place on April 17th, 2016 Program and Abstracts Program: Program of the 29th annual meeting Time Lecturer Lecture Title 8:45- Refreshments & Gathering 9:05 Session 1 -Astrobiology (Doron Lancet, Chair; Amri Wandel, Organizer) 9:05- Gonen Ashkenasy Opening Remarks 9:15 (BGU) 9:15- Ravit Helled Methane-Rich Planets and the Characterization of Exoplanets 9:45 (TAU) 9:45- Sohan Jheeta (NoR Formation of Glycolaldehyde (HOCH2CHO) from Pure 10:10 HGT, LUCA) Methanol in Astrophysical Ice Analogues 10:10- Joseph Is Liquid Water Essential for Life? A Reassessment 10:35 Gale (HUJI) 10:35- Coffee break 11:00 Session 2 - Evolution (Addy Pross, Chair) 11:00- Robert Pascal Identifying the Kinetic, Thermodynamic and Chemical 11:40 (CNRS Conditions for Stability and Complexity in Living Systems Montpellier) 11:40- Omer Markovitch Predicting Proto-Species Emergence in Complex Networks 12:05 (Newcastle) 12:05- Amir Aharoni Engineering a Species Barrier in Yeast 12:30 (BGU) 12:30- Jayanta Nanda Spontaneous Evolution of β-Sheet Forming Self Replicating 12:55 (BGU) Peptides 12:55- Lunch 14:05 Session 3 - Origins of Order and Complexity (Gonen Ashkenasy, Chair; Tal Mor, Organizer) 14:05- Prof. Zvi HaCohen, Greetings 14:15 Rector (BGU) 14:15- Doron Composomics: a Common Biotic Thread 14:45 Lancet (WIS) 14:45- Avshalom Elitzur Living State Physics: Does Life's Uniqueness Elude Scientific 15:10 (IYAR) Definition? 15:10- Tal Mor Origins of Translation: Speculations about the First and the 15:35 -
The Ethics of Terraforming and Areoforming in an Age of Climate Change
Engineering Planets, Engineering Ourselves: The Ethics of Terraforming and Areoforming in an Age of Climate Change Patrick D. Murphy (University of Central Florida)1 Abstract The concept of terraforming, the engineered transformation of alien planets into habitats suitable for human settlement, has taken on new meaning in science fiction and contemporary culture as climate change has indicated that human beings are currently transforming this planet but without a clear plan for sustaining inhabitability. Literary depictions by Kim Stanley Robinson of both climate change and terraforming raise ethical questions about the engineering of this and other planets, while the science fiction novels of Joan Slonczewski raise ethical questions about engineering human beings to adapt to alien environments. Together, they provide ways of thinking about the intertwined ethical questions of engineering the biosphere and engineering the species in the context of human and environmental sustainability. In particular, some works, such as the novels of Karen Traviss, raise the issue of how much the human species might have to engineer itself to pay the price of its unplanned engineering of planet Earth. Nearly twenty years ago Bill McKibben claimed that "we are at the end of nature" (8). In support of this seemingly hyperbolic statement, he referred to a 1957 scientific paper which claimed that "Human beings are now carrying out a large scale geophysical experiment" (qtd. in McKibben 10), by pumping rapidly increasing amounts of carbon dioxide into the atmosphere. 1 Patrick Murphy, Department of English, University of Central Florida, Building: CNH301 P.O. Box 161346 Orlando, FL 32816-1346 [email protected] 54 Many people, myself included, thought McKibben had gone over the top. -
The War of the Worlds Postcolonialism, Americanism, and Terrorism in Modern Science Fiction Film
Durkstra 4167430 | 1 The War of the Worlds Postcolonialism, Americanism, and Terrorism in Modern Science Fiction Film Sytse Durkstra English Language and Culture Supervisor | Chris Louttit Sytse Durkstra | s4167430 | Email [email protected] Durkstra 4167430 | 2 ENGLISH LANGUAGE AND CULTURE Teacher who will receive this document: Chris Louttit Title of document: The War of the Worlds: Postcolonialism, Americanism, and Terrorism in Modern Science Fiction Film Name of course: BA Thesis English Language and Culture Date of submission: 15 June 2015 The work submitted here is the sole responsibility of the undersigned, who has neither committed plagiarism nor colluded in its production. Signed Name of student: Sytse Durkstra Student number: 4167430 Durkstra 4167430 | 3 And this Thing I saw! How can I describe it? A monstrous tripod, higher than many houses, striding over the young pine trees, and smashing them aside in its career; a walking engine of glittering metal, reeling now across the heather, articulate ropes of steel dangling from it, and the clattering tumult of its passage mingling with the riot of the thunder. A flash, and it came out vividly, heeling over one way with two feet in the air, to vanish and reappear almost instantly, as it seemed with the next flash, a hundred yards nearer. - H.G. Wells, The War of the Worlds But who shall dwell in these worlds if they be inhabited? . Are we or they Lords of the World? . And how are all things made for man? - Kepler In our obsession with antagonisms of the moment, we often forget how much unites all the members of humanity. -
The Past Decade and the Future of Cosmology and Astrophysics
Towards a New Enlightenment? A Transcendent Decade The Past Decade and the Future of Cosmology and Astrophysics Martin Rees Martin Rees is a cosmologist and space scientist. After studying at Cambridge University, he held various posts in the UK and elsewhere, before returning to Cambridge, where he has been a professor, Head of the Institute of Astronomy, and Master of Trinity College. He has contributed to our understanding of galaxy formation, black holes, high-energy phenomena in the cosmos, and the concept of the multiverse. He has received substantial international recognition for his research. He has been much involved in science-related policy, being a member of the UK’s House of Lords and (during 2005–10) President of the Royal Society, the independent scientific academy of the UK Martin Rees and the Commonwealth. Apart from his research publications, he writes and University of Cambridge lectures widely for general audiences, and is the author of eight books, the most recent being On the Future (2018). Recommended books: Universe, Martin Rees, Dorling Kindersley, 2012; On the Future, Martin Rees, Princeton University Press, 2018. In the last decade, there has been dramatic progress in exploring the cosmos. Highlights include close-up studies of the planets and moons of our Solar System; and (even more dramatic) the realization that most stars are orbited by planets, and that there may be millions of Earth-like planets in our Galaxy. On a still larger scale, we have achieved a better understanding of how galaxies have developed, over 13.8 billion years of cosmic history, from primordial fluctuations. -
Westminsterresearch the Astrobiology Primer V2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., De La Rubia Leigh, A., Bond
WestminsterResearch http://www.westminster.ac.uk/westminsterresearch The Astrobiology Primer v2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., de la Rubia Leigh, A., Bond, J., Dartnell, L., Goldman, A.D., Lynch, K., Naud, M.-E., Paulino-Lima, I.G., Kelsi, S., Walter-Antonio, M., Abrevaya, X.C., Anderson, R., Arney, G., Atri, D., Azúa-Bustos, A., Bowman, J.S., Brazelton, W.J., Brennecka, G.A., Carns, R., Chopra, A., Colangelo-Lillis, J., Crockett, C.J., DeMarines, J., Frank, E.A., Frantz, C., de la Fuente, E., Galante, D., Glass, J., Gleeson, D., Glein, C.R., Goldblatt, C., Horak, R., Horodyskyj, L., Kaçar, B., Kereszturi, A., Knowles, E., Mayeur, P., McGlynn, S., Miguel, Y., Montgomery, M., Neish, C., Noack, L., Rugheimer, S., Stüeken, E.E., Tamez-Hidalgo, P., Walker, S.I. and Wong, T. This is a copy of the final version of an article published in Astrobiology. August 2016, 16(8): 561-653. doi:10.1089/ast.2015.1460. It is available from the publisher at: https://doi.org/10.1089/ast.2015.1460 © Shawn D. Domagal-Goldman and Katherine E. Wright, et al., 2016; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by- nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited. The WestminsterResearch online digital archive at the University of Westminster aims to make the research output of the University available to a wider audience. -
God and Design: the Teleological Argument and Modern Science
GOD AND DESIGN Is there reason to think a supernatural designer made our world? Recent discoveries in physics, cosmology, and biochemistry have captured the public imagination and made the design argument—the theory that God created the world according to a specific plan—the object of renewed scientific and philosophical interest. Terms such as “cosmic fine-tuning,” the “anthropic principle,” and “irreducible complexity” have seeped into public consciousness, increasingly appearing within discussion about the existence and nature of God. This accessible and serious introduction to the design problem brings together both sympathetic and critical new perspectives from prominent scientists and philosophers including Paul Davies, Richard Swinburne, Sir Martin Rees, Michael Behe, Elliott Sober, and Peter van Inwagen. Questions raised include: • What is the logical structure of the design argument? • How can intelligent design be detected in the Universe? • What evidence is there for the claim that the Universe is divinely fine-tuned for life? • Does the possible existence of other universes refute the design argument? • Is evolutionary theory compatible with the belief that God designed the world? God and Design probes the relationship between modern science and religious belief, considering their points of conflict and their many points of similarity. Is God the “master clockmaker” who sets the world’s mechanism on a perfectly enduring course, or a miraculous presence continually intervening in and altering the world we know? Are science and faith, or evolution and creation, really in conflict at all? Expanding the parameters of a lively and urgent contemporary debate, God and Design considers the ways in which perennial questions of origin continue to fascinate and disturb us. -
Monday, November 13, 2017 WHAT DOES IT MEAN to BE HABITABLE? 8:15 A.M. MHRGC Salons ABCD 8:15 A.M. Jang-Condell H. * Welcome C
Monday, November 13, 2017 WHAT DOES IT MEAN TO BE HABITABLE? 8:15 a.m. MHRGC Salons ABCD 8:15 a.m. Jang-Condell H. * Welcome Chair: Stephen Kane 8:30 a.m. Forget F. * Turbet M. Selsis F. Leconte J. Definition and Characterization of the Habitable Zone [#4057] We review the concept of habitable zone (HZ), why it is useful, and how to characterize it. The HZ could be nicknamed the “Hunting Zone” because its primary objective is now to help astronomers plan observations. This has interesting consequences. 9:00 a.m. Rushby A. J. Johnson M. Mills B. J. W. Watson A. J. Claire M. W. Long Term Planetary Habitability and the Carbonate-Silicate Cycle [#4026] We develop a coupled carbonate-silicate and stellar evolution model to investigate the effect of planet size on the operation of the long-term carbon cycle, and determine that larger planets are generally warmer for a given incident flux. 9:20 a.m. Dong C. F. * Huang Z. G. Jin M. Lingam M. Ma Y. J. Toth G. van der Holst B. Airapetian V. Cohen O. Gombosi T. Are “Habitable” Exoplanets Really Habitable? A Perspective from Atmospheric Loss [#4021] We will discuss the impact of exoplanetary space weather on the climate and habitability, which offers fresh insights concerning the habitability of exoplanets, especially those orbiting M-dwarfs, such as Proxima b and the TRAPPIST-1 system. 9:40 a.m. Fisher T. M. * Walker S. I. Desch S. J. Hartnett H. E. Glaser S. Limitations of Primary Productivity on “Aqua Planets:” Implications for Detectability [#4109] While ocean-covered planets have been considered a strong candidate for the search for life, the lack of surface weathering may lead to phosphorus scarcity and low primary productivity, making aqua planet biospheres difficult to detect. -
Does the Rapid Appearance of Life on Earth Suggest That Life Is Common in the Universe?
ASTROBIOLOGY Volume 2, Number 3, 2002 © Mary Ann Liebert, Inc. Does the Rapid Appearance of Life on Earth Suggest that Life Is Common in the Universe? CHARLES H. LINEWEAVER 1,2 and TAMARA M. DAVIS 1 ABSTRACT It is sometimes assumed that the rapidity of biogenesis on Earth suggests that life is common in the Universe. Here we critically examine the assumptions inherent in this if-life-evolved- rapidly-life-must-be-common argument. We use the observational constraints on the rapid- ity of biogenesis on Earth to infer the probability of biogenesis on terrestrial planets with the same unknown probability of biogenesis as the Earth. We find that on such planets, older than ,1 Gyr, the probability of biogenesis is .13% at the 95% confidence level. This quan- tifies an important term in the Drake Equation but does not necessarily mean that life is com- mon in the Universe. Key Words: Biogenesis—Drake Equation. Astrobiology 2, 293–304. THE BIOGENESIS LOTTERY duction–oxidation pairs are common (Nealson and Conrad, 1999). UCHOFCURRENTASTROBIOLOGICALRESEARCH Mis focused on learning more about the early It is difficult to translate this circumstantial ev- evolution of the Earth and about the origin of life. idence into an estimate of how common life is in We may be able to extrapolate and generalize our the Universe. Without definitive detections of ex- knowledge of how life formed here to how it traterrestrial life we can say very little about how might have formed elsewhere. Indirect evidence common it is or even whether it exists. Our exis- suggesting that life may be common in the Uni- tence on Earth can tell us little about how com- verse includes: mon life is in the Universe or about the proba- bility of biogenesis on a terrestrial planet because, Sun-like stars are common. -
The Drake Equation the Drake Equation, Which We Encountered in the Very First Lecture of This Class, Is a Way to Take the Questi
The Drake Equation The Drake equation, which we encountered in the very first lecture of this class, is a way to take the question “How many communicative civilizations are there currently in our galaxy?” and break it into several factors that we estimate as best we can. In this class we will go into detail about this equation. We will find that we now have a decent idea of the values of a couple of the factors, but that many are still guesswork. We’ll do our best to make our guesses informed. We will also discover that some people have reformulated the equation by adding a number of other factors they consider crucial to having technologically adept life. The remarkable and subtle effect of this is that, depending on how many factors you think appropriate, you can get the conclusions you want while appearing reasonable and conservative throughout. That is, if you think many civilizations exist, you can use the Drake equation to demonstrate this. If you think we are the only ones, you can get the equation to say that as well. With this in mind, we should approach the Drake equation as a way of framing our discussion as opposed to as a method of determining the answer rigorously. The equation itself and its factors The original form of the equation was written by Frank Drake in 1960 in preparation for a meeting in Green Bank, West Virginia. It says: ∗ N = R × fp × ne × fl × fi × fc × L . (1) Here: • N is the number of currently active, communicative civilizations in our galaxy. -
Fermi's Paradox Is a Daunting Problem – Under Whatever Label
Fermi's Paradox Is a Daunting Problem – Under Whatever Label Milan M. Dirkovid1 Astronomical Observatory of Belgrade, Volgina 7, 11000 Belgrade, Serbia 1. Introduction Gray (2015) argued that Fermi's paradox (FP) is a misnomer, and it is not a valid paradox. Gray also speculated that the argument was misattributed to Fermi, whose lunchtime remarks did not pertain to the existence of extraterrestrial intelligence, but to the feasibility of interstellar travel. Instead, the paradox is ascribed to Hart and Tipler, and it is further suggested that the paradox is not a “real” problem or research subject and should not be used in debates about SETI projects. The arguments given are unpersuasive, ahistorical, and, in at least one instance, clearly hinge on literalistic and uncharitable reading of evidence. Instead, I argue the following three points: (i) Contrary to Gray’s assertion, the historical issue of naming of ideas or concepts is completely divorced from their epistemic status. (ii) FP is easily and smoothly generalized into the “Great Silence” paradox, so it makes no sense either theoretically or empirically to separate the two. (iii) In sharp contrast to the main implication of Gray’s paper, FP has become more aggravated lately due to advances in astrobiology. Research that deals with FP has greatly expanded in recent years on both a theoretical and observational stage (Davies 2010, 2012; Vukotid and Dirkovid 2012; Barlow 2013; Hair and Hedman 2013; Davies and Wagner 2013; Armstrong and Sandberg 2013; Lampton 2013; Cartin 2014; Nunn, Guy, and Bell 2014; Wright et al. 2014; Spivey 2015; Griffith et al.