Cosmology and Ecology
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A Rapid, Low-Cost Approach to Permanently Extend Life Beyond Earth
A Rapid, Low-Cost Approach to Permanently Extend Life Beyond Earth Gregory A. Dorais, Ph.D. [email protected] Autonomous Systems & Robotics Research Scientist Intelligent Systems Division NASA Ames Research Center 11/16/2018 Outline • The value proposition for permanently extending life beyond Earth • Closed ecosystems • An approach to study sustainable, closed ecosystems • The problem of long-term life in space • A mission design concept to study long-term life in space • Next steps 2 Notable Cassini Image 7/19/2013 Cassini Spacecraft: Launched 1997, Saturn orbit insertion 2004, and impacted Saturn 2017. 3 Location of All Known Life in the Universe Pale Blue Dot 4 Location of All Known Life in the Universe Pale Blue Assertion: Earth is a multigenome seedpod. Dot Big question: Will it germinate or die? Fundamental questions of space biology: • What happens to life from Earth, beyond Earth? • Can a self-sufficient biome persist beyond Earth? 5 Apollo 8: Earthrise December 24, 1968 Earth Biosphere Assertions: • It is the most sophisticated complex adaptive system known to exist in the entire universe. • It is extremely precious and should be treated as such. • It has persisted for over 4 billion years, but may now have reached a critical juncture in its development. The Value Proposition: • Distributing multiple, sustainable, small-scale reproductions of the Earth biosphere on and beyond Earth can help preserve it. This image is credited with stimulating environmental movements world-wide. 6 Wheel of Misfortune Really bad things have happened on Earth and can happen with little notice (at least 5 mass extinction events). -
A Study of John Leslie's Infinite Minds, a Philosophical Cosmology
Document généré le 1 oct. 2021 09:18 Laval théologique et philosophique Infinite Minds, Determinism & Evil A Study of John Leslie’s Infinite Minds, A Philosophical Cosmology Leslie Armour La question de Dieu Volume 58, numéro 3, octobre 2002 URI : https://id.erudit.org/iderudit/000634ar DOI : https://doi.org/10.7202/000634ar Aller au sommaire du numéro Éditeur(s) Faculté de philosophie, Université Laval Faculté de théologie et de sciences religieuses, Université Laval ISSN 0023-9054 (imprimé) 1703-8804 (numérique) Découvrir la revue Citer cette note Armour, L. (2002). Infinite Minds, Determinism & Evil: A Study of John Leslie’s Infinite Minds, A Philosophical Cosmology. Laval théologique et philosophique, 58(3), 597–603. https://doi.org/10.7202/000634ar Tous droits réservés © Laval théologique et philosophique, Université Laval, Ce document est protégé par la loi sur le droit d’auteur. L’utilisation des 2002 services d’Érudit (y compris la reproduction) est assujettie à sa politique d’utilisation que vous pouvez consulter en ligne. https://apropos.erudit.org/fr/usagers/politique-dutilisation/ Cet article est diffusé et préservé par Érudit. Érudit est un consortium interuniversitaire sans but lucratif composé de l’Université de Montréal, l’Université Laval et l’Université du Québec à Montréal. Il a pour mission la promotion et la valorisation de la recherche. https://www.erudit.org/fr/ Laval théologique et philosophique, 58, 3 (octobre 2002) : 597-603 ◆ note critique INFINITE MINDS, DETERMINISM & EVIL A STUDY OF JOHN LESLIE’S INFINITE MINDS, A PHILOSOPHICAL COSMOLOGY * Leslie Armour The Dominican College of Philosophy and Theology Ottawa ohn Leslie’s Infinite Minds is a refreshingly daring book. -
Science and Religion in the Face of the Environmental Crisis
Roger S. Gottlieb, ed., The Oxford Handbook of Religion and Ecology. New York and Oxford: Oxford University Press, 2006. Pages 376-397. CHAPTER 17 .................................................................................................. SCIENCE AND RELIGION IN THE FACE OF THE ENVIRONMENTAL CRISIS ..................................................................................................... HOLMES ROLSTON III BOTH science and religion are challenged by the environmental crisis, both to reevaluate the natural world and to reevaluate their dialogue with each other. Both are thrown into researching fundamental theory and practice in the face of an upheaval unprecedented in human history, indeed in planetary history. Life on Earth is in jeopardy owing to the behavior of one species, the only species that is either scientific or religious, the only species claiming privilege as the "wise spe- cies," Homo sapiens. Nature and the human relation to nature must be evaluated within cultures, classically by their religions, currently also by the sciences so eminent in Western culture. Ample numbers of theologians and ethicists have become persuaded that religion needs to pay more attention to ecology, and many ecologists recognize religious dimensions to caring for nature and to addressing the ecological crisis. Somewhat ironically, just when humans, with their increasing industry and technology, seemed further and further from nature, having more knowledge about natural processes and more power to manage them, just when humans were more and more rebuilding their environments, thinking perhaps to escape nature, the natural world has emerged as a focus of concern. Nature remains the milieu of 376 SCIENCE AND RELIGION 377 culture—so both science and religion have discovered. In a currently popular vocabulary, humans need to get themselves "naturalized." Using another meta- phor, nature is the "womb" of culture, but a womb that humans never entirely leave. -
Cosmos Carl Sagan - Free Pdf Download
[pdf] Cosmos Carl Sagan - free pdf download Cosmos Ebook Download, online free Cosmos, Read Cosmos Book Free, Cosmos Ebooks, Read Best Book Cosmos Online, Pdf Books Cosmos, PDF Cosmos Full Collection, Cosmos Free PDF Online, by Carl Sagan pdf Cosmos, Download Cosmos E-Books, Cosmos pdf read online, Download Online Cosmos Book, Read Best Book Online Cosmos, Download Cosmos Online Free, Read Cosmos Full Collection Carl Sagan, by Carl Sagan pdf Cosmos, Free Download Cosmos Books [E-BOOK] Cosmos Full eBook, PDF Download Cosmos Free Collection, PDF Cosmos Full Collection, Free Download Cosmos Ebooks Carl Sagan, CLICK FOR DOWNLOAD mobi, kindle, azw, epub Description: This is no exaggeration, but when you search for something new or the first time...well it has been there It even came as an absolute pleasure this way, right For some reason my personal favourite character Jack Sparrowhas become such melded with Captain America 2 - I had always wanted him before he was just about done making them....I finally found his identity that will never go away......but we get closer after months of being together during her final day at DC She loves everything she does--and if they ever meet again on their return voyage back home then only half amigos are possible once more..we have decided exactly what happens next which means goodbye by now. Enjoy Letm out your welcome here from The Wrap blog Catch-the-Wrap. Stay up to date while watching live DCGIRL This weeks episode takes our look at some of the craziest mysteries lurking along the way that will make its debut on Sunday Episode 1The Curse of Saint Louis I don't believe I'm going anywhere. -
Physical Cosmology Physics 6010, Fall 2017 Lam Hui
Physical Cosmology Physics 6010, Fall 2017 Lam Hui My coordinates. Pupin 902. Phone: 854-7241. Email: [email protected]. URL: http://www.astro.columbia.edu/∼lhui. Teaching assistant. Xinyu Li. Email: [email protected] Office hours. Wednesday 2:30 { 3:30 pm, or by appointment. Class Meeting Time/Place. Wednesday, Friday 1 - 2:30 pm (Rabi Room), Mon- day 1 - 2 pm for the first 4 weeks (TBC). Prerequisites. No permission is required if you are an Astronomy or Physics graduate student { however, it will be assumed you have a background in sta- tistical mechanics, quantum mechanics and electromagnetism at the undergrad- uate level. Knowledge of general relativity is not required. If you are an undergraduate student, you must obtain explicit permission from me. Requirements. Problem sets. The last problem set will serve as a take-home final. Topics covered. Basics of hot big bang standard model. Newtonian cosmology. Geometry and general relativity. Thermal history of the universe. Primordial nucleosynthesis. Recombination. Microwave background. Dark matter and dark energy. Spatial statistics. Inflation and structure formation. Perturba- tion theory. Large scale structure. Non-linear clustering. Galaxy formation. Intergalactic medium. Gravitational lensing. Texts. The main text is Modern Cosmology, by Scott Dodelson, Academic Press, available at Book Culture on W. 112th Street. The website is http://www.bookculture.com. Other recommended references include: • Cosmology, S. Weinberg, Oxford University Press. • http://pancake.uchicago.edu/∼carroll/notes/grtiny.ps or http://pancake.uchicago.edu/∼carroll/notes/grtinypdf.pdf is a nice quick introduction to general relativity by Sean Carroll. • A First Course in General Relativity, B. -
Cosmos: a Spacetime Odyssey (2014) Episode Scripts Based On
Cosmos: A SpaceTime Odyssey (2014) Episode Scripts Based on Cosmos: A Personal Voyage by Carl Sagan, Ann Druyan & Steven Soter Directed by Brannon Braga, Bill Pope & Ann Druyan Presented by Neil deGrasse Tyson Composer(s) Alan Silvestri Country of origin United States Original language(s) English No. of episodes 13 (List of episodes) 1 - Standing Up in the Milky Way 2 - Some of the Things That Molecules Do 3 - When Knowledge Conquered Fear 4 - A Sky Full of Ghosts 5 - Hiding In The Light 6 - Deeper, Deeper, Deeper Still 7 - The Clean Room 8 - Sisters of the Sun 9 - The Lost Worlds of Planet Earth 10 - The Electric Boy 11 - The Immortals 12 - The World Set Free 13 - Unafraid Of The Dark 1 - Standing Up in the Milky Way The cosmos is all there is, or ever was, or ever will be. Come with me. A generation ago, the astronomer Carl Sagan stood here and launched hundreds of millions of us on a great adventure: the exploration of the universe revealed by science. It's time to get going again. We're about to begin a journey that will take us from the infinitesimal to the infinite, from the dawn of time to the distant future. We'll explore galaxies and suns and worlds, surf the gravity waves of space-time, encounter beings that live in fire and ice, explore the planets of stars that never die, discover atoms as massive as suns and universes smaller than atoms. Cosmos is also a story about us. It's the saga of how wandering bands of hunters and gatherers found their way to the stars, one adventure with many heroes. -
Cosmic Microwave Background
1 29. Cosmic Microwave Background 29. Cosmic Microwave Background Revised August 2019 by D. Scott (U. of British Columbia) and G.F. Smoot (HKUST; Paris U.; UC Berkeley; LBNL). 29.1 Introduction The energy content in electromagnetic radiation from beyond our Galaxy is dominated by the cosmic microwave background (CMB), discovered in 1965 [1]. The spectrum of the CMB is well described by a blackbody function with T = 2.7255 K. This spectral form is a main supporting pillar of the hot Big Bang model for the Universe. The lack of any observed deviations from a 7 blackbody spectrum constrains physical processes over cosmic history at redshifts z ∼< 10 (see earlier versions of this review). Currently the key CMB observable is the angular variation in temperature (or intensity) corre- lations, and to a growing extent polarization [2–4]. Since the first detection of these anisotropies by the Cosmic Background Explorer (COBE) satellite [5], there has been intense activity to map the sky at increasing levels of sensitivity and angular resolution by ground-based and balloon-borne measurements. These were joined in 2003 by the first results from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP)[6], which were improved upon by analyses of data added every 2 years, culminating in the 9-year results [7]. In 2013 we had the first results [8] from the third generation CMB satellite, ESA’s Planck mission [9,10], which were enhanced by results from the 2015 Planck data release [11, 12], and then the final 2018 Planck data release [13, 14]. Additionally, CMB an- isotropies have been extended to smaller angular scales by ground-based experiments, particularly the Atacama Cosmology Telescope (ACT) [15] and the South Pole Telescope (SPT) [16]. -
9. the Cosmic Microwave Background
A5682: Introduction to Cosmology Course Notes 9. The Cosmic Microwave Background Reading: Chapter 8, sections 8.0-8.3. (We will cover 8.4 and 8.5 later.) “Re”combination After Big Bang Nucleosynthesis, the universe was still much too hot for the formation of neutral atoms. As expansion continued, the background radiation photons redshifted and the temperature dropped. Naively, one would expect p + e− → H when kT ∼ 13.6eV. Just as with deuterium synthesis, however, the high value of nγ/nb implies that the exponential tail of the photon distribution can dissociate hydrogen atoms. Less naively, we expect p + e− → H when kT ∼ 13.6eV/(− ln η) ∼ 0.65eV, corresponding to (1 + z) ≈ 2700. A more accurate version of this argument given in the textbook (section 9.3) yields a predicted redshift of (1 + z) ≈ 1370 for hydrogen formation. In practice, there are several complicating factors, e.g., any recombination direct to the ground state produces a photon that can immediately ionize another neutral atom unless the photon survives long enough to be redshifted below 13.6 eV. A proper, somewhat tricky calculation of cosmic recombination shows that there is a fairly rapid transition from a free electron fraction xe ≈ 1 to xe ≈ 0 at z ≈ 1100, with most of the transition occuring over a redshift range ∆z ≈ 80. In the laboratory, or in regions ionized by hot stars or quasars or shocks, the process p + e− → H is usually referred to as “recombination.” In the early universe, the protons and electrons were never in the form of hydrogen to begin with, so this process should arguably be called “combination” rather than “recombination.” But “combination” sounds rather silly, so “recombination” is still the standard term for this tran- sition. -
Music and Environment: Registering Contemporary Convergences
JOURNAL OF OF RESEARCH ONLINE MusicA JOURNALA JOURNALOF THE MUSIC OF MUSICAUSTRALIA COUNCIL OF AUSTRALIA ■ Music and Environment: Registering Contemporary Convergences Introduction H O L L I S T A Y L O R & From the ancient Greek’s harmony of the spheres (Pont 2004) to a first millennium ANDREW HURLEY Babylonian treatise on birdsong (Lambert 1970), from the thirteenth-century round ‘Sumer Is Icumen In’ to Handel’s Water Music (Suites HWV 348–50, 1717), and ■ Faculty of Arts Macquarie University from Beethoven’s Pastoral Symphony (No. 6 in F major, Op. 68, 1808) to Randy North Ryde 2109 Newman’s ‘Burn On’ (Newman 1972), musicians of all stripes have long linked ‘music’ New South Wales Australia and ‘environment’. However, this gloss fails to capture the scope of recent activity by musicians and musicologists who are engaging with topics, concepts, and issues [email protected] ■ relating to the environment. Faculty of Arts and Social Sciences University of Technology Sydney Despite musicology’s historical preoccupation with autonomy, our register of musico- PO Box 123 Broadway 2007 environmental convergences indicates that the discipline is undergoing a sea change — New South Wales one underpinned in particular by the1980s and early 1990s work of New Musicologists Australia like Joseph Kerman, Susan McClary, Lawrence Kramer, and Philip Bohlman. Their [email protected] challenges to the belief that music is essentially self-referential provoked a shift in the discipline, prompting interdisciplinary partnerships to be struck and methodologies to be rethought. Much initial activity focused on the role that politics, gender, and identity play in music. -
Lecture 19 Big Bang Cosmology
PHY100 ― The Nature of the Physical World Lecture 19 Big Bang Cosmology Arán García-Bellido PHY100 1 News Exam 2: you can do better! Presentations April 14: Great Physicist life, Controlled fusion April 19: Nuclear power, Search for ET life April 21: Music, Nuclear terrorism 2 per day 20 min+discussion/Q&A Want to meet with all groups this week Contact me PHY100 2 Cosmology Scientific study of the large scale structure of the universe Attempt to understand the origin, evolution and fate of the universe The universe: all matter, space, time and energy Remember first lecture: Tycho Brahe (1546-1601): careful observation of sun, moon, planets Johannes Kepler (1571-1630): elliptical orbits, 3 laws of planetary motion Isaac Newton (1643-1727): Universal law of gravitation + laws of motion explained Kepler's laws of planetary motion Albert Einstein (1879-1955): In an accelerated rocket ship, light would seem to travel on a curved path Gravity = accelerated frame Gravity curves space PHY100 3 Gravity bends light From outside Light is not bent because of the gravitational force 'per se' Light moves on a geodesic (=shortest distance between two points) So Einstein interprets gravitation as a curvature of spacetime Gravity warps spacetime Light just follows the curvature of space From inside PHY100 4 General Relativity: tests Bending of light by gravitational field 4 Gravitational redshift of light 4 Perihelion advance of Mercury 4 Gravitational waves ? PHY100 5 Light travels at a finite speed Object Lookback time Sun 8 minutes Alpha Centauri -
19. Big-Bang Cosmology 1 19
19. Big-Bang cosmology 1 19. BIG-BANG COSMOLOGY Revised September 2009 by K.A. Olive (University of Minnesota) and J.A. Peacock (University of Edinburgh). 19.1. Introduction to Standard Big-Bang Model The observed expansion of the Universe [1,2,3] is a natural (almost inevitable) result of any homogeneous and isotropic cosmological model based on general relativity. However, by itself, the Hubble expansion does not provide sufficient evidence for what we generally refer to as the Big-Bang model of cosmology. While general relativity is in principle capable of describing the cosmology of any given distribution of matter, it is extremely fortunate that our Universe appears to be homogeneous and isotropic on large scales. Together, homogeneity and isotropy allow us to extend the Copernican Principle to the Cosmological Principle, stating that all spatial positions in the Universe are essentially equivalent. The formulation of the Big-Bang model began in the 1940s with the work of George Gamow and his collaborators, Alpher and Herman. In order to account for the possibility that the abundances of the elements had a cosmological origin, they proposed that the early Universe which was once very hot and dense (enough so as to allow for the nucleosynthetic processing of hydrogen), and has expanded and cooled to its present state [4,5]. In 1948, Alpher and Herman predicted that a direct consequence of this model is the presence of a relic background radiation with a temperature of order a few K [6,7]. Of course this radiation was observed 16 years later as the microwave background radiation [8]. -
1 Exploring the Cosmos: the Rhetoric of Successful
EXPLORING THE COSMOS: THE RHETORIC OF SUCCESSFUL SCIENCE TELEVISION By ALEXANDREA MATTHEWS A THESIS PRESENTED TO THE GRADUATE SCHOOL OF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF ARTS IN MASS COMMUNICATION UNIVERSITY OF FLORIDA 2015 1 © 2015 Alexandrea Matthews 2 To my mom, Dina Matthews, for the never-ending love, encouragement, and support 3 ACKNOWLEDGEMENTS I thank my chair, Dr. Debbie Treise, who not only guided me through my thesis but my entire graduate school experience. She has been patient and always accommodating, answering my many questions by e-mail almost immediately, even on weekends, and always found time for me despite her busy schedule. Through the research, coding, and analysis, she has always offered me invaluable insight and editing. I could not be more grateful to have had such a caring, supportive, and experienced thesis chair, advisor, and professor. Thank you for always going above and beyond in these roles. I also thank my other two committee members, Dr. Johanna Cleary and Dr. Elizabeth Lada. They have been supportive and enthusiastic about my research from the beginning and have offered me guidance that really shaped my methodology and research. Dr. Cleary gave me insight from her expertise in telecommunications and offered many great suggestions. Dr. Lada helped me from her expertise in astronomy, as both a committee member and a professor, who gave me the knowledge to approach my thesis from a more informed perspective. I am so thankful to have had such an experienced, diverse committee which could offer me guidance from multiple areas.