The Search for Alien Life Requires Stand the Elements Vision, Blinding Them to the and Magnetic Crystals
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MMM #278 Since December 1986 SEPTEMBER 2014 – P 1
MMM #278 Since December 1986 SEPTEMBER 2014 – p 1 Two worlds of the Inner Solar System that present enormous challenges for human visitors, explorers, and settlers Feature Articles: 2 In Focus: Venus & Mercury: Why Limit Human Frontiers to Moon and Mars? 3 Venus: The Sources of Radical Transformation are already “on Location” 5 Mercury: Discovery of a hidden Settlement Sweet Spot; “Location, Location, Location” 7 Moon Base Costs: Dave Dietzler Below: Previous Articles about Venus have focused on “Aerostat stations” high above the surface, where air pressure and temperatures are human-friendly Above left: a Venus aerostat station - right: at an altitude where temperatures and pressures are benign For past articles, Visit http://www.moonsociety.org/publications/mmm_classics/ or /mmm_themes/ MMM #278 Since December 1986 SEPTEMBER 2014 – p 2 About Moon Miners’ Manifesto - “The Moon - it’s not Earth, but it’s Earth’s!” • MMM’s VISION: “expanding the human economy through of-planet resources”; early heavy reliance on Lunar materials; early use of Mars system and asteroid resources; and permanent settlements supporting this economy. • MMM’s MISSION: to encourage “spin-up” entrepreneurial development of the novel technologies needed and promote the economic-environmental rationale of space and lunar settlement. • Moon Miners’ Manifesto CLASSICS: The non-time-sensitive articles and editorials of MMM’s first twenty years plus have been re-edited, reillustrated, and republished in 23 PDF format volumes, for free downloading from this location: http://www.MoonSociety.org/publications/mmm_classics/ • MMM THEME Issues: 14 collections of articles according to themes: ..../publications/mmm_themes/ • MMM Glossary: new terms, old terms/new meanings: www.moonsociety.org/publications/m3glossary.html • MMM retains its editorial independence and serves many groups, each with its own philosophy, agenda, and programs. -
Biologically Enhanced Energy and Carbon Cycling on Titan?
1 Biologically Enhanced Energy and Carbon Cycling on Titan? Dirk Schulze-Makuch1 and David H. Grinspoon2 1 Dept. of Geological Sciences, Washington State Universty, Pullman, WA 99164, 2Dept. of Space Studies, Southwest Research Institute, Boulder, Colorado With the Cassini-Huygens Mission in orbit around Saturn, the large moon Titan, with its reducing atmosphere, rich organic chemistry, and heterogeneous surface, moves into the astrobiological spotlight. Environmental conditions on Titan and Earth were similar in many respects 4 billion years ago, the approximate time when life originated on Earth. Life may have originated on Titan during its warmer early history and then developed adaptation strategies to cope with the increasingly cold conditions. If organisms originated and persisted, metabolic strategies could exist that would provide sufficient energy for life to persist, even today. Metabolic reactions might include the catalytic hydrogenation of photochemically produced acetylene, or involve the recombination of radicals created in the atmosphere by UV radiation. Metabolic activity may even contribute to the apparent youth, smoothness, and high activity of Titan’s surface via biothermal energy. Environmental conditions are generally thought to be conducive for life if it can be shown that (a) polymeric chemistry, (b) an energy source, and (c) a liquid solvent are present in appreciable quantities (1). Polymeric chemistry has not been confirmed yet for Titan but is most likely present given the complex carbon chemistry in Titan’s atmosphere and on its surface. Abundant energy sources are present at least in the form of UV radiation and photochemistry, and probably endogenic geological activity. Water as a liquid solvent may be limited, but liquid mixtures of water and ammonia are likely(2), and the recent Cassini radar images suggesting the presence of a young surface and ongoing cryovolcanism (3, 4) point towards near-surface liquid reservoirs. -
First Life in Primordial-Planet Oceans: the Biological Big Bang Gibson/Wickramasinghe/Schild First Life in Primordial-Planet Oceans: the Biological Big Bang
Journal of Cosmology First life in primordial-planet oceans: the biological big bang Gibson/Wickramasinghe/Schild First life in primordial-planet oceans: the biological big bang Carl H. Gibson 1,2 1 University of California San Diego, La Jolla, CA 92093-0411, USA [email protected], http://sdcc3.ucsd.edu/~ir118 N. Chandra Wickramasinghe3,4 3Cardiff Centre for Astrobiology, 24 Llwynypia Road, Lisvane, Cardiff CF14 0SY [email protected] Rudolph E. Schild5,6 5 Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 6 [email protected] Abstract: A scenario is presented for the formation of first life in the universe based on hydro- gravitational-dynamics (HGD) cosmology. From HGD, the dark matter of galaxies is H-He gas dominated planets (primordial-fog-particle PFPs) in million solar mass clumps (protoglobularstar- cluster PGCs), which formed at the plasma to gas transition temperature 3000 K. Stars result from mergers of these hot-gas-planets. Over-accretion causes stars to explode as supernovae that scatter life-chemicals (C, N, O, P, S, Ca, Fe etc.) to other planets in PGC clumps and beyond. These chemicals were first collected gravitationally by merging PFPs to form H-saturated, high-pressure, dense oceans of critical-temperature 647 K water over iron-nickel cores at ~ 2 Myr. Stardust fertil- izes the formation of first life in a cosmic hot-ocean soup kitchen comprised of all planets and their moons in meteoric communication, > 10100 kg in total. Ocean freezing at 273 K slows this biologi- cal big bang at ~ 8 Myr. HGD cosmology confirms that the evolving seeds of life are scattered on intergalactic scales by Hoyle-Wickramasinghe cometary panspermia. -
From the Moon to the Moons: Encedalus, Ganymede and Europa
Journal of Cosmology, 2010, Vol 5, pages xxx In PRESS Cosmology, January 13, 2010 From the Moon to the Moons: Encedalus, Ganymede and Europa. The Search for Life and Reliable Biomarkers J. Chela-Flores, Ph.D., The Abdus Salam ICTP, Strada Costiera 11, 34014 Trieste, Italia, and Instituto de Estudios Avanzados, IDEA, Caracas 1015A, República Bolivariana de Venezuela Abstract The recent renewal of interest in exploring the Moon has led to further novel possibilities for the exploration of the Solar System. It is in the outer Solar System where the biggest challenges await our efforts, both in the development of instrumentation and in the clarification of the biosignatures that should be clear indications of life, as opposed to non-life signals. We argue that in the present-day larger scope of cosmology we can undertake one of the most important missions of the space sciences within our own solar system, namely the search for and discovery of a second genesis. This may be accomplished by landing on Europa's surface. We conclude that the implementation of penetrators in future exploration of the outer solar system is worthy of all the financial and technical support that will be needed, both at the national, as well as at the international level. Keywords: Astrobiology, instrumentation, exploration of the solar system, Europa, Enceladus, Biosignatures 1. Introduction It seems appropriate for a journal devoted to cosmology to encompass the field of astrobiology and to move beyond the "anthropic principle" of quantum physics, the standard astroparticle physics and astrophysics that dominate the field of classical cosmology. -
Astrobiology and the Search for Life on Others Worlds
1 EDISON HIGH SCHOOL, HUNTINGTON BEACH, CALIFORNIA, USA Mr. Matheny, Seth Campbell, Connor Hadley, Jackson Sipple ASTROBIOLOGY AND THE SEARCH FOR LIFE ON OTHER WORLDS Finding intelligent life has always been a major dream for all space scientists. The idea of extraterrestrial life contacting us is a fascinating concept that has filled our dreams and science fiction novels since the first telescope was used. The attempts to find intelligence off Earth are collectively known as SETI, or the Search for Extraterrestrial Intelligence. The largest projects use the idea that electromagnetic radiation as communication can be used as a form of contact from an intelligent extraterrestrial source. The basis behind this theory is the fact that these radio waves tend to move in a rather uniform pattern that can penetrate most atmospheres. Broadcasting these waves would be an efficient source of interplanetary communication. Electromagnetic radiation is a reliable way to contact potential intelligent life. For one, waves created by manmade devices such as the television, radio, and other appliances could be detected from space and the waves could be identified from natural waves hinting that they come from an intelligent source. Current SETI projects and future ideas include the constant transmitting of a signal that could be detected by an extraterrestrial source, as well as the development of a message in a ‘universal language’ that is one of friendship that could be delivered to an alien source upon contact. Due to the fact that intelligent life requires a certain environment, a lot of areas in our 2 known universe can be removed from the list of those which might house extraterrestrial life in a form other than bacteria. -
Titan: a Hazy Waterworld That We Can Visit 1 Introduction
Exoplanets in our Backyard 2020 (LPI Contrib. No. 2195) 3015.pdf TITAN: A HAZY WATERWORLD THAT WE CAN VISIT Jason W. Barnes1, Elizabeth P. Turtle2, Melissa G. Trainer3, Ralph D. Lorenz2, Sarah Horst¨ 4, Shannon M. MacKenzie2, and the Dragonfly Science Team. 1University of Idaho, Moscow, ID, USA ([email protected]), 2Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA, 3NASA Goddard Space Flight Center, Greenbelt, MD, USA, 4Johns Hopkins University, Baltimore, Maryland, USA 1 INTRODUCTION There are precious few examples of planets with both distinct surfaces and thick atmospheres in the Solar Sys- tem: just Venus, Earth, Mars, and Saturn’s moon Titan. These four therefore represent our only opportunities to explore close-up the diversity of physical and chemical processes that we expect occur on trillions of extrasolar planets in the Milky Way. Titan’s contributions to this endeavor derive from its (1) organic chemistry, (2) in- terior water ocean, (3) surface-atmosphere interactions, and (4) hazy methane-rich atmosphere. Titan’s particular strength with respect to exoplan- Figure 1: Artist’s conception of Dragonfly on the surface of Titan, ets derives from its accessibility. The Cassini/Huygens within an interdune in the Shangri-La sand sea. mission explored Titan from Saturn orbit and within the atmosphere, respectively. A future Titan orbiter mission will hopefully follow up on Cassini’s discoveries [e.g. 1], periment in abiotic organic synthesis. Entire planets like providing global imaging and topography, atmospheric Titan may be common in extrasolar systems [3, 4, 5]. measurements and characterization, and gravity probing On Titan, carbon can interact with liquid water on of the interior. -
Strategies for Detecting Biological Molecules on Titan
ASTROBIOLOGY Volume 18, Number 5, 2018 ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2017.1758 Strategies for Detecting Biological Molecules on Titan Catherine D. Neish,1 Ralph D. Lorenz,2 Elizabeth P. Turtle,2 Jason W. Barnes,3 Melissa G. Trainer,4 Bryan Stiles,5 Randolph Kirk,6 Charles A. Hibbitts,2 and Michael J. Malaska5 Abstract Saturn’s moon Titan has all the ingredients needed to produce ‘‘life as we know it.’’ When exposed to liquid water, organic molecules analogous to those found on Titan produce a range of biomolecules such as amino acids. Titan thus provides a natural laboratory for studying the products of prebiotic chemistry. In this work, we examine the ideal locales to search for evidence of, or progression toward, life on Titan. We determine that the best sites to identify biological molecules are deposits of impact melt on the floors of large, fresh impact craters, specifically Sinlap, Selk, and Menrva craters. We find that it is not possible to identify biomolecules on Titan through remote sensing, but rather through in situ measurements capable of identifying a wide range of biological molecules. Given the nonuniformity of impact melt exposures on the floor of a weathered impact crater, the ideal lander would be capable of precision targeting. This would allow it to identify the locations of fresh impact melt deposits, and/or sites where the melt deposits have been exposed through erosion or mass wasting. Determining the extent of prebiotic chemistry within these melt deposits would help us to understand how life could originate on a world very different from Earth. -
Life Without Water? 18 March 2010, by Henry Bortman
Life Without Water? 18 March 2010, by Henry Bortman found a way to take hold on Titan. Water may all be frozen solid, but methane and ethane are liquids. In the past few years, instruments on NASA’s Cassini spacecraft and images captured by ESA’s Huygens probe have revealed an astonishing world with a complete liquid cycle, much like the hydrologic cycle on Earth, but based on methane and ethane rather than on water. “What Cassini actually found on Titan, from 2004 onwards, was a methane-ethane cycle that very much echoes the kind of hydrologic cycle we see on the Earth,” says Jonathan Lunine, currently at the University of Rome Tor Vergata while on leave from the University of Arizona. Cassini has revealed rivers and lakes of methane-ethane, the lakes evaporating to form clouds, the clouds raining The irregular black shapes in this Cassini radar image of hydrocarbons back down onto the surface, flowing Titan’s northern polar region are believed to be liquid through rivers and collecting in lakes. It is the only methane-ethane lakes. Credit: NASA/JPL/USGS world in our solar system other than Earth where a liquid cycle like this takes place. There’s just no water. On Saturn’s giant moon Titan, it is so cold that But there are plenty of hydrocarbons. Methane and water is frozen as hard as granite. And yet there is ethane are the simplest hydrocarbon molecules. By a complete liquid cycle of methane and ethane. themselves, they are of limited biological interest. Scientists wonder whether there could also be life. -
Origins of Life: a Problem for Physics
Origins of Life: A Problem for Physics Sara Imari Walker School of Earth and Space Exploration and Beyond Center for Fundamental Concepts in Science, Arizona State University, Tempe AZ USA; Blue Marble Space Institute of Science, Seattle WA USA E-mail: [email protected] Abstract. The origins of life stands among the great open scientific questions of our time. While a number of proposals exist for possible starting points in the pathway from non-living to living matter, these have so far not achieved states of complexity that are anywhere near that of even the simplest living systems. A key challenge is identifying the properties of living matter that might distinguish living and non-living physical systems such that we might build new life in the lab. This review is geared towards covering major viewpoints on the origin of life for those new to the origin of life field, with a forward look towards considering what it might take for a physical theory that universally explains the phenomenon of life to arise from the seemingly disconnected array of ideas proposed thus far. The hope is that a theory akin to our other theories in fundamental physics might one day emerge to explain the phenomenon of life, and in turn finally permit solving its origins. arXiv:1705.08073v1 [q-bio.PE] 23 May 2017 CONTENTS 2 Contents 1 Introduction 2 2 Knowns and unknowns in solving the origin of life 4 2.1 One planet, one sample: The significance of anthropic bias . .5 2.2 Two paths to a solution . -
Primordial Planets, Comets and Moons Foster Life in the Cosmos
Primordial planets, comets and moons foster life in the cosmos Carl H. Gibsona*, N. Chandra Wickramasingheb and Rudolph E. Schildc a UCSD, La Jolla, CA, 92093-0411, USA; b Cardiff Univ., Cardiff, UK; c Harvard, Cambridge, MA, USA ABSTRACT A key result of hydrogravitational dynamics cosmology relevant to astrobiology is the early formation of vast numbers of hot primordial-gas planets in million-solar-mass clumps as the dark matter of galaxies and the hosts of first life. Photon viscous forces in the expanding universe of the turbulent big bang prevent fragmentations of the plasma for mass scales smaller than protogalaxies. At the plasma to gas transition 300,000 years after the big bang, the 107 decrease in kinematic viscosity ν explains why ~3x107 planets are observed to exist per star in typical galaxies like the Milky Way, not eight or nine. Stars form by a binary accretional cascade from Earth-mass primordial planets to progressively larger masses that collect and recycle the stardust chemicals of life produced when stars overeat and explode. The astonishing complexity of molecular biology observed on Earth is possible to explain only if enormous numbers of primordial planets and their fragments have hosted the formation and wide scattering of the seeds of life virtually from the beginning of time. Geochemical and biological evidence suggests that life on Earth appears at the earliest moment it can survive, in highly evolved forms with complexity requiring a time scale in excess of the age of the galaxy. This is quite impossible within standard cold-dark-matter cosmology where planets are relatively recent, rare and cold, completely lacking mechanisms for intergalactic transport of life forms. -
Meeting Abstracts
228th AAS San Diego, CA – June, 2016 Meeting Abstracts Session Table of Contents 100 – Welcome Address by AAS President Photoionized Plasmas, Tim Kallman (NASA 301 – The Polarization of the Cosmic Meg Urry GSFC) Microwave Background: Current Status and 101 – Kavli Foundation Lecture: Observation 201 – Extrasolar Planets: Atmospheres Future Prospects of Gravitational Waves, Gabriela Gonzalez 202 – Evolution of Galaxies 302 – Bridging Laboratory & Astrophysics: (LIGO) 203 – Bridging Laboratory & Astrophysics: Atomic Physics in X-rays 102 – The NASA K2 Mission Molecules in the mm II 303 – The Limits of Scientific Cosmology: 103 – Galaxies Big and Small 204 – The Limits of Scientific Cosmology: Town Hall 104 – Bridging Laboratory & Astrophysics: Setting the Stage 304 – Star Formation in a Range of Dust & Ices in the mm and X-rays 205 – Small Telescope Research Environments 105 – College Astronomy Education: Communities of Practice: Research Areas 305 – Plenary Talk: From the First Stars and Research, Resources, and Getting Involved Suitable for Small Telescopes Galaxies to the Epoch of Reionization: 20 106 – Small Telescope Research 206 – Plenary Talk: APOGEE: The New View Years of Computational Progress, Michael Communities of Practice: Pro-Am of the Milky Way -- Large Scale Galactic Norman (UC San Diego) Communities of Practice Structure, Jo Bovy (University of Toronto) 308 – Star Formation, Associations, and 107 – Plenary Talk: From Space Archeology 208 – Classification and Properties of Young Stellar Objects in the Milky Way to Serving -
ASTRONOMY 141: Life in the Universe Fall Quarter 2010 · Mo Tu We Th Fr 1:30 - 2:18 Pm · Stillman Hall 100
ASTRONOMY 141: Life in the Universe Fall Quarter 2010 · Mo Tu We Th Fr 1:30 - 2:18 pm · Stillman Hall 100 Instructor: Professor Barbara Ryden Office: 4035 McPherson Lab (4th floor), 140 W. 18th Avenue Office hours: Mo Fr 9 – 11 am, Tu We 3:30 – 5:30 pm, or by appointment Telephone: 292-4562 Email: [email protected] Graduate Teaching Associate: Courtney Epstein Office: 4020 McPherson Lab Office hours: Mo Th Fr 11 – 12:30, or by appointment Telephone: 292-7785 Email: [email protected] Required text: Life in the Universe (Second Edition), by Bennett & Shostak (ISBN 0805347534) Class website: www.astronomy.ohio-state.edu/∼ryden/ast141/ The website will contain notes for each lecture, the course syllabus, the as- signed problem sets, and additional astronomy links. Lectures: Please silence your cellphone and turn off any wireless de- vices during lecture. (Exceptions will be made for assistive technology for the vision- or hearing-impaired.) Grading policy: Your course grade will be determined from the results of four in-class multiple-choice quizzes (40%), four take-home problem sets (30%), and a final exam (30%). The quizzes will be held on Friday, October 8, Friday, October 22, Friday, November 5, and Friday, November 19. If you know in advance you will miss a quiz because of attendance at a university-sponsored activity, please contact the professor prior to the scheduled quiz date in order to schedule a makeup quiz. If you miss a quiz due to a sudden illness or other emergency, contact the professor as soon as possible after the missed exam, in order to schedule a makeup quiz.