57. Understanding the Natural Ancient Origin of Oil Versus a Biblical
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Gold T. Rotating Neutron Stars As the Origin of the Pulsating Radio Sources
CC/NUMBER 8 ® FEBRUARY 22, 1993 This Week's Citation Classic Gold T. Rotating neutron stars as the origin of the pulsating radio sources. Nature 218:731-2, 1968; and Gold T. Rotating neutron stars and the nature of pulsars. Nature 221:25-7, 1969. [Center for Radiophysics and Space Research: and Cornell-Sydney University Astronomy Center. Cornell University, Ithaca. NY] Enigmatic, rapidly pulsating radio sources were preferred to attribute these sources to interpreted as rotating beacons sweeping over distant galaxies, not to stellar objects. the Earth, radiating out from rapidly rotating, The pulsars now seemed to repre- extremely collapsed stars ("neutron stars"). Nu- merous detailed predictions followed from this sent just the stellar objects I had dis- model, and all were soon verified. The model cussed then. Calculations existed for also accounted closely for the previously unex- the collapsed "neutron stars" that in- plained luminosity of the Crab Nebula. [The dicated approximately their size, as SCI® indicates that these papers have been small as a few kilometers, and their cited in more than 240 and 150 publications, mass, on the order of a solar mass.4 respectively.] Astronomers generally thought that even if they existed, they could never be discovered. However hot, a star so small could not be seen at astronomi- The Nature of Pulsars cal distances. But they had not con- sidered the energy concentration re- Thomas Gold sulting from the collapse: enormous Center for Radiophysics magnetic field strengths and a spin and Space Research energy quite comparable with the en- Cornell University tire content of nuclear energy of the Ithaca, NY 14853 star before its collapse. -
Understanding the Application of Raman Spectroscopy to the Detection of Traces of Life
ASTROBIOLOGY Volume 10, Number 2, 2010 ª Mary Ann Liebert, Inc. DOI: 10.1089=ast.2009.0344 Understanding the Application of Raman Spectroscopy to the Detection of Traces of Life Craig P. Marshall,1 Howell G.M. Edwards,2 and Jan Jehlicka3 Abstract Investigating carbonaceous microstructures and material in Earth’s oldest sedimentary rocks is an essential part of tracing the origins of life on our planet; furthermore, it is important for developing techniques to search for traces of life on other planets, for example, Mars. NASA and ESA are considering the adoption of miniaturized Raman spectrometers for inclusion in suites of analytical instrumentation to be placed on robotic landers on Mars in the near future to search for fossil or extant biomolecules. Recently, Raman spectroscopy has been used to infer a biological origin of putative carbonaceous microfossils in Early Archean rocks. However, it has been demonstrated that the spectral signature obtained from kerogen (of known biological origin) is similar to spectra obtained from many poorly ordered carbonaceous materials that arise through abiotic processes. Yet there is still confusion in the literature as to whether the Raman spectroscopy of carbonaceous materials can indeed delineate a signature of ancient life. Despite the similar nature in spectra, rigorous structural interrogation between the thermal alteration products of biological and nonbiological organic materials has not been undertaken. There- fore, we propose a new way forward by investigating the second derivative, deconvolution, and chemometrics of the carbon first-order spectra to build a database of structural parameters that may yield distinguishable characteristics between biogenic and abiogenic carbonaceous material. -
Basic Geochemical Evaluation of Unconventional Resource Plays Stephan H
Basic Geochemical Evaluation of Unconventional Resource Plays Stephan H. Nordeng Introduction These changes provide clues that may answer questions such as: Basin-centered petroleum accumulations such as the Bakken Formation in the Williston Basin of North Dakota have recently been Is a given kerogen capable of producing petroleum? recognized as being important in the future development of energy resources. There are several features that these petroleum systems If so, what are the likely types of petroleum that may have in common. The systems typically include the deposition result? of organic-rich rocks that form the core of the petroleum system when subjected to elevated temperatures for suffi cient periods of Did a given source rock generate petroleum? time. This allows for the source rock to “mature” to the point that oil is generated. Once a suffi cient amount of generation has If so, how fast and possibly how much? occurred the oil is expelled into neighboring rocks and, in instances when these rocks are poorly permeable, the oil accumulates under Source Rock Evaluation high pressures. The three interconnected processes of deposition, Probably the most important aspect of evaluating a potential maturation, and expulsion may all be studied using various types source rock involves determining the amount and character of of geochemical analyses. organic matter that could have been available, given the proper conditions, to generate oil and gas. One of the fi rst things to Deposition of a potential source rock involves a tightly constrained consider is just how much organic carbon is currently present set of circumstances. These include high rates of biological in the rock. -
The Deep, Hot Biosphere (Geochemistry/Planetology) THOMAS GOLD Cornell University, Ithaca, NY 14853 Contributed by Thomas Gold, March 13, 1992
Proc. Natl. Acad. Sci. USA Vol. 89, pp. 6045-6049, July 1992 Microbiology The deep, hot biosphere (geochemistry/planetology) THOMAS GOLD Cornell University, Ithaca, NY 14853 Contributed by Thomas Gold, March 13, 1992 ABSTRACT There are strong indications that microbial gasification. As liquids, gases, and solids make new contacts, life is widespread at depth in the crust ofthe Earth, just as such chemical processes can take place that represent, in general, life has been identified in numerous ocean vents. This life is not an approach to a lower chemical energy condition. Some of dependent on solar energy and photosynthesis for its primary the energy so liberated will increase the heating of the energy supply, and it is essentially independent of the surface locality, and this in turn will liberate more fluids there and so circumstances. Its energy supply comes from chemical sources, accelerate the processes that release more heat. Hot regions due to fluids that migrate upward from deeper levels in the will become hotter, and chemical activity will be further Earth. In mass and volume it may be comparable with all stimulated there. This may contribute to, or account for, the surface life. Such microbial life may account for the presence active and hot regions in the Earth's crust that are so sharply of biological molecules in all carbonaceous materials in the defined. outer crust, and the inference that these materials must have Where such liquids or gases stream up to higher levels into derived from biological deposits accumulated at the surface is different chemical surroundings, they will continue to repre- therefore not necessarily valid. -
Science Loses Some Friends Francis Crick, Thomas Gold, and Philip Abelson
Monthly Planet October 2004 Science Loses Some Friends Francis Crick, Thomas Gold, and Philip Abelson By Iain Murray he scientifi c world lost three impor- Throughout his career, Abelson used which suggests that the universe and Ttant fi gures in recent weeks, as scientifi c principles to determine genu- the laws of physics have always existed Francis Crick, Thomas Gold, and Philip ine new developments from hype and in the same, steady state. This has since Abelson have all passed away. In their publicity stunts (he was famously dis- been supplanted as the dominant cos- careers, each demonstrated the best that missive of the scientifi c value of the race mological paradigm by the Big Bang science has to offer humanity. Their loss to the moon). In that, he should prove a theory. illustrates how much worse off the state role model for true scientists. After working at the Royal Greenwich of science is today than during their Observatory, Gold moved to the United glory years. Thomas Gold States to become Professor of Astron- Astronomer Thomas Gold had an omy at Harvard. From there he moved Philip Abelson equally distinguished career, in fi elds as to Cornell, where he demonstrated that Philip Abelson was a scientist of truly diverse as engineering, physiology, and the newly discovered “pulsar” phenom- broad talents. One of America’s fi rst cosmology; and he was never afraid of enon must contain a rotating neutron nuclear physicists, he discovered the being called a maverick. A fellow of both star (a star more massive than the sun element Neptunium and designed the the Royal Society and the National Acad- but just 10 km in diameter). -
Notes of a Fringe -Watcher
MARTIN GARDNER Notes of a Fringe -Watcher The Anomalies of Chip Arp We have watched the farther galaxies I don't know what the 'C stands for, but fleeing away from us, wild herds of panic all his friends call him 'Chip.' He's in horses—or a trick of distance deceived danger of losing all those friends, if he the prism. keeps up what he's doing now! "Now mind you, I am kidding, be —Robinson Jeffers cause I am very fond of Chip Arp. In fact, we were graduate students at Caltech N HIS SPLENDID book The Drama together. But in those years he was nice." I of the Universe (1978) the late George An astronomer at Hale Observatories, Abell, an astronomer who served on the in California, Chip Arp is still adding to editorial board of this magazine, specu his collection of crazy objects, and still lates what generates the enormous ener making sharp rapier jabs at his more gies emitted by quasars (quasi-stellar orthodox colleagues. (Actual sword fenc sources). Quasars are almost surely the ing, by the way, is one of his major hob most distant known objects in the uni bies.) Like Thomas Gold, the subject of verse. Their gigantic redshifts indicate this column two issues back, Arp is a that some are moving outward at veloci competent, well-informed scientist who ties close to 90 percent of the speed of delights in the role of gadfly. His peculiar light. They occupy positions believed to anomalies are quasars that seem to be be very near the "edge" of the light connected by bridges of luminous gas barrier, a boundary beyond which noth but that have markedly different red- ing could ever be observed from our shifts, or high-redshift quasars that ap galaxy. -
Native Polycyclic Aromatic Hydrocarbons (PAH) in Coals – a Hardly Recognized Source of Environmental Contamination
SCIENCE OF THE TOTAL ENVIRONMENT 407 (2009) 2461– 2473 available at www.sciencedirect.com www.elsevier.com/locate/scitotenv Review Native polycyclic aromatic hydrocarbons (PAH) in coals – A hardly recognized source of environmental contamination C. Achtena,b, T. Hofmanna,⁎ a University of Vienna, Department of Environmental Geosciences, Althanstr. 14, 1090 Vienna, Austria b University of Münster, Department of Applied Geology, Corrensstr. 24, 48149 Münster, Germany ARTICLE DATA ABSTRACT Article history: Numerous environmental polycyclic aromatic hydrocarbon (PAH) sources have been Received 15 October 2008 reported in literature, however, unburnt hard coal/ bituminous coal is considered only Received in revised form rarely. It can carry native PAH concentrations up to hundreds, in some cases, thousands of 29 November 2008 mg/kg. The molecular structures of extractable compounds from hard coals consist mostly Accepted 5 December 2008 of 2–6 polyaromatic condensed rings, linked by ether or methylene bridges carrying methyl Available online 4 February 2009 and phenol side chains. The extractable phase may be released to the aquatic environment, be available to organisms, and thus be an important PAH source. PAH concentrations and Keywords: patterns in coals depend on the original organic matter type, as well as temperature and Native PAH pressure conditions during coalification. The environmental impact of native unburnt coal- Bituminous coal bound PAH in soils and sediments is not well studied, and an exact source apportionment is Hard coal hardly possible. In this paper, we review the current state of the art. Sediment © 2008 Elsevier B.V. All rights reserved. Soil Contents 1. Introduction .........................................................2462 2. Reserves and production ..................................................2462 3. -
Can High Pressures Enhance the Long-Term Survival of Microorganisms?
Can High Pressures Enhance The Long-Term Survival of Microorganisms? Robert M. Hazen & Matt Schrenk Carnegie Institution & NASA Astrobiology Institute Pardee Keynote Symposium: Evidence for Long-Term Survival of Microorganisms and Preservation of DNA Philadelphia – October 24, 2006 Objectives I. Review the nature and distribution of life at high pressures. II. Examine the extreme pressure limits of cellular life. III. Compare experimental approaches to study microbial behavior at high P and T. IV. Explore how biomolecules and their reactions might change at high pressure? I. High-Pressure Life HMS Challenger – 1870s 20 MPa (~200 atmospheres) High-Pressure Life Deep-Sea Hydrothermal Vents – 1977 High-Pressure Life Discoveries of Microbial Life in Crustal Rocks – 1990s P ~ 100 MPa Witwatersrand Deep Microbiology Project Energy from radiolytic cleavage of water. Lin, Onstott et al. (2006) Science Thomas Gold’s Hypothesis: Organic Synthesis in the Mantle ß>300 MPa Thomas Gold (1999) NY:Springer-Verlag. Life at High Pressures on other Worlds? Deep, wet environments may exist on Mars, Europa, etc. I. What is the Nature and Distribution of Life at High-Pressure? Deep life, especially microbial life, is abundant throughout the upper crust . II. What are the Extreme Pressure Limits of Life? How deep might microbes exist in Earth’s crust? Pressure Can Enhance T Stability [Pledger et al. (1994) FEMS Microbiology [Margosch et al. (2006) Appl. Environ. Ecology 14, 233-242.] Microbiology 72, 3476-3481.] Life’s Extreme Pressure Limits 60 km Fast, cold slabs have regions of P > 2 GPa & T < 150°C [Stein & Stein (1996) AGU Monograph 96] Pressure Limits of Life Hydrothermal Opposed-Anvil Cell Pressure Limits of Life E. -
Edward Milne's Influence on Modern Cosmology
ANNALS OF SCIENCE, Vol. 63, No. 4, October 2006, 471Á481 Edward Milne’s Influence on Modern Cosmology THOMAS LEPELTIER Christ Church, University of Oxford, Oxford OX1 1DP, UK Received 25 October 2005. Revised paper accepted 23 March 2006 Summary During the 1930 and 1940s, the small world of cosmologists was buzzing with philosophical and methodological questions. The debate was stirred by Edward Milne’s cosmological model, which was deduced from general principles that had no link with observation. Milne’s approach was to have an important impact on the development of modern cosmology. But this article shows that it is an exaggeration to intimate, as some authors have done recently, that Milne’s rationalism went on to infiltrate the discipline. Contents 1. Introduction. .........................................471 2. Methodological and philosophical questions . ..................473 3. The outcome of the debate .................................476 1. Introduction In a series of articles, Niall Shanks, John Urani, and above all George Gale1 have analysed the debate stirred by Edward Milne’s cosmological model.2 Milne was a physicist we can define, at a philosophical level, as an ‘operationalist’, a ‘rationalist’ and a ‘hypothetico-deductivist’.3 The first term means that Milne considered only the observable entities of a theory to be real; this led him to reject the notions of curved space or space in expansion. The second term means that Milne tried to construct a 1 When we mention these authors without speaking of one in particular, we will use the expression ‘Gale and co.’ 2 George Gale, ‘Rationalist Programmes in Early Modern Cosmology’, The Astronomy Quarterly,8 (1991), 193Á218. -
Dark Universe: Science & Literacy Activity for Grades 9-12
Dark Universe Science & Literacy Activity GRADES 9-12 OVERVIEW Common Core State Standards: This activity, which is aligned to the Common Core State Standards (CCSS) WHST.9-12.2, WHST.9-12.8, WHST.9-12.9, for English Language Arts, introduces students to scientific knowledge and RST.9-12.1, RST.9-12.2, RST.9-12.4, RST.9-12.7, language related to the study of cosmology. Students will read content-rich RST.9-12.10 texts, view the Dark Universe space show, and use what they have learned New York State Science Core Curriculum: to complete a CCSS-aligned writing task, creating an illustrated text about PS 1.2a how scientists study the history of the universe. Next Generation Science Standards: Materials in this activity include: PE HS-ESS1-2 • Teacher instructions for: DCI ESS1.A: The Universe and Its Stars o Pre-visit student reading The Big Bang theory is supported by o Viewing the Dark Universe space show observations of distant galaxies receding o Post-visit writing task from our own, of the measured composition • Text for student reading: “Case Study: The Cosmic Microwave Background ” of stars and non-stellar gases, and of the • Student Writing Guidelines maps of spectra of the primordial radiation (cosmic microwave background) that still • Teacher rubric for writing assessment fills the universe. SUPPORTS FOR DIVERSE LEARNERS: An Overview This resource has been designed to engage all learners with the principles of Universal Design for Learning in mind. It represents information in multiple ways and offers multiple ways for your students to engage with content as they read about, discuss, view, and write about scientific concepts. -
CV Background
Steven Soter CV 2013 Research Associate, Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024. Visiting Professor, Environmental Studies Program, New York University, 285 Mercer Street, 9th Floor, New York, NY 10003, and Email: <[email protected]>. Tel: 212-769-5230. RECENT ACTIVITIES Research in astronomy and geoarchaeology. Teaching at NYU: courses on Scientific Thinking and Speculation, Geology and Antiquity in the Mediterranean, Life in the Universe, Climate Change, and Energy and Environment. BACKGROUND AND EDUCATION Born in Los Angeles, California, May 1943 BSc in Astronomy/Physics, 1965 University of California at Los Angeles (Advisors: George Abell and Peter Goldreich) PhD in Astronomy, 1971 Cornell University, Ithaca, New York (Advisors: Thomas Gold, Carl Sagan, Joseph Burns) PREVIOUS POSITIONS 1964-66 Research Assistant, Radio Astronomy Project, Aerospace Corporation, El Segundo, California 1966-71 Research Assistant, Center for Radiophysics and 1973-79 Space Research, Cornell University, Ithaca, N.Y. 1971-73 Postdoctoral Fellow, Miller Institute for Basic Research in Science, UC Berkeley 1973-79 Assistant Editor, ICARUS: International Journal of Solar System Studies (Carl Sagan, editor) 1977-80 Co-Writer and Head of Research, COSMOS Television Series, KCET/Los Angeles 1980-87 Senior Research Associate, Center for Radiophyscs and Space Research, Cornell University 1988-97 Special Assistant to the Director, National Air and Space Museum, Smithsonian Institution, Washington, DC 1997-03 Scientist, Hayden Planetarium American Museum of Natural History, New York 2004-13 Research Associate, Department of Astrophysics, American Museum of Natural History, New York 2005-07 Scientist-in-Residence, Center for Ancient Studies, New York University, New York 2008-12 Visiting Professor, Environmental Studies Program, New York University, New York . -
Shale Kerogen – Hydraulic Fracturing Fluid Interactions and Contaminant Release
SHALE KEROGEN – HYDRAULIC FRACTURING FLUID INTERACTIONS AND CONTAMINANT RELEASE Megan K. Dustin1, John R. Bargar2, Adam D. Jew,1,2 Anna L. Harrison1,2, Claresta Joe-Wong1, Dana L. Thomas1, Gordon E. Brown, Jr.1,2,3, and Katharine Maher4* 1 Department of Geological Sciences, School of Earth, Energy & Environmental Sciences, Stanford University, Stanford, CA 94305-2115, USA 2 Stanford Synchrotron Radiation Lightsource, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94062, USA 3 Department of Photon Science, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94062, USA 4 Department of Earth Systems Science, School of Earth, Energy & Environmental Sciences, Stanford University, Stanford, CA 94305-2115, USA *Corresponding author: [email protected] Abstract The recent increase in unconventional oil and gas exploration and production has prompted a large amount of research on hydraulic fracturing, but the majority of chemical reactions between shale minerals and organic matter with fracturing fluids are not well understood. Organic matter, primarily in the form of kerogen, dominates the transport pathways for oil and gas; thus any alteration of kerogen (both physical and chemical properties) upon exposure to fracturing fluid may impact hydrocarbon extraction. In addition, kerogen is enriched in metals, making it a potential source of heavy metal contaminants to produced waters. In this study, we reacted two different kerogen isolates of contrasting type and maturity (derived from Green River and Marcellus shales) with a synthetic hydraulic fracturing fluid for two weeks in order to determine the effect of fracturing fluids on both shale organic matter and closely associated minerals.