Interview with Gerald J. Wasserburg
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Carnegie Institution of Washington Department of Terrestrial Magnetism Washington, DC 20015-1305
43 Carnegie Institution of Washington Department of Terrestrial Magnetism Washington, DC 20015-1305 This report covers astronomical research carried out during protostellar outflows have this much momentum out to rela- the period July 1, 1994 – June 30, 1995. Astronomical tively large distances. Planetary nebulae do not, but with studies at the Department of Terrestrial Magnetism ~DTM! their characteristic high post-shock temperatures, collapse of the Carnegie Institution of Washington encompass again occurs. Hence all three outflows appear to be able to observational and theoretical fields of solar system and trigger the collapse of molecular clouds to form stars. planet formation and evolution, stars and star formation, Foster and Boss are continuing this work and examining galaxy kinematics and evolution, and various areas where the possibility of introducing 26Al into the early solar system these fields intersect. in a heterogeneous manner. Some meteoritical inclusions ~chondrules! show no evidence for live 26Al at the time of their formation. So either the chondrules formed after the 1. PERSONNEL aluminium had decayed away, or the solar nebula was not Staff Members: Sean C. Solomon ~Director!, Conel M. O’D. Alexander, Alan P. Boss, John A. Graham, Vera C. Rubin, uniformly populated with the isotope. Foster & Boss are ex- Franc¸ois Schweizer, George W. Wetherill ploring the injection of shock wave particles into the collaps- Postdoctoral Fellows: Harold M. Butner, John E. Chambers, ing solar system. Preliminary results are that ;40% of the Prudence N. Foster, Munir Humayun, Stacy S. McGaugh, incident shock particles are swallowed by the collapsing Bryan W. Miller, Elizabeth A. Myhill, David L. -
Lecture 9—Is the Earth Rare?
41st Saas-Fee Course From Planets to Life 3-9 April 2011 Lecture 9—Is the Earth Rare? List of Rare Earth arguments/ Nitrogen abundance/ Frequency of large impacts/ Chaotic obliquity fluctuations J. F. Kasting The Gaia hypothesis First presented in the 1970s by James Lovelock 1979 1988 • Life itself is what stabilizes planetary environments • Corollary: A planet might need to be inhabited in order to remain habitable The Medea and Rare Earth hypotheses Peter Ward 2009 2000 Medea hypothesis: Life is harmful to the Earth! Rare Earth hypothesis: Complex life (animals, including humans) is rare in the universe Additional support for the Rare Earth hypothesis • Lenton and Watson think that complex life (animal life) is rare because it requires a series of unlikely evolutionary events – the origin of life – the origin of the genetic code – the development of oxygenic photosynthesis) – the origin of eukaryotes – the origin of sexuality 2011 Rare Earth/Gaia arguments 1. Plate tectonics is rare --We have dealt with this already. Plate tectonics is not necessarily rare, but it requires liquid water. Thus, a planet needs to be within the habitable zone. 2. Other planets may lack magnetic fields and may therefore have harmful radiation environments and be subject to loss of atmosphere – We have talked about this one also. Venus has retained its atmosphere. The atmosphere itself provides protection against cosmic rays 3. The animal habitable zone (AHZ) is smaller than the habitable zone (HZ) o – AHZ definition: Ts = 0-50 C o – HZ definition: Ts = 0-100 C. But this is wrong! For a 1-bar atmosphere like Earth, o water loss begins when Ts reaches 60 C. -
Annual Report 2013.Pdf
ATOMIC HERITAGE FOUNDATION Preserving & Interpreting Manhattan Project History & Legacy preserving history ANNUAL REPORT 2013 WHY WE SHOULD PRESERVE THE MANHATTAN PROJECT “The factories and bombs that Manhattan Project scientists, engineers, and workers built were physical objects that depended for their operation on physics, chemistry, metallurgy, and other nat- ural sciences, but their social reality - their meaning, if you will - was human, social, political....We preserve what we value of the physical past because it specifically embodies our social past....When we lose parts of our physical past, we lose parts of our common social past as well.” “The new knowledge of nuclear energy has undoubtedly limited national sovereignty and scaled down the destructiveness of war. If that’s not a good enough reason to work for and contribute to the Manhattan Project’s historic preservation, what would be? It’s certainly good enough for me.” ~Richard Rhodes, “Why We Should Preserve the Manhattan Project,” Bulletin of the Atomic Scientists, May/June 2006 Photographs clockwise from top: J. Robert Oppenheimer, General Leslie R. Groves pinning an award on Enrico Fermi, Leona Woods Marshall, the Alpha Racetrack at the Y-12 Plant, and the Bethe House on Bathtub Row. Front cover: A Bruggeman Ranch property. Back cover: Bronze statues by Susanne Vertel of J. Robert Oppenheimer and General Leslie Groves at Los Alamos. Table of Contents BOARD MEMBERS & ADVISORY COMMITTEE........3 Cindy Kelly, Dorothy and Clay Per- Letter from the President..........................................4 -
Chapter 9: the Origin and Evolution of the Moon and Planets
Chapter 9 THE ORIGIN AND EVOLUTION OF THE MOON AND PLANETS 9.1 In the Beginning The age of the universe, as it is perceived at present, is perhaps as old as 20 aeons so that the formation of the solar system at about 4.5 aeons is a comparatively youthful event in this stupendous extent of time [I]. Thevisible portion of the universe consists principally of about 10" galaxies, which show local marked irregularities in distribution (e.g., Virgo cluster). The expansion rate (Hubble Constant) has values currently estimated to lie between 50 and 75 km/sec/MPC [2]. The reciprocal of the constant gives ages ranging between 13 and 20 aeons but there is uncertainty due to the local perturbing effects of the Virgo cluster of galaxies on our measurement of the Hubble parameter [I]. The age of the solar system (4.56 aeons), the ages of old star clusters (>10" years) and the production rates of elements all suggest ages for the galaxy and the observable universe well in excess of 10" years (10 aeons). The origin of the presently observable universe is usually ascribed, in current cosmologies, to a "big bang," and the 3OK background radiation is often accepted as proof of the correctness of the hypothesis. Nevertheless, there are some discrepancies. The observed ratio of hydrogen to helium which should be about 0.25 in a "big-bang" scenario may be too high. The distribution of galaxies shows much clumping, which would indicate an initial chaotic state [3], and there are variations in the spectrum of the 3OK radiation which are not predicted by the theory. -
An Integrated Chemical and Stable-Isotope Model of the Origin of Midocean Ridge Hot Spring Systems
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 90, NO. B14, PAGES 12,583-12,606, DECEMBER 10, 1985 An Integrated Chemical and Stable-Isotope Model of the Origin of Midocean Ridge Hot Spring Systems TERESASUTER BOWERS 1 AND HUGH P. TAYLOR,JR. Division of Geologicaland Planetary Sciences,California Institute of Technology,Pasadena Chemical and isotopic changes accompanying seawater-basalt interaction in axial midocean ridge hydrothermal systemsare modeled with the aid of chemical equilibria and mass transfer computer programs,incorporating provision for addition and subtractionof a wide-range of reactant and product minerals, as well as cation and oxygen and hydrogen isotopic exchangeequilibria. The models involve stepwiseintroduction of fresh basalt into progressivelymodified seawater at discrete temperature inter- vals from 100ø to 350øC, with an overall water-rock ratio of about 0.5 being constrainedby an assumed •80,2 o at 350øCof +2.0 per mil (H. Craig,personal communication, 1984). This is a realisticmodel because:(1) the grade of hydrothermal metamorphism increasessharply downward in the oceanic crust; (2) the water-rock ratio is high (> 50) at low temperaturesand low (<0.5) at high temperatures;and (3) it allows for back-reaction of earlier-formed minerals during the course of reaction progress.The results closelymatch the major-elementchemistry (Von Damm et al., 1985) and isotopic compositions(Craig et al., 1980) of the hydrothermalsolutions presently emanating from ventsat 21øN on the East Pacific Rise. The calculatedsolution chemistry,for example, correctly predicts completeloss of Mg and SO,• and substantial increases in Si and Fe; however, discrepanciesexist in the predicted pH (5.5 versus 3.5 measured)and state of saturation of the solution with respectto greenschist-faciesminerals. -
Dynamical Models of Terrestrial Planet Formation
Dynamical Models of Terrestrial Planet Formation Jonathan I. Lunine, LPL, The University of Arizona, Tucson AZ USA, 85721. [email protected] David P. O’Brien, Planetary Science Institute, Tucson AZ USA 85719 Sean N. Raymond, CASA, University of Colorado, Boulder CO USA 80302 Alessandro Morbidelli, Obs. de la Coteˆ d’Azur, Nice, F-06304 France Thomas Quinn, Department of Astronomy, University of Washington, Seattle USA 98195 Amara L. Graps, SWRI, Boulder CO USA 80302 Revision submitted to Advanced Science Letters May 23, 2009 Abstract We review the problem of the formation of terrestrial planets, with particular emphasis on the interaction of dynamical and geochemical models. The lifetime of gas around stars in the process of formation is limited to a few million years based on astronomical observations, while isotopic dating of meteorites and the Earth-Moon system suggest that perhaps 50-100 million years were required for the assembly of the Earth. Therefore, much of the growth of the terrestrial planets in our own system is presumed to have taken place under largely gas-free conditions, and the physics of terrestrial planet formation is dominated by gravitational interactions and collisions. The ear- liest phase of terrestrial-planet formation involve the growth of km-sized or larger planetesimals from dust grains, followed by the accumulations of these planetesimals into ∼100 lunar- to Mars- mass bodies that are initially gravitationally isolated from one-another in a swarm of smaller plan- etesimals, but eventually grow to the point of significantly perturbing one-another. The mutual perturbations between the embryos, combined with gravitational stirring by Jupiter, lead to orbital crossings and collisions that drive the growth to Earth-sized planets on a timescale of 107 − 108 years. -
The Iron Planet Sex and Skin Color
PERIODICALS Yet, this is the key to the lesson, Kass says. necessary condition for national self- "God's dispersion of the nations is the PO- awareness and the possibility of a politics litical analog to the creation of woman: in- that will. hearken to the voice of what is stituting otherness and opposition, it is the eternal, true, and good." SCIENCE & TECHNOLOGY ''Mercu~'~Heart of Iron" by Clark R. Chapman, in Asfrononzy The Iron Planet (Nov. 19881, 1027 N. 7th St., Milwaukee, Wisc. 53233. More than a decade after America's un- plays a vita1 role in the two leading theo- manned Mariner 10 flew near the planet ries of the origins of the solar system. Ac- Mercury during 1974-75, scientists have fi- cording to one theory, formulated by cos- nally digested all of the data from the mochemist John Lewis during the 1970~~ flight. And they are starting to ask some the solar system was created in a more or big questions, reports Chapman, of Tuc- less orderly fashion. Lewis believes that son's Planetary Science Institute. the planets formed out of gases that cooled Located about midway between the and condensed. At some point, billions of Earth and the Sun, Mercury is a "truly bi- years ago, the sun flared up briefly, blast- zarre" planet. Its rock cmst is unusually ing away many gases. According to Lewis's thin; a "metallic iron core" accounts for theory, there should not be any sulfur, or 70 percent of the planet's weight. anything like it, on Mercury. The most surprising discovery made by A more recent theory, propounded by Mariner 10 was that the tiny planet has a George Wetherill of the Carnegie Institu- magnetic field, like Earth's but much tion, is that the solar system emerged from weaker. -
Alfred O. C. Nier
CHEMICAL HERITAGE FOUNDATION ALFRED O. C. NIER Transcript of Interviews Conducted by Michael A. Grayson and Thomas Krick at University of Minnesota Minneapolis, Minnesota on 7, 8, 9, and 10 April 1989 (With Subsequent Corrections and Additions) ACKNOWLEDGMENT This oral history is one in a series initiated by the Chemical Heritage Foundation on behalf of the American Society for Mass Spectrometry. The series documents the personal perspectives of individuals related to the advancement of mass spectrometric instrumentation, and records the human dimensions of the growth of mass spectrometry in academic, industrial, and governmental laboratories during the twentieth century. This project is made possible through the generous support of the American Society for Mass Spectrometry Upon Alfred O.C. Nier’s death in 1994, this oral history was designated Free Access. Please note: Users citing this interview for purposes of publication are obliged under the terms of the Chemical Heritage Foundation Oral History Program to credit CHF using the format below: Alfred O.C. Nier, interview by Michael A. Grayson and Thomas Krick at the University of Minnesota, Minneapolis, Minnesota, 7-10 April 1989 (Philadelphia: Chemical Heritage Foundation, Oral History Transcript # 0112). Chemical Heritage Foundation Oral History Program 315 Chestnut Street Philadelphia, Pennsylvania 19106 The Chemical Heritage Foundation (CHF) serves the community of the chemical and molecular sciences, and the wider public, by treasuring the past, educating the present, and inspiring the future. CHF maintains a world-class collection of materials that document the history and heritage of the chemical and molecular sciences, technologies, and industries; encourages research in CHF collections; and carries out a program of outreach and interpretation in order to advance an understanding of the role of the chemical and molecular sciences, technologies, and industries in shaping society. -
Sources of Variation in the Stable Isotopic Composition of Plants*
CHAPTER 2 Sources of variation in the stable isotopic composition of plants* JOHN D. MARSHALL, J. RENÉE BROOKS, AND KATE LAJTHA Introduction The use of stable isotopes of carbon, nitrogen, oxygen, and hydrogen to study physiological processes has increased exponentially in the past three decades. When Harmon Craig (1953, 1954), a geochemist and early pioneer of natural abundance stable isotopes, fi rst measured isotopic values of plant materials, he found that plants tended to have a fairly narrow δ13C range of −25 to −35‰. In these initial surveys, he was unable to fi nd large taxonomic or environmental effects on these values. Since that time ecologists have identi- fi ed clear isotopic signatures based not only on different photosynthetic pathways, but also on ecophysiological differences, such as photosynthetic water-use effi ciency (WUE) and sources of water and nitrogen used. As large empirical databases have accumulated and our theoretical understanding of isotopic composition has improved, scientists have continued to discover mismatches between theoretical and observed values, as well as confounding effects from sources and factors not previously considered. In the best tradi- tion of science, these discoveries have led to important new insights into physiological or ecological processes, as well as new uses of stable isotopes in plant ecophysiology. This chapter reviews the most common applications of stable isotope analysis in plant ecophysiology. Carbon isotopes Photosynthetic pathways 13 Plants contain less C than the atmospheric CO2 on which they rely for photosynthesis. They are therefore “depleted” of 13C relative to the atmo- sphere. This depletion is caused by enzymatic and physical processes that discriminate against 13C in favor of 12C. -
Chemical Heritage Foundation William S. Knowles
CHEMICAL HERITAGE FOUNDATION WILLIAM S. KNOWLES Transcript of an Interview Conducted by Michael A. Grayson at St. Louis, Missouri on 30 January 2008 (With Subsequent Corrections and Additions) This interview has been designated as Free Access. One may view, quote from, cite, or reproduce the oral history with the permission of CHF. Please note: Users citing this interview for purposes of publication are obliged under the terms of the Chemical Heritage Foundation Oral History Program to credit CHF using the format below: William S. Knowles, interview by Michael A. Grayson at St. Louis, Missouri, 30 January 2008 (Philadelphia: Chemical Heritage Foundation, Oral History Transcript # 0406). Chemical Heritage Foundation Oral History Program 315 Chestnut Street Philadelphia, Pennsylvania 19106 The Chemical Heritage Foundation (CHF) serves the community of the chemical and molecular sciences, and the wider public, by treasuring the past, educating the present, and inspiring the future. CHF maintains a world-class collection of materials that document the history and heritage of the chemical and molecular sciences, technologies, and industries; encourages research in CHF collections; and carries out a program of outreach and interpretation in order to advance an understanding of the role of the chemical and molecular sciences, technologies, and industries in shaping society. WILLIAM S. KNOWLES 1917 Born in Taunton, Massachusetts on 1 June Education 1939 A.B., Harvard University, Chemistry 1942 Ph.D., Columbia University, Steroids Professional Experience Monsanto, Dayton 1942-1944 Chemical Research and Development Monsanto, St. Louis 1944-1951 Organic Division Harvard University 1951-1952 Academic Leave, Total Synthesis of Steroids, R.B. Woodward Monsanto, St. -
Biosphere: How Life Alters Climate
THIS IS THE TEXT OF AN ESSAY IN THE WEB SITE “THE DISCOVERY OF GLOBAL WARMING” BY SPENCER WEART, HTTP://WWW.AIP.ORG/HISTORY/CLIMATE. AUGUST 2021. HYPERLINKS WITHIN THAT SITE ARE NOT INCLUDED IN THIS FILE. FOR AN OVERVIEW SEE THE BOOK OF THE SAME TITLE (HARVARD UNIV. PRESS, REV. ED. 2008). COPYRIGHT © 2003-2021 SPENCER WEART & AMERICAN INSTITUTE OF PHYSICS. Biosphere: How Life Alters Climate People had long speculated that the climate might be altered where forests were cut down, marshes drained or land irrigated. Scientists were skeptical. During the first half of the 20th century, they studied climate as a system of mechanical physics and mineral chemistry, churning along heedless of the planet’s thin film of living organisms. Then around 1960, evidence of a rise in carbon dioxide showed that at least one species, humanity, could indeed alter global climate. As scientists looked more deeply into how carbon moved in and out of the atmosphere, they discovered many ways that other organisms could also exert powerful influences. Forests in particular were deeply involved in the carbon cycle, and from the 1970s onward, scientists argued over just what deforestation might mean for climate. By the 1980s, it was certain that all the planet’s ecosystems were major players in the climate changes that would determine their own future. CARBON DIOXIDE AND THE BIOSPHERE (1938-1950S) - CAN PEOPLE CHANGE CLIMATE? - WHERE DOES THE CARBON GO? (1971-1980S) - METHANE (1979-1980S) - GAIA (1972-1980S) - GLOBAL WARMING FEEDBACKS “In our century the biosphere has acquired an entirely new meaning; it is being revealed as a planetary phenomenon of cosmic character.” — W.I. -
Water Is Not H2O†
y Water is Not H2O Michael Weisberg ([email protected]) Stanford University 1. Introduction In defending semantic externalism, philosophers of language have often assumed that there is a straightforward connection between scientific kinds and the natural kinds recognized by ordinary language users.1 For example, the claim that water is H2O assumes that the ordinary language kind water corresponds to a chemical kind, which contains all the molecules with molecular formula H2O as its members. This assumption about the coordination between ordinary language kinds and scientific kinds is important for the externalist program, because it is what allows us to discover empirically the extensions of ordinary language kind terms. While I am sympathetic to the semantic externalist project, I think that the discussion of chemical kinds by philosophers of language has been rather badly oversimplified, hiding difficulties that arise when we try to coordinate scientific kinds with the natural kinds recognized by ordinary language users.2 In this paper, I will examine these difficulties by looking more closely at the chemist’s notion of water. To help with this examination, I will begin by making explicit a principle on which I believe semantic externalists rely. The coordina- tion principle is the thesis that scientific kinds and the natural kinds recognized by natural language users line up or can be mapped onto one another one-to-one. A brief examination of an externalist picture of kind reference will show how the coordination principle is relied on. y Many thanks to Peter Godfrey-Smith, Michael Strevens, Anthony Everett, and Deena Skolnick who helped me to clarify the main ideas of this paper tremendously.