What If the Earth Stopped Spinning? 3 Maser to Predict Milky Way's Fate 8
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New Candidate Pits and Caves at High Latitudes on the Near Side of the Moon
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2733.pdf NEW CANDIDATE PITS AND CAVES AT HIGH LATITUDES ON THE NEAR SIDE OF THE MOON. 1,2 1,3,4 1 2 Wynnie Avent II and Pascal Lee , S ETI Institute, Mountain View, VA, USA, V irginia Polytechnic Institute 3 4 and State University Blacksburg, VA, USA. M ars Institute, N ASA Ames Research Center. Summary: 35 new candidate pits are identified in Anaxagoras and Philolaus, two high-latitude impact structures on the near side of the Moon. Introduction: Since the discovery in 2009 of the Marius Hills Pit (Haruyama et al. 2009), a.k.a. the “Haruyama Cavern”, over 300 hundred pits have been identified on the Moon (Wagner & Robinson 2014, Robinson & Wagner 2018). Lunar pits are small (10 to 150 m across), steep-walled, negative relief features (topographic depressions), surrounded by funnel-shaped outer slopes and, unlike impact craters, no raised rim. They are interpreted as collapse features resulting from the fall of the roof of shallow (a few Figure 1: Location of studied craters (Polar meters deep) subsurface voids, generally lava cavities. projection). Although pits on the Moon are found in mare basalt, impact melt deposits, and highland terrain of the >300 Methods: Like previous studies searching for pits pits known, all but 16 are in impact melts (Robinson & (Wagner & Robinson 2014, Robinson & Wagner 2018, Wagner 2018). Many pits are likely lava tube skylights, Lee 2018a,b,c), we used imaging data collected by the providing access to underground networks of NASA Lunar Reconnaissance Orbiter (LRO) Narrow tunnel-shaped caves, including possibly complex Angle Camera (NAC). -
Frontiers of Quantum and Mesoscopic Thermodynamics 29 July - 3 August 2013, Prague, Czech Republic
Frontiers of Quantum and Mesoscopic Thermodynamics 29 July - 3 August 2013, Prague, Czech Republic Under the auspicies of Ing. Milosˇ Zeman President of the Czech Republic Milan Stˇ echˇ President of the Senate of the Parliament of the Czech Republic Prof. Ing. Jirˇ´ı Drahos,ˇ DrSc., dr. h. c. President of the Academy of Sciences of the Czech Republic Dominik Cardinal Duka OP Archbishop of Prague Supported by • Committee on Education, Science, Culture, Human Rights and Petitions of the Senate of the Parliament of the Czech Republic • Institute of Physics, the Academy of Sciences of the Czech Republic • Institute for Theoretical Physics, University of Amsterdam, The Netherlands • Department of Physics, Texas A&M University, USA • Institut de Physique Theorique,´ CEA/CNRS Saclay, France Topics • Foundations of quantum physics • Non-equilibrium statistical physics • Quantum thermodynamics • Quantum measurement, entanglement and coherence • Dissipation, dephasing, noise and decoherence • Quantum optics • Macroscopic quantum behavior, e.g., cold atoms, Bose-Einstein condensates • Physics of quantum computing and quantum information • Mesoscopic, nano-electromechanical and nano-optical systems • Biological systems, molecular motors • Cosmology, gravitation and astrophysics Scientific Committee Chair: Theo M. Nieuwenhuizen (University of Amsterdam) Co-Chair: Vaclav´ Spiˇ ckaˇ (Institute of Physics, Acad. Sci. CR, Prague) Raymond Dean Astumian (University of Maine, Orono) Roger Balian (IPhT, Saclay) Gordon Baym (University of Illinois at Urbana -
Project Selene: AIAA Lunar Base Camp
Project Selene: AIAA Lunar Base Camp AIAA Space Mission System 2019-2020 Virginia Tech Aerospace Engineering Faculty Advisor : Dr. Kevin Shinpaugh Team Members : Olivia Arthur, Bobby Aselford, Michel Becker, Patrick Crandall, Heidi Engebreth, Maedini Jayaprakash, Logan Lark, Nico Ortiz, Matthew Pieczynski, Brendan Ventura Member AIAA Number Member AIAA Number And Signature And Signature Faculty Advisor 25807 Dr. Kevin Shinpaugh Brendan Ventura 1109196 Matthew Pieczynski 936900 Team Lead/Operations Logan Lark 902106 Heidi Engebreth 1109232 Structures & Environment Patrick Crandall 1109193 Olivia Arthur 999589 Power & Thermal Maedini Jayaprakash 1085663 Robert Aselford 1109195 CCDH/Operations Michel Becker 1109194 Nico Ortiz 1109533 Attitude, Trajectory, Orbits and Launch Vehicles Contents 1 Symbols and Acronyms 8 2 Executive Summary 9 3 Preface and Introduction 13 3.1 Project Management . 13 3.2 Problem Definition . 14 3.2.1 Background and Motivation . 14 3.2.2 RFP and Description . 14 3.2.3 Project Scope . 15 3.2.4 Disciplines . 15 3.2.5 Societal Sectors . 15 3.2.6 Assumptions . 16 3.2.7 Relevant Capital and Resources . 16 4 Value System Design 17 4.1 Introduction . 17 4.2 Analytical Hierarchical Process . 17 4.2.1 Longevity . 18 4.2.2 Expandability . 19 4.2.3 Scientific Return . 19 4.2.4 Risk . 20 4.2.5 Cost . 21 5 Initial Concept of Operations 21 5.1 Orbital Analysis . 22 5.2 Launch Vehicles . 22 6 Habitat Location 25 6.1 Introduction . 25 6.2 Region Selection . 25 6.3 Locations of Interest . 26 6.4 Eliminated Locations . 26 6.5 Remaining Locations . 27 6.6 Chosen Location . -
Robert Patrick (Bob) Goldstein James L
Robert Patrick (Bob) Goldstein James L. Peacock III Distinguished Professor Biology Department University of North Carolina at Chapel Hill Chapel Hill, NC 27599-3280 USA email bobg @ unc.edu, phone 919 843-8575 http://www.bio.unc.edu/faculty/goldstein/ PROFESSIONAL EXPERIENCE 1999-current Faculty, UNC Chapel Hill Biology Department and Member, Lineberger Comprehensive Cancer Center EDUCATION PhD: University of Texas at Austin, 1992, Zoology BS: Union College, Schenectady, New York, 1988, Biology RESEARCH TRAINING 1996-1999 Miller Institute Postdoctoral Research Fellow, University of California, Berkeley, Department of Molecular and Cell Biology, Laboratory of Dr. David Weisblat. 1992-1996 Postdoctoral Fellow, MRC Laboratory of Molecular Biology, Cambridge, England. Laboratory of Dr. John White 1992-1993. Independent 1993-1996. 1988-1992 PhD student, University of Texas at Austin. Laboratory of Dr. Gary Freeman. AWARDS 2018 Chapman Family Teaching Award, UNC Chapel Hill 2016 James L. Peacock III Distinguished Professor 2008 Elected Life Member of Clare Hall, Cambridge University 2007 Guggenheim Fellow 2007 Visiting Fellow, Clare Hall, Cambridge University 2005 Phillip and Ruth Hettleman Prize for Artistic and Scholarly Achievement by Young Faculty at UNC Chapel Hill 2000-2004 Pew Scholar 2000-2002 March of Dimes Basil O'Connor Scholar 1996-1998 Miller Institute Research Fellow, University of California, Berkeley 1996 Medical Research Council Postdoctoral Fellow, Cambridge, England 1995 Development Traveling Fellow 1994-1996 Human Frontiers -
Delayed-Choice Gedanken Experiments and Their Realizations
REVIEWS OF MODERN PHYSICS, VOLUME 88, JANUARY–MARCH 2016 Delayed-choice gedanken experiments and their realizations Xiao-song Ma* Institute for Quantum Optics and Quantum Information (IQOQI), Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria, Department of Electrical Engineering, Yale University, 15 Prospect Street, New Haven, Connecticut 06520, USA, and National Laboratory of Solid State Microstructures, School of Physics, Collaborative Innovation Center of Advanced Microstructures, Nanjing University, Nanjing 210093, China † Johannes Kofler Max Planck Institute of Quantum Optics (MPQ), Hans-Kopfermann-Straße 1, 85748 Garching, Germany ‡ Anton Zeilinger Vienna Center of Quantum Science and Technology (VCQ), University of Vienna, Boltzmanngasse 5, 1090 Vienna, Austria and Institute for Quantum Optics and Quantum Information (IQOQI), Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria (published 3 March 2016) The wave-particle duality dates back to Einstein’s explanation of the photoelectric effect through quanta of light and de Broglie’s hypothesis of matter waves. Quantum mechanics uses an abstract description for the behavior of physical systems such as photons, electrons, or atoms. Whether quantum predictions for single systems in an interferometric experiment allow an intuitive under- standing in terms of the particle or wave picture depends on the specific configuration which is being used. In principle, this leaves open the possibility that quantum systems always behave either definitely as a particle or definitely as a wave in every experimental run by a priori adapting to the specific experimental situation. This is precisely what is tried to be excluded by delayed-choice experiments, in which the observer chooses to reveal the particle or wave character of a quantum system—or even a continuous transformation between the two—at a late stage of the experiment. -
Determining the Structural Stability of Lunar Lava Tubes
46th Lunar and Planetary Science Conference (2015) 2174.pdf DETERMINING THE STRUCTURAL STABILITY OF LUNAR LAVA TUBES. D. M. Blair1*, L. Chappaz2, R. Sood2, C. Milbury1, H. J. Melosh1, K. C. Howell2, and A. M. Freed1. 1,* Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA, [email protected]; 2School of Aeronautics and Astronautics, Purdue University, West Lafayette, IN, USA. Introduction: Recent in-depth analysis of lunar wider lava tube or a thinner roof, but do not quantify gravity data from the Gravity Recovery And Interior what difference an arched roof would make. Laboratory (GRAIL) spacecraft has suggested the In caves on Earth that occur in bedded rock, failure possibility of lava tubes on the Moon with diameters in of the cave’s roof tends to occur one bed at a time, excess of 1 km [1, 2]. Could such features be progressing upwards [9]. This means that the structurally stable? What is the theoretical maximum mechanical “roof thickness” of a lava tube should be size of a lunar lava tube? Here we attempt to address considered to be the thickness of the flows that form those questions and improve on prior estimates of the the roof and not the total depth at which the tube is same by using modern numerical modeling techniques. buried. Lava flows thicknesses on the moon vary over Background: The presence of sublunarean voids a broad range, from 1–14 m in the skylights in Mare has recently been confirmed via the observation of Tranquilitatis and elsewhere [5] to ~80–600 m in "skylights" in several lunar maria [3, 4, 5]. -
Works of Love
reader.ad section 9/21/05 12:38 PM Page 2 AMAZING LIGHT: Visions for Discovery AN INTERNATIONAL SYMPOSIUM IN HONOR OF THE 90TH BIRTHDAY YEAR OF CHARLES TOWNES October 6-8, 2005 — University of California, Berkeley Amazing Light Symposium and Gala Celebration c/o Metanexus Institute 3624 Market Street, Suite 301, Philadelphia, PA 19104 215.789.2200, [email protected] www.foundationalquestions.net/townes Saturday, October 8, 2005 We explore. What path to explore is important, as well as what we notice along the path. And there are always unturned stones along even well-trod paths. Discovery awaits those who spot and take the trouble to turn the stones. -- Charles H. Townes Table of Contents Table of Contents.............................................................................................................. 3 Welcome Letter................................................................................................................. 5 Conference Supporters and Organizers ............................................................................ 7 Sponsors.......................................................................................................................... 13 Program Agenda ............................................................................................................. 29 Amazing Light Young Scholars Competition................................................................. 37 Amazing Light Laser Challenge Website Competition.................................................. 41 Foundational -
Investigating the Neutral Sodium Emissions Observed at Comets
Investigating the neutral sodium emissions observed at comets K. S. Birkett M.Sci. Physics, Imperial College London, UK (2012) Department of Space and Climate Physics University College London Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey. RH5 6NT. United Kingdom THESIS Submitted for the degree of Doctor of Philosophy, University College London 2017 2 I, Kimberley Si^anBirkett, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. 3 Abstract Neutral sodium emission is typically very easy to detect in comets, and has been seen to form a distinct neutral sodium tail at some comets. If the source of neutral cometary sodium could be determined, it would shed light on the composition of the comet, therefore allowing deeper understanding of the conditions present in the early solar system. Detection of neutral sodium emission at other solar system objects has also been used to infer chemical and physical processes that are difficult to measure directly. Neutral cometary sodium tails were first studied in depth at comet Hale-Bopp, but to date the source of neutral sodium in comets has not been determined. Many authors considered that orbital motion may be a significant factor in conclusively identifying the source of neutral sodium, so in this work details of the development of the first fully heliocentric distance and velocity dependent orbital model, known as COMPASS, are presented. COMPASS is then applied to a range of neutral sodium observations, includ- ing spectroscopic measurements at comet Hale-Bopp, wide field images of comet Hale- Bopp, and SOHO/LASCO observations of neutral sodium tails at near-Sun comets. -
80 Stephen Paget Memorial Lecture and Openness Awards Ceremony 5
80th Stephen Paget Memorial Lecture and Openness Awards Ceremony 5th December 2016 Royal College of Physicians, London #ConcordatOpenness Programme 18:00 Arrival and Refreshments 18:30 Welcome Address 18:40 Openness Awards Internal or sector engagement activity Public engagement activity Media engagement or media stories Website or use of new media Individual award 19:00 80th Paget Lecture by Professor Sir Mark Walport Animal Research – Then and Now 20:00 Drinks Reception 21:30 End The Stephen Paget Memorial Lecture The Stephen Paget Memorial Lecture is a scientific lecture to commemorate the life of Dr Stephen Paget. Stephen Paget (1855 – 1926) was the founder of the Research Defence Society, a forerunner of Understanding Animal Research. He believed passionately that better science and understanding of physiology would lead to better medical treatments. After his death in 1926, he was greatly missed by his medical colleagues and the scientific community. The first Stephen Paget memorial lecture was given in 1927 to commemorate his life and allow leading bio-medical scientists of the day to talk about their research. The Openness Awards The Concordat on Openness launched in May 2014 and has to date brought together 109 organisations in a pledge to be more open and transparent about the use of animals in research. This year the Openness Awards celebrate five recipients that have met the Concordat commitments and encouraged the widespread sharing of best practice. Professor Sir Mark Walport, FRS, FMedSci Sir Mark is the Chief Scientific Adviser to HM Government and Head of the Government Office for Science. Previously, Sir Mark was Director of the Wellcome Trust. -
Frontiers of Quantum and Mesoscopic Thermodynamics 14 - 20 July 2019, Prague, Czech Republic
Frontiers of Quantum and Mesoscopic Thermodynamics 14 - 20 July 2019, Prague, Czech Republic Under the auspicies of Ing. Miloš Zeman President of the Czech Republic Jaroslav Kubera President of the Senate of the Parliament of the Czech Republic Milan Štˇech Vice-President of the Senate of the Parliament of the Czech Republic Prof. RNDr. Eva Zažímalová, CSc. President of the Czech Academy of Sciences Dominik Cardinal Duka OP Archbishop of Prague Supported by • Committee on Education, Science, Culture, Human Rights and Petitions of the Senate of the Parliament of the Czech Republic • Institute of Physics, the Czech Academy of Sciences • Department of Physics, Texas A&M University, USA • Institute for Theoretical Physics, University of Amsterdam, The Netherlands • College of Engineering and Science, University of Detroit Mercy, USA • Quantum Optics Lab at the BRIC, Baylor University, USA • Institut de Physique Théorique, CEA/CNRS Saclay, France Topics • Non-equilibrium quantum phenomena • Foundations of quantum physics • Quantum measurement, entanglement and coherence • Dissipation, dephasing, noise and decoherence • Many body physics, quantum field theory • Quantum statistical physics and thermodynamics • Quantum optics • Quantum simulations • Physics of quantum information and computing • Topological states of quantum matter, quantum phase transitions • Macroscopic quantum behavior • Cold atoms and molecules, Bose-Einstein condensates • Mesoscopic, nano-electromechanical and nano-optical systems • Biological systems, molecular motors and -
Extra-Terrestrial Meteors
LIST OF CONTRIBUTORS apostolos christou Armagh Observatory and Planetarium College Hill, BT61 9DG Northern Ireland, UK jeremie vaubaillon IMCCE, Observatoire de Paris Paris 75014, France paul withers Astronomy Department, Boston University 725 Commonwealth Avenue Boston MA 02215, USA ricardo hueso Fisica Aplicada I Escuela de Ingenieria de Bilbao Plaza Ingeniero Torres Quevedo 1 48013 Bilbao, Spain rosemary killen NASA/Goddard Space Flight Center Planetary Magnetospheres, Code 695 Greenbelt MD 20771, USA arXiv:2010.14647v1 [astro-ph.EP] 27 Oct 2020 1 1 Extra-Terrestrial Meteors 1.1 Introduction cometary orbits, all-but-invisible except where the particles are packed densely enough to be detectable, typically near The beginning of the space age 60 years ago brought about the comet itself (Sykes and Walker, 1992; Reach and Sykes, a new era of discovery for the science of astronomy. Instru- 2000; Gehrz et al., 2006). Extending meteor observations ments could now be placed above the atmosphere, allowing to other planetary bodies allows us to map out these access to new regions of the electromagnetic spectrum and streams and investigate the nature of comets whose mete- unprecedented angular and spatial resolution. But the im- oroid streams do not intersect the Earth. Observations of pact of spaceflight was nowhere as important as in planetary showers corresponding to the same stream at two or more and space science, where it now became possible – and this planets will allow to study a stream’s cross-section. In ad- is still the case, uniquely among astronomical disciplines – dition, the models used to extract meteoroid parameters to physically touch, sniff and directly sample the bodies and from the meteor data are fine-tuned, to a certain degree, for particles of the solar system. -
D a R K N E S S V I S I B L E : I N S T R U M E N Tat
DARKNESS VISIBLE: INSTRUMENTATION AND THERMAL DESIGN TO ACCESS THE HIDDEN MOON Jeffrey E. Van Cleve1, Jonathan D. 1 2 In poetic language, people often talk about “The Dark Side of the Moon,” while their astronomical meaning is the “Far Side of the Moon.” In this workshop, we are literally discussing the dark Weinberg , Clive R. Neal , Richard 3 1 Moon – the entire Moon during the 14-day lunar night at the equator, and the regions of eternal darkness in polar craters that are rich in volatiles1 which may be rich in volatiles for use as C. Elphic , Gary Mills , Kevin resources, and as a valuable record of the Moon’s history. The dark Moon has been hidden for most of the history of spaceflight, as no human missions and few robotic missions have persisted Weed1, David Glaister1 through even one lunar night, and no missions whatsoever have landed in the permanently-shadowed regions. In this poster, we discuss “Night” mission concepts, previously developed by the 1 authors with NASA funding, that remain directly relevant to NASA robotic and human science and exploration of the Moon - a long-lived (> 6 y) lunar geophysical network and a Discovery-class Ball Aerospace, Boulder CO mission for the in-situ investigation of volatiles in the lunar polar cold traps. We also discuss Ball instrument and thermal technology enabling survival, situational awareness, and operations in 2Notre Dame the dark Moon, including low-light and thermal cameras, flash lidars, advanced multi-layer insulation (MLI), and phase-change material “hockey pucks” that can damp out thermal transients to 3 help moving platforms scuttle through dark regions for 24 h or so on their way between illuminated area such as “the peaks of eternal light” near the lunar south pole, without expending NASA-Ames precious stored electrical power for heat.