EUGENE SCIENCE CENTER We Are Aliens – a Guide for Educators Prepared by Haley Sharp, Eugene Science Center Planetarium Direct
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A Preliminary Report of the Battle of the Crater, 30 July 1864
Holding the Line A Preliminary Report of The Battle of the Crater 30 July 1864 Adrian Mandzy, Ph. D. Michelle Sivilich, Ph. D. Benjamin Lewis Fitzpatrick, Ph. D. Dan Sivilich Floyd Patrick Davis Kelsey P. Becraft Dakota Leigh Goedel Jeffrey A. McFadden Jessey C. Reed Jaron A. Rucker A PRELIMINARY REPORT ON THE SURVEY OF THE BATTLE OF THE CRATER, 30 JULY 1864 By Adrian Mandzy, Ph.D., Michelle Sivilich, Ph. D., Floyd Patrick Davis, Kelsey P. Becraft, Dakota Leigh Goedel, Jeffrey A. McFadden, Jessey C. Reed, and Jaron A. Rucker With a Contributions by Daniel Sivilich and Dr. Benjamin Lewis Fitzpatrick Report prepared for the Northeast Region Archeology Program National Park Service 115 John Street, 4th Floor Lowell, Massachusetts 01852-1195 _______________________________ Adrian Mandzy Principal Investigator ARPA Permit 2014.PETE.01 2 Abstract In March 2015, faculty and students from Morehead State University’s History program, along with members of the Battlefield Restoration and Archeological Volunteer Organization (BRAVO) conducted a survey of The Crater Battlefield. Fought on 30 July 1864, during the Siege of Petersburg, the Battle of the Crater, according to the National Park Service, is one of the most important events of the Civil War. The participation of African-American troops in the battle and the subsequent execution of black prisoners highlights the racial animosities that were the underpinning causes of this conflict. The goal of this project is to document the level of integrity of any archaeological resources connected with this field of conflict and to examine how far the Union troops advance beyond the mouth of the Crater. -
Astronomy Unusually High Magnetic Fields in the Coma of 67P/Churyumov-Gerasimenko During Its High-Activity Phase C
Astronomy Unusually high magnetic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase C. Goetz, B. Tsurutani, Pierre Henri, M. Volwerk, E. Béhar, N. Edberg, A. Eriksson, R. Goldstein, P. Mokashi, H. Nilsson, et al. To cite this version: C. Goetz, B. Tsurutani, Pierre Henri, M. Volwerk, E. Béhar, et al.. Astronomy Unusually high mag- netic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase. Astronomy and Astrophysics - A&A, EDP Sciences, 2019, 630, pp.A38. 10.1051/0004-6361/201833544. hal- 02401155 HAL Id: hal-02401155 https://hal.archives-ouvertes.fr/hal-02401155 Submitted on 9 Dec 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A&A 630, A38 (2019) Astronomy https://doi.org/10.1051/0004-6361/201833544 & © ESO 2019 Astrophysics Rosetta mission full comet phase results Special issue Unusually high magnetic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase C. Goetz1, B. T. Tsurutani2, P. Henri3, M. Volwerk4, E. Behar5, N. J. T. Edberg6, A. Eriksson6, R. Goldstein7, P. Mokashi7, H. Nilsson4, I. Richter1, A. Wellbrock8, and K. -
Thermal Regeneration of Sulfuric Acid Hydrates After Irradiation ⇑ Mark J
Icarus 219 (2012) 561–566 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Thermal regeneration of sulfuric acid hydrates after irradiation ⇑ Mark J. Loeffler , Reggie L. Hudson Astrochemistry Laboratory, NASA Goddard Space Flight Center, Mail Code 691, Greenbelt, MD 20771, United States article info abstract Article history: In an attempt to more completely understand the surface chemistry of the jovian icy satellites, we have Received 17 January 2012 investigated the effect of heating on two irradiated crystalline sulfuric acid hydrates, H2SO4Á4H2O and Revised 13 March 2012 H2SO4ÁH2O. At temperatures relevant to Europa and the warmer jovian satellites, post-irradiation heating Accepted 25 March 2012 recrystallized the amorphized samples and increased the intensities of the remaining hydrate’s infrared Available online 10 April 2012 absorptions. This thermal regeneration of the original hydrates was nearly 100% efficient, indicating that over geological times, thermally-induced phase transitions enhanced by temperature fluctuations will Keywords: reform a large fraction of crystalline hydrated sulfuric acid that is destroyed by radiation processing. Europa The work described is the first demonstration of the competition between radiation-induced amorphiza- Ices, IR spectroscopy Jupiter, Satellites tion and thermally-induced recrystallization in icy ionic solids relevant to the outer Solar System. Impact processes Published by Elsevier Inc. Cosmic rays 1. Introduction ic, salty, or acidic, could be transported to a surface by a variety of mechanisms (Kargel et al., 2000; Greenburg, 2010). Primordial sub- Remote sensing of Jupiter’s icy satellites has revealed that even surface SO2 (Noll et al., 1995) and CO2 (Moore et al., 1999) could though their surfaces are composed mostly of water ice (Kuiper, also be carried upward by geological processes. -
Early Observations of the Interstellar Comet 2I/Borisov
geosciences Article Early Observations of the Interstellar Comet 2I/Borisov Chien-Hsiu Lee NSF’s National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ 85719, USA; [email protected]; Tel.: +1-520-318-8368 Received: 26 November 2019; Accepted: 11 December 2019; Published: 17 December 2019 Abstract: 2I/Borisov is the second ever interstellar object (ISO). It is very different from the first ISO ’Oumuamua by showing cometary activities, and hence provides a unique opportunity to study comets that are formed around other stars. Here we present early imaging and spectroscopic follow-ups to study its properties, which reveal an (up to) 5.9 km comet with an extended coma and a short tail. Our spectroscopic data do not reveal any emission lines between 4000–9000 Angstrom; nevertheless, we are able to put an upper limit on the flux of the C2 emission line, suggesting modest cometary activities at early epochs. These properties are similar to comets in the solar system, and suggest that 2I/Borisov—while from another star—is not too different from its solar siblings. Keywords: comets: general; comets: individual (2I/Borisov); solar system: formation 1. Introduction 2I/Borisov was first seen by Gennady Borisov on 30 August 2019. As more observations were conducted in the next few days, there was growing evidence that this might be an interstellar object (ISO), especially its large orbital eccentricity. However, the first astrometric measurements do not have enough timespan and are not of same quality, hence the high eccentricity is yet to be confirmed. This had all changed by 11 September; where more than 100 astrometric measurements over 12 days, Ref [1] pinned down the orbit elements of 2I/Borisov, with an eccentricity of 3.15 ± 0.13, hence confirming the interstellar nature. -
Toxicological Review of Chloral Hydrate (CAS No. 302-17-0) (PDF)
EPA/635/R-00/006 TOXICOLOGICAL REVIEW OF CHLORAL HYDRATE (CAS No. 302-17-0) In Support of Summary Information on the Integrated Risk Information System (IRIS) August 2000 U.S. Environmental Protection Agency Washington, DC DISCLAIMER This document has been reviewed in accordance with U.S. Environmental Protection Agency policy and approved for publication. Mention of trade names or commercial products does not constitute endorsement or recommendation for use. Note: This document may undergo revisions in the future. The most up-to-date version will be made available electronically via the IRIS Home Page at http://www.epa.gov/iris. ii CONTENTS—TOXICOLOGICAL REVIEW for CHLORAL HYDRATE (CAS No. 302-17-0) FOREWORD .................................................................v AUTHORS, CONTRIBUTORS, AND REVIEWERS ................................ vi 1. INTRODUCTION ..........................................................1 2. CHEMICAL AND PHYSICAL INFORMATION RELEVANT TO ASSESSMENTS ..... 2 3. TOXICOKINETICS RELEVANT TO ASSESSMENTS ............................3 4. HAZARD IDENTIFICATION ................................................6 4.1. STUDIES IN HUMANS - EPIDEMIOLOGY AND CASE REPORTS .................................................6 4.2. PRECHRONIC AND CHRONIC STUDIES AND CANCER BIOASSAYS IN ANIMALS ................................8 4.2.1. Oral ..........................................................8 4.2.2. Inhalation .....................................................12 4.3. REPRODUCTIVE/DEVELOPMENTAL STUDIES ..........................13 -
Confronting Antisemitism in Modern Media, the Legal and Political Worlds an End to Antisemitism!
Confronting Antisemitism in Modern Media, the Legal and Political Worlds An End to Antisemitism! Edited by Armin Lange, Kerstin Mayerhofer, Dina Porat, and Lawrence H. Schiffman Volume 5 Confronting Antisemitism in Modern Media, the Legal and Political Worlds Edited by Armin Lange, Kerstin Mayerhofer, Dina Porat, and Lawrence H. Schiffman ISBN 978-3-11-058243-7 e-ISBN (PDF) 978-3-11-067196-4 e-ISBN (EPUB) 978-3-11-067203-9 DOI https://10.1515/9783110671964 This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. For details go to https://creativecommons.org/licenses/by-nc-nd/4.0/ Library of Congress Control Number: 2021931477 Bibliographic information published by the Deutsche Nationalbibliothek The Deutsche Nationalbibliothek lists this publication in the Deutsche Nationalbibliografie; detailed bibliographic data are available on the Internet at http://dnb.dnb.de. © 2021 Armin Lange, Kerstin Mayerhofer, Dina Porat, Lawrence H. Schiffman, published by Walter de Gruyter GmbH, Berlin/Boston The book is published with open access at www.degruyter.com Cover image: Illustration by Tayler Culligan (https://dribbble.com/taylerculligan). With friendly permission of Chicago Booth Review. Printing and binding: CPI books GmbH, Leck www.degruyter.com TableofContents Preface and Acknowledgements IX LisaJacobs, Armin Lange, and Kerstin Mayerhofer Confronting Antisemitism in Modern Media, the Legal and Political Worlds: Introduction 1 Confronting Antisemitism through Critical Reflection/Approaches -
Muslim Scientists and Thinkers
MUSLIM SCIENTISTS AND THINKERS Syed Aslam Second edition 2010 Copyright 2010 by Syed Aslam Publisher The Muslim Observer 29004 W. Eight Mile Road Farmington, MI 48336 Cover Statue of Ibn Rushd Cordoba, Spain ISBN 978-1-61584-980-2 Printed in India Lok-Hit Offset Shah-e-Alam Ahmedabad Gujarat ii Dedicated to Ibn Rushd and other Scientists and Thinkers of the Islamic Golden Age iii CONTENTS Acknowledgments ................................................VI Foreword .............................................................VII Introduction ..........................................................1 1 Concept of Knowledge in Islam ............................8 2 Abu Musa Jabir Ibn Hayyan..................................25 3 Al-Jahiz abu Uthman Ibn Bahar ...........................31 4 Muhammad Ibn Musa al-Khwarizmi....................35 5 Abu Yaqoub Ibn Ishaq al-Kindi ............................40 6 Muhammad bin Zakaria Razi ...............................45 7 Jabir ibn Sinan al-Batani.......................................51 8 Abu Nasar Mohammad ibn al-Farabi....................55 9 Abu Wafa ibn Ismail al-Buzjani ...........................61 10 Abu Ali al-Hasan ibn al-Haytham .......................66 11 Abu Rayhan ibn al-Biruni ....................................71 12 Ali al-Hussain ibn Sina ........................................77 13 Abu Qasim ibn al-Zahrawi ..................................83 iv 14 Omar Khayyam ...................................................88 15 Abu Hamid al-Ghazali .........................................93 -
Hydrate Risk Assessment and Restart-Procedure Optimization Of
Hydrate Risk Assessment and Restart- Procedure Optimization of an Offshore Well Using a Transient Hydrate Prediction Model L.E. Zerpa, E.D. Sloan, C.A. Koh, and A.K. Sum, Colorado School of Mines Summary This paper focuses on the application of the gas-hydrate model A produced-hydrocarbon stream from a wellhead encounters for- to study the hydrate-plugging risk of an offshore well with a typ- mation of solid gas-hydrate deposits, which plug flowlines and ical geometry and fluid properties from the Caratinga field located which are one of the most challenging problems in deep subsea fa- in the Campos basin, Brazil. Three different periods of the well cilities. This paper describes a gas-hydrate model for oil-dominated life are considered: an early stage with low production gas/oil ratio systems, which can be used for the design and optimization of facil- (GOR) and low water cut, a middle stage with an increased GOR, ities focusing on the prevention, management, and remediation of and a late stage with higher GOR and higher water cut. The hy- hydrates in flowlines. Using a typical geometry and fluid properties drate-plugging risk is estimated from the calculation of three per- of an offshore well from the Caratinga field located in the Campos formance measures (pressure drop along flowline, hydrate volume basin in Brazil, the gas-hydrate model is applied to study the hy- fraction in pipe, and hydrate-slurry relative viscosity) in an attempt drate-plugging risk at three different periods of the well life. Addi- to quantify the plugging risk. -
Synthesis of Methane Hydrate from Ice Powder Accelerated by Doping
www.nature.com/scientificreports OPEN Synthesis of Methane Hydrate from Ice Powder Accelerated by Doping Ethanol into Methane Gas Received: 2 May 2019 Yen-An Chen1, Liang-Kai Chu1, Che-Kang Chu1, Ryo Ohmura2 & Li-Jen Chen 1,2 Accepted: 13 August 2019 Clathrate hydrate is considered to be a potential medium for gas storage and transportation. Slow Published: xx xx xxxx kinetics of hydrate formation is a hindrance to the commercialized process development of such applications. The kinetics of methane hydrate formation from the reaction of ice powder and methane gas doped with/without saturated ethanol vapor at constant pressure of 16.55 ± 0.20 MPa and constant temperature ranging from −15 to −1.0 °C were investigated. The methane hydrate formation can be dramatically accelerated by simply doping ethanol into methane gas with ultralow ethanol concentration (<94 ppm by mole fraction) in the gas phase. For ethanol-doped system 80.1% of ice powder were converted into methane hydrate after a reaction time of 4 h, while only 26.6% of ice powder was converted into methane hydrate after a reaction time of 24 h when pure methane gas was used. Furthermore, this trace amount of ethanol could also substantially suppress the self-preservation efect to enhance the dissociation rate of methane hydrate (operated at 1 atm and temperatures below the ice melting point). In other words, a trace amount of ethanol doped in methane gas can act as a kinetic promoter for both the methane hydrate formation and dissociation. Clathrate hydrates are ice-like nonstoichiometric crystalline compounds formed by guest molecules encapsulated in the hydrogen bonded water cages at elevated pressures and low temperatures1. -
Diamond Craters Oregon's Geologic
Text by Ellen M. Benedict, 1985 Features at stops correspond to points on a clock ago, a huge mass of hot gases, volcanic ashes, bits face. Imagine that you are standing in the middle of a of pumice and other pyroclastics (fire-broken rock) Travel And Hiking Hints clock face. Twelve o’clock is the road in front of you violently erupted. The blast – greater than the May and 6 o’clock the road behind. If you always align the 18, 1980, eruption of Mt. St. Helens – deposited a Diamond Craters is located in the high desert country clock face with the road, you should be able to locate layer of pyroclastics 30 to 130 feet thick over an area about 55 miles southeast of Burns, Oregon. It’s an the features. almost 7,000 square miles! isolated place and some precautions should be taken . when traveling in the area. Start Tour. Mileage begins halfway Pyroclastics are between milepost 40 and 41 on State normal behavior Diamond Craters has no tourist facilities. The nearest Highway 205 at the junction to Diamond. for magmas place where gasoline is sold is at Frenchglen. Turn left. (subsurface That’s the opinion held by scores of molten rocks) Keep your scientists and educators who have visited Diamond, Oregon, a small ranching community, was of rhyolitic (a vehicle on named in 1874 for Mace McCoy’s Diamond brand. volcanic material and studied the area. It has the “best and hard-packed The nearby craters soon became known as Diamond related to granite) most diverse basaltic volcanic features in the road surfaces Craters. -
Interstellar Comet 2I/Borisov Exhibits a Structure Similar to Native Solar System Comets⋆
Mon. Not. R. Astron. Soc. 000, 1–5 (201X) Printed 4 April 2020 (MN LATEX style file v2.2) Interstellar Comet 2I/Borisov exhibits a structure similar to native Solar System comets⋆ F. Manzini1†, V. Oldani1, P. Ochner2,3, and L.R.Bedin2 1Stazione Astronomica di Sozzago, Cascina Guascona, I-28060 Sozzago (Novara), Italy 2INAF-Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy 3Department of Physics and Astronomy-University of Padova, Via F. Marzolo 8, I-35131 Padova, Italy Letter: Accepted 2020 April 1. Received 2020 April 1; in original form 2019 November 22. ABSTRACT We processed images taken with the Hubble Space Telescope (HST) to investigate any morphological features in the inner coma suggestive of a peculiar activity on the nucleus of the interstellar comet 2I/Borisov. The coma shows an evident elongation, in the position angle (PA) ∼0◦-180◦ direction, which appears related to the presence of a jet originating from a single active source on the nucleus. A counterpart of this jet directed towards PA ∼10◦ was detected through analysis of the changes of the inner coma morphology on HST images taken in different dates and processed with different filters. These findings indicate that the nucleus is probably rotating with a spin axis projected near the plane of the sky and oriented at PA ∼100◦-280◦, and that the active source is lying in a near-equatorial position. Subsequent observations of HST allowed us to determine the direction of the spin axis at RA = 17h20m ±15◦ and Dec = −35◦ ±10◦. Photometry of the nucleus on HST images of 12 October 2019 only span ∼7 hours, insufficient to reveal a rotational period. -
Closing the Gap Between Ground Based and In-Situ Observations of Cometary Dust Activity: Investigating Comet 67P to Gain a Deeper Understanding of Other Comets
Closing the gap between ground based and in-situ observations of cometary dust activity: Investigating comet 67P to gain a deeper understanding of other comets. Raphael Marschall & Oleksandra Ivanova et al. Abstract When cometary dust particles are ejected from the surface they are accelerated because of the surrounding gas flow from sublimating ices. As these particles travel millions of kilometres from their origin into the solar system they produce the magnificent tails commonly associated with comets. During their long journey the dust particles transition through different regimes of changing dominant forces such as gas drag, cometary gravity, solar radiation pressure, and solar gravity. The transition and link between the different regimes is to this day poorly understood. There are two main reasons for this. Firstly, the problem covers a vast range in spatial and temporal scales that need to be matched taking into account multiple transitions of the force regime. Furthermore, observational data covering these large spatial and temporal scales for at least one comet and thus characterising it in great detail has been lacking until recently. For comet 67P/Churyumov-Gerasimenko (hereafter 67P) a small number of large scale struc- tures in the outer dust coma and tail have been found from ground based observations. Con- versely ESA's Rosetta mission has shown many small scale structures defining the innermost coma close to the nucleus surface. This disconnect between the observations on these different scales has yet to be understood and explained. Solving this problem thus requires an interdisciplinary approach. This ISSI team shall bring together experts of the recent observational data from ground and in-situ of comet 67P as well as theorists that are able to model the dynamical processes over these different scales.