6Th Grade Science Distance Learning Packet Week 2
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Illuminating Eclipses: Astronomy and Chronology in King Lear
Brief Chronicles Vol. II (2010) 32 Illuminating Eclipses: Astronomy and Chronology in King Lear Hanno Wember ohann Gottfried Herder wrote his famous essay Shakespeare in 1772. He was (as Wieland, Lessing and, of course, Goethe and Schiller) one of the 18th century German writers “who first embraced Shakespeare and welcomed his Jgenius as a dramatist.”1 In his 1980 introduction to Herder’s essay, Konrad Nussbächer wrote: “Shakespeare is not, as it appeared in the 18th century, a natural genius growing up in the wild, but a highly cultured, artful Renaissance poet and practitioner of the stage.” Astronomy was one of the liberal arts and sciences a “highly cultured” man of Renaissance England was expected to know. This essay will review a few illuminating examples of Shakespeare’s profound knowledge of astronomy, and will examine a new astronomical reference that could shed significant new light on Shakespearean chronology. Shakespeare’s Astronomy In many regards Shakespeare had a better knowledge of the relationship between the moon and the tides2 than his distinguished contemporary Galileo (1564 - 1642), who tried to explain the tides by the two motions of the earth, correlating to the day and the year.3 This was an erroneous explanation for ebb and flow. But while Galileo refused to acknowledge any tidal influence of the moon, Bernardo knew better, referring to the moon as the Brief Chronicles Vol. II (2010) 33 moist star Upon whose influence Neptune’s empire stands (Hamlet, I.1.135)4 To Prince Henry, likewise, the moon commands the tides: The fortune of us that are moon’s men doth ebb and flow like the sea, being governed as the sea is by the moon…..Now in as low an ebb as the foot of the ladder, and by and by in as high a flow as the ridge of the gallows. -
Variation of Secondary Cosmic Gamma Ray Flux During Lunar Eclipse
Variation of secondary cosmic gamma ray flux during lunar eclipse S. Roy* , S. Chatterjee , S. Chakraborty** , S. Biswas , S. Das , S. K. Ghosh , S. Raha Department of Physics (CAPSS), Bose Institute, Kolkata, India. E-mail: [email protected] Introduction Astronomical events such as Solar eclipses and Lunar eclipses provide the opportunity for studying the disturbance produced in the atmosphere and its effect on cosmic ray intensity. There are earlier reports on decrease in secondary cosmic gamma ray (SCGR) flux during solar eclipse and enhancement of the same during lunar eclipse [1-4]. We have measured the variation of SCGR flux during two lunar eclipses that took place in India in the year 2018, one on 31st of January and the other on 27th of July. Both the measurements have been carried out in the Detector laboratory of Bose Institute, Kolkata, India, using NaI (Tl) scintillator detector. We observed slight increment of SCGR during the lunar eclipse of January. We did not observe any significant changes in SCGR during lunar eclipse of July. Experimental Setup ❖ NaI(Tl) scintillator detector is used. Size of the crystal: 5.1cm × 5.1cm ❖ Gamma ray sources used for detector calibration: 137Cs (662 keV), ❖ PMT bias: +600V. Signals are amplified and shaped before sending 60Co (1173 keV and 1332 keV) and 22Na (551 keV) them to MCA for energy spectrum accumulation ORTEC-556 ORTEC-671 Schematic of the signal processing electronics Picture of the experimental setup Gamma ray spectra with different configurations of lead shielding ADC -
DNVGL-OS-E402 Diving Systems
OFFSHORE STANDARDS DNVGL-OS-E402 Edition January 2017 Diving systems The content of this service document is the subject of intellectual property rights reserved by DNV GL AS ("DNV GL"). The user accepts that it is prohibited by anyone else but DNV GL and/or its licensees to offer and/or perform classification, certification and/or verification services, including the issuance of certificates and/or declarations of conformity, wholly or partly, on the basis of and/or pursuant to this document whether free of charge or chargeable, without DNV GL's prior written consent. DNV GL is not responsible for the consequences arising from any use of this document by others. The electronic pdf version of this document, available free of charge from http://www.dnvgl.com, is the officially binding version. DNV GL AS FOREWORD DNV GL offshore standards contain technical requirements, principles and acceptance criteria related to classification of offshore units. © DNV GL AS January 2017 Any comments may be sent by e-mail to [email protected] This service document has been prepared based on available knowledge, technology and/or information at the time of issuance of this document. The use of this document by others than DNV GL is at the user's sole risk. DNV GL does not accept any liability or responsibility for loss or damages resulting from any use of this document. CHANGES – CURRENT This document supersedes DNV-OS-E402 Offshore standard for Diving systems, October 2010 and DNV-DS- E403 Standard for Surface Diving Systems, July 2012 Changes in this document are highlighted in red colour. -
Viewing an Eclipse Safely
ECLIPSES SOLAR an eclipse safely How to observe SOLAR ECLIPSE, OCTOBER 2014, BY LEMAN NORTHWAY Solar eclipses are quite rare and are often a major event. The SOLAR ECLIPSES Moon passes right in front of the Sun, blotting out its disc. Every time a solar eclipse occurs there are various things to look for. However, it is extremely dangerous to just go out and look up. The Sun is so bright that just looking at it can blind you, so you’ll need to prepare beforehand. There are various ways to observe eclipses safely, using both everyday materials and telescopes or binoculars. So read this leaflet Introduction to find out what happens during an eclipse and how you can see all the stages of the event safely. This booklet was written by the Royal Astronomical Society with The Society for Popular Astronomy and is endorsed by the British Astronomical Association The Royal Astronomical The Society for Popular Formed in 1890, the Society, founded in Astronomy is for British Astronomical 1820, encourages and beginners of all ages. Our Association has an promotes the study of aim is to make astronomy international reputation astronomy, solar-system fun, and our magazine, for the quality of science, geophysics and Popular Astronomy, is full its observational closely related branches of information to help and scientific work. of science. you get to know the Membership is open to www.ras.org.uk sky and get involved. We even have a special Young all persons interested in HIGGS-BOSON.COM JOHNSON: PAUL BY D Stargazers section, run by TV’s Lucie Green. -
Ant-Xxv/3 - Lohafex)
613 2010 The Expedition of the Research Vessel "Polarstern" to the Antarctic in 2009 (ANT-XXV/3 - LOHAFEX) Edited by Victor Smetacek and Syed Wajih A. Naqvi with contributions of the participants ALFRED-WEGENER-INSTITUT FÜR POLAR- UND MEERESFORSCHUNG In der Helmholtz-Gemeinschaft D-27570 BREMERHAVEN Bundesrepublik Deutschland ISSN 1866-3192 Hinweis Notice Die Berichte zur Polar- und Meeresforschung The Reports on Polar and Marine Research are issued werden vom Alfred-Wegener-Institut für Polar-und by the Alfred Wegener Institute for Polar and Marine Meeresforschung in Bremerhaven* in Research in Bremerhaven*, Federal Republic of unregelmäßiger Abfolge herausgegeben. Germany. They appear in irregular intervals. Sie enthalten Beschreibungen und Ergebnisse der They contain descriptions and results of investigations in vom Institut (AWI) oder mit seiner Unterstützung polar regions and in the seas either conducted by the durchgeführten Forschungsarbeiten in den Institute (AWI) or with its support. Polargebieten und in den Meeren. The following items are published: Es werden veröffentlicht: — expedition reports (incl. station lists and — Expeditionsberichte (inkl. Stationslisten route maps) und Routenkarten) — expedition results (incl. — Expeditionsergebnisse Ph.D. theses) (inkl. Dissertationen) — scientific results of the Antarctic stations and of — wissenschaftliche Ergebnisse der other AWI research stations Antarktis-Stationen und anderer Forschungs-Stationen des AWI — reports on scientific meetings — Berichte wissenschaftlicher Tagungen Die Beiträge geben nicht notwendigerweise die The papers contained in the Reports do not necessarily Auffassung des Instituts wieder. reflect the opinion of the Institute. The „Berichte zur Polar- und Meeresforschung” continue the former „Berichte zur Polarforschung” * Anschrift / Address Alfred-Wegener-Institut Editor in charge: für Polar- und Meeresforschung Dr. -
Semi-Analytical Solution of Optimization on Moon-Pool Shaped Wec
POLISH MARITIME RESEARCH Special Issue 2016 S1 (91) 2016 Vol. 23; pp. 25-31 10.1515/pomr-2016-0042 SEMI-ANALYTICAL SOLUTION OF OPTIMIZATION ON MOON-POOL SHAPED WEC W.C. ZHANG, H.X. Liu, X.W. ZHANG, L. ZHANG College of Shipbuilding Engineering, Harbin Engineering University, Harbin,China ABSTRACT In order to effectively extract and maximize the energy from ocean waves, a new kind of oscillating-body WEC (wave energy converter) with moon pool has been put forward. The main emphasis in this paper is placed on inserting the damping into the equation of heaving motion applied for a complex wave energy converter and expressions for velocity potential added mass, damping coefficients associated with exciting forces were derived by using eigenfunction expansion matching method. By using surface-wave hydrodynamics, the exact theoretical conditions were solved to allow the maximum energy to be absorbed from regular waves. To optimize the ability of the wave energy conversion, oscillating system models under different radius-ratios are calculated and comparatively analyzed. Numerical calculations indicated that the capture width reaches the maximum in the vicinity of the natural frequency and the new kind of oscillating-body WEC has a positive ability of wave energy conversion. Keywords: wave energy; eigenfunction expansion; moon pool; conversion ability; optimization INTRODUCTION heaving motion. Oscillating-body WEC can take advantage of the body with resonant and periodic motion caused by the With worldwide demand for energy and electricity ocean waves with large forces at slow speeds to capture energy. unabated, over the past decades, so much considerable Comparing to other types of WECs, the oscillating body is attention and effort have been devoted to the problem of usually small in size and often used in arrays. -
1986Aj 92.120Id the Astronomical Journal Volume 92, Number 5 November 1986 Modeling Pluto-Charon Mutual Eclipse Events. I. First
THE ASTRONOMICAL JOURNAL VOLUME 92, NUMBER 5 NOVEMBER 1986 92.120ID MODELING PLUTO-CHARON MUTUAL ECLIPSE EVENTS. I. FIRST-ORDER MODELS R. Scott Dunbar and Edward F. Tedesco Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 1986AJ Received 29 May 1986; revised 7August 1986 ABSTRACT We present numerical and analytical models describing the light curves resulting from mutual events between close planetary binaries, with particular application to the Pluto-Charon system. These models are referred to as “first-order” models because they incorporate the effects of shadowing in such sys- tems, in contrast to “zeroth-order” models, which do not include shadowing. The shadows cast between close binaries of similar size (as in the case of Pluto and Charon) can be treated as extensions of the eclipsing bodies themselves at small solar phase angles. Shadowing plays a major role in the morphology of mutual event light curves. The numerical approach is a straightforward, but computationally inten- sive, discrete-element integration. The analytical approach uses a conceptually simple model of three circular disks, representing the planet, satellite, and shadow, and computes the complex geometric relationship among these three disks to obtain the eclipse magnitude at each time step. The results of the two models agree to well within the expected light-curve measurement error. A preliminary model fit to the depths of five mutual eclipse events observed in 1985 and 1986 gives eclipse light-curve-derived estimates of the orbit radius C = 16.5 + 0.5 Pluto radii, the radius ratio B0 = 0.65 + 0.03, and the Charon:Pluto albedo ratio K — 0.55 + 0.15. -
Solar and Lunar Eclipses Reading
Eclipses What would you think if you were walking home from school on a sunny afternoon and the sun began to disappear? Would you be frightened? On rare occasions, the moon completely blocks the sun. The sky grows as dark as night even in the middle of a clear day. The air gets cool and the sky becomes an eerie color. If you don’t know what is happening, you can become very frightened. The moon doesn’t usually go directly between Earth and the sun or directly behind Earth. As the diagram below shows, the moon’s orbit around Earth is slightly tilted with respect to Earth’s orbit around the sun. As a result, in most months the moon revolves completely around Earth without the moon moving into Earth’s shadow or the moon’s shadow hitting Earth. When the moon’s shadow hits Earth or Earth’s shadow hits the moon, an eclipse occurs. An eclipse (ih klips) occurs when an object in space comes between the sun and a third object, and casts a shadow on that object. There are two types of eclipses: solar eclipses and lunar eclipses. (The words solar and lunar come from the Latin words for “sun” and “moon.”) The Tilt of the Moon’s Orbit The moon’s orbit is tilted with respect to Earth’s orbit. So the moon rarely goes directly between Earth and the sun. Solar Eclipses During a new moon, the moon is almost exactly between Earth and the sun. But most months, as you have seen, the moon travels a little above or below the sun in the sky. -
The Moon and Eclipses
Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole. -
Metabolic Diversity of Heterotrophic Bacterioplankton Over Winter and Spring in the Coastal Arctic Ocean
Environmental Microbiology (2008) 10(4), 942–949 doi:10.1111/j.1462-2920.2007.01513.x Metabolic diversity of heterotrophic bacterioplankton over winter and spring in the coastal Arctic Ocean Maria Montserrat Sala,1* Ramon Terrado,2 advection, and sedimentation events that contributed Connie Lovejoy,2 Fernando Unrein1,3 and organic matter that enhanced bacterial metabolism. Carlos Pedrós-Alió1 1Departament de Biologia Marina i Oceanografia, Institut Introduction de Ciències del Mar (CSIC), Passeig Marítim de la Barceloneta 37-49, 08003 Barcelona, Spain. Arctic Ocean ecosystems are particularly sensitive to 2Dépt de Biologie and Québec Océan, Université Laval, climate changes, for example small temperature differ- Québec City, Québec G1K 7P4, Canada. ences may have large effects on the thickness and extent 3Instituto de Investigaciones Biotecnológicas-Instituto of sea ice (Smetacek and Nicol, 2005). Snow and ice cover Tecnológico de Chascomús (IIB-INTECH), Camino de are biologically important, influencing light availabity and Circunvalación Laguna Km 6 (B 7130 IWA) Chascomús, the timing of phytoplankton production in the Arctic Buenos Aires, Argentina. (Carmack et al., 2004). Primary production in oceanic areas constitutes the main organic source for bacteri- oplankton growth (Bird and Kalff, 1984; Cole et al., 1988), Summary mainly owing to direct bacterial use of dissolved com- Metabolic diversity of heterotrophic bacterioplankton pounds released by growing phytoplankton cells (Baines was tracked from early winter through spring with and Pace, 1991). However, recent evidence suggests that Biolog Ecoplates under the seasonally ice covered bacteria do not respond immediately to phytoplankton arctic shelf in the Canadian Arctic (Franklin Bay, production in cold waters (Bird and Karl, 1999; Pomeroy Beaufort Sea). -
• Zrmanjin Zov • Prince Rupert Expedition • TBM Avenger
• Zrmanjin Zov • Prince Rupert Expedition • TBM Avenger • Mystifying Leviathans of Cay Sal • Submerged Ghost Town of Minnewanka Landing • Introduction to Tech Video • New Cave – Old Species • Harvest Refugia • Ricks Spring Exploration • Wreck Fest 2009 • B-24 Liberator “DRIP” • Rouse Simmons Publisher’s Notes This summer has been a busy dive season with excursions from the Florida Keys and Silent World’s Wreckfest 2009 where we explored some of the deeper shipwrecks in the upper Florida Keys. Then it was on to the rough scrub jungles of the Dominican Republic where we beat the bush and crawled through every small subterranean hole we could discover in search of virgin cave passages. And we found more than we could have hoped for! The discovery of ancient animal fossils, extinct in all of the Caribbean islands, would bring us back a month later to recover these unique artifacts for the Domini- can Republic’s archeological department and the Museum of Publisher................. Curt Bowen Dominican Man. Finally, southeast to the amazing Blue Holes of the Co-Publisher............ Linda Bowen Cay Sal Bank where divers pushed some of these mysterious giants to extreme depths. Copy Editor..................... Victoria Leigh Chief Staff Writer............ John Rawlings Chief Photojournalist...... Jeff Toorish Of course, in addition to traveling to all these far-flung points of the Video Chief of Staff........ David Ulloa globe, there was the gathering of editorial materials from ADM Web Master..................... Jakub Rehacek writers and contributors, the operations of Rebreatherworld.com, First Grade.................. Savannah Bowen and continued promotion of the ADM Exploration Foundation. Add ADM Staff Writers & Photographers in the hundreds of hours that are required for me to complete the Mel Clark • Erik Foreman magazine layout from cover to cover…. -
Polarstern PS113 Punta Arenas - Bremerhaven 07 May 2018 - 11 June 2018
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Electronic Publication Information Center EXPEDITION PROGRAMME PS113 Polarstern PS113 Punta Arenas - Bremerhaven 07 May 2018 - 11 June 2018 Coordinator: Rainer Knust Chief Scientist: Volker Strass Bremerhaven, Januar 2018 Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung Am Handelshafen 12 D-27570 Bremerhaven Telefon: ++49 471 4831- 0 Telefax: ++49 471 4831 – 1149 E-Mail: [email protected] Website: http://www.awi.de Email Coordinator: [email protected] Email Chief Scientist: [email protected] PS113 South-North Atlantic Transit 07 May 2018 - 11 June 2018 Punta Arenas - Bremerhaven Chief scientist Volker Strass Coordinator Rainer Knust Contents 1. Überblick und Fahrtverlauf 2 Summary and itinerary 3 2. System-testing and commissioning of the multidisciplinary towed ocean profiler of the AWI (topawi) 5 3. Phytooptics 6 4. Plankton-Genomics: Pro- and eukaryotic diversity along a latitudinal gradient in the Atlantic Ocean 9 5. WaMoS: Radar-based measurements of surface waves and currents 10 6. OCEANET-Atmosphere: Autonomous measurement platforms for energy and material exchange between ocean and atmosphere 12 7. MIcrotops: Measurements of atmospheric column integrated aerosol properties and water vapor 14 Planned additional activity, if possible: Monitoring clouds cover, structure and cloud base altitude 15 8. Argo float deployments 16 9. Bathymetric Mapping and sub-bottom profiling 17 10. Benthic fish: Climate sensitivity in various fishes from the Antarctic Peninsula - Molecular ecology and cellular mechanisms 18 11. Teilnehmende Institute / Participating Institutions 20 12 Fahrtteilnehmer / Cruise Participants 22 13 Schiffsbesatzung / Ship's Crew 23 1 PS113 Expedition Programme 1.