Ancient Korean Meteor Shower Records
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Korean Nova Records in A.D. 1073 and A.D. 1074: R Aquarii
A&A 435, 207–214 (2005) Astronomy DOI: 10.1051/0004-6361:20042455 & c ESO 2005 Astrophysics Korean nova records in A.D. 1073 and A.D. 1074: R Aquarii Hong-Jin Yang1, Myeong-Gu Park2, Se-Hyung Cho1, and Changbom Park3 1 Korea Astronomy and Space Science Institute, 61-1 Hwaam, Yuseong, Daejeon 305-348, Korea e-mail: [hjyang;cho]@kasi.re.kr 2 Department of Astronomy and Atmospheric Sciences, Kyungpook National University, Daegu 702-701, Korea e-mail: [email protected] 3 School of Physics, Korea Institute for Advanced Study, Seoul 130-722, Korea e-mail: [email protected] Received 30 November 2004 / Accepted 31 December 2004 Abstract. R Aqr is known to be a symbiotic binary system with an associated extended emission nebula, possibly produced by a historic outburst. To find the associated historic records, we searched for and compiled all Guest Star and Peculiar Star records in three Korean official history books that cover almost two thousand years, Samguksagi, Goryeosa, Joseonwangjosillok. In addition to the record of A.D. 1073, previously noted by Li (1985, Chin. Astron. Astrophys., 9, 322), we have found in Goryeosa another candidate record of A.D. 1074, which has the same positional description as that of A.D. 1073 with an additional brightness description. We examined various aspects of the two records and conclude that they both are likely to be the records of outburst of R Aqr. This means that there were two successive outbursts in A.D. 1073 and in A.D. 1074, separated by approximately one year. -
Teachers' Guide to Meteor Showers Leonids Meteor Shower
Education and Public Outreach Look Up! Event Guides Teachers’ Guide to Meteor Showers Leonids Meteor Shower - November 17/18, 2015 What is a meteor shower? A meteor shower is a predictable celestial event in which a relatively large number of meteors streak across the sky on a given night or series of nights. Meteor showers appear to originate from one point (called the radiant) in the night sky, often a constellation. Meteor showers get their name from the constellation from which they appear to originate. Meteor showers are caused by debris called meteoroids entering Earth’s atmosphere at extremely high speeds. This debris usually comes from comets that intersect Earth’s orbit. As Earth orbits the Sun, it collides with the debris left by passing comets and the result are meteors streaking through Earth’s atmosphere. Most meteors are smaller than a grain of sand, so almost all of them disintegrate before having a chance to hit the ground. In 2015, the annual Leonid meteor shower will peak the night of November 17/18. The Leonids are so named because they appear to originate from the constellation of Leo (the lion). The debris responsible for the Leonids comes from the comet Tempel- Tuttle. It is possible to view about 20 meteors in one hour at the peak of the Leonids meteor shower. Upcoming Events Find information and resources about upcoming celestial events and NASA mission milestones to share with your students at http://www.lpi.usra.edu/education/look_up. Meteor Showers/Comets in Your Classroom! Use the resources below to enable your students to explore meteor showers. -
Download This Article in PDF Format
A&A 598, A40 (2017) Astronomy DOI: 10.1051/0004-6361/201629659 & c ESO 2017 Astrophysics Separation and confirmation of showers? L. Neslušan1 and M. Hajduková, Jr.2 1 Astronomical Institute, Slovak Academy of Sciences, 05960 Tatranska Lomnica, Slovak Republic e-mail: [email protected] 2 Astronomical Institute, Slovak Academy of Sciences, Dubravska cesta 9, 84504 Bratislava, Slovak Republic e-mail: [email protected] Received 6 September 2016 / Accepted 30 October 2016 ABSTRACT Aims. Using IAU MDC photographic, IAU MDC CAMS video, SonotaCo video, and EDMOND video databases, we aim to separate all provable annual meteor showers from each of these databases. We intend to reveal the problems inherent in this procedure and answer the question whether the databases are complete and the methods of separation used are reliable. We aim to evaluate the statistical significance of each separated shower. In this respect, we intend to give a list of reliably separated showers rather than a list of the maximum possible number of showers. Methods. To separate the showers, we simultaneously used two methods. The use of two methods enables us to compare their results, and this can indicate the reliability of the methods. To evaluate the statistical significance, we suggest a new method based on the ideas of the break-point method. Results. We give a compilation of the showers from all four databases using both methods. Using the first (second) method, we separated 107 (133) showers, which are in at least one of the databases used. These relatively low numbers are a consequence of discarding any candidate shower with a poor statistical significance. -
Calendrical Calculations: the Millennium Edition Edward M
Errata and Notes for Calendrical Calculations: The Millennium Edition Edward M. Reingold and Nachum Dershowitz Cambridge University Press, 2001 4:45pm, December 7, 2006 Do I contradict myself ? Very well then I contradict myself. (I am large, I contain multitudes.) —Walt Whitman: Song of Myself All those complaints that they mutter about. are on account of many places I have corrected. The Creator knows that in most cases I was misled by following. others whom I will spare the embarrassment of mention. But even were I at fault, I do not claim that I reached my ultimate perfection from the outset, nor that I never erred. Just the opposite, I always retract anything the contrary of which becomes clear to me, whether in my writings or my nature. —Maimonides: Letter to his student Joseph ben Yehuda (circa 1190), Iggerot HaRambam, I. Shilat, Maaliyot, Maaleh Adumim, 1987, volume 1, page 295 [in Judeo-Arabic] If you find errors not given below or can suggest improvements to the book, please send us the details (email to [email protected] or hard copy to Edward M. Reingold, Department of Computer Science, Illinois Institute of Technology, 10 West 31st Street, Suite 236, Chicago, IL 60616-3729 U.S.A.). If you have occasion to refer to errors below in corresponding with the authors, please refer to the item by page and line numbers in the book, not by item number. Unless otherwise indicated, line counts used in describing the errata are positive counting down from the first line of text on the page, excluding the header, and negative counting up from the last line of text on the page including footnote lines. -
The Solar System
5 The Solar System R. Lynne Jones, Steven R. Chesley, Paul A. Abell, Michael E. Brown, Josef Durech,ˇ Yanga R. Fern´andez,Alan W. Harris, Matt J. Holman, Zeljkoˇ Ivezi´c,R. Jedicke, Mikko Kaasalainen, Nathan A. Kaib, Zoran Kneˇzevi´c,Andrea Milani, Alex Parker, Stephen T. Ridgway, David E. Trilling, Bojan Vrˇsnak LSST will provide huge advances in our knowledge of millions of astronomical objects “close to home’”– the small bodies in our Solar System. Previous studies of these small bodies have led to dramatic changes in our understanding of the process of planet formation and evolution, and the relationship between our Solar System and other systems. Beyond providing asteroid targets for space missions or igniting popular interest in observing a new comet or learning about a new distant icy dwarf planet, these small bodies also serve as large populations of “test particles,” recording the dynamical history of the giant planets, revealing the nature of the Solar System impactor population over time, and illustrating the size distributions of planetesimals, which were the building blocks of planets. In this chapter, a brief introduction to the different populations of small bodies in the Solar System (§ 5.1) is followed by a summary of the number of objects of each population that LSST is expected to find (§ 5.2). Some of the Solar System science that LSST will address is presented through the rest of the chapter, starting with the insights into planetary formation and evolution gained through the small body population orbital distributions (§ 5.3). The effects of collisional evolution in the Main Belt and Kuiper Belt are discussed in the next two sections, along with the implications for the determination of the size distribution in the Main Belt (§ 5.4) and possibilities for identifying wide binaries and understanding the environment in the early outer Solar System in § 5.5. -
Meteoroid Stream Formation Due to the Extraction of Space Resources from Asteroids
Meteoroid Stream Formation Due to the Extraction of Space Resources from Asteroids Logan Fladeland(1), Aaron C. Boley(2), and Michael Byers(3) (1) UBC, Department of Physics and Astronomy, 6224 Agricultural Rd, Vancouver, BC V6T 1Z1 (Canada), [email protected] (2) UBC, Department of Physics and Astronomy, 6224 Agricultural Rd, Vancouver, BC V6T 1Z1 (Canada), [email protected] (3) UBC, Department of Political Science, 1866 Main Mall C425, Vancouver, BC V6T 1Z1 (Canada), [email protected] ABSTRACT Asteroid mining is not necessarily a distant prospect. Building on the earlier mission Hayabusa, two spacecraft (Hayabusa2 and OSIRIS-REx) have recently rendezvoused with near-Earth asteroids and will return samples to Earth. While there is significant science motivation for these missions, there are also resource interests. Space agencies and commercial entities are particularly interested in ices and water-bearing minerals that could be used to produce rocket fuel in deep space. The internationally coordinated roadmaps of major space agencies depend on utilizing the natural resources of such celestial bodies. Several companies have already created plans for intercepting and extracting water and minerals from near-Earth objects, as even a small asteroid could have high economic worth. The low surface gravity of asteroids could make the release of mining waste and the subsequent formation of debris streams a consequence of asteroid mining. Proposed strategies that would contain material during extraction could be inefficient or could still require the purposeful jettison of mining waste to avoid the need to manage unwanted mass. Since all early mining targets are expected to be near-Earth asteroids due to their orbital accessibility, these streams could be Earth-crossing and create risks for Earth and lunar satellite populations, as well as humans and equipment on the lunar surface. -
Meteor Showers' Activity and Forecasting
Meteoroids 2007 – Barcelona, June 11-15 About the cover: The recent fall of the Villalbeto de la Peña meteorite on January 4, 2004 (Spain) is one of the best documented in history for which atmospheric and orbital trajectory, strewn field area, and recovery circumstances have been described in detail. Photometric and seismic measurements together with radioisotopic analysis of several recovered specimens suggest an original mass of about 760 kg. About fifty specimens were recovered from a strewn field of nearly 100 km2. Villalbeto de la Peña is a moderately shocked (S4) equilibrated ordinary chondrite (L6) with a cosmic-ray-exposure age of 48±5 Ma. The chemistry and mineralogy of this genuine meteorite has been characterized in detail by bulk chemical analysis, electron microprobe, electron microscopy, magnetism, porosimetry, X-ray diffraction, infrared, Raman, and 57Mössbauer spectroscopies. The picture of the fireball was taken by M.M. Ruiz and was awarded by the contest organized by the Spanish Fireball Network (SPMN) for the best photograph of the event. The Moon is also visible for comparison. The picture of the meteorite was taken as it was found by the SPMN recovery team few days after the fall. 2 Meteoroids 2007 – Barcelona, June 11-15 FINAL PROGRAM Monday, June 11 Auditorium conference room 9h00-9h50 Reception 9h50-10h00 Opening event Session 1: Observational Techniques and Meteor Detection Programs Morning session Session chairs: J. Borovicka and W. Edwards 10h00-10h30 Pavel Spurny (Ondrejov Observatory, Czech Republic) et al. “Fireball observations in Central Europe and Western Australia – instruments, methods and results” (invited) 10h30-10h45 Josep M. -
Dan-Gun Dan-Gun Is Named After the Holy Dan-Gun, the Legendary Founder of Korea in the Year of 2333 B.C
Dan-Gun Dan-Gun is named after the holy Dan-Gun, the legendary founder of Korea in the year of 2333 B.C. The history of the Dan-Gun Dangun Wanggeom was the legendary founder of Gojoseon, the first kingdom of Korea, in present-day Liaoning, Manchuria, and the Korean Peninsula. He is said to be the grandson of the god of heaven, and to have founded the kingdom in 2333 BC. Although the term Dangun commonly refers to the founder, some believe it was a title used by all rulers of Gojoseon, and that Wanggeom was the proper name of the founder. Dangun’s ancestry begins with his grandfather Hwanin, the “Lord of Heaven” (a name which also appears in Indian Buddhist texts). Hwanin had a son Hwanung who yearned to live on the earth among the valleys and the mountains. Hwanin permitted Hwanung and 3000 followers to descend onto Baekdu Mountain, then called Taebaek Mountain, where Hwanung founded Sinsi (“City of God”). Along with his ministers of clouds, rain, and wind, he instituted laws and moral codes and taught humans various arts, medicine, and agriculture. One day both a bear and a tiger came to Hwanung’s residence in prayer and asked to be transformed into humans. The god agreed to this gift but on the condition that they remain out of the sun for 100 days and eat only a sacred bunch of mug- worts and 20 garlic cloves. To this the animals agreed and followed his advice. The tiger was unable to keep up with the conditions, but the bear – a female called Ung- nyo – after only 21 days was transformed into a woman. -
17. a Working List of Meteor Streams
PRECEDING PAGE BLANK NOT FILMED. 17. A Working List of Meteor Streams ALLAN F. COOK Smithsonian Astrophysical Observatory Cambridge, Massachusetts HIS WORKING LIST which starts on the next is convinced do exist. It is perhaps still too corn- page has been compiled from the following prehensive in that there arc six streams with sources: activity near the threshold of detection by pho- tography not related to any known comet and (1) A selection by myself (Cook, 1973) from not sho_m to be active for as long as a decade. a list by Lindblad (1971a), which he found Unless activity can be confirmed in earlier or from a computer search among 2401 orbits of later years or unless an associated comet ap- meteors photographed by the Harvard Super- pears, these streams should probably be dropped Sehmidt cameras in New Mexico (McCrosky and from a later version of this list. The author will Posen, 1961) be much more receptive to suggestions for dele- (2) Five additional radiants found by tions from this list than he will be to suggestions McCrosky and Posen (1959) by a visual search for additions I;o it. Clear evidence that the thresh- among the radiants and velocities of the same old for visual detection of a stream has been 2401 meteors passed (as in the case of the June Lyrids) should (3) A further visual search among these qualify it for permanent inclusion. radiants and velocities by Cook, Lindblad, A comment on the matching sets of orbits is Marsden, McCrosky, and Posen (1973) in order. It is the directions of perihelion that (4) A computer search -
Meteor Showers # 11.Pptx
20-05-31 Meteor Showers Adolf Vollmy Sources of Meteors • Comets • Asteroids • Reentering debris C/2019 Y4 Atlas Brett Hardy 1 20-05-31 Terminology • Meteoroid • Meteor • Meteorite • Fireball • Bolide • Sporadic • Meteor Shower • Meteor Storm Meteors in Our Atmosphere • Mesosphere • Atmospheric heating • Radiant • Zenithal Hourly Rate (ZHR) 2 20-05-31 Equipment Lounge chair Blanket or sleeping bag Hot beverage Bug repellant - ThermaCELL Camera & tripod Tracking Viewing Considerations • Preparation ! Locate constellation ! Take a nap and set alarm ! Practice photography • Location: dark & unobstructed • Time: midnight to dawn https://earthsky.org/astronomy- essentials/earthskys-meteor-shower- guide https://www.amsmeteors.org/meteor- showers/meteor-shower-calendar/ • Where to look: 50° up & 45-60° from radiant • Challenges: fatigue, cold, insects, Moon • Recording observations ! Sky map, pen, red light & clipboard ! Time, position & location ! Recording device & time piece • Binoculars Getty 3 20-05-31 Meteor Showers • 112 confirmed meteor showers • 695 awaiting confirmation • Naming Convention ! C/2019 Y4 (Atlas) ! (3200) Phaethon June Tau Herculids (m) Parent body: 73P/Schwassmann-Wachmann Peak: June 2 – ZHR = 3 Slow moving – 15 km/s Moon: Waning Gibbous June Bootids (m) Parent body: 7p/Pons-Winnecke Peak: June 27– ZHR = variable Slow moving – 14 km/s Moon: Waxing Crescent Perseid by Brian Colville 4 20-05-31 July Delta Aquarids Parent body: 96P/Machholz Peak: July 28 – ZHR = 20 Intermediate moving – 41 km/s Moon: Waxing Gibbous Alpha -
Long Grazing and Slow Trail Fireball Over Portugal Spectra of Slow
e-Zine for meteor observers meteornews.org Vol. 4 / January 2017 A bright fireball photographed by four stations of the Danish Meteor network on December 25 at 2:11 UT. Long grazing and slow trail OCT outburst model comparisons fireball over Portugal in the years 2005, 2016, 2017 Spectra of slow bolides Worldwide radio results The PRO-AM Lunar Impact autumn 2016 project Exoss Fireball events 2016 – 4 eMeteorNews Contents Spectra of slow bolides Jakub Koukal ........................................................................................................................................... 117 Visual observing reports Paul Jones ............................................................................................................................................... 123 Fireball events Compiled by Paul Roggemans ................................................................................................................ 130 CAMS BeNeLux September results Carl Johannink ........................................................................................................................................ 134 October Camelopardalis outburst model comparisons in the years 2005, 2016, 2017 Esko Lyytinen .......................................................................................................................................... 135 CAMS Benelux contributed 4 OCT orbits Carl Johannink ....................................................................................................................................... -
Arxiv:2104.05964V3 [Cs.CL] 7 May 2021 1 Introduction Discover the Important Historical Events Over the Last Hundreds of Years
Restoring and Mining the Records of the Joseon Dynasty via Neural Language Modeling and Machine Translation Kyeongpil Kang Kyohoon Jin Soyoung Yang Scatter Lab Chung-Ang University KAIST Seoul, South Korea Seoul, South Korea Daejeon, South Korea [email protected] [email protected] [email protected] Soojin Jang Jaegul Choo Youngbin Kim Chung-Ang University KAIST Chung-Ang University Seoul, South Korea Daejeon, South Korea Seoul, South Korea [email protected] [email protected] [email protected] Abstract records in a digital form for long-term preservation. A representative example is the Google Books Li- Understanding voluminous historical records brary Project1. However, despite the importance of provides clues on the past in various aspects, such as social and political issues and even the historical records, it has been challenging to natural science facts. However, it is generally properly utilize the records for the following rea- difficult to fully utilize the historical records, sons. First, the nontrivial amounts of the documents since most of the documents are not written are partially damaged and unrecognizable due to in a modern language and part of the contents unfortunate historical events or environments, such are damaged over time. As a result, restoring as wars and disasters, as well as the weak durability the damaged or unrecognizable parts as well as of paper documents. These factors result in difficul- translating the records into modern languages are crucial tasks. In response, we present a ties to translate and understand the records. Second, multi-task learning approach to restore and as most of the records are written in ancient and out- translate historical documents based on a self- dated languages, non-experts are difficult to read attention mechanism, specifically utilizing two and understand them.