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Religion and Science in Abraham Ibn Ezra's Sefer Ha-Olam
RELIGION AND SCIENCE IN ABRAHAM IBN EZRA'S SEFER HA-OLAM (INCLUDING AN ENGLISH TRANSLATION OF THE HEBREW TEXT) Uskontotieteen pro gradu tutkielma Humanistinen tiedekunta Nadja Johansson 18.3.2009 1 CONTENTS 1 INTRODUCTION ............................................................................................................... 3 1.1 Abraham Ibn Ezra and Sefer ha-Olam ........................................................................ 3 1.2 Previous research ......................................................................................................... 5 1.3 The purpose of this study ............................................................................................. 8 2 SOURCE, METHOD AND THEORETICAL FRAMEWORK ....................................... 10 2.1 Primary source: Sefer ha-Olam (the Book of the World) ........................................... 10 2.1.1 Edition, manuscripts, versions and date .............................................................. 10 2.1.2 Textual context: the astrological encyclopedia .................................................... 12 2.1.3 Motivation: technical handbook .......................................................................... 14 2.2 Method ....................................................................................................................... 16 2.2.1 Translation and historical analysis ...................................................................... 16 2.2.2 Systematic analysis ............................................................................................. -
What's in This Issue?
A JPL Image of surface of Mars, and JPL Ingenuity Helicioptor illustration. July 11th at 4:00 PM, a family barbeque at HRPO!!! This is in lieu of our regular monthly meeting.) (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory) This is a pot-luck. Club will provide briskett and beverages, others will contribute as the spirit moves. What's In This Issue? President’s Message Member Meeting Minutes Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night SubReddit and Discord BRAS Member Astrophotos ARTICLE: Astrophotography with your Smart Phone Observing Notes: Canes Venatici – The Hunting Dogs Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society BRAS YouTube Channel Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 23 July 2021 President’s Message Hey everybody, happy fourth of July. I hope ya’ll’ve remembered your favorite coping mechanism for dealing with the long hot summers we have down here in the bayou state, or, at the very least, are making peace with the short nights that keep us from enjoying both a good night’s sleep and a productive observing/imaging session (as if we ever could get a long enough break from the rain for that to happen anyway). At any rate, we figured now would be as good a time as any to get the gang back together for a good old fashioned potluck style barbecue: to that end, we’ve moved the July meeting to the Sunday, 11 July at 4PM at HRPO. -
The Astronomy of the Kamilaroi and Euahlayi Peoples and Their Neighbours
The Astronomy of the Kamilaroi and Euahlayi Peoples and Their Neighbours By Robert Stevens Fuller A thesis submitted to the Faculty of Arts at Macquarie University for the degree of Master of Philosophy November 2014 © Robert Stevens Fuller i I certify that the work in this thesis entitled “The Astronomy of the Kamilaroi and Euahlayi Peoples and Their Neighbours” has not been previously submitted for a degree nor has it been submitted as part of requirements for a degree to any other university or institution other than Macquarie University. I also certify that the thesis is an original piece of research and it has been written by me. Any help and assistance that I have received in my research work and the preparation of the thesis itself has been appropriately acknowledged. In addition, I certify that all information sources and literature used are indicated in the thesis. The research presented in this thesis was approved by Macquarie University Ethics Review Committee reference number 5201200462 on 27 June 2012. Robert S. Fuller (42916135) ii This page left intentionally blank Contents Contents .................................................................................................................................... iii Dedication ................................................................................................................................ vii Acknowledgements ................................................................................................................... ix Publications .............................................................................................................................. -
2005 FEBBRAIO Sab Lun Mar Gio 1 Maria Madre Di Dio 17 S
S L P s.p.a. Assicurazioni Spese Legali Peritali e Rischi Accessori Sede e Dir. Gen: 10121 Torino - C.so Matteotti 3 bis - Tel. 011.548.003 - 011.548.748 - Fax 011.548.760 - e-mail: [email protected] SLP Assicurazioni SpA Compagnia Specializzata nel ramo Tutela Giudiziaria Capricorno (Capricornus, Cap) Acquario (Aquarius, Aqr) ALGEDI SADALMELIK M 2 DENEB ALGEDI SADACHBIA DABIH SADALSUUD NASHIRA O ANCHA ALBALI NGC 7009 M 72 SKAT M30 NGC 7293 IL MITO GRECO: IL MITO GRECO: Pan, dio della mitologia greca di carattere infernale ed orgiastico, stava banchettando sull’Olimpo insieme ad altri dei. Improvvisamente Rappresenta Ganimede, il giovane adolescente della cui bellezza si innamorò Zeus, il quale per soddisfare la propria passione amorosa, apparve Tifone, essere mostruoso, mezzo uomo e mezzo belva. Gli Dei, atterriti, fuggirono, trasformandosi in animali: Apollo diventò un assunta la forma di un’aquila, lo rapì e lo trasportò sull’Olimpo. Qui Ganimede, nominato coppiere degli Dei, si occupava personalmente di nibbio, Ermes un ibis, Ares un pesce. Pan (da cui il termine “panico”), terrorizzato, si gettò in un fiume prima di trasformarsi completamnte versare il nettare nella coppa di Zeus. Altre leggende identificano l’Acquario nello stesso Zeus intento a versare l’acqua vitale per la Terra. La in capra e fu così che le sue estremità inferiori assunsero la forma della coda di un pesce. Zeus, stupito e compiaciuto per la metamorfosi, Costellazione era conosciuta anche dagli antichi Babilonesi ed Egizi che nell’Acquario, il Portatore d’Acqua, raffiguravano un uomo che versava decise di collocare in cielo la “capra d’acqua”. -
Catalogue CACIB Web.Pdf
Организатор выставки: Федерация охотничьего собаководства (РФОС) Москва, Головинское шоссе 1, +7 916 1443315, [email protected] Организационный комитет: Е. Домогацкая (председатель), М. Мартынова, Е. Гришина Генеральный спонсор выставки: FARMINA PET FOODS www.farmina.com СУДЬИ / JUDGES: Сисси АДРАМИТЛИ / Sissy ADRAMITLI (Греция) Кнут Зигурд ВИЛЬБЕРГ / Knut Sigurd WILBERG (Норвегия-Великобритания) Артем ГАЛКИН / Artyom GALKIN (Россия) Станислав ГОРОДИЛОВ / Stanislav GORODILOV (Россия) Юлия ГУСЕВА / Julia GUSEVA (Россия) Хельге КВИВЕСЕН / Helge KVIVESEN (Норвегия) Жан Клод КЛЯЙН / Jean Claude KLEIN (Франция) Дина КОРНА / Dina KORNA (Эстония) Евгений КУПЛЯУСКАС / Eugene KUPLYAUSKAS (Россия) Джузеппе МАСИЯ / Guiseppe MASIA (Италия) Мауро МОСТУРА / Mauro MOSTURA (Италия) Микаэль Аллеруп НИЛЬСЕН / Michael Allerup NIELSEN (Дания) Франческо Ди Паола НУЦЦО / Francesco Di Paola NUZZO (Италия) Евгений ПУДЕЕВ / Eugene PUDEEV (Россия) Петер ФРИДРИХ / Peter FRIEDRICH (Германия) Реваз ХОМАСУРИДЗЕ / Revaz KHOMASURIDZE (Россия) Мария ЧЕККАРЕЛЛИ / Maria CECCARELLI (Италия) Дамьяна ШВЕГЕЛЬ ЖНИДАРШИЧ / Damjana ŠVEGELJ ŽNIDARŠIČ (Словения) Владимир ШИЯН / Vladimir SHYIAN (Украина) Дитер ШНАЙДЕР / Dieter SCHNEIDER (Германия) Йохен ЭБЕРХАРДТ / Jochen EBERHARDT (Германия) Яна ЯНЕК / Jana JANEK (Словакия) Таль ЯФФЕ / Tal YAFFE (Израиль) Место проведения выставки / Show ground: Москва, КВЦ «Сокольники», пав. 4, 3 и 11 / Moscow, ECC “Sokolniki”, halls 4, 3, 11 Москва / Moscow, 25.01.2020 РЕГЛАМЕНТ ПРОВЕДЕНИЯ ВЫСТАВКИ ПАМЯТИ Л.П.САБАНЕЕВА 1. ОБЩИЕ ПОЛОЖЕНИЯ 1.1. Регламент составлен на основе действующего Положения о сертификатных выставках Российской кинологической федерации (РКФ). 1.2. Выставка проводится в соответствии с календарным планом РКФ / FCI на 2020 год. 1.3. Дата и место проведения выставки: 25 января 2020 г., Москва, КВЦ «Сокольники», павильоны 4, 3, 11. 1.4. Организатор – Федерация охотничьего собаководства (РФОС). Председатель оргкомитета – президент РФОС Е.Г.Домогацкая. -
December 2014 BRAS Newsletter
December, 2014 Next Meeting: December 8th at 7PM at the HRPO Artist rendition of the Philae lander from the ESA's Rosetta mission. Click on the picture to go see the latest info. What's In This Issue? Astro Short- Mercury: Snow Globe Dynamo? Secretary's Summary Message From HRPO Globe At Night Recent Forum Entries Orion Exploration Test Flight Event International Year of Light 20/20 Vision Campaign Observing Notes by John Nagle Mercury: Snow Globe Dynamo? We already knew Mercury was bizarre. A planet of extremes, during its day facing the sun, its surface temperature tops 800°F —hot enough to melt lead—but during the night, the temperature plunges to -270°F, way colder than dry ice. Frozen water may exist at its poles. And its day (from sunrise to sunrise) is twice as long as its year. Now add more weirdness measured by NASA’s recent MESSENGER spacecraft: Mercury’s magnetic field in its northern hemisphere is triple its strength in the southern hemisphere. Numerical models run by postdoctoral researcher Hao Cao, working in the lab of Christopher T. Russell at UC Los Angeles, offer an explanation: inside Mercury’s molten iron core it is “snowing,” and the resultant convection is so powerful it causes the planet’s magnetic dynamo to break symmetry and concentrate in one hemisphere. “Snowing” inside Mercury With a diameter only 40 percent greater than the Moon’s, Mercury is the smallest planet in the solar system (now that Pluto was demoted). But its gravitational field is more than double the Moon’s. -
Variable Stars Across the Observational HR Diagram
Variable stars across the observational HR diagram Laurent Eyer1, Nami Mowlavi1;2 1 Observatoire de Gen`eve, Universit´ede Gen`eve, 1290 Sauverny, Switzerland 2 ISDC, Universit´ede Gen`eve, 1290 Versoix, Switzerland E-mail: [email protected] Abstract. An overview of pulsating variable stars across the observational Hertzprung-Russel (HR) diagram is presented, together with a summary of their global properties. The HR diagram is presented with a third colour-coded dimension, visualizing the fraction of variable, the amplitude of variability or the period of variability. The distribution of variable stars in the other observational diagrams, such as the Period-Amplitude diagram, is also presented. Some of the progresses performed in the field of variable stars during the last decade are briefly summarized, and future projects that will improve our knowledge of variable stars are mentioned. 1. Introduction There are in the literature several global descriptions of variable stars. We can mention four books, one by Richter, Wenzel and Hoffmeister (1985, out of print), one by Sterken and Jaschek [1], one by Percy ([2]) and one, soon to come, by Aerts et al. [3]. There have also been two excellent and detailed reviews by Gautschy and Saio ([4], [5]) about a decade ago. With the advent of Charge-Coupled Devices (CCDs) and large scale surveys like the Optical Gravitational Lensing Experiment (OGLE), the Massive Compact Halo Object project (MACHO) or the "Exp´eriencepour la Recherche d'Objets Sombres" (EROS), the subject of variable star studies is now under a remarkable expansion. As we will see the expansion will continue in the coming decade because there are many future projects which will sample frequently large regions of the sky. -
Arxiv:1709.07265V1 [Astro-Ph.SR] 21 Sep 2017 an Der Sternwarte 16, 14482 Potsdam, Germany E-Mail: [email protected] 2 Smitha Subramanian Et Al
Noname manuscript No. (will be inserted by the editor) Young and Intermediate-age Distance Indicators Smitha Subramanian · Massimo Marengo · Anupam Bhardwaj · Yang Huang · Laura Inno · Akiharu Nakagawa · Jesper Storm Received: date / Accepted: date Abstract Distance measurements beyond geometrical and semi-geometrical meth- ods, rely mainly on standard candles. As the name suggests, these objects have known luminosities by virtue of their intrinsic proprieties and play a major role in our understanding of modern cosmology. The main caveats associated with standard candles are their absolute calibration, contamination of the sample from other sources and systematic uncertainties. The absolute calibration mainly de- S. Subramanian Kavli Institute for Astronomy and Astrophysics Peking University, Beijing, China E-mail: [email protected] M. Marengo Iowa State University Department of Physics and Astronomy, Ames, IA, USA E-mail: [email protected] A. Bhardwaj European Southern Observatory 85748, Garching, Germany E-mail: [email protected] Yang Huang Department of Astronomy, Kavli Institute for Astronomy & Astrophysics, Peking University, Beijing, China E-mail: [email protected] L. Inno Max-Planck-Institut f¨urAstronomy 69117, Heidelberg, Germany E-mail: [email protected] A. Nakagawa Kagoshima University, Faculty of Science Korimoto 1-1-35, Kagoshima 890-0065, Japan E-mail: [email protected] J. Storm Leibniz-Institut f¨urAstrophysik Potsdam (AIP) arXiv:1709.07265v1 [astro-ph.SR] 21 Sep 2017 An der Sternwarte 16, 14482 Potsdam, Germany E-mail: [email protected] 2 Smitha Subramanian et al. pends on their chemical composition and age. To understand the impact of these effects on the distance scale, it is essential to develop methods based on differ- ent sample of standard candles. -
The Electric Sun Hypothesis
Basics of astrophysics revisited. II. Mass- luminosity- rotation relation for F, A, B, O and WR class stars Edgars Alksnis [email protected] Small volume statistics show, that luminosity of bright stars is proportional to their angular momentums of rotation when certain relation between stellar mass and stellar rotation speed is reached. Cause should be outside of standard stellar model. Concept allows strengthen hypotheses of 1) fast rotation of Wolf-Rayet stars and 2) low mass central black hole of the Milky Way. Keywords: mass-luminosity relation, stellar rotation, Wolf-Rayet stars, stellar angular momentum, Sagittarius A* mass, Sagittarius A* luminosity. In previous work (Alksnis, 2017) we have shown, that in slow rotating stars stellar luminosity is proportional to spin angular momentum of the star. This allows us to see, that there in fact are no stars outside of “main sequence” within stellar classes G, K and M. METHOD We have analyzed possible connection between stellar luminosity and stellar angular momentum in samples of most known F, A, B, O and WR class stars (tables 1-5). Stellar equatorial rotation speed (vsini) was used as main parameter of stellar rotation when possible. Several diverse data for one star were averaged. Zero stellar rotation speed was considered as an error and corresponding star has been not included in sample. RESULTS 2 F class star Relative Relative Luminosity, Relative M*R *eq mass, M radius, L rotation, L R eq HATP-6 1.29 1.46 3.55 2.950 2.28 α UMi B 1.39 1.38 3.90 38.573 26.18 Alpha Fornacis 1.33 -
April 2019 BRAS Newsletter
Monthly Meeting April 8th at 7PM at HRPO (Monthly meetings are on 2nd Mondays, Highland Road Park Observatory). Speaker: Merrill Hess will speak on “The life cycle of stars." What's In This Issue? President’s Message Secretary's Summary Outreach Report Astrophotography Group Asteroid and Comet News Light Pollution Committee Report Globe at Night Recent BRAS Forum Entries Messages from the HRPO Science Academy Friday Night Lecture Series Special Presentation 13 April: “Skygazing—A Pursuer’s Guide” International Astronomy Day” American Radio Relay League Field Day Observing Notes – Cancer the Crab & Mythology Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Newsletter of the Baton Rouge Astronomical Society April 2019 © 2019 President’s Message As we move into spring hopefully the run of cloudy nights we had this winter will end. At the last meeting we finally did the drawing for the Meade ETX 90EC, which was won by Joel Tews. Congratulations and thanks to all who bought raffle tickets. I would like take this moment to congratulate Coy Wagoner on being published in the March 2019 Reflector. BRAS CRAWFISH BOIL There will be a crawfish boil on May 18, 2019 at the home of Michele and John. Club will provide the crawfish and trimmings, with side dishes by attendees. Put it on your calendar now, please. We will need a head count to know how many crawfish to buy. More details and a map will follow in next month’s newsletter. Raffle winner was Joel Tews VOLUNTEER AT HRPO: If any of the members wish to volunteer at HRPO, please speak to Chris Kersey, BRAS Liaison for BREC, to fill out the paperwork. -
May 2019 OBSERVER
THE OBSERVER OF THE TWIN CITY AMATEUR ASTRONOMERS Volume 44, Number 5 May 2019 INSIDE THIS ISSUE: 1«Editor’s Choice: Image of the Month – Leo Triplet 2«President’s Note 3«Calendar of Celestial Events – May 2019 3«New & Renewing Members/Dues Blues/E-Mail List 4«This Month’s Phases of the Moon 4«This Month’s Solar Phenomena 4«AstroBits – News from Around the TCAA 5«E/PO for April 2019 5«TCAA Image Gallery 9«WentZel and Wenning at NEAF 11«May 2019 with Jeffrey L. Hunt 12«Throwback Thursday 16«Public Viewing Sessions Schedule for 2019 17«TCAA Calendar of Events for 2019 18«TCAA Treasurer’s Report as of April 29, 2019 19«Renewing Your TCAA Membership 19«TCAA Active on Facebook IMAGE OF THE MONTH: EDITOR’S CHOICE – LEO TRIPLET This month’s image was produced by Tim Stone. Tim writes: This famous triplet of galaxies is known as ‘The Leo Trio,’ a catchy name for a wildly unlikely group of three large galaxies: M65, M66, and NGC 3628. All three are interacting with each other, and are quite close to each other, at least as far as large galaxies go. M65 and 66 are about 160,000 light years apart, about the same as the distance between us and the Magellanic Clouds. Imagine the view of each other these two galaxies enjoy! NGC 3628 is a bit farther from the two, about 300,000 years. If we think our view of M31 is unbelievable, suitably positioned astronomers in these galaxies enjoy a vastly superior view of their neighbors! M66 has been deeply disrupted by the interactions with its two neighbors. -
Observational Diagnostics of Gas in Protoplanetary Disks
Noname manuscript No. (will be inserted by the editor) Observational diagnostics of gas in protoplanetary disks Andr´esCarmona October 2008. Review written for the proceedings of the conference "Origin and Evolution of Planets 2008", Ascona, Switzerland, 2008. Abstract Protoplanetary disks are composed primar- disk last?, how much material is available for forming ily of gas (99% of the mass). Nevertheless, relatively giant planets?, how do the density and the temperature few observational constraints exist for the gas in disks. of the disk vary as a function of the radius?, what are In this review, I discuss several observational diagnos- the dynamics of the disk?. tics in the UV, optical, near-IR, mid-IR, and (sub)-mm Although we have learned important insights from wavelengths that have been employed to study the gas disks from dust observations (see for example the re- in the disks of young stellar objects. I concentrate in views by Henning et al. 2006 and Natta et al. 2007), diagnostics that probe the inner 20 AU of the disk, the dust presents several limitations: (i) dust spectral fea- region where planets are expected to form. I discuss the tures are broad; consequently, dust emission does not potential and limitations of each gas tracer and present provide kinematical information; (ii) dust properties are prospects for future research. expected to change during the planet formation pro- Keywords solar system formation · protoplanetary cess; therefore, quantities such as the gas-to-dust ra- disks · observations · gas · spectroscopy tio (needed to derive the disk mass from dust contin- uum emission in the (sub)-mm) are expected to strongly vary with respect to the conditions of the Interstellar Medium (ISM).