DOCSLIB.ORG

Notes Du Mont Royal ←

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Notes Du Mont Royal ← Notes du mont Royal www.notesdumontroyal.com 쐰 Cette œuvre est hébergée sur « No- tes du mont Royal » dans le cadre d’un exposé gratuit sur la littérature. SOURCE DES IMAGES Google Livres HERODOTI HISTORIARUM LIBRI 1X. GRAECE ET LATINE. T o M U s V 1. Adnotationes ad lib. v-- 1 X. ARGENTORATI TYPIS PHILIPPI ILCOBI DLRNILÔHc 41 EMW R o D o T1 ,MUSAnu SI’VI ,HISTORIARUM LIBRI 1X.* l AI) VETERUM CODICUM FIDEM DENUO EECENSUIT LECTIONÏS VÀRIETATE CONTINUA INTERPRÉTATIONE LATINA ADNOTATIONIBUS ’ JVVESSELINGII ET VALCKENARII ALIORUMQUE ET SUIS ILLUSTRAVIT IOHANNES SCHWEIGHAEUSER IN ACAD. ARGENT. ET 38Mo PROT. LITERAR. GRAEC. PROF. ACADÉMIAE REG. INSCRIPT. ET HUM. LITERAR. ADSCR- TOMUs SEXTUS. ARGENTORATIÆT PARISIIS "un TREUTTEL ET wÜnTz, murerons, MDCCCXVL’ ’ HERODOTI HISTORIAR. T. VI. P. I. ADNOTATIONES AD LIB.V-VIIÇ c. 171.’ l *’T’. 3 ADNOTATIONES AD H’ERODOTI LIBRUM QUINTUM. CAP. L 5. 01 au) :31 d’un; Ergono’voç) Men haec nonne. mini stribiligq: locum enim misère esse lacunosum , cui sarciendo nullum nunc œmedium. Mihi alia mens. Quid illud tandem , unde lacunae suspicio P Uberior-ne de Paco- m’bus conmembratio? At illa conmodiore loco et tempore cap. 1 2. sequetur; quam hic si deposuisset , longius ab in-. stituto de Perinthiis sermone aberrasset. Verum abstineo me in re cuivîs apertissima. WESS. 17. vô’v finirent 1-6 397w) Docte Valckenarius banc illu- stravit dictionem ad Tragici Phoeniss. vs. 447. Eustathina num muant..." [lin. 1 8.] Codices aversantur , non ma- lumlalioqui, et cum vulgato, scribarum arbitrio, mal. tifariam conmutatum apud Cl. Dukerum ad Thuçydid. lib. 1. 5o. et Diodorum X111. 16. Forte famen Eustath. marmita" voluit, in quo et Union; liquidior engainez, ab eo notata, quem quidem altero. Statim aux). :5 r r: Arch. non absurn ’ dum 0b consequens o’n’yovç, nîsi in Musis zoAAôv sedem cre- berrime occuparet. W ESS. 18. æœxuvlrun îæzxszçs’owt a; lInu’ovtç) In bis observatà aragpîxmç Eustalhio in Iliad. 8’. pag. 272 , 22. est illa carte fortuita, qualem alibi dixit M; crouà’udzïa’uv lem, in! (in? mal nain Ën 7291199479 augumeoô’mv, in 0d. I. p. 566 , 18. Stu- diose quaesîtas recentioribus, commodum oblates allite- ramones non prorsus evitarunt veteres: pmeter ceteros Reiskiu: apta quacdatn cum in rem collegit in Miscell. Lips. Nov. V1. p. 1 13. Quod sequitur, rohxôv Engins-au. Herodoteum est, ut "me. 566059116011! V. 102. Usitatius m).- N; ingénus est et apud Hcrod. V. 77. forum et hic, olim Herod. T. V1. P. I. I A .2 4 ADNOTATIONES lectum : "Mir exhibe: Cod. Amis. In talibus autan in» Ail sacpe male transiit in «enfin Ingenio Marklandi di- gne venusls est correctio, [Ev. Math. x, 31.] "nô "poo- SlmCÀP. Slalom". 111. l seqq. 8min» VALC 3? il»; ahurir i074.K. de.), Unius si Thraces imperio concordes regmntur, Hmdoto iu- dice, alguazil! 7’ a?! (in son) orang? naine?» minot ibis». Huic sententiae suons, niai l’allor, opposuit mordilla lib. Il. cap. 97., dum si Bannis: (inquit, de Thraciluu loquens : ) Mwim lylnro xçnuqirm argotise: au) «in; (distinctif incuit 3? même un) «nous; andin zani 3nde: jurai fait Enduis : nul- lam addit gentem esse nec in Europa neque in Anis, quse posset 2:60am Juo’ymmvoô’n ne?!" intrigua. Sun! apud Thu- cydidan multa, quibus suum ab historiai: paire dissen- sum aemulus non noluerit significatum: vere Aristide; T. 111. p. 650. , in 3’ in": opium n; Omûûy du; du sa) tu! «in; ni; Wpuoîç: neque tantum opimes, sed et Hel- lanici , Hecatazi, similiumque, quin ipsius etiam Herodoti, xœraœço’num. Nostri locus obverssbatur Faustine, lib. I. icap. 9.] p. 22. scribenti : Gpaxôv rÔ’v tain-m 063M; «Mou; sic) 15v 05090km, 31’144»; Kim»), and; Jim il»; Ïv émia-al- éas". Optima Groriov. in his [lin. 2.] and" pro modem: sedquod in proximis posuit, [lin. 5.] iv 76mm, si Groe- cum esset in tali phrasi , hic cette sensum non admitteret tolerahilem. Redibit, opiner, scriptio vers: aluni ni, "q. ra oïmpdv d’0: un) insinuer Mm lyylnyrau: nulle mode contingere poterit faire, r3 in” id; oignent, a? envias aurai vairé.2. si 33 ün’V b6;A singez") L C AllubescitK. Ionicum simulas-o ex Vind. et Arch.; ac paene, ut si Opinions fuisse olim opiner, sdigit. Praecedens il»; non monitor, ut nec similis. Tale lib. 111. 1 13.13 32 i719" yin; 167v il!» - - - Oopioufl. Inmsnem Thraum multitudimm Forum» I. 9. silentio non pressit. Quam autem caussam, cur inexpugnsbiles non sint, No- ster in medium ;ponit, cadem in numerosissimn Scythag rum gente apud Thucydide»: lib. Il. 97. , cui in Cod. Canal. ndscriptum, qui 2109.5! 1’05" m2 ’Hpo’Èoraç un, veto con- Yeniet, ubi artel figurais corrigetur. W ES S. 9. K ne? un orlon) Slephani Kgncraivq. Thracum urbs, ex Hérodote, nusquam in Musis. ngmm’avg, KPnnmau’zv en; AD HERODOT.V..3.4. 1 5 schedis Med., Kganuvmfiv lib. VIL 124. m7. et V111. 116. videbimus. rçmrœvlœy sa? Marin (eidem enim regi, uti posteriori? loco innuit’ur, parebat) Thucydide: 1111.11. 99. iungit; ubi doctissimus Wasse multa , oblitus Attici scri- ptoris 16 brandy au) Kçnnwvmdv lib. IV. 109., quo r9»- s-rma’œ nonnihil debilitatur. WESS. --- Conf. lib. I. cap. 57, 5. et ibi notata. Apud Steph. Byz. vero forsitan sic scriptum oportebat: K profil". WO’Àlç (ses... 3mn: 3E sin: si Kçsia’rwv «29’ ’Hçoâo’rp: quod inde etism fit probabile, quad pro altera forma Kpnnaiyn testimonium invocatur Lymphronis.CÀP. IV. 4. aurai 3è 73v ytvo’utra’v S. roi’ ml Junon.) Istam consuetudinem , ut huius vitae malis congruam, laudaverat Euripides in Cresphonte: Nam n06 decebat coe- tus celebrantes domum Lugere , ubi esset aliquis in lucem edi- tu, Humanae vitae varia. reputantes mala. At, qui lobons mortejinisset graves, Hum: omni arnicas lande et latitia erse- qui. Haec ubi leguntur in Ciceron. Tusc. I. c. 48., Graeca dedit accumtius scripta Io. Davis. quam fecerant Croc. in Stob. p. 495., aut Catcher. Advers. Mise. cap. x. T6, Qsivra’ 99m5?! si; in” imam sans? , non 18v gava-a, pmebent Aeschin. i Son.- in Axiocho pag. 142. Plut. T. l]. p. 56. n. Dieu. Chrys. p05. 27 6.- 11. et Aristid. T. 111. pag. 526. Lugebant infantem notant Transi, secundum Herodotum, [lin. 7.] dvnidflSWI 102 airûemsiïu mina: mils»: imam scripturam satis adfirmavit D108. Herod. p. 84.; altera, nivoayso’nmi, non Gmecà, sicut nultis mendosis, nbusus est Wetsten. in Lucae Ev, suiv, 45. Qui Herodoœn quoque transscripsit Stoboeus , hsec e Nicolao dederat Damase. p. 605. Kawa-soufi. "si; ni) 79min»; 91min, rad; 3! MWŒGWIÇ Mmçlfovw. Haine populi n0- men Zenoûio Cent. V. Prov. p. 125 , 2. restituendum putat Druides; ex Herodoto Trousorum nomes; Ampl. Bouhia. in Cicemn. Tusc. p. 88,. VALC K. 7. 0313114614001)- Expuli ineptum illud cheminerez, ’ Idignissimum obscurissimi inventoris tenebris. Credo ope- ns vocabulo sordes adspersisse, minime a Galeo et aliis dateras. »De Tunis, et, qui corum morem illustrant, Euripidis cultissimis e Cresphonte versibus , pmestat moere. Uberrime Bouhierius et Domine ’ad Ciceronis Disput. Tub cul. lib. I. cap. 48. et, corum’ vestigin prennent, [filmons 6 ADNOTATIONES in Anion. psg. 250. [ad Epicteti Dissert. lib. 1V. cap. 5.] WESS. 8. 75’ xgünrovn) Obsequor sebedis et scriptori, oui. crebrum; max cap. 8. si aime si amidure": et lib. l. 140. si! d’un filetai ni imbu-won tu!!! 1V. 103. Q1188 quidm nbunde videntur. WE S S. CÀP. V. 2. in; 7vmi’xat: gnons; aunaie) Esdem de Paeonibus c. 16. Vere huque de Thracia, W li par: Mm; A0010: 107.1017; il; Juif muséum; Euripide: Androm. vs. 31 5. Vere Strabo, iE irroflzç in Menandri lbbuln Gemm Pari, l’ami yole mais 01333 Il; Il mi 508, si 33m1: Wzïm. 363ml n, arnica; min Lib. VII. pag. 455. c. [p. 297. cd. Cam] Quai! palygamiae studium, Grnecorum plerisque odiosum, in barbaris nunc et olim celebrabatur. WESS. 5. 5 n; mirlwv iomltfo paillera) Dorum Aeolumve lehm valent, ubi poterit: quad rcduxi, commstis Ioni- ci. Gelarum Iegem, r3 lancez?!" mir sarrazin: a; 635?, Sto- phon. Byz. attigit in Perla, de certamine silens, qunle in Indis receptissimum nostra et superiore aetate in Diodon’ lib. XIX. 34., ubî vide, et qune nuperrime Cl. P. Barman- nus Secund. ad Antholog. lib. l. p. 185. WESS. Ibid. lamina )- Hoc ex Atdi potuent Ed. maclai: quad in alias irrepserat lOc’Mro, vol-hum nabis in Parti Le. xicon ’întroduxit velu! Ionicum 00mm, et chaman. An- ctor idoneus Hnaclides docct Daricn fuisse 001m1, me... : Aeolica, ÔIIÀIMMK, 1169214141. Hunc etism tongens Herodoti locum , Stobaeus, pag. 614., ex Nicolao Damase. Indorum uxores memornt , hoc certamine Thrcissis mugis nobilitatas. Cicero Tusc. V. 27. Cam est cuius arum air morulas, in cer- tomen iudiciumque veniunt , quam plurimum ille diluer-in - o - . quae est victriæ, en luta, prosequenlibus suis, 1Mo cum vin in rogum imponitur ; victae moulue discedunt. [bi plurn Do- vis. p. 402 , et ad Actioni Var. Hist. V11. 18. notant Schef- fer et Perizon. Tale certamen inter dans Indus mulieres in Eumenis exercitu narrst Diodorus Sic. XlX. c. 33. et 54. Malta magis mirabile, quad de tribus eiusdcm familise vGraecis mulieribus memarîae tradidit Pausanias lib. 1V. [cap. 2.] p. 284. , quae mira: roi; nivîça’m Ëawaiç imitatrices:- ’ En". VALC K. l ° 621?. 7. mû ri air 3071x9œ1, zdysyîç) Attenti- A?!) 112.1101101: v.4.3. 1 dans Onirocr. I. 9. "(ennui «qui ont). si 11378117; 1mm; , be- ne quidem, quamquam non soli. Tbracum ni; moïses; rai; indigos; cramai-rus userais, and rendra: armions imitiez; retoquera and méfient, in» air BEN-ion; un) in 89min.» M514, ex visu Dia Chymst. propanitOr. XlV. p. 235.11. Caussam veto et originem cor-uns stigmatum , sed fabulo- sam, Pkamcles in Stob. Serin. LXII. p. 400. Verum de bis locupletissime Io. Rhodius in Scribonii Lorgi Conposit. Med. 231. p. 510.
Load more

Recommended publications
  • Copyrighted Material
    Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED
    [Show full text]
  • ARTICLE in PRESS EPSL-09719; No of Pages 8 Earth and Planetary Science Letters Xxx (2009) Xxx–Xxx
    ARTICLE IN PRESS EPSL-09719; No of Pages 8 Earth and Planetary Science Letters xxx (2009) xxx–xxx Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl 1 Regular articles 2 Could Pantheon Fossae be the result of the Apollodorus crater^-forming impact within 3 the Caloris Basin, Mercury? 4 Andrew M. Freed a,⁎, Sean C. Solomon b, Thomas R. Watters c, Roger J. Phillips d, Maria T. Zuber e 5 a Department of Earth and Atmospheric Sciences, Purdue University, West Lafayette, IN 47907, USA 6 b Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA 7 c Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA 8 d Planetary Science Directorate, Southwest Research Institute, Boulder, CO 80302, USA 9 e Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 10 article info abstract OOF 11 12 Article history: 25 The ^~40^-km-diameter Apollodorus impact crater lies near the center of Pantheon Fossae, a complex of 13 Accepted 20 February 2009 radiating linear troughs itself at the approximate center of the 1500-km-diameter Caloris basin on Mercury. 26 14 Available online xxxx Here we use a series of finite element models to explore the idea that the Apollodorus crater-forming impact 27 15 induced the formation of radially oriented graben by altering a pre-existing extensional stress state. Graben 28 16 Editor: T. Spohn in the outer portions of the Caloris basin, which displayPR predominantly circumferential orientations, have 29 191718 been taken as evidence that the basin interior was in a state of horizontal extensional stress as a result of 30 20 Keywords: fi 31 21 Mercury uplift.
    [Show full text]
  • Impact Melt Emplacement on Mercury
    Western University Scholarship@Western Electronic Thesis and Dissertation Repository 7-24-2018 2:00 PM Impact Melt Emplacement on Mercury Jeffrey Daniels The University of Western Ontario Supervisor Neish, Catherine D. The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Jeffrey Daniels 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Daniels, Jeffrey, "Impact Melt Emplacement on Mercury" (2018). Electronic Thesis and Dissertation Repository. 5657. https://ir.lib.uwo.ca/etd/5657 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Impact cratering is an abrupt, spectacular process that occurs on any world with a solid surface. On Earth, these craters are easily eroded or destroyed through endogenic processes. The Moon and Mercury, however, lack a significant atmosphere, meaning craters on these worlds remain intact longer, geologically. In this thesis, remote-sensing techniques were used to investigate impact melt emplacement about Mercury’s fresh, complex craters. For complex lunar craters, impact melt is preferentially ejected from the lowest rim elevation, implying topographic control. On Venus, impact melt is preferentially ejected downrange from the impact site, implying impactor-direction control. Mercury, despite its heavily-cratered surface, trends more like Venus than like the Moon.
    [Show full text]
  • Thomas Robert Watters
    THOMAS ROBERT WATTERS Address: Center for Earth and Planetary Studies National Air and Space Museum Smithsonian Institution P. O. Box 37012, Washington, DC 20013-7012 Education: George Washington University, Ph.D., Geology (1981-1985). Bryn Mawr College, M.A., Geology (1977-1979). West Chester University, B.S. (magna cum laude), Earth Sciences (1973-1977). Experience: Senior Scientist, Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution (1998-present). Chairman, Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution (1989-1998). Research Geologist, Center for Earth and Planetary Studies, Smithsonian Institution, Planetary Geology and Tectonics, Structural Geology, Tectonophysics (1981-1989). Research Assistant, Department of Terrestrial Magnetism, Carnegie Institution of Washington, Chemical Analysis and Fission Track Studies of Meteorites (1980-1981). Research Fellowship, American Museum of Natural History, Electron Microprobe and Petrographic Study of Aubrites and Related Meteorites (1978-1980). Teaching Assistant, Bryn Mawr College (1977-1979), Physical and Historical Geology, Crystallography and Optical Crystallography. Undergraduate Assistant, West Chester University (1973-1977), Teaching Assistant in General and Advanced Astronomy, Physical and Historical Geology. Honors: William P. Phillips Memorial Scholarship (West Chester University); National Air and Space Museum Certificate of Award 1983, 1986, 1989, 1991, 1992, 2002, 2004; American Geophysical Union Editor's Citation for Excellence in Refereeing - Journal Geophysical Research-Planets, 1992; Smithsonian Exhibition Award - Earth Today: A Digital View of Our Dynamic Planet, 1999; Certificate of Appreciation, Geological Society of America, 2005, 2006; Elected to Fellowship in the Geological Society of America, 2007. The Johns Hopkins University Applied Physics Laboratory 2009 Publication Award - Outstanding Research Paper, “Return to Mercury: A Global Perspective on MESSENGER’s First Mercury Flyby (S.C.
    [Show full text]
  • Geology of the Caloris Basin, Mercury: Ysis and Spectral Ratios Were Used to Highlight the Most Important Trends in the Data (17)
    SPECIALSECTION photometrically corrected to normalized re- REPORT flectance at a standard geometry (30° incidence angle, 0° emission angle) and map-projected. From the 11-color data, principal component anal- Geology of the Caloris Basin, Mercury: ysis and spectral ratios were used to highlight the most important trends in the data (17). The first A View from MESSENGER principal component dominantly represents bright- ness variations, whereas the second principal com- Scott L. Murchie,1 Thomas R. Watters,2 Mark S. Robinson,3 James W. Head,4 Robert G. Strom,5 ponent (PC2) isolates the dominant color variation: Clark R. Chapman,6 Sean C. Solomon,7 William E. McClintock,8 Louise M. Prockter,1 the slope of the spectral continuum. Several higher Deborah L. Domingue,1 David T. Blewett1 components isolate fresh craters; a simple color ratio combines these and highlights all fresh The Caloris basin, the youngest known large impact basin on Mercury, is revealed in MESSENGER craters. PC2 and a 480-nm/1000-nm color ratio images to be modified by volcanism and deformation in a manner distinct from that of lunar thus represent the major observed spectral var- impact basins. The morphology and spatial distribution of basin materials themselves closely match iations (Fig. 1B). lunar counterparts. Evidence for a volcanic origin of the basin's interior plains includes embayed The images show that basin exterior materials, craters on the basin floor and diffuse deposits surrounding rimless depressions interpreted to be including the Caloris Montes, Nervo, and von of pyroclastic origin. Unlike lunar maria, the volcanic plains in Caloris are higher in albedo than Eyck Formations, all share similar color proper- surrounding basin materials and lack spectral evidence for ferrous iron-bearing silicates.
    [Show full text]
  • A Two-Dimensional, Linear–Elastic Model to Explain Radial Extensional Fractures, Pantheon Fossae, Caloris Basin, Mercury Brianne Mcdonough
    Undergraduate Review Volume 6 Article 21 2010 A Two-Dimensional, Linear–Elastic Model to Explain Radial Extensional Fractures, Pantheon Fossae, Caloris Basin, Mercury Brianne McDonough Follow this and additional works at: http://vc.bridgew.edu/undergrad_rev Part of the Geology Commons, and the The unS and the Solar System Commons Recommended Citation McDonough, Brianne (2010). A Two-Dimensional, Linear–Elastic Model to Explain Radial Extensional Fractures, Pantheon Fossae, Caloris Basin, Mercury. Undergraduate Review, 6, 107-112. Available at: http://vc.bridgew.edu/undergrad_rev/vol6/iss1/21 This item is available as part of Virtual Commons, the open-access institutional repository of Bridgewater State University, Bridgewater, Massachusetts. Copyright © 2010 Brianne McDonough A Two-Dimensional, Linear– Elastic Model to Explain Radial Extensional Fractures, Pantheon Fossae, Caloris Basin, Mercury BRIANNE MCDONOUGH Brianne McDonough n this study, two-dimensional linear elasticity theory is used to model the lithospheric stress field that produces radial extensional fractures observed is a graduating Earth at Pantheon Fossae in the Caloris Basin of Mercury. These fractures were Science major with imaged by the MESSENGER mission flyby of Mercury on January 14, 2008 a concentration in Iand show radial fractures extending outward from a 40-kilometer impact crater Geology. Through named Apollodorus. Recent studies have proposed several different mechanisms to explain these fractures, including magmatic processes, central basin uplift, and the Adrian Tinsley Program, Brianne stresses produced by the formation of the impact crater itself. completed her project titled, A Two- Dimensional, Linear-Elastic Model to The model presented here attempts to describe the state of the stress field, independent of the physical mechanism that produced it.
    [Show full text]
  • Rest of the Solar System” As We Have Covered It in MMM Through the Years
    As The Moon, Mars, and Asteroids each have their own dedicated theme issues, this one is about the “rest of the Solar System” as we have covered it in MMM through the years. Not yet having ventured beyond the Moon, and not yet having begun to develop and use space resources, these articles are speculative, but we trust, well-grounded and eventually feasible. Included are articles about the inner “terrestrial” planets: Mercury and Venus. As the gas giants Jupiter, Saturn, Uranus, and Neptune are not in general human targets in themselves, most articles about destinations in the outer system deal with major satellites: Jupiter’s Io, Europa, Ganymede, and Callisto. Saturn’s Titan and Iapetus, Neptune’s Triton. We also include past articles on “Space Settlements.” Europa with its ice-covered global ocean has fascinated many - will we one day have a base there? Will some of our descendants one day live in space, not on planetary surfaces? Or, above Venus’ clouds? CHRONOLOGICAL INDEX; MMM THEMES: OUR SOLAR SYSTEM MMM # 11 - Space Oases & Lunar Culture: Space Settlement Quiz Space Oases: Part 1 First Locations; Part 2: Internal Bearings Part 3: the Moon, and Diferent Drums MMM #12 Space Oases Pioneers Quiz; Space Oases Part 4: Static Design Traps Space Oases Part 5: A Biodynamic Masterplan: The Triple Helix MMM #13 Space Oases Artificial Gravity Quiz Space Oases Part 6: Baby Steps with Artificial Gravity MMM #37 Should the Sun have a Name? MMM #56 Naming the Seas of Space MMM #57 Space Colonies: Re-dreaming and Redrafting the Vision: Xities in
    [Show full text]
  • RAYMOND V. SCHODER, S.J. (1916-1987) Classical Studies Department
    y RAYMOND V. SCHODER, S.J. (1916-1987) Classical Studies Department SLIDE COLLECTION OF FIFTH CENTURY SCULPTURES 113 slides Prepared by Laszlo Sulyok Ace. No. 89-15 Computer Name:SCULPTSC.SCH 1 Metal Box Loca lion: 17B The following slides of Fifth Century Sculptures arc from the collection of Fr. Raymond V. Schoder, S.J. They are arranged numerically in the order in which they were received at the archives. The list below provides a brief description of the categorical breakdown of the slides and is copied verbatim from Schoder's own notes on the material.· The collection also contains some replicas of the original artifacts. I. SCULPT: Owl, V c (A crop.) # 2. SCULPT: 'Leonidas' (Sparta) c.400 3. SCULPT: Vc: Boy ded. by Lysikleidcs at Rhamnous, c. 420:30" (A) 4. SCULPT: Vc. Girl, Rhamnous (A) 5. SCULPT: V c. hd, c.475 (Cyrene) 6. SCULPT: Peplophoros * B arberini, c. 475 (T) 7. SCUPLT: Horse, fr. Thasos Hcracles T. pediment, c. 465 (Thas) 8. SCULPT: Base for loutrophoros, Attic, c. 410: Hermes (1), Dead w. apples (Elysian?) (A) 9. SCULPT: Aphrod. on Turtle, aft. or.c. 410 1459 (E. Berlin) 10. SCULPT: fem. fig. fr. frieze Arcs T? (Ag) II. SCULPT: V c. style hd: Diomedes (B) 12. SCULPT: v C. Hercules (Mykonos) 13. SCULPT: V c. style goddcs hd. colossal: Roman copy (Istb) 14. SCULPT: Vc Goddes; Farn. 6269; Rom. (N) 15. SCULPT: Gk. Here. pre-Lysippus (Csv) 16. SCULPT: Choiseui-Gouffier Apollo·· aft early V c (BM) 17. SCULPT: Choiseui/Gouffier Apollo, c. 460 (BM) 18.
    [Show full text]
  • The Universe Contents 3 HD 149026 B
    History . 64 Antarctica . 136 Utopia Planitia . 209 Umbriel . 286 Comets . 338 In Popular Culture . 66 Great Barrier Reef . 138 Vastitas Borealis . 210 Oberon . 287 Borrelly . 340 The Amazon Rainforest . 140 Titania . 288 C/1861 G1 Thatcher . 341 Universe Mercury . 68 Ngorongoro Conservation Jupiter . 212 Shepherd Moons . 289 Churyamov- Orientation . 72 Area . 142 Orientation . 216 Gerasimenko . 342 Contents Magnetosphere . 73 Great Wall of China . 144 Atmosphere . .217 Neptune . 290 Hale-Bopp . 343 History . 74 History . 218 Orientation . 294 y Halle . 344 BepiColombo Mission . 76 The Moon . 146 Great Red Spot . 222 Magnetosphere . 295 Hartley 2 . 345 In Popular Culture . 77 Orientation . 150 Ring System . 224 History . 296 ONIS . 346 Caloris Planitia . 79 History . 152 Surface . 225 In Popular Culture . 299 ’Oumuamua . 347 In Popular Culture . 156 Shoemaker-Levy 9 . 348 Foreword . 6 Pantheon Fossae . 80 Clouds . 226 Surface/Atmosphere 301 Raditladi Basin . 81 Apollo 11 . 158 Oceans . 227 s Ring . 302 Swift-Tuttle . 349 Orbital Gateway . 160 Tempel 1 . 350 Introduction to the Rachmaninoff Crater . 82 Magnetosphere . 228 Proteus . 303 Universe . 8 Caloris Montes . 83 Lunar Eclipses . .161 Juno Mission . 230 Triton . 304 Tempel-Tuttle . 351 Scale of the Universe . 10 Sea of Tranquility . 163 Io . 232 Nereid . 306 Wild 2 . 352 Modern Observing Venus . 84 South Pole-Aitken Europa . 234 Other Moons . 308 Crater . 164 Methods . .12 Orientation . 88 Ganymede . 236 Oort Cloud . 353 Copernicus Crater . 165 Today’s Telescopes . 14. Atmosphere . 90 Callisto . 238 Non-Planetary Solar System Montes Apenninus . 166 How to Use This Book 16 History . 91 Objects . 310 Exoplanets . 354 Oceanus Procellarum .167 Naming Conventions . 18 In Popular Culture .
    [Show full text]
  • Evaluation of the Origin Hypotheses of Pantheon Fossae, Central Caloris Basin, Mercury
    Icarus 209 (2010) 262–270 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Evaluation of the origin hypotheses of Pantheon Fossae, central Caloris basin, Mercury Christian Klimczak *, Richard A. Schultz, Amanda L. Nahm 1 Geomechanics – Rock Fracture Group, Department of Geological Sciences and Engineering, MS172, University of Nevada, Reno, NV 89557, USA article info abstract Article history: The origin of Pantheon Fossae, a complex structure consisting of radial graben in the center of the Caloris Received 24 October 2009 basin, Mercury, has been debated since the structure was first imaged by the MESSENGER spacecraft. Revised 16 April 2010 Three different formation hypotheses have been suggested, i.e. an origin associated with the Apollodorus Accepted 20 April 2010 impact into a previously domed Caloris basin floor, graben formation as surface expressions of dike intru- Available online 24 April 2010 sions and basin-interior uplift alone. In order to test the scenarios, detailed observations from the cur- rently available imagery were compared to the proposed formation mechanisms. We evaluate these Keywords: origin hypotheses by means of detailed interpretations of the graben characteristics and patterns, by Mercury comparing to radial structures from Earth and Venus, and by mechanical analyses for each formation Tectonics hypothesis. Results indicate that the formation of Pantheon Fossae as the result of doming in the central part of the Caloris basin is more likely than it having formed in association with a radially symmetric stress field centered at or near the Apollodorus crater, that would have been created by a magma cham- ber or been superimposed on a pre-existing dome due to impact mechanics.
    [Show full text]
  • Duration of Activity on Lobate-Scarp Thrust Faults on Mercury
    PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Duration of activity on lobate-scarp thrust 10.1002/2015JE004828 faults on Mercury Key Points: Maria E. Banks1,2, Zhiyong Xiao3,4,5, Thomas R. Watters1, Robert G. Strom3, Sarah E. Braden6, • MESSSENGER data reveal stratigraphic 7 8,9 9,10 9,11 relations between lobate scarps Clark R. Chapman , Sean C. Solomon , Christian Klimczak , and Paul K. Byrne and craters 1 • Such relations constrain the timing Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, District of 2 3 and duration of Mercury’s global Columbia, USA, Planetary Science Institute, Tucson, Arizona, USA, Lunar and Planetary Laboratory, University of Arizona, contraction Tucson, Arizona, USA, 4School of Earth Sciences, China University of Geosciences, Wuhan, Hubei, China, 5Centre for Earth • Global contraction deformed Evolution and Dynamics, University of Oslo, Oslo, Norway, 6School of Earth and Space Exploration, Arizona State University, ’ Mercury s surface over much of the 7 8 last 3–4 Gyr Tempe, Arizona, USA, Department of Space Studies, Southwest Research Institute, Boulder, Colorado, USA, Lamont- Doherty Earth Observatory, Columbia University, Palisades, New York, USA, 9Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, District of Columbia, USA, 10Department of Geology, University of Georgia, Athens, Georgia, USA, 11Lunar and Planetary Institute, Universities Space Research Association, Houston, Texas, USA Correspondence to: M. E. Banks, [email protected] Abstract Lobate scarps, landforms interpreted as the surface manifestation of thrust faults, are widely distributed across Mercury and preserve a record of its history of crustal deformation. Their formation is Citation: primarily attributed to the accommodation of horizontal shortening of Mercury’s lithosphere in response to Banks, M.
    [Show full text]
  • The Book of Dead Philosophers
    Praise for Simon Critchley's THE BOOK OF DEAD PHILOSOPHERS "A provocative and engrossing invitation to think about the human condition and what philosophy can and can't do to illuminate it." —Financial Times "Concise, witty and oddly heartening." —New Statesman (A 2008 Book of the Year) "Full of wonderful absurdities.... Extremely enjoyable." —The Independent (London) "Simon Critchley is probably the sharpest and most lucid philosopher writing in English today." —Tom McCarthy, author of Remainder "Ingenious. Packed with great stories." —Time Out London "A tremendous addition to an all too sparse literature. Brilliant, entertaining, informative." —New Humanist (UK) "A fabulous concept. [Critchley writes] with dash, humour and an eye for scandalous detail." —The Vancouver Sun "[Critchley is] among the hippest of (living) British philosophers." —The Book Bench, newyorker.com "Surprisingly good fun. Worthy of the prose writings of Woody Allen. .. Not the least of the pleasures of this odd book, lighthearted and occasionally facetious as it is, is that in surveying a chronological history of philoso• phers it provides a sweep through the entire history of philosophy itself." —The Irish Times "Critchley has a lightness of touch, a nimbleness of thought, and a mocking graveyard humour that puts you in mind of Hamlet with a skull." —The Independent on Sunday (London) Simon Critchley "The Book of Dead Philosophers is something of a magic trick: on the surface an amusing and bemused series of blackout sketches of philosophers' often rather humble THE BOOK OF and/or brutal deaths, it actually is an utterly serious, DEAD PHILOSOPHERS deeply moving, cant-free attempt to return us to the gor- geousness of material existence, to our creatureliness, to our clownish bodies, to the only immortality available to us (immersion in the moment).
    [Show full text]