Other Moons Prepared by Romanian Team
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Arxiv:1912.09192V2 [Astro-Ph.EP] 24 Feb 2020
Draft version February 25, 2020 Typeset using LATEX preprint style in AASTeX62 Photometric analyses of Saturn's small moons: Aegaeon, Methone and Pallene are dark; Helene and Calypso are bright. M. M. Hedman,1 P. Helfenstein,2 R. O. Chancia,1, 3 P. Thomas,2 E. Roussos,4 C. Paranicas,5 and A. J. Verbiscer6 1Department of Physics, University of Idaho, Moscow, ID 83844 2Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca NY 14853 3Center for Imaging Science, Rochester Institute of Technology, Rochester NY 14623 4Max Planck Institute for Solar System Research, G¨ottingen,Germany 37077 5APL, John Hopkins University, Laurel MD 20723 6Department of Astronomy, University of Virginia, Charlottesville, VA 22904 ABSTRACT We examine the surface brightnesses of Saturn's smaller satellites using a photometric model that explicitly accounts for their elongated shapes and thus facilitates compar- isons among different moons. Analyses of Cassini imaging data with this model reveals that the moons Aegaeon, Methone and Pallene are darker than one would expect given trends previously observed among the nearby mid-sized satellites. On the other hand, the trojan moons Calypso and Helene have substantially brighter surfaces than their co-orbital companions Tethys and Dione. These observations are inconsistent with the moons' surface brightnesses being entirely controlled by the local flux of E-ring par- ticles, and therefore strongly imply that other phenomena are affecting their surface properties. The darkness of Aegaeon, Methone and Pallene is correlated with the fluxes of high-energy protons, implying that high-energy radiation is responsible for darkening these small moons. Meanwhile, Prometheus and Pandora appear to be brightened by their interactions with nearby dusty F ring, implying that enhanced dust fluxes are most likely responsible for Calypso's and Helene's excess brightness. -
Table of Contents
Solar System Table of Contents Publisher's Note Editors' Introduction List of Contributors Complete List of Contents Archeaostronomy (new) Asteroids Auroras Big Bang Brown Dwarfs Callisto (new) Ceres (new) Comet Halley Comet Shoemaker-Levy 9 (new) Comets Coordinate Systems Coronal Holes and Coronal Mass Ejections (new) Cosmic Rays Cosmology Dwarf Planets (new) Earth-Moon Relations (new) Earth-Sun Relations Earth System Science Earth's Age Earth's Atmosphere Earth's Composition Earth's Core Earth's Core-Mantle Boundary Earth's Crust Earth's Crust-Mantle Boundary(new) Earth's Differentiation Earth's Magnetic Field: Origins Earth's Magnetic Field: Secular Variation Earth's Magnetic Field at Present Earth's Magnetosphere Earth's Mantle Earth's Oceans Earth's Origin Earth's Rotation Earth's Shape Earth's Structure Eclipses Electromagnetic Radiation: Thermal Emissions (new) Electromagnetic Radiation: Nonthermal Emissions (new) Enceladus (new) Eris and Dysnomia (new) Europa Extrasolar Planet Detection Methods (new) Extrasolar Planetary Systems Extraterrestrial Life in the Solar System Gamma-Ray Bursters Ganymede (new) General Relativity Gravity Measurement Greenhouse Effect Habitable Zones (new) Hertzsprung-Russell Diagram Iapetus (new) Impact Cratering Infrared Astronomy Interstellar Clouds and the Interstellar Medium Interplanetary Environment (new) Io Jovian Planets Jupiter's Atmosphere Jupiter's Great Red Spot Jupiter's Interior (new) Jupiter's Magnetic Field and Radiation Belts Jupiter's Ring System (new) Jupiter's Satellites Kuiper Belt -
Cassini Update
Cassini Update Dr. Linda Spilker Cassini Project Scientist Outer Planets Assessment Group 22 February 2017 Sols%ce Mission Inclina%on Profile equator Saturn wrt Inclination 22 February 2017 LJS-3 Year 3 Key Flybys Since Aug. 2016 OPAG T124 – Titan flyby (1584 km) • November 13, 2016 • LAST Radio Science flyby • One of only two (cf. T106) ideal bistatic observations capturing Titan’s Northern Seas • First and only bistatic observation of Punga Mare • Western Kraken Mare not explored by RSS before T125 – Titan flyby (3158 km) • November 29, 2016 • LAST Optical Remote Sensing targeted flyby • VIMS high-resolution map of the North Pole looking for variations at and around the seas and lakes. • CIRS last opportunity for vertical profile determination of gases (e.g. water, aerosols) • UVIS limb viewing opportunity at the highest spatial resolution available outside of occultations 22 February 2017 4 Interior of Hexagon Turning “Less Blue” • Bluish to golden haze results from increased production of photochemical hazes as north pole approaches summer solstice. • Hexagon acts as a barrier that prevents haze particles outside hexagon from migrating inward. • 5 Refracting Atmosphere Saturn's• 22unlit February rings appear 2017 to bend as they pass behind the planet’s darkened limb due• 6 to refraction by Saturn's upper atmosphere. (Resolution 5 km/pixel) Dione Harbors A Subsurface Ocean Researchers at the Royal Observatory of Belgium reanalyzed Cassini RSS gravity data• 7 of Dione and predict a crust 100 km thick with a global ocean 10’s of km deep. Titan’s Summer Clouds Pose a Mystery Why would clouds on Titan be visible in VIMS images, but not in ISS images? ISS ISS VIMS High, thin cirrus clouds that are optically thicker than Titan’s atmospheric haze at longer VIMS wavelengths,• 22 February but optically 2017 thinner than the haze at shorter ISS wavelengths, could be• 8 detected by VIMS while simultaneously lost in the haze to ISS. -
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 -
Chapter 4. Hatred in Hesiod
This electronic thesis or dissertation has been downloaded from Explore Bristol Research, http://research-information.bristol.ac.uk Author: Kilgallon, Silvie Title: Hatred in Hesiod General rights Access to the thesis is subject to the Creative Commons Attribution - NonCommercial-No Derivatives 4.0 International Public License. A copy of this may be found at https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode This license sets out your rights and the restrictions that apply to your access to the thesis so it is important you read this before proceeding. Take down policy Some pages of this thesis may have been removed for copyright restrictions prior to having it been deposited in Explore Bristol Research. However, if you have discovered material within the thesis that you consider to be unlawful e.g. breaches of copyright (either yours or that of a third party) or any other law, including but not limited to those relating to patent, trademark, confidentiality, data protection, obscenity, defamation, libel, then please contact [email protected] and include the following information in your message: •Your contact details •Bibliographic details for the item, including a URL •An outline nature of the complaint Your claim will be investigated and, where appropriate, the item in question will be removed from public view as soon as possible. Hatred in Hesiod Silvie Kilgallon A dissertation submitted to the University of Bristol in accordance with the requirements for award of the degree of Doctor of Philosophy in the Faculty of Arts, January 2019. Word Count: 75,322. 2 Abstract: This thesis examines the conception and role of hatred in the Theogony and Works and Days of Hesiod. -
HOMERIC-ILIAD.Pdf
Homeric Iliad Translated by Samuel Butler Revised by Soo-Young Kim, Kelly McCray, Gregory Nagy, and Timothy Power Contents Rhapsody 1 Rhapsody 2 Rhapsody 3 Rhapsody 4 Rhapsody 5 Rhapsody 6 Rhapsody 7 Rhapsody 8 Rhapsody 9 Rhapsody 10 Rhapsody 11 Rhapsody 12 Rhapsody 13 Rhapsody 14 Rhapsody 15 Rhapsody 16 Rhapsody 17 Rhapsody 18 Rhapsody 19 Rhapsody 20 Rhapsody 21 Rhapsody 22 Rhapsody 23 Rhapsody 24 Homeric Iliad Rhapsody 1 Translated by Samuel Butler Revised by Soo-Young Kim, Kelly McCray, Gregory Nagy, and Timothy Power [1] Anger [mēnis], goddess, sing it, of Achilles, son of Peleus— 2 disastrous [oulomenē] anger that made countless pains [algea] for the Achaeans, 3 and many steadfast lives [psūkhai] it drove down to Hādēs, 4 heroes’ lives, but their bodies it made prizes for dogs [5] and for all birds, and the Will of Zeus was reaching its fulfillment [telos]— 6 sing starting from the point where the two—I now see it—first had a falling out, engaging in strife [eris], 7 I mean, [Agamemnon] the son of Atreus, lord of men, and radiant Achilles. 8 So, which one of the gods was it who impelled the two to fight with each other in strife [eris]? 9 It was [Apollo] the son of Leto and of Zeus. For he [= Apollo], infuriated at the king [= Agamemnon], [10] caused an evil disease to arise throughout the mass of warriors, and the people were getting destroyed, because the son of Atreus had dishonored Khrysēs his priest. Now Khrysēs had come to the ships of the Achaeans to free his daughter, and had brought with him a great ransom [apoina]: moreover he bore in his hand the scepter of Apollo wreathed with a suppliant’s wreath [15] and he besought the Achaeans, but most of all the two sons of Atreus, who were their chiefs. -
'Myth' and 'Religion'
THOUGHTS ON MYTH AND RELIGION IN EARLY GREEK HISTORIOGRAPHY Robert L. FOWLER University of Bristol [email protected] RESUMEN: El artículo examina el nacimiento del concepto de mythos/mito en el contexto de la historiografía y la mitografía de la Grecia arcaica. La posibilidad de oponerse a relatos tradicionales es un factor crítico en este proceso y se relaciona estrechamente con los esfuerzos de los autores por fijar su autoridad. Se compara la práctica de Heródoto con la de los primeros mitógrafos y, aunque hay amplias similitudes, hay diferencias cruciales en el tratamiento de los asuntos religiosos. Los escrúpulos personales de Heródoto responden en parte a su bien conocida reserva en lo referente a los dioses, pero es también relevante su actitud acerca de la tarea del historiador y su noción de cómo los dioses intervienen en la historia. Mientras que los mitógrafos tratan de historicizar la mitología, Heródoto trata de modo notable de desmitologizar la historia, separando ambas, pero al mismo tiempo definiendo con más profundidad que nunca sus auténticas interconexiones. Esta situación sugiere algunas consideraciones generales acerca de la relación entre mito y ritual en Grecia. ABSTRACT: The article examines the emerging concept of mythos/myth in the context of early Greek historiography and mythography. The possibility of contesting traditional stories is a critical factor in this process, and is closely related to the efforts of writers to establish their authority. Herodotos’ practice is compared with that of the early mythographers, and though there are some broad similarities, there are crucial differences in their approach to religious matters. -
L RES~ARCH Coljncll ·
NA~IOf\i'At ACADEMIES OF SCIENCE AND ENGiNEERING 7 ·.· ·.·. : NATIONAL RES~ARCH ColJNCll · of the UNITED STATES OF AMERICA UNITED• STATES NATIONAL COMMITTEEI . International Union of Radio Sden<:e Nationa.1 Radio Science Meeting 13-15 January 1982 · f l··.. ·· Sponsored by USNC/URSI in cooperation with r Institute of Electrical and Electronics Engineers University of· Colorado Boulder, Colorado U.S.A. ~· 1' National Radio Science Meeting 13-15 January 19 82 Condensed Technical Program TUESDAY, 12 JANUARY 0900 CCIR U.S. Study Group 5 OT 8-8 CCIR U.S. Study ,Gr.oup 6 Radio Building 2000-2400 USNC/URSI Meeting Broker Inn WEDNESDAY, 13 JANUARY 0900-1200 A-1 Time Domai~ 1-ieasurements CRl-42 B-1 Scattering CR2-28 B-2 Electromagnetic Theory CR2-28 C-1 Topics in Information Theory CR0-30 F-1 Propagation Theory and Models CR2-26 J-1 Millimeter-Wave Astronomy UMC Ballroom 1330-1700 A-2 Microwave/Millimeter Wave Measurements CRl-42 B-3 Antenna Theory and Practice CR2-28 B-4 Inverse Scattering CR2-6 C-2 Digital HF: Equaltz ation and Reiated CR0-30 Techniques E-1 EM Noise in the Sea CRl-40 F-2 Ground-Based Remote Sensing CR2-26 H-1 VLF-ELF Wave Injection Into the CRl-46 Magnetosphere J-2 Very Long Baseline Interferometry UMC 157 1700 Commission A Business Meeting CRl-42 Commission C Business Meeting CR0-30 Commission E Business Meeting CRl-40 Commission F Business Meeting CR2-26 Commission H Business Meeting CRl-46 1800-2000 Reception Engineering Center 2000-2200 IEEE Wave Propagation Standards Committee CRl-46 TH.URSDAY, 14 JANUARY 0830-1200 A-3 -
Beauty on Display Plato and the Concept of the Kalon
BEAUTY ON DISPLAY PLATO AND THE CONCEPT OF THE KALON JONATHAN FINE Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2018 © 2018 Jonathan Fine All rights reserved ABSTRACT BEAUTY ON DISPLAY: PLATO AND THE CONCEPT OF THE KALON JONATHAN FINE A central concept for Plato is the kalon – often translated as the beautiful, fine, admirable, or noble. This dissertation shows that only by prioritizing dimensions of beauty in the concept can we understand the nature, use, and insights of the kalon in Plato. The concept of the kalon organizes aspirations to appear and be admired as beautiful for one’s virtue. We may consider beauty superficial and concern for it vain – but what if it were also indispensable to living well? By analyzing how Plato uses the concept of the kalon to contest cultural practices of shame and honour regulated by ideals of beauty, we come to see not only the tensions within the concept but also how attractions to beauty steer, but can subvert, our attempts to live well. TABLE OF CONTENTS Acknowledgements ii 1 Coordinating the Kalon: A Critical Introduction 1 1 The Kalon and the Dominant Approach 2 2 A Conceptual Problem 10 3 Overview 24 2 Beauty, Shame, and the Appearance of Virtue 29 1 Our Ancient Contemporaries 29 2 The Cultural Imagination 34 3 Spirit and the Social Dimension of the Kalon 55 4 Before the Eyes of Others 82 3 Glory, Grief, and the Problem of Achilles 100 1 A Tragic Worldview 103 2 The Heroic Ideal 110 3 Disgracing Achilles 125 4 Putting Poikilia in its Place 135 1 Some Ambivalences 135 2 The Aesthetics of Poikilia 138 3 The Taste of Democracy 148 4 Lovers of Sights and Sounds 173 5 The Possibility of Wonder 182 5 The Guise of the Beautiful 188 1 A Psychological Distinction 190 2 From Disinterested Admiration to Agency 202 3 The Opacity of Love 212 4 Looking Good? 218 Bibliography 234 i ACKNOWLEDGEMENTS “To do philosophy is to explore one’s own temperament,” Iris Murdoch suggested at the outset of “Of ‘God’ and ‘Good’”. -
1. Some of the Definitions of the Different Types of Objects in the Solar
1. Some of the definitions of the different types of objects in has the greatest orbital inclination (orbit at the the solar system overlap. Which one of the greatest angle to that of Earth)? following pairs does not overlap? That is, if an A) Mercury object can be described by one of the labels, it B) Mars cannot be described by the other. C) Jupiter A) dwarf planet and asteroid D) Pluto B) dwarf planet and Kuiper belt object C) satellite and Kuiper belt object D) meteoroid and planet 10. Of the following objects in the solar system, which one has the greatest orbital eccentricity and therefore the most elliptical orbit? 2. Which one of the following is a small solar system body? A) Mercury A) Rhea, a moon of Saturn B) Mars B) Pluto C) Earth C) Ceres (an asteroid) D) Pluto D) Mathilde (an asteroid) 11. What is the largest moon of the dwarf planet Pluto 3. Which of the following objects was discovered in the called? twentieth century? A) Chiron A) Pluto B) Callisto B) Uranus C) Charon C) Neptune D) Triton D) Ceres 12. If you were standing on Pluto, how often would you see 4. Pluto was discovered in the satellite Charon rise above the horizon each A) 1930. day? B) 1846. A) once each 6-hour day as Pluto rotates on its axis C) 1609. B) twice each 6-hour day because Charon is in a retrograde D) 1781. orbit C) once every 2 days because Charon orbits in the same direction Pluto rotates but more slowly 5. -
The Rings and Inner Moons of Uranus and Neptune: Recent Advances and Open Questions
Workshop on the Study of the Ice Giant Planets (2014) 2031.pdf THE RINGS AND INNER MOONS OF URANUS AND NEPTUNE: RECENT ADVANCES AND OPEN QUESTIONS. Mark R. Showalter1, 1SETI Institute (189 Bernardo Avenue, Mountain View, CA 94043, mshowal- [email protected]! ). The legacy of the Voyager mission still dominates patterns or “modes” seem to require ongoing perturba- our knowledge of the Uranus and Neptune ring-moon tions. It has long been hypothesized that numerous systems. That legacy includes the first clear images of small, unseen ring-moons are responsible, just as the nine narrow, dense Uranian rings and of the ring- Ophelia and Cordelia “shepherd” ring ε. However, arcs of Neptune. Voyager’s cameras also first revealed none of the missing moons were seen by Voyager, sug- eleven small, inner moons at Uranus and six at Nep- gesting that they must be quite small. Furthermore, the tune. The interplay between these rings and moons absence of moons in most of the gaps of Saturn’s rings, continues to raise fundamental dynamical questions; after a decade-long search by Cassini’s cameras, sug- each moon and each ring contributes a piece of the gests that confinement mechanisms other than shep- story of how these systems formed and evolved. herding might be viable. However, the details of these Nevertheless, Earth-based observations have pro- processes are unknown. vided and continue to provide invaluable new insights The outermost µ ring of Uranus shares its orbit into the behavior of these systems. Our most detailed with the tiny moon Mab. Keck and Hubble images knowledge of the rings’ geometry has come from spanning the visual and near-infrared reveal that this Earth-based stellar occultations; one fortuitous stellar ring is distinctly blue, unlike any other ring in the solar alignment revealed the moon Larissa well before Voy- system except one—Saturn’s E ring. -
Abstracts of the 50Th DDA Meeting (Boulder, CO)
Abstracts of the 50th DDA Meeting (Boulder, CO) American Astronomical Society June, 2019 100 — Dynamics on Asteroids break-up event around a Lagrange point. 100.01 — Simulations of a Synthetic Eurybates 100.02 — High-Fidelity Testing of Binary Asteroid Collisional Family Formation with Applications to 1999 KW4 Timothy Holt1; David Nesvorny2; Jonathan Horner1; Alex B. Davis1; Daniel Scheeres1 Rachel King1; Brad Carter1; Leigh Brookshaw1 1 Aerospace Engineering Sciences, University of Colorado Boulder 1 Centre for Astrophysics, University of Southern Queensland (Boulder, Colorado, United States) (Longmont, Colorado, United States) 2 Southwest Research Institute (Boulder, Connecticut, United The commonly accepted formation process for asym- States) metric binary asteroids is the spin up and eventual fission of rubble pile asteroids as proposed by Walsh, Of the six recognized collisional families in the Jo- Richardson and Michel (Walsh et al., Nature 2008) vian Trojan swarms, the Eurybates family is the and Scheeres (Scheeres, Icarus 2007). In this theory largest, with over 200 recognized members. Located a rubble pile asteroid is spun up by YORP until it around the Jovian L4 Lagrange point, librations of reaches a critical spin rate and experiences a mass the members make this family an interesting study shedding event forming a close, low-eccentricity in orbital dynamics. The Jovian Trojans are thought satellite. Further work by Jacobson and Scheeres to have been captured during an early period of in- used a planar, two-ellipsoid model to analyze the stability in the Solar system. The parent body of the evolutionary pathways of such a formation event family, 3548 Eurybates is one of the targets for the from the moment the bodies initially fission (Jacob- LUCY spacecraft, and our work will provide a dy- son and Scheeres, Icarus 2011).