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3.1 Discipline Science Results
CASSINI FINAL MISSION REPORT 2019 1 SATURN Before Cassini, scientists viewed Saturn’s unique features only from Earth and from a few spacecraft flybys. During more than a decade orbiting the gas giant, Cassini studied the composition and temperature of Saturn’s upper atmosphere as the seasons changed there. Cassini also provided up-close observations of Saturn’s exotic storms and jet streams, and heard Saturn’s lightning, which cannot be detected from Earth. The Grand Finale orbits provided valuable data for understanding Saturn’s interior structure and magnetic dynamo, in addition to providing insight into material falling into the atmosphere from parts of the rings. Cassini’s Saturn science objectives were overseen by the Saturn Working Group (SWG). This group consisted of the scientists on the mission interested in studying the planet itself and phenomena which influenced it. The Saturn Atmospheric Modeling Working Group (SAMWG) was formed to specifically characterize Saturn’s uppermost atmosphere (thermosphere) and its variation with time, define the shape of Saturn’s 100 mbar and 1 bar pressure levels, and determine when the Saturn safely eclipsed Cassini from the Sun. Its membership consisted of experts in studying Saturn’s upper atmosphere and members of the engineering team. 2 VOLUME 1: MISSION OVERVIEW & SCIENCE OBJECTIVES AND RESULTS CONTENTS SATURN ........................................................................................................................................................................... 1 Executive -
Radiative Forcing of the Stratosphere of Jupiter, Part I: Atmospheric
*(Revised) Manuscript, clean version Click here to download (Revised) Manuscript, clean version: Manuscript.pdf Click here to view linked References 1 2 3 4 5 Radiative Forcing of the Stratosphere of Jupiter, Part I: 6 7 Atmospheric Cooling Rates from Voyager to Cassini 8 9 10 a, b a c d e 11 X. Zhang *, C.A. Nixon , R.L. Shia , R.A. West , P.G. J. Irwin , R.V. Yelle , M.A. 12 a,c a 13 Allen , Y.L. Yung 14 15 16 17 18 a Division of Geological and Planetary Sciences, California Institute of Technology, 19 20 Pasadena, CA, 91125, USA 21 b 22 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 23 c 24 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, 25 Pasadena, CA 91109, USA 26 d 27 Atmospheric, Oceanic, and Planetary Physics, University of Oxford, Clarendon 28 29 Laboratory, Parks Road, Oxford, OX1 3PU,UK 30 e 31 Department of Planetary Sciences, University of Arizona, Tucson, Arizona, USA 32 33 34 35 36 *Corresponding author at: Division of Geological and Planetary Sciences, California 37 38 Institute of Technology, Pasadena, CA, 91125, USA. 39 40 E-mail address: [email protected] (X. Zhang) 41 42 43 44 45 46 47 Submitted to: 48 49 Plan. Space Sci. (PSS) Special issue on Outer planets systems 50 51 52 53 54 55 56 57 58 59 60 61 62 63 1 64 65 1 2 3 4 Abstract 5 6 7 8 We developed a line-by-line heating and cooling rate model for the stratosphere of 9 10 Jupiter, based on two complete sets of global maps of temperature, C2H2 and C2H6, 11 12 retrieved from the Cassini and Voyager observations in the latitude and vertical plane, 13 with a careful error analysis. -
Migration of a Moonlet in a Ring of Solid Particles: Theory And
Migration of a moonlet in a ring of solid particles : Theory and application to Saturn’s propellers. Aur´elien Crida Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK Laboratoire Cassiop´ee, Universit´ede Nice Sophia-antipolis / CNRS / Observatoire de la Cˆote d’Azur, B.P. 4229, 06304 Nice Cedex 4, France [email protected] John C. B. Papaloizou Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK Hanno Rein Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK S´ebastien Charnoz Laboratoire AIM-UMR 7158, CEA/CNRS/Universit´eParis Diderot, IRFU/Service d’Astrophysique, CEA/Saclay, 91191 Gif-sur-Yvette Cedex, France Julien Salmon Laboratoire AIM-UMR 7158, CEA/CNRS/Universit´eParis Diderot, IRFU/Service d’Astrophysique, CEA/Saclay, 91191 Gif-sur-Yvette Cedex, France ABSTRACT Hundred meter sized objects have been identified by the Cassini spacecraft in Saturn’s A ring through the so-called “propeller” features they create in the ring. These moonlets should migrate, arXiv:1006.1573v1 [astro-ph.EP] 8 Jun 2010 due to their gravitational interaction with the ring ; in fact, some orbital variation have been detected. The standard theory of type I migration of planets in protoplanetary disks can’t be applied to the ring system, as it is pressureless. Thus, we compute the differential torque felt by a moonlet embedded in a two-dimensional disk of solid particles, with flat surface density profile, both analytically and numerically. -
Moons of Saturn National Aeronautics and Space Administration Moons of Saturn
National Aeronautics and Space Administration Moons of Saturn www.nasa.gov National Aeronautics and Space Administration Moons of Saturn www.nasa.gov Saturn, the sixth planet from the Sun, is home to a vast array of • Phoebe orbits the planet in a direction opposite that of Saturn’s • Closest Moon to Saturn Pan intriguing and unique worlds. From the cloud-shrouded surface larger moons, as do several of the recently discovered moons. Pan’s Distance from Saturn 133,583 km (83,022 mi) of Titan to crater-riddled Phoebe, each of Saturn’s moons tells • Mimas has an enormous crater on one side, the result of an • Fastest Orbit Pan another piece of the story surrounding the Saturn system. impact that nearly split the moon apart. Pan’s Orbit Around Saturn 13.8 hours Christiaan Huygens discovered the first known moon of Saturn. • Enceladus displays evidence of active ice volcanism: Cassini • Number of Moons Discovered by Voyager 3 The year was 1655 and the moon is Titan. Jean-Dominique Cas- observed warm fractures where evaporating ice evidently escapes (Atlas, Prometheus, and Pandora) sini made the next four discoveries: Iapetus (1671), Rhea (1672), and forms a huge cloud of water vapor over the south pole. • Number of Moons Discovered by Cassini (So Far) 4 Dione (1684), and Tethys (1684). Mimas and Enceladus were • Hyperion has an odd flattened shape and rotates chaotically, (Methone, Pallene, Polydeuces, and the moonlet 2005S1) both discovered by William Herschel in 1789. The next two probably due to a recent collision. discoveries came at intervals of 50 or more years — Hyperion ABOUT THE IMAGES • Pan orbits within the main rings and helps sweep materials out 1 An ultraviolet (1848) and Phoebe (1898). -
Accretion of Saturn's Mid-Sized Moons During the Viscous
Accretion of Saturn’s mid-sized moons during the viscous spreading of young massive rings: solving the paradox of silicate-poor rings versus silicate-rich moons. Sébastien CHARNOZ *,1 Aurélien CRIDA 2 Julie C. CASTILLO-ROGEZ 3 Valery LAINEY 4 Luke DONES 5 Özgür KARATEKIN 6 Gabriel TOBIE 7 Stephane MATHIS 1 Christophe LE PONCIN-LAFITTE 8 Julien SALMON 5,1 (1) Laboratoire AIM, UMR 7158, Université Paris Diderot /CEA IRFU /CNRS, Centre de l’Orme les Merisiers, 91191, Gif sur Yvette Cedex France (2) Université de Nice Sophia-antipolis / C.N.R.S. / Observatoire de la Côte d'Azur Laboratoire Cassiopée UMR6202, BP4229, 06304 NICE cedex 4, France (3) Jet Propulsion Laboratory, California Institute of Technology, M/S 79-24, 4800 Oak Drive Pasadena, CA 91109 USA (4) IMCCE, Observatoire de Paris, UMR 8028 CNRS / UPMC, 77 Av. Denfert-Rochereau, 75014, Paris, France (5) Department of Space Studies, Southwest Research Institute, Boulder, Colorado 80302, USA (6) Royal Observatory of Belgium, Avenue Circulaire 3, 1180 Uccle, Bruxelles, Belgium (7) Université de Nantes, UFR des Sciences et des Techniques, Laboratoire de Planétologie et Géodynamique, 2 rue de la Houssinière, B.P. 92208, 44322 Nantes Cedex 3, France (8) SyRTE, Observatoire de Paris, UMR 8630 du CNRS, 77 Av. Denfert-Rochereau, 75014, Paris, France (*) To whom correspondence should be addressed ([email protected]) 1 ABSTRACT The origin of Saturn’s inner mid-sized moons (Mimas, Enceladus, Tethys, Dione and Rhea) and Saturn’s rings is debated. Charnoz et al. (2010) introduced the idea that the smallest inner moons could form from the spreading of the rings’ edge while Salmon et al. -
Proquest Dissertations
Detailed study of the Yarkovsky effect on asteroids and solar system implications Item Type text; Dissertation-Reproduction (electronic) Authors Spitale, Joseph Nicholas Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 07/10/2021 08:04:24 Link to Item http://hdl.handle.net/10150/279835 INFORMATION TO USERS This manuscript has t)een reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand comer and continuing from left to right in equal sections with small overiaps. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6" x 9' black and white photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. -
The Formation of the Martian Moons Rosenblatt P., Hyodo R
The Final Manuscript to Oxford Science Encyclopedia: The formation of the Martian moons Rosenblatt P., Hyodo R., Pignatale F., Trinh A., Charnoz S., Dunseath K.M., Dunseath-Terao M., & Genda H. Summary Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not tens of moons of various sizes like for the giant planets, but two small moons: Phobos and Deimos. How did form such a system? This question is still being investigated on the basis of the Earth-based and space-borne observations of the Martian moons and of the more modern theories proposed to account for the formation of other moon systems. The most recent scenario of formation of the Martian moons relies on a giant impact occurring at early Mars history and having also formed the so-called hemispheric crustal dichotomy. This scenario accounts for the current orbits of both moons unlike the scenario of capture of small size asteroids. It also predicts a composition of disk material as a mixture of Mars and impactor materials that is in agreement with remote sensing observations of both moon surfaces, which suggests a composition different from Mars. The composition of the Martian moons is however unclear, given the ambiguity on the interpretation of the remote sensing observations. The study of the formation of the Martian moon system has improved our understanding of moon formation of terrestrial planets: The giant collision scenario can have various outcomes and not only a big moon as for the Earth. -
TRANSIT the Newsletter Of
TRANSIT The Newsletter of 05 July2007 Analemma over Ukraine Front page image: If you took a picture of the Sun at the same time each day, would it remain in the same position? The answer is no, and the shape traced out by the Sun over the course of a year is called an analemma. The Sun's apparent shift is caused by the Earth's motion around the Sun when combined with the tilt of the Earth's rotation axis. The Sun will appear at its highest point of the analemma during summer and at its lowest during winter. Vasilij Rumyantsev ( Crimean Astrophysical Obsevatory) Editorial Last meeting: 8 June 2007 - Keith Johnson delivered a talk on "Astrophotography" whilst seated in front of his computer. He walked us through the technique of using the free Registax software in processing AVIs obtained with a simple and inexpensive Webcam. His choice of subjects to work with were fascinating, an occultation of Saturn by the Moon and a series of Saturn captures. When first seen by non-astroimagers the processing seems hyper- technical but with a good guide through the process by an enthusiast like Keith showed it can be easily learned and that the software itself is very intuitive. The final results always justify the efforts involved judging from Keith’s completed images. Next meeting : Friday, September 14, 2007 subject and presenter to be announced by the Secretary in his Summer Newsletter. Location, Wynyard Planetarium Letters to the Editor : From John Crowther :- We had a 24 page Transit last month completing our 2006-2007 season before the summer break. -
Origin and Evolution of Saturn's Ring System
Origin and Evolution of Saturn’s Ring System Chapter 17 of the book “Saturn After Cassini-Huygens” Saturn from Cassini-Huygens, Dougherty, M.K.; Esposito, L.W.; Krimigis, S.M. (Ed.) (2009) 537-575 Sébastien CHARNOZ * Université Paris Diderot/CEA/CNRS Paris, France Luke DONES Southwest Research Institute Colorado, USA Larry W. ESPOSITO University of Colorado Colorado, USA Paul R. ESTRADA SETI Institute California, USA Matthew M. HEDMAN Cornell University New York, USA (*): to whom correspondence should be addressed : [email protected] 1 ABSTRACT: The origin and long-term evolution of Saturn’s rings is still an unsolved problem in modern planetary science. In this chapter we review the current state of our knowledge on this long- standing question for the main rings (A, Cassini Division, B, C), the F Ring, and the diffuse rings (E and G). During the Voyager era, models of evolutionary processes affecting the rings on long time scales (erosion, viscous spreading, accretion, ballistic transport, etc.) had suggested that Saturn’s rings are not older than 10 8 years. In addition, Saturn’s large system of diffuse rings has been thought to be the result of material loss from one or more of Saturn’s satellites. In the Cassini era, high spatial and spectral resolution data have allowed progress to be made on some of these questions. Discoveries such as the “propellers” in the A ring, the shape of ring-embedded moonlets, the clumps in the F Ring, and Enceladus’ plume provide new constraints on evolutionary processes in Saturn’s rings. At the same time, advances in numerical simulations over the last 20 years have opened the way to realistic models of the rings’ fine scale structure, and progress in our understanding of the formation of the Solar System provides a better-defined historical context in which to understand ring formation. -
Chronophilia; Or, Biding Time in a Solar System
Chronophilia; or, Biding Time in a Solar System MARCUS HALL Department of Evolutionary Biology and Environmental Studies, University of Zurich, Switzerland Abstract Having evolved in a dynamic solar system, all life on earth has adapted to and de- pends on recurring and repeating cycles of light, heat, and gravity. Our sleep cycles, repro- ductive cycles, and emotional cycles are all linked in varying ways to planetary motion even though we continually disrupt, modify, or extend these cycles to go about our personal and collective business. This essay explores how our sense of time is both physiological and cul- tural, with deep ramifications for confronting such challenges as jet lag, navigation, calendar construction, shift work, and even life span. Although chronobiologists have posited the existence of a Zeitgeber, or external master clock that serves to reset our internal clocks, it hasbecomeclearthatanymasterclockreliesasmuchonnaturalelements(suchasarising sun) as cultural elements (such as an alarm clock). Moreover the “circa” of circadian rhythms, suggests that our activities and emotions recur, not in exact twenty-four-hour cycles, but in more plastic and approximate cycles that, according to circumstance and individual, may span somewhat longer or shorter periods than one earthly rotation. Or as one chronobiolo- gist explains, “Any one physiologic variable is characterized by a spectrum of rhythms that aregeneticallyanchored,sociologicallysynchronized...andinfluenced by heliogeophysical effects.” As we contemplate faster and further travel and other activities that disrupt our biorhythms, we need to develop greater awareness of chronophilia, our attachment to rhythm, our love of familiar time. Keywords chronobiology, biorhythm, circadian, desynchrony, jet lag, shift work, sense of time ven before the newborn infant takes his or her first gasps of air, he or she has settled E into recurring patterns of rest and activity. -
Moons and Rings
The Rings of Saturn 5.1 Saturn, the most beautiful planet in our solar system, is famous for its dazzling rings. Shown in the figure above, these rings extend far into space and engulf many of Saturn’s moons. The brightest rings, visible from Earth in a small telescope, include the D, C and B rings, Cassini’s Division, and the A ring. Just outside the A ring is the narrow F ring, shepherded by tiny moons, Pandora and Prometheus. Beyond that are two much fainter rings named G and E. Saturn's diffuse E ring is the largest planetary ring in our solar system, extending from Mimas' orbit to Titan's orbit, about 1 million kilometers (621,370 miles). The particles in Saturn's rings are composed primarily of water ice and range in size from microns to tens of meters. The rings show a tremendous amount of structure on all scales. Some of this structure is related to gravitational interactions with Saturn's many moons, but much of it remains unexplained. One moonlet, Pan, actually orbits inside the A ring in a 330-kilometer-wide (200-mile) gap called the Encke Gap. The main rings (A, B and C) are less than 100 meters (300 feet) thick in most places. The main rings are much younger than the age of the solar system, perhaps only a few hundred million years old. They may have formed from the breakup of one of Saturn's moons or from a comet or meteor that was torn apart by Saturn's gravity. -
DIRECT EVIDENCE for GRAVITATIONAL INSTABILITY and MOONLET FORMATION in SATURN’S RINGS
The Astrophysical Journal Letters, 718:L176–L180, 2010 August 1 doi:10.1088/2041-8205/718/2/L176 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A. DIRECT EVIDENCE FOR GRAVITATIONAL INSTABILITY AND MOONLET FORMATION IN SATURN’s RINGS K. Beurle, C. D. Murray, G. A. Williams, M. W. Evans1, N. J. Cooper, and C. B. Agnor Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK; [email protected] Received 2010 March 3; accepted 2010 June 30; published 2010 July 14 ABSTRACT New images from the Cassini spacecraft reveal optically thick clumps, capable of casting shadows, and associated structures in regions of Saturn’s F ring that have recently experienced close passage by the adjacent moon Prometheus. Using these images and modeling, we show that Prometheus’ perturbations create regions of enhanced density and low relative velocity that are susceptible to gravitational instability and the formation of distended, yet long-lived, gravitationally coherent clumps. Subsequent collisional damping of these low-density clumps may facilitate their collapse into ∼10–20 km contiguous moonlets. The observed behavior of the F ring is analogous to the case of a marginally stable gas disk being driven to instability and collapse via perturbations from an embedded gas giant planet. Key words: instabilities – planets and satellites: dynamical evolution and stability – planets and satellites: formation – planets and satellites: rings – planet–disk interactions 1. INTRODUCTION (Murray et al. 2008; Charnoz et al. 2005; Charnoz 2009); (2) additional analysis of high-resolution Cassini images of the F Saturn’s ring system is the only local example of an astro- ring (Figure 3 of Murray et al.