Cassini Images Show Moon on a Roll
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
A Wunda-Full World? Carbon Dioxide Ice Deposits on Umbriel and Other Uranian Moons
Icarus 290 (2017) 1–13 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus A Wunda-full world? Carbon dioxide ice deposits on Umbriel and other Uranian moons ∗ Michael M. Sori , Jonathan Bapst, Ali M. Bramson, Shane Byrne, Margaret E. Landis Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA a r t i c l e i n f o a b s t r a c t Article history: Carbon dioxide has been detected on the trailing hemispheres of several Uranian satellites, but the exact Received 22 June 2016 nature and distribution of the molecules remain unknown. One such satellite, Umbriel, has a prominent Revised 28 January 2017 high albedo annulus-shaped feature within the 131-km-diameter impact crater Wunda. We hypothesize Accepted 28 February 2017 that this feature is a solid deposit of CO ice. We combine thermal and ballistic transport modeling to Available online 2 March 2017 2 study the evolution of CO 2 molecules on the surface of Umbriel, a high-obliquity ( ∼98 °) body. Consid- ering processes such as sublimation and Jeans escape, we find that CO 2 ice migrates to low latitudes on geologically short (100s–1000 s of years) timescales. Crater morphology and location create a local cold trap inside Wunda, and the slopes of crater walls and a central peak explain the deposit’s annular shape. The high albedo and thermal inertia of CO 2 ice relative to regolith allows deposits 15-m-thick or greater to be stable over the age of the solar system. -
Privacy Policy
Privacy Policy Culmia Privacy Policy Culmia Desarrollos Inmobiliarios, S.L.U. (hereinafter, “the manager”), with headquarters in Madrid, Calle Génova, 27, Company Tax No. B-67186999, is an integral manager of property assets and a member of a Property Group to which it provides its services. The manager provides its services to the following property developers who are members of its Group: Company Company Company Company Tax Tax No. No. Saturn Holdco S.A.U. A88554100 Antea Activos Inmobiliarios B88554324 S.L.U. Thrym Activos Inmobiliarios S.L.U. B88554142 Redes Promotora 1 Ma, B88093117 S.L.U. Erriap Activos Inmobiliarios S.L.U. B88554159 Redes Promotora 2 Ma, B88093174 S.L.U. Daphne Activos Inmobiliarios S.L.U. B88554167 Redes Promotora 3 Ma, B88093265 S.L.U. Dione Activos Inmobiliarios S.L.U. B88554183 Redes Promotora 4 Ma, B88093356 S.L.U. Fornjot Activos Inmobiliarios S.L.U. B88554191 Redes Promotora 5 Ma, B88093471 S.L.U. Greip Activos Inmobiliarios S.L.U. B88554217 Redes Promotora 6 Ma, B88145073 S.L.U. Hiperion Activos Inmobiliarios B88554233 Redes Promotora 7 Ma, B88145123 S.L.U. S.L.U. Loge Activos Inmobiliarios S.L.U. B88554241 Redes Promotora 8 Ma, B88145263 S.L.U. Kiviuq Activos Inmobiliarios S.L.U. B88554258 Redes Promotora 9, S.L.U. B88159728 Narvi Activos Inmobiliarios S.L.U. B88554266 Redes 2 2018 Iberica 2 B88160221 S.L.U. Polux Activos Inmobiliarios S.L.U. B88554282 Redes 2 2018 Iberica 3 B88160239 S.L.U. Siarnaq Activos Inmobiliarios S.L.U. B88554290 Redes 2 Promotora B88160247 Inversiones 2018 IV S.L.U. -
Margaret Kivelson
Margaret Galland Kivelson 6/27/2013 Margaret Kivelson- Dynamics - MoP 2011 – Boston University 1 Rotationally driven magnetospheres! (Mauk et al., (Saturn, Chapter 11) state: “while it is true that Saturn’s magnetosphere is intermediate between those of Earth and Jupiter in terms of size (whether measured by RP; RPP, or RMP), it is not intermediate in any meaningful dynamical sense. It is clearly rotationally driven like Jupiter’s, not solar-wind–driven like Earth’s.” Margaret Kivelson- Dynamics - MoP 6/27/2013 2011 – Boston University 2 This Vasyliunas (1983) diagram is a necessary element of any discussion of the magnetospheres of gas giants! It captures some critical features implicitly or explicitly: A significant source of heavy plasma deep within the magnetopause (Io, Enceladus) is spun up to some fraction of corotation speed by field-aligned currents coupling magnetosphere and ionosphere. Rotation dominates the dynamics – drives plasmoid releases down the tail. Solar wind shapes the boundaries but does not dominate the dynamics. Margaret Kivelson- Dynamics - MoP 6/27/2013 2011 – Boston University 3 Thomas et al., 2004 Schneider and Trager, 1995 In the pickup process, ions acquire perp. thermal speed of local rotation speed. 2 Energy added N pum() Pickup energy is shared with background plasma. Typically heats plasma. Melin6/27/2013 et al., 2009 4 Much is well established, but puzzles remain. Discuss a few features energy density of plasma and why it changes vs. radial distance, vs. local time, periodicities, Anomalies in regions of high dust density. Margaret Kivelson- Dynamics - MoP 6/27/2013 2011 – Boston University 5 At Earth, temperature (more correctly Below a plot from Kane et al (1995) thermal energy per particle) decreases of Voyager data at Jupiter, modeled with but not at Jupiter or Saturn. -
Mars Exploration Office Jet Propulsion Laboratory California Institute of Technology Pasadena, California
TECHNOLOGIES FOR MARSEXPLORATION AND SAMPLE RETURN Carl F. Ruoff, Technology Manager Mars Exploration Office Jet Propulsion Laboratory California Institute of Technology Pasadena, California ABSTRACT history, to understand how the planet evolved physically, and to locate potentially useful resources. A comprehensive program of robotic Mars exploration is The common thread among these is water: How much being undertaken inorder to address important scientific existed, when, where, and in what form? In addition to questions, to investigate whether or not life exists or ever remote sensing, answering these questions will require existed on Mars, and to pave the way for eventual human surface and subsurface sampling, in-situ analysis, and presence. The program, which is likely to include returning samples to Earth for analysis in terrestrial establishing robotic outposts, will require many technical laboratories. advances. This paper briefly describes key missions in the Mars exploration program, including robotic outposts, and As currently envisioned, the exploration strategy begins discusses near- and far-term technologies needed for theirwith a series of robotic missions which gradually implementation. evolve into the sustained presence of robotic outposts. The early missions will perform science investigations, INTRODUCTION acquire and returnsamples, and will provide engineering The first decades of the new Millennium will see a data on system and technology performance in the vigorous program of robotic Mars exploration, Martian environment. They will also establish undertaken both for compelling scientific reasons as communication and navigation capabilities and will well as to pave the way, over the long term, for human make it possible to select promising sites for additional missions and potential human habitation. -
Cassini Observations of Saturn's Irregular Moons
EPSC Abstracts Vol. 12, EPSC2018-103-1, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 Cassini Observations of Saturn's Irregular Moons Tilmann Denk (1) and Stefano Mottola (2) (1) Freie Universität Berlin, Germany ([email protected]), (2) DLR Berlin, Germany 1. Introduction two prograde irregulars are slower than ~13 h, while the periods of all but two retrogrades are faster than With the ISS-NAC camera of the Cassini spacecraft, ~13 h. The fastest period (Hati) is much slower than we obtained photometric lightcurves of 25 irregular the disruption rotation barrier for asteroids (~2.3 h), moons of Saturn. The goal was to derive basic phys- indicating that Saturn's irregulars may be rubble piles ical properties of these objects (like rotational periods, of rather low densities, possibly as low as of comets. shapes, pole-axis orientations, possible global color variations, ...) and to get hints on their formation and Table: Rotational periods of 25 Saturnian irregulars evolution. Our campaign marks the first utilization of an interplanetary probe for a systematic photometric Moon Approx. size Rotational period survey of irregular moons. name [km] [h] Hati 5 5.45 ± 0.04 The irregular moons are a class of objects that is very Mundilfari 7 6.74 ± 0.08 distinct from the inner moons of Saturn. Not only are Loge 5 6.9 ± 0.1 ? they more numerous (38 versus 24), but also occupy Skoll 5 7.26 ± 0.09 (?) a much larger volume within the Hill sphere of Suttungr 7 7.67 ± 0.02 Saturn. -
Planetary Magnetospheres
CLBE001-ESS2E November 9, 2006 17:4 100-C 25-C 50-C 75-C C+M 50-C+M C+Y 50-C+Y M+Y 50-M+Y 100-M 25-M 50-M 75-M 100-Y 25-Y 50-Y 75-Y 100-K 25-K 25-19-19 50-K 50-40-40 75-K 75-64-64 Planetary Magnetospheres Margaret Galland Kivelson University of California Los Angeles, California Fran Bagenal University of Colorado, Boulder Boulder, Colorado CHAPTER 28 1. What is a Magnetosphere? 5. Dynamics 2. Types of Magnetospheres 6. Interaction with Moons 3. Planetary Magnetic Fields 7. Conclusions 4. Magnetospheric Plasmas 1. What is a Magnetosphere? planet’s magnetic field. Moreover, unmagnetized planets in the flowing solar wind carve out cavities whose properties The term magnetosphere was coined by T. Gold in 1959 are sufficiently similar to those of true magnetospheres to al- to describe the region above the ionosphere in which the low us to include them in this discussion. Moons embedded magnetic field of the Earth controls the motions of charged in the flowing plasma of a planetary magnetosphere create particles. The magnetic field traps low-energy plasma and interaction regions resembling those that surround unmag- forms the Van Allen belts, torus-shaped regions in which netized planets. If a moon is sufficiently strongly magne- high-energy ions and electrons (tens of keV and higher) tized, it may carve out a true magnetosphere completely drift around the Earth. The control of charged particles by contained within the magnetosphere of the planet. -
A Healthy Outlook NASA’S FY16 Budget Funds JPL’S Ongoing Work, Future Initiatives
FEBRUARY Jet Propulsion 2015 Laboratory VOLUME 45 NUMBER 2 A healthy outlook NASA’s FY16 budget funds JPL’s ongoing work, future initiatives By Mark Whalen The White House’s budget request for fiscal year 2016 includes “Last year was an exciting year and I think this year is going to full funding for all of JPL’s ongoing missions as well as continuing be even more exciting,” JPL Director Charles Elachi told employ- support for development of a mission to Jupiter’s moon Europa ees in an all-hands meeting. next decade. Continued on page 2 BUDGET Continued from page 1 2 The request includes about $5.2 billion Space Research Organization; Orbiting sion,” Elachi said. “In order to deploy as- for science overall, of which $1.95 billion Carbon Observatory 3; the Surface Wa- sets on Mars for humans, you need a lot Universe is requested for Earth science and $1.36 ter Ocean Topography mission; and a of tonnage. Electric propulsion is the most billion for planetary science. NASA’s total Gravity Recovery and Climate Experiment efficient way to transport heavy mass.” FY 2016 budget requests $18.5 billion. follow-on mission. The proposed asteroid mission’s two “NASA did pretty well in this very tight All ongoing Mars activities and op- major objectives, he added, are illustrat- budget environment,” said Elachi, noting erations at JPL are fully funded, as is ing high-power electric propulsion and an increase of $450 million relative to FY the continuing development of the Mars providing a platform to assess astronauts 14. -
In Search of a Cure IIT 2010
Features F ALL 2005 IIT MAGAZINE Associate Vice President of Communications and Marketing Catherine Braendel Director of Marketing Marlis Manley Broadhead Managing Editor Chelsea Kalberloh Jackson Contributing Editors Catherine Bruck Beth Duncan Jon Kavanaugh Anne Johnson Theresa Minarik Melanie Nimrodi Abigail Nall Linda Packer Beth Wittbrodt Art Editor Theresa Minarik Design 18 Panebianco, Inc. IIT Magazine is published three times Cover: The Crowded Sky a year by the Office of Communications Cell phones, laptops, radios, and and Marketing. © 2005 airplanes—even microwaves—are Send Letters To all competing for increasingly con- IIT Magazine gested air space. Researchers at Office of Communications and Marketing IIT’s Wireless Interference Labora- 3300 South Federal Street Main Building, Suite 503 tory are studying how to prevent Chicago, IL 60616-3793 a frequency overload. 22 Or Email [email protected] Big Things in Small Packages Send Alumni News To What could the ultra-small neutrino [email protected]. tell us about the universe? Professor 12 Chris White is shooting them from Founded in 1890, Illinois Institute of Technology is a private Chicago to Minnesota in hopes of In Search of a Cure Ph.D.-granting university that awards finding out. IIT is steadily building its reputation degrees in engineering, the sciences, math- ematics, architecture, law, design, psycholo- in cancer research. Bolstered by sev- gy, and business. IIT takes an interprofes- eral high-profile grants, researchers 24 sional approach to research and teaching. at IITRI and faculty and students in By reaching across geographic boundaries, engineering and the life sciences are A Man for Mars academic disciplines, and the professions, investigating new ways to detect, Now more than ever, the world is IIT prepares students for leadership roles in an increasingly complex global workplace treat, and prevent this disease. -
Planets Days Mini-Conference (Friday August 24)
Planets Days Mini-Conference (Friday August 24) Session I : 10:30 – 12:00 10:30 The Dawn Mission: Latest Results (Christopher Russell) 10:45 Revisiting the Oort Cloud in the Age of Large Sky Surveys (Julio Fernandez) 11:00 25 years of Adaptive Optics in Planetary Astronomy, from the Direct Imaging of Asteroids to Earth-Like Exoplanets (Franck Marchis) 11:15 Exploration of the Jupiter Trojans with the Lucy Mission (Keith Noll) 11:30 The New and Unexpected Venus from Akatsuki (Javier Peralta) 11:45 Exploration of Icy Moons as Habitats (Athena Coustenis) Session II: 13:30 – 15:00 13:30 Characterizing ExOPlanet Satellite (CHEOPS): ESA's first s-class science mission (Kate Isaak) 13:45 The Habitability of Exomoons (Christopher Taylor) 14:00 Modelling the Rotation of Icy Satellites with Application to Exoplanets (Gwenael Boue) 14:15 Novel Approaches to Exoplanet Life Detection: Disequilibrium Biosignatures and Their Detectability with the James Webb Space Telescope (Joshua Krissansen-Totton) 14:30 Getting to Know Sub-Saturns and Super-Earths: High-Resolution Spectroscopy of Transiting Exoplanets (Ray Jayawardhana) 14:45 How do External Giant Planets Influence the Evolution of Compact Multi-Planet Systems? (Dong Lai) Session III: 15:30 – 18:30 15:30 Titan’s Global Geology from Cassini (Rosaly Lopes) 15:45 The Origins Space Telescope and Solar System Science (James Bauer) 16:00 Relationship Between Stellar and Solar System Organics (Sun Kwok) 16:15 Mixing of Condensible Constituents with H/He During Formation of Giant Planets (Jack Lissauer) -
Spaceport News America's Gateway to the Universe
MissionUpdate Vol. 36, No. 17 August 29, 1997 Shuttle-Mir Spaceport News America's gateway to the universe. Leading the world in preparing and launching missions to Earth and beyond. John F. Kennedy Space Center Internal EVA conducted: Mir 24 cosmonauts Anatoly Solovyev and Pavel Vinogradov and U.S. astronaut Michael Foale continue the process of verifying restoration of electrical power to the Russian Busy week at Space Station Mir after an intravehicular activity Aug. 22. Troubleshooting of the oxygen- generating system also was under America’s way, and an extravehicular activity was tentatively set for the first week of September to conduct an spaceport inspection of leak sites on the damaged Spektr module. STS-86 ONE Shuttle rolled out to the launch pad Aug. 18 and another returned to KSC the following day. The Space Shuttle Atlantis (above) is now at Pad 39A, undergoing final preparations for launch Sept. 25 on the seventh Shuttle-Mir docking mission, STS-86. The Terminal Countdown Demonstration Test is scheduled for Sept. 9- Atlantis (20th flight OV-104) 10. At about 7:08 a.m., Aug. 19, Discovery (right) 87th Shuttle flight touched down on Runway 33 of KSC's Shuttle Landing Pad 39A Facility, bringing Mission STS-85 to a successful 7th Mir Docking conclusion. Researchers were delighted with the Launch: Sept. 25, 10:34 p.m. performance of the primary scientific instruments flown Crew: Wetherbee; Bloomfield; on the 86th Shuttle flight, the Cryogenic Infrared Parazynski; Titov; Chretien Spectrometers and Telescopes for the Atmosphere (France); Lawrence; Wolf. (CRISTA)-SPAS and the Middle Atmosphere High Commander Wetherbee flew on Resolution Spectrograph Investigation (MAHRSI), both of STS-63, the Shuttle flight that which performed flawlessly. -
Starscan Johnson Space Center Astronomical Society VOLUME 22, NUMBER 4 April 2006
Starscan Johnson Space Center Astronomical Society VOLUME 22, NUMBER 4 April 2006 IN THIS ISSUE Top Stories and Special Interest Reports 3 — Texas Sized Astrophotos in New Mexico 6 — Deep South Texas Star Gaze 6 — California Nebula — Trivia 7 — JSCAS Star Parties 8 — Visual Observing April 2006 19 — Comet 73/P Schwassmann-Wachmann 20 — Members Gallery In the News 12 — Double Helix Nebula Near Center of the Milky Way 13 — SSC Astronomer Discovers a River of Stars 14 — A Shocking Surprise in Stephan's Quintet 15 — Hubble’s Latest Look At Pluto’s Moons Supports A Common Birth 15 — Years of Observing Combined Into Best-Yet Look at Mars Canyon 16— Galaxy on Fire! NASA's Spitzer Reveals Stellar Smoke 17 — Mars Rovers Get New Manager During Challenging Period Club News and Information 18 — Upcoming Events 18— Magazine Subscriptions 19 — IDA News 19 — Member Recognition 19 — Houston Area Astronomy Clubs 22 — Next Meeting 22 — Officers 22 — Agenda 22 — Starscan Submissions 22 — Cover Image Texas-Sized Astrophotos in New Mexico Shane Ramotowski It is common for astronomers to want bigger, bigger, bigger. I too seem to be affected by this condition. Most astronomers get aperture fever. I don’t seem to have contracted that particular disease — I went from a 4 inch reflector to a 6 inch Maksutov-Cassegrain and then to a 5 inch refractor. No, I seem to have a different affliction: film format fever! I’ve been doing 35mm photography since I was in elementary school. A few years ago, I stepped up to medium format with a Mamiya 645 medium format camera. -
Mars Rover Opportunity Working at 'Matijevic Hill' Site 30 September 2012
Mars rover Opportunity working at 'Matijevic Hill' site 30 September 2012 reminiscent of, but different from, the iron-rich spheres nicknamed "blueberries" at the rover's landing site nearly 22 driving miles ago (35 kilometers). The small spheres at Matijevic Hill have different composition and internal structure. Opportunity's science team is evaluating a range of possibilities for how they formed. The spheres are up to about an eighth of an inch (3 millimeters) in diameter. The "blueberries" found earlier are concretions formed by the action of mineral-laden water inside rocks, but that is only one of the ways nature can make small, rounded particles. One working hypothesis, out of several, is that the new-found spherules are also concretions but with a different Rock fins up to about 1 foot (30 centimeters) tall composition. Others include that they may be dominate this scene from the panoramic camera accretionary lapilli formed in volcanic ash eruptions, (Pancam) on NASA's Mars Exploration Rover Opportunity. The component images were taken during impact spherules formed in impact events, or the 3,058th Martian day, or sol, of Opportunity's work on devitrification spherules resulting from formation of Mars (Aug. 23, 2012). The view spans an area of terrain crystals from formerly melted material. There are about 30 feet (9 meters) wide. Orbital investigation of the other possibilities, too. area has identified a possibility of clay minerals in this area of the Cape York segment of the western rim of "Right now we have multiple working hypotheses, Endeavour Crater. The view combines exposures taken and each hypothesis makes certain predictions through Pancam filters centered on wavelengths of 753 about things like what the spherules are made of nanometers (near infrared), 535 nanometers (green) and and how they are distributed," said Opportunity's 432 nanometers (violet).