Top 5 Elements in the Atmosphere of Saturn
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JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
Photophoretic Spectroscopy in Atmospheric Chemistry – High-Sensitivity Measurements of Light Absorption by a Single Particle
Atmos. Meas. Tech., 13, 3191–3203, 2020 https://doi.org/10.5194/amt-13-3191-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Photophoretic spectroscopy in atmospheric chemistry – high-sensitivity measurements of light absorption by a single particle Nir Bluvshtein, Ulrich K. Krieger, and Thomas Peter Institute for Atmospheric and Climate Science, ETH Zurich, 8092, Switzerland Correspondence: Nir Bluvshtein ([email protected]) Received: 28 February 2020 – Discussion started: 4 March 2020 Revised: 30 April 2020 – Accepted: 16 May 2020 – Published: 18 June 2020 Abstract. Light-absorbing organic atmospheric particles, the UV–vis wavelength range, attributing them with a nega- termed brown carbon, undergo chemical and photochemi- tive (cooling) radiative effect. However, light-absorbing or- cal aging processes during their lifetime in the atmosphere. ganic aerosol, termed brown carbon (BrC), with wavelength- The role these particles play in the global radiative balance dependent light absorption (λ−2 − λ−6) in the UV–vis wave- and in the climate system is still uncertain. To better quan- length range (Chen and Bond, 2010; Hoffer et al., 2004; tify their radiative forcing due to aerosol–radiation interac- Kaskaoutis et al., 2007; Kirchstetter et al., 2004; Lack et al., tions, we need to improve process-level understanding of ag- 2012b; Moosmuller et al., 2011; Sun et al., 2007), may be the ing processes, which lead to either “browning” or “bleach- dominant light absorber downwind of urban and industrial- ing” of organic aerosols. Currently available laboratory tech- ized areas and in biomass burning plumes (Feng et al., 2013). -
Enceladus, Moon of Saturn
National Aeronautics and and Space Space Administration Administration Enceladus, Moon of Saturn www.nasa.gov Enceladus (pronounced en-SELL-ah-dus) is an icy moon of Saturn with remarkable activity near its south pole. Covered in water ice that reflects sunlight like freshly fallen snow, Enceladus reflects almost 100 percent of the sunlight that strikes it. Because the moon reflects so much sunlight, the surface temperature is extremely cold, about –330 degrees F (–201 degrees C). The surface of Enceladus displays fissures, plains, corrugated terrain and a variety of other features. Enceladus may be heated by a tidal mechanism similar to that which provides the heat for volca- An artist’s concept of Saturn’s rings and some of the icy moons. The ring particles are composed primarily of water ice and range in size from microns to tens of meters. In 2004, the Cassini spacecraft passed through the gap between the F and G rings to begin orbiting Saturn. noes on Jupiter’s moon Io. A dramatic plume of jets sprays water ice and gas out from the interior at ring material, coating itself continually in a mantle Space Agency. The Jet Propulsion Laboratory, a many locations along the famed “tiger stripes” at of fresh, white ice. division of the California Institute of Technology, the south pole. Cassini mission data have provided manages the mission for NASA. evidence for at least 100 distinct geysers erupting Saturn’s Rings For images and information about the Cassini on Enceladus. All of this activity, plus clues hidden Saturn’s rings form an enormous, complex struc- mission, visit — http://saturn.jpl.nasa.gov/ in the moon’s gravity, indicates that the moon’s ture. -
The Solar System Cause Impact Craters
ASTRONOMY 161 Introduction to Solar System Astronomy Class 12 Solar System Survey Monday, February 5 Key Concepts (1) The terrestrial planets are made primarily of rock and metal. (2) The Jovian planets are made primarily of hydrogen and helium. (3) Moons (a.k.a. satellites) orbit the planets; some moons are large. (4) Asteroids, meteoroids, comets, and Kuiper Belt objects orbit the Sun. (5) Collision between objects in the Solar System cause impact craters. Family portrait of the Solar System: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, (Eris, Ceres, Pluto): My Very Excellent Mother Just Served Us Nine (Extra Cheese Pizzas). The Solar System: List of Ingredients Ingredient Percent of total mass Sun 99.8% Jupiter 0.1% other planets 0.05% everything else 0.05% The Sun dominates the Solar System Jupiter dominates the planets Object Mass Object Mass 1) Sun 330,000 2) Jupiter 320 10) Ganymede 0.025 3) Saturn 95 11) Titan 0.023 4) Neptune 17 12) Callisto 0.018 5) Uranus 15 13) Io 0.015 6) Earth 1.0 14) Moon 0.012 7) Venus 0.82 15) Europa 0.008 8) Mars 0.11 16) Triton 0.004 9) Mercury 0.055 17) Pluto 0.002 A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). (1) The terrestrial planets are made primarily of rock and metal. -
Planetary Rings
CLBE001-ESS2E November 10, 2006 21:56 100-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 Rings Carolyn C. Porco Space Science Institute Boulder, Colorado Douglas P. Hamilton University of Maryland College Park, Maryland CHAPTER 27 1. Introduction 5. Ring Origins 2. Sources of Information 6. Prospects for the Future 3. Overview of Ring Structure Bibliography 4. Ring Processes 1. Introduction houses, from coalescing under their own gravity into larger bodies. Rings are arranged around planets in strikingly dif- Planetary rings are those strikingly flat and circular ap- ferent ways despite the similar underlying physical pro- pendages embracing all the giant planets in the outer Solar cesses that govern them. Gravitational tugs from satellites System: Jupiter, Saturn, Uranus, and Neptune. Like their account for some of the structure of densely-packed mas- cousins, the spiral galaxies, they are formed of many bod- sive rings [see Solar System Dynamics: Regular and ies, independently orbiting in a central gravitational field. Chaotic Motion], while nongravitational effects, includ- Rings also share many characteristics with, and offer in- ing solar radiation pressure and electromagnetic forces, valuable insights into, flattened systems of gas and collid- dominate the dynamics of the fainter and more diffuse dusty ing debris that ultimately form solar systems. Ring systems rings. Spacecraft flybys of all of the giant planets and, more are accessible laboratories capable of providing clues about recently, orbiters at Jupiter and Saturn, have revolutionized processes important in these circumstellar disks, structures our understanding of planetary rings. -
Final Report of the Opgt/Mjs Plasma Wave Science Team
1 September 1972 FINAL REPORT OF THE OPGT/MJS PLASMA WAVE SCIENCE TEAM Prepared by F. L. Scarf, Team Leader for National Aeronautical and Space Administration Washington, D.C. 205*t6 Contract NASW 2228 Space Sciences Department TRW Systems Group One Space Park Redondo Beach, California 902?8 4 Page 1 1. TEAM ORGANIZATION AND MEMBERSHIP The Plasma Wave Team Leader is Dr. F. L. Scarf of TRW Systems, and the official team members are Dr. D. A. Gurnett (University of Iowa), Dr. R. A. Helliwell (Stanford University), Dr. R. E. Holzer (UCLA), Dr. P. J. Kellogg (University of Minnesota), Dr. E. J. Smith (JPL), and Dr. E. Ungstrup (Danish Space Research Institute). Mr. A. M. A. Frandsen of JPL serves as Team Member and Experiment Representative. In addition, the Plasma Wave Team solicited the continuing support and assistance of several other outstanding scientists, and we have designated these participants as Team Associates; the Associates are Dr. N. M. Brice (Cornell University), Dr. D. Cartwright (University of Minnesota), Dr. R. W. Fredricks (TRW), Dr. H. B. Liemohn (Boeing), Dr. C. F. Kennel (UCLA), and Dr. R. Thome (UCLA) . 2. GENERAL TEAM ACTIVITIES FEBRUARY 1972-AUGUST 31, 1972 (See the mid-year report for a summary of the earlier work) During this period Dr. Scarf attended all SSG Meetings except the last one, where Dr. E. J. Smith represented the Plasma Wave Team. There were a number of Team Meetings and several additional .conferences at JPL concerning EMI and other potential spacecraft problems. The major development during this interval involved the decision not to go ahead with the Grand Tour. -
Atmospheric Chemistry
Atmospheric Chemistry John Lee Grenfell Technische Universität Berlin Atmospheres and Habitability (Earthlike) Atmospheres: -support complex life (respiration) -stabilise temperature -maintain liquid water -we can measure their spectra hence life-signs Modern Atmospheric Composition CO2 Modern Atmospheric Composition O2 CO2 N2 CO2 N2 CO2 Modern Atmospheric Composition O2 CO2 N2 CO2 N2 P 93bar 1bar 6mb 1.5bar surface CO2 Tsurface 735K 288K 220K 94K Early Earth Atmospheric Compositions Magma Hadean Archaean Proterozoic Snowball CO2 Early Earth Atmospheric Compositions Magma Hadean Archaean Proterozoic Snowball Silicate CO2 CO2 N2 N2 Steam H2ON2 O2 O2 CO2 Additional terrestrial-type atmospheres Jurassic Earth Early Mars Early Venus Jungleworld Desertworld Waterworld Superearth Modern Atmospheric Composition Today we will talk about these CO2 Reading List Yuk Yung (Caltech) and William DeMore “Photochemistry of Planetary Atmospheres” Richard P. Wayne (Oxford) “Chemistry of Atmospheres” T. Gredel and Paul Crutzen (Mainz) “Chemie der Atmosphäre” Processes influencing Photochemistry Photons Protection Delivery Escape Clouds Photochemistry Surface OCEAN Biology Volcanism Some fundamentals… ALKALI METALS The Periodic Table NOBLE GASES One outer electron Increasing atomic number 8 outer electrons: reactive Rows called PERIODS unreactive GROUPS: similar Halogens chemical C, Si etc. have 4 outer electrons properties SO CAN FORM STABLE CHAINS Chemical Structure and Reactivity s and p orbitals d orbitals The Aufbau Method works OK for the first 18 elements -
Chapter 1 – Introduction
1 Chapter 1 – Introduction 1.1 – Scientific Background Knowledge of gas phase compounds and their chemical reactions are pivotal to our understanding of chemistry. The conditions these molecules are in can vary dramatically, from temperatures as low as 10 K in the depths of the interstellar medium, to more than 1000 K in the combustion of hydrocarbons in engines. The chemistry in these systems is dominated by highly reactive, unstable compounds, leading to fast and complex chemistry occurring. In order to accurately understand these systems, we must be able to observe these unstable species and measure the kinetics of their formation and destruction. While molecular spectra and reaction rate constants of these reactive compounds can be computed with theoretical calculations, they must be benchmarked with experimental measurements to determine their accuracy. To that end, one major focus in experimental gas phase chemistry is to better understand these unstable molecules and their reactions in systems such as atmospheric chemistry and astrochemistry. 1.1a – Atmospheric Chemistry Understanding Earth’s atmosphere and the chemistry behind it has been a major topic in gas phase chemistry since the mid-20th century, when the impact of fossil fuel usage and air pollution resulting from the Industrial Revolution became apparent. The dominant molecule in Earth’s atmosphere is N2 (77% of the atmosphere) followed by O2 (21%) and argon (1%). The remaining components are largely stable molecules, such as CO2 and H2O. 2 Figure 1.1: The average temperature (left) and pressure (right) profiles of the Earth’s lower atmosphere, consisting of the troposphere and stratosphere. -
Jacques Tiziou Space Collection
Jacques Tiziou Space Collection Isaac Middleton and Melissa A. N. Keiser 2019 National Air and Space Museum Archives 14390 Air & Space Museum Parkway Chantilly, VA 20151 [email protected] https://airandspace.si.edu/archives Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Biographical / Historical.................................................................................................... 1 Scope and Contents........................................................................................................ 2 Arrangement..................................................................................................................... 2 Names and Subjects ...................................................................................................... 2 Container Listing ............................................................................................................. 4 Series : Files, (bulk 1960-2011)............................................................................... 4 Series : Photography, (bulk 1960-2011)................................................................. 25 Jacques Tiziou Space Collection NASM.2018.0078 Collection Overview Repository: National Air and Space Museum Archives Title: Jacques Tiziou Space Collection Identifier: NASM.2018.0078 Date: (bulk 1960s through -
Appulses of Jupiter and Saturn
IN ORIGINAL FORM PUBLISHED IN: arXiv:(side label) [physics.pop-ph] Sternzeit 46, No. 1+2 / 2021 (ISSN: 0721-8168) Date: 6th May 2021 Appulses of Jupiter and Saturn Joachim Gripp, Emil Khalisi Sternzeit e.V., Kiel and Heidelberg, Germany e-mail: gripp or khalisi ...[at]sternzeit-online[dot]de Abstract. The latest conjunction of Jupiter and Saturn occurred at an optical distance of 6 arc minutes on 21 December 2020. We re-analysed all encounters of these two planets between -1000 and +3000 CE, as the extraordinary ones (< 10′) take place near the line of nodes every 400 years. An occultation of their discs did not and will not happen within the historical time span of ±5,000 years around now. When viewed from Neptune though, there will be an occultation in 2046. Keywords: Jupiter-Saturn conjunction, Appulse, Trigon, Occultation. Introduction reason is due to Earth’s orbit: while Jupiter and Saturn are locked in a 5:2-mean motion resonance, the Earth does not The slowest naked-eye planets Jupiter and Saturn made an join in. For very long periods there could be some period- impressive encounter in December 2020. Their approaches icity, however, secular effects destroy a cycle, e.g. rotation have been termed “Great Conjunctions” in former times of the apsides and changes in eccentricity such that we are and they happen regularly every ≈20 years. Before the left with some kind of “semi-periodicity”. discovery of the outer ice giants these classical planets rendered the longest known cycle. The separation at the instant of conjunction varies up to 1 degree of arc, but the Close Encounters latest meeting was particularly tight since the planets stood Most pass-bys of Jupiter and Saturn are not very spectac- closer than at any other occasion for as long as 400 years. -
A Pictorial History of Rockets
he mighty space rockets of today are the result A Pictorial Tof more than 2,000 years of invention, experi- mentation, and discovery. First by observation and inspiration and then by methodical research, the History of foundations for modern rocketry were laid. Rockets Building upon the experience of two millennia, new rockets will expand human presence in space back to the Moon and Mars. These new rockets will be versatile. They will support Earth orbital missions, such as the International Space Station, and off- world missions millions of kilometers from home. Already, travel to the stars is possible. Robotic spacecraft are on their way into interstellar space as you read this. Someday, they will be followed by human explorers. Often lost in the shadows of time, early rocket pioneers “pushed the envelope” by creating rocket- propelled devices for land, sea, air, and space. When the scientific principles governing motion were discovered, rockets graduated from toys and novelties to serious devices for commerce, war, travel, and research. This work led to many of the most amazing discoveries of our time. The vignettes that follow provide a small sampling of stories from the history of rockets. They form a rocket time line that includes critical developments and interesting sidelines. In some cases, one story leads to another, and in others, the stories are inter- esting diversions from the path. They portray the inspirations that ultimately led to us taking our first steps into outer space. NASA’s new Space Launch System (SLS), commercial launch systems, and the rockets that follow owe much of their success to the accomplishments presented here. -
America's Greatest Projects and Their Engineers - VII
America's Greatest Projects and Their Engineers - VII Course No: B05-005 Credit: 5 PDH Dominic Perrotta, P.E. Continuing Education and Development, Inc. 22 Stonewall Court Woodcliff Lake, NJ 076 77 P: (877) 322-5800 [email protected] America’s Greatest Projects & Their Engineers-Vol. VII The Apollo Project-Part 1 Preparing for Space Travel to the Moon Table of Contents I. Tragedy and Death Before the First Apollo Flight A. The Three Lives that Were Lost B. Investigation, Findings & Recommendations II. Beginning of the Man on the Moon Concept A. Plans to Land on the Moon B. Design Considerations and Decisions 1. Rockets – Launch Vehicles 2. Command/Service Module 3. Lunar Module III. NASA’s Objectives A. Unmanned Missions B. Manned Missions IV. Early Missions V. Apollo 7 Ready – First Manned Apollo Mission VI. Apollo 8 - Orbiting the Moon 1 I. Tragedy and Death Before the First Apollo Flight Everything seemed to be going well for the Apollo Project, the third in a series of space projects by the United States intended to place an American astronaut on the Moon before the end of the 1960’s decade. Apollo 1, known at that time as AS (Apollo Saturn)-204 would be the first manned spaceflight of the Apollo program, and would launch a few months after the flight of Gemini 12, which had occurred on 11 November 1966. Although Gemini 12 was a short duration flight, Pilot Buzz Aldrin had performed three extensive EVA’s (Extra Vehicular Activities), proving that Astronauts could work for long periods of time outside the spacecraft.