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Lab 7: Gravity and Jupiter's Moons
Lab 7: Gravity and Jupiter's Moons Image of Galileo Spacecraft Gravity is the force that binds all astronomical structures. Clusters of galaxies are gravitationally bound into the largest structures in the Universe, Galactic Superclusters. The galaxies themselves are held together by gravity, as are all of the star systems within them. Our own Solar System is a collection of bodies gravitationally bound to our star, Sol. Cutting edge science requires the use of Einstein's General Theory of Relativity to explain gravity. But the interactions of the bodies in our Solar System were understood long before Einstein's time. In chapter two of Chaisson McMillan's Astronomy Today, you went over Kepler's Laws. These laws of gravity were made to describe the interactions in our Solar System. P2=a3/M Where 'P' is the orbital period in Earth years, the time for the body to make one full orbit. 'a' is the length of the orbit's semi-major axis, for nearly circular orbits the orbital radius. 'M' is the total mass of the system in units of Solar Masses. Jupiter System Montage picture from NASA ID = PIA01481 Jupiter has over 60 moons at the last count, most of which are asteroids and comets captured from Written by Meagan White and Paul Lewis Page 1 the Asteroid Belt. When Galileo viewed Jupiter through his early telescope, he noticed only four moons: Io, Europa, Ganymede, and Callisto. The Jupiter System can be thought of as a miniature Solar System, with Jupiter in place of the Sun, and the Galilean moons like planets. -
Galileo and the Telescope
Galileo and the Telescope A Discussion of Galileo Galilei and the Beginning of Modern Observational Astronomy ___________________________ Billy Teets, Ph.D. Acting Director and Outreach Astronomer, Vanderbilt University Dyer Observatory Tuesday, October 20, 2020 Image Credit: Giuseppe Bertini General Outline • Telescopes/Galileo’s Telescopes • Observations of the Moon • Observations of Jupiter • Observations of Other Planets • The Milky Way • Sunspots Brief History of the Telescope – Hans Lippershey • Dutch Spectacle Maker • Invention credited to Hans Lippershey (c. 1608 - refracting telescope) • Late 1608 – Dutch gov’t: “ a device by means of which all things at a very great distance can be seen as if they were nearby” • Is said he observed two children playing with lenses • Patent not awarded Image Source: Wikipedia Galileo and the Telescope • Created his own – 3x magnification. • Similar to what was peddled in Europe. • Learned magnification depended on the ratio of lens focal lengths. • Had to learn to grind his own lenses. Image Source: Britannica.com Image Source: Wikipedia Refracting Telescopes Bend Light Refracting Telescopes Chromatic Aberration Chromatic aberration limits ability to distinguish details Dealing with Chromatic Aberration - Stop Down Aperture Galileo used cardboard rings to limit aperture – Results were dimmer views but less chromatic aberration Galileo and the Telescope • Created his own (3x, 8-9x, 20x, etc.) • Noted by many for its military advantages August 1609 Galileo and the Telescope • First observed the -
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3 f~ ~:~~NEA~yA:=~~~T?c:NA:=~~:c:Q:.,I~~; . }RS:~cN ------------------------RELEASE NO, I FOR RELEASE' January 4, 1971 [ \_ ('. '~ '· APOLLO 14 STATUS REPORT Apollo 14 astronaut crew activities include physical examination at MSC, guidance and navigation system briefing, contingency (one-man) EVA simulation on January 5; lunar descent flight simulations with flight controller participation on January 6; lunar orbit and descent orbit insertion simulations with the flight controllers on January 7; EVA simulation with the flight controllers on January 8; and press interviews on January 9 at MSC Hypergolic propellants-- those which ignite spontaneously when the fuel and oxydizer meet-- will be loaded in the Apollo 14 spacecraft and in the auxiliary propulsion system of the Saturn third stage from January 4 to 8. Then RP-1 fuel will be loaded aboard the Saturn V first stage on January 9. Also during the week, spacecraft pyrotechnics will be installed, Saturn first stage engines will be leak-checked. and flight stowage of the modularized equipment stowage assembly in the lunar module descent stage will be accomplished. Preparations of the Apollo 14 space vehicle continue to proceed satisfactorily for a scheduled launching January 31 from Kennedy Space Center Launch Complex 39. Fifteen potential Skylab astronauts are scheduled to visit Sacramento Peak Observatory, Sunspot. New Mexico for solar telescope training on January ' and 7. The second stage for the 13th Saturn V rocket departed the NASA Mississippi Test Facility December 30 aboard the barge Poseidon for the Kennedy Space Center. The stage is scheduled to arrive January 5 and go into temporary storage in the VAB The stage is planned for use in the Skylab program as part of the Saturn V rocket to place the orbital workshop into Earth orbit in late 1972. -
Callisto: a Guide to the Origin of the Jupiter System
A PAPER SUBMITTED TO THE DECADAL SURVEY ON PLANETARY SCIENCE AND ASTROBIOLOGY Callisto: A Guide to the Origin of the Jupiter System David E Smith 617-803-3377 Department of Earth, Atmospheric and PLanetary Sciences Massachusetts Institute of Technology, Cambridge MA 02139 [email protected] Co-authors: Francis Nimmo, UCSC, [email protected] Krishan Khurana, UCLA, [email protected] Catherine L. Johnson, PSI, [email protected] Mark Wieczorek, OCA, Fr, [email protected] Maria T. Zuber, MIT, [email protected] Carol Paty, University of Oregon, [email protected] Antonio Genova, Univ Rome, It, [email protected] Erwan Mazarico, NASA GSFC, [email protected] Louise Prockter, LPI, [email protected] Gregory A. Neumann, NASA GSFC Emeritus, [email protected] John E. Connerney, Adnet Systems Inc., [email protected] Edward B. Bierhaus, LMCO, [email protected] Sander J. Goossens, UMBC, [email protected] MichaeL K. Barker, NASA GSFC, [email protected] Peter B. James, Baylor, [email protected] James Head, Brown, [email protected] Jason Soderblom, MIT, [email protected] July 14, 2020 Introduction Among the GaLiLean moons of Jupiter, it is outermost CaLListo that appears to most fulLy preserve the record of its ancient past. With a surface aLmost devoid of signs of internaL geologic activity, and hints from spacecraft data that its interior has an ocean whiLe being only partiaLLy differentiated, CaLListo is the most paradoxicaL of the giant rock-ice worlds. How can a body with such a primordiaL surface harbor an ocean? If the interior was warm enough to form an ocean, how could a mixed rock and ice interior remain stable? What do the striking differences between geologicaLLy unmodified CaLListo and its sibling moon Ganymede teLL us about the formation of the GaLiLean moons and the primordiaL conditions at the time of the formation of CaLListo and the accretion of giant planet systems? The answers can be provided by a CaLListo orbitaL mission. -
Student Worksheets, Assessments, and Answer Keys
Apollo Mission Worksheet Team Names _________________________ Your team has been assigned Apollo Mission _______ Color _________________ 1. Go to google.com/moon and find your mission, click on it and then zoom in. 2. Find # 1, this will give you information to answer the questions below. 3. On your moon map, find the location of the mission landing site and locate this spot on your map. Choose a symbol and the correct color for your mission (each mission has a specific symbol and you can use this if you like or make up your own). In the legend area put your symbol and mission number. 4. Who were the astronauts on the mission? The astronauts on the mission were ______________________________________ ______________________________________________________________________ 5. When did the mission take place? The mission took place from _______________________________________________ 6. How many days did the mission last? The mission lasted ______________________________________________________ 7. Where did the mission land? The mission landed at____________________________________________________ 8. Why did the mission land here? They landed at this location because ________________________________________ ___________________________________________________________________________ _______________________________________________________________________ 9. What was the goal of the mission? The goal of the mission was_______________________________________________ ______________________________________________________________________ ___________________________________________________________________________ -
Dwarf Planet Ceres
Dwarf Planet Ceres drishtiias.com/printpdf/dwarf-planet-ceres Why in News As per the data collected by NASA’s Dawn spacecraft, dwarf planet Ceres reportedly has salty water underground. Dawn (2007-18) was a mission to the two most massive bodies in the main asteroid belt - Vesta and Ceres. Key Points 1/3 Latest Findings: The scientists have given Ceres the status of an “ocean world” as it has a big reservoir of salty water underneath its frigid surface. This has led to an increased interest of scientists that the dwarf planet was maybe habitable or has the potential to be. Ocean Worlds is a term for ‘Water in the Solar System and Beyond’. The salty water originated in a brine reservoir spread hundreds of miles and about 40 km beneath the surface of the Ceres. Further, there is an evidence that Ceres remains geologically active with cryovolcanism - volcanoes oozing icy material. Instead of molten rock, cryovolcanoes or salty-mud volcanoes release frigid, salty water sometimes mixed with mud. Subsurface Oceans on other Celestial Bodies: Jupiter’s moon Europa, Saturn’s moon Enceladus, Neptune’s moon Triton, and the dwarf planet Pluto. This provides scientists a means to understand the history of the solar system. Ceres: It is the largest object in the asteroid belt between Mars and Jupiter. It was the first member of the asteroid belt to be discovered when Giuseppe Piazzi spotted it in 1801. It is the only dwarf planet located in the inner solar system (includes planets Mercury, Venus, Earth and Mars). Scientists classified it as a dwarf planet in 2006. -
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. -
Salt Triggered Melting of Permafrost in the Chaos Regions of Mars
Lunar and Planetary Science XXXVII (2006) 2218.pdf SALT TRIGGERED MELTING OF PERMAFROST IN THE CHAOS REGIONS OF MARS. Popa I.C., Università degli Studi "G. d'Annunzio" Chieti-Pescara, Pescara, Viale Pindaro 42, Italy. ([email protected]) Introduction: Mars surface bears traces of many landing site (Chryse Planitia) is the place where Ares fluvial-like features, geomorphic identified as outflow outflow channel is depositing its transporting channels, valley networks etc. Among these a particular materials. The following Martian landers Pathfinder one stands above others from the dimensional point of [6] and MER A Spirit [7], and MER B Opportunity [8] view. Outflow channels bear unique water erosion also revealed high soluble salts contents in places characteristics, that led Baker and Milton (1974) [1] to possibly genetically connected. Recently OMEGA believe that are caused by a surface runoff of large aboard Mars Express spacecraft has proven the amounts of water, in short geological time. Water existence of gypsum and other highly soluble salts (e.g origin, necessary for these processes was the topic of kieserite and epsomite) in localized deposits in places around Valles Marineris, and Iani Chaos [9]. many works. Among these theories one generally Freezing point depression of water solutions: accepted idea considers that water is originating from The freezing point of pure water at 1 bar is 0°C melting of permafrost layers positioned in the places of (273K). This melting point can be easily depressed by today chaos’. Here is an investigation that takes into adding impurities or soluble salts to the solvent. In the account the exoergic salt-ice dissolution reaction, along case of halite (NaCl) salt it is known that a 10% NaCl with freezing point depression of formed salty solutions, solution lowers the melting point of about -6°C (267K) as a complentary or a stand-alone process in chaos- and a 20% salt solution lowers it to -16°C (257K). -
THE PENNY MOON and QUARTER EARTH School Adapted from a Physics Forum Activity At
~ LPI EDUCATION/PUBLIC OUTREACH SCIENCE ACTIVITIES ~ Ages: 5th grade – high THE PENNY MOON AND QUARTER EARTH school Adapted from a Physics Forum activity at: http://www.phvsicsforums.com/ Duration: 10 minutes OVERVIEW — The students will use a penny and a quarter to model the Moon’s rotation on its axis and Materials: revolution around the Earth, and demonstrate that the Moon keeps the same face toward One penny and one the Earth. quarter per pair of students OBJECTIVE — Overhead projector, or The students will: elmo, or video Demonstrate the motion of the Moon’s rotation and revolution. projector Compare what we would see of the Moon if it did not rotate to what we see when its period of rotation is the same as its orbital period. Projected image of student overhead BEFORE YOU START: Do not introduce this topic along with the reason for lunar phases; students may become confused and assume that the Moon’s rotation is related to its phases. Prepare to show the student overhead projected for the class to see. ACTIVITY — 1. Ask your students to describe which parts of the Moon they see. Does the Moon turn? Can we see its far side? Allow time for your students to discuss this and share their opinions. 2. Hand out the pennies and quarters so that each pair of students has both. Tell the students that they will be creating a model of the Earth and Moon. Which object is Earth? [the quarter] Which one is the Moon? [the penny] 3. Turn on the projected student overhead. -
Through Astronaut Eyes: Photographing Early Human Spaceflight
Purdue University Purdue e-Pubs Purdue University Press Book Previews Purdue University Press 6-2020 Through Astronaut Eyes: Photographing Early Human Spaceflight Jennifer K. Levasseur Follow this and additional works at: https://docs.lib.purdue.edu/purduepress_previews This document has been made available through Purdue e-Pubs, a service of the Purdue University Libraries. Please contact [email protected] for additional information. THROUGH ASTRONAUT EYES PURDUE STUDIES IN AERONAUTICS AND ASTRONAUTICS James R. Hansen, Series Editor Purdue Studies in Aeronautics and Astronautics builds on Purdue’s leadership in aeronautic and astronautic engineering, as well as the historic accomplishments of many of its luminary alums. Works in the series will explore cutting-edge topics in aeronautics and astronautics enterprises, tell unique stories from the history of flight and space travel, and contemplate the future of human space exploration and colonization. RECENT BOOKS IN THE SERIES British Imperial Air Power: The Royal Air Forces and the Defense of Australia and New Zealand Between the World Wars by Alex M Spencer A Reluctant Icon: Letters to Neil Armstrong by James R. Hansen John Houbolt: The Unsung Hero of the Apollo Moon Landings by William F. Causey Dear Neil Armstrong: Letters to the First Man from All Mankind by James R. Hansen Piercing the Horizon: The Story of Visionary NASA Chief Tom Paine by Sunny Tsiao Calculated Risk: The Supersonic Life and Times of Gus Grissom by George Leopold Spacewalker: My Journey in Space and Faith as NASA’s Record-Setting Frequent Flyer by Jerry L. Ross THROUGH ASTRONAUT EYES Photographing Early Human Spaceflight Jennifer K. -
Io Observer SDT to Steer a Comprehensive Mission Concept Study for the Next Decadal Survey
Io as a Target for Future Exploration Rosaly Lopes1, Alfred McEwen2, Catherine Elder1, Julie Rathbun3, Karl Mitchell1, William Smythe1, Laszlo Kestay4 1 Jet Propulsion Laboratory, California Institute of Technology 2 University of Arizona 3 Planetary Science Institute 4 US Geological Survey Io: the most volcanically active body is solar system • Best example of tidal heating in solar system; linchpin for understanding thermal evolution of Europa • Effects reach far beyond Io: material from Io feeds torus around Jupiter, implants material on Europa, causes aurorae on Jupiter • Analog for some exoplanets – some have been suggested to be volcanically active OPAG recommendation #8 (2016): OPAG urges NASA PSD to convene an Io Observer SDT to steer a comprehensive mission concept study for the next Decadal Survey • An Io Observer mission was listed in NF-3, Decadal Survey 2003, the NOSSE report (2008), Visions and Voyages Decadal Survey 2013 (for inclusion in the NF-5 AO) • Io Observer is a high OPAG priority for inclusion in the next Decadal Survey and a mission study is an important first step • This study should be conducted before next Decadal and NF-5 AO and should include: o recent advances in technology provided by Europa and Juno missions o advances in ground-based techniques for observing Io o new resources to study Io in future, including JWST, small sats, miniaturized instruments, JUICE Most recent study: Decadal Survey Io Observer (2010) (Turtle, Spencer, Khurana, Nimmo) • A mission to explore Io’s active volcanism and interior structure (including determining whether Io has a magma ocean) and implications for the tidal evolution of the Jupiter-Io-Europa- Ganymede system and ancient volcanic processes on the terrestrial planets. -
The Periglacial Landscape of Utopia Planitia; Geologic Evidence for Recent Climate Change on Mars
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 1-23-2013 12:00 AM The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars. Mary C. Kerrigan The University of Western Ontario Supervisor Dr. Marco Van De Wiel The University of Western Ontario Joint Supervisor Dr. Gordon R Osinski The University of Western Ontario Graduate Program in Geography A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Mary C. Kerrigan 2013 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Climate Commons, Geology Commons, Geomorphology Commons, and the Physical and Environmental Geography Commons Recommended Citation Kerrigan, Mary C., "The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars." (2013). Electronic Thesis and Dissertation Repository. 1101. https://ir.lib.uwo.ca/etd/1101 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]. THE PERIGLACIAL LANDSCAPE OF UTOPIA PLANITIA; GEOLOGIC EVIDENCE FOR RECENT CLIMATE CHANGE ON MARS by Mary C. Kerrigan Graduate Program in Geography A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science The School of Graduate and Postdoctoral Studies The University of Western Ontario London, Ontario, Canada © Mary C. Kerrigan 2013 ii THE UNIVERSITY OF WESTERN ONTARIO School of Graduate and Postdoctoral Studies CERTIFICATE OF EXAMINATION Joint Supervisor Examiners ______________________________ Dr.