Sha'áłchíní Welcome to Science Class! What If… My Teacher Gets Kicked August 27, 2020 out of Zoom?

Total Page:16

File Type:pdf, Size:1020Kb

Sha'áłchíní Welcome to Science Class! What If… My Teacher Gets Kicked August 27, 2020 out of Zoom? April 26, 2021 Yá’át’ééh! sha'áłchíní Welcome to science class! What if… My teacher gets kicked August 27, 2020 out of Zoom? Then.. 1. If you get assigned as the host end the meeting. 2. Everyone immediately log out of Zoom. 3. Re-enter the class in 5 minutes. 4. If you do not get back into the meeting after continuous tries, class is cancelled. 5. Refer to agenda slides from website. In case Mrs. Yazzie loses internet connection: ● someone becomes host ● host monitors class until Mrs. Yazzie returns or four minutes have passed ● after 4 minutes host ends class ● everyone tries to re-enter class ● if Mrs. Yazzie doesn’t return after another 4 minutes, class is ended for the day Sun. Mon. Tues. Wed. Thurs. Fri. Sat. 1 Intervention 2 3 Science Project PTC 4-7PM Check-In 4 5 6 7 8 9 10 No school Intervention Science Project Check-In 11 12 13 14 15 16 17 Intervention Science Project Due 40 points 18 19 20 21 22 23 24 Intervention 25 26 27 28 29 30 Community Forum Last Intervention NO SCHOOL 5:30pm No School Sun. Mon. Tues. Wed. Thurs. Fri. Sat. 25 26 27 28 29 30 1 Community Forum Last Day of Intervention 5:30PM No School 2 3 4 5 6 7 8 Last Day of Science Zoom No School 9 10 11 12 13 14 15 Mother’s No Zoom No Zoom No Zoom Return school laptops Day NWEA- Math NWEA-RDG NWEA-LANG No School 16 17 18 19 20 21 22 ALL WORK DUE No School 23 24 25 26 27 28 29 30 31 Last Day of School 8th Grade Promotion Announcements ● April 28th-Community Forum ● Friday, April 30th-NO SCHOOL ● Thurs., May 27th- 8th Grade Promotion ● Thurs., May 27th - Last Day of School Agenda -Announcements and Calendar -Student Objective & Essential Question -Intro to Vocabulary -Dwarf Planets -Kahoot! On a scale from 1-10 with 10 being excellent, how was your weekend? UPDATE! ● INGENUITY-2nd Flight Success! ● Perseverance makes oxygen! Student Objective Day 1, Monday: I can describe the relationship of objects in the solar system. Essential Questions: 1 The Structure of the Solar System How are the inner planets different from the outer planets? 2 The Inner Planets How are the inner planets similar? 3 The Outer Planets How are the outer planets similar? 4 Dwarf Planets and Other Objects What is a dwarf planet? What are the characteristics of comets and asteroids? Big Ideas ● The distances between these bodies are huge. ● The solar system consists of the sun and a collection of objects, including planets, their moons, and asteroids that are held in orbit around the sun by its gravitational pull on them ● What natural phenomena do the motions of objects in the solar system produce? Weekly asteroid small, astronomical comet object rocky object that unit average made of gas, orbits the Sun in Vocabulary distance from dust, and ice that the asteroid belt moves around the between Mars Earth to the Sun in an and Jupiter Sun—about 150 million km oval-shaped orbit impact crater star object in meteor streak of meteoroid small, round depression space made of light in Earth’s rocky particle that formed by the gases in which atmosphere made moves through impact of a nuclear fusion by a glowing space meteorite on the reactions occur meteoroid meteorite surface of a that emit meteoroid that planet, moon, or energy strikes a planet or other space object moon Comets Solar System Asteroids Dwarf Planets The International Astronomical Union (IAU) defines a dwarf planet as an object that orbits a star. When a dwarf planet formed, there was enough mass and gravity for it to form a sphere. A dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. Astronomers classify Pluto, Ceres, Eris, Makemake, and Haumea (how MAY ah) as dwarf planets. Pluto was once considered to be a planet, but now it has the status of a dwarf planet. All dwarf planets are smaller than Earth’s moon. The figure below locates Ceres, Pluto, and Eris. These dwarf planets each have a rocky core surrounded by a thick layer of ice. It's primarily made up of icy objects, dwarf planets, dust, and comets. The total mass of all the material in the Kuiper Belt today is estimated to be no more than about 10 percent of the mass of Earth. Physical Characteristics •5 - Recognized Dwarf Planets –Ceres, Pluto, Haumea, Makemake, Eris •Classification Criteria –Directly orbits the Sun (not a satellite) –Relatively round in shape –Has not cleared its orbital path •Term applied to Solar System objects in 2006 •Ceres : 2.77 AU •Orbital Period = 4.60 years Dwarf Planet Orbits •Pluto : 39.48 AU •Orbital Period = 248.09 years •Haumea : 43.13 AU •Orbital Period = 283.28 years •Makemake : 45.79 AU •Orbital Period = 309.9 years •Eris : 67.67 AU Orbital Period = 557 years 1 AU = Distance to Earth from the Sun •Ceres •Diameter : 590 miles Surface and Atmosphere •Temperature Range : -106 ˚C to -34 ˚C •Pluto •Diameter : 1,430 miles •Average Temperature : - 229 ˚C •Haumea •Diameter : 1,218 x 943 miles •Average Temperature : - 223 ˚C •Makemake •Diameter : 882 miles •Average Temperature : – 239 ˚C •Eris •Diameter : 1,445 miles •Average Temperature : -231 ˚C •Ceres Dwarf Planet Discovery •Giuseppe Piazzi (January 1, 1801) •Pluto •Clyde Tombaugh (February 18, 1930) •Haumea •Mike Brown et al (December 28, 2004) •Makemake •Mike Brown, Chad Trujilo, David Rabinowitz (March 31, 2005) •Eris •Mike Brown, Chad Trujilo, David Rabinowitz (January 5, 2005) Dwarf Planet Facts •394 possible dwarf planets in the Solar System •All dwarf planets located in Kuiper Belt •Except Ceres (Asteroid Belt) •No dwarf planet has been visited by a space probe •2015 : Dawn (Ceres) & New Horizons (Pluto) •Number of known natural satellites (moons) •Ceres : 0 •Pluto : 5 (Charon, Nix, Hydra, Kerberos, Styx) •Haumea : 2 (Hi’iaka, Namaka) •Makemake : 0 •Eris : 1 (Dysnomia) VIDEOS Assignment Kahoot.
Recommended publications
  • DOUGLAS P. HAMILTON Career Summary Professor, University of Maryland, Astronomy Dept., 9/1995 – Present
    CURRICULUM VITAE: DOUGLAS P. HAMILTON Career Summary Professor, University of Maryland, Astronomy Dept., 9/1995 { Present. Postdoctoral Scholar, MPI Kernphysik, Heidelberg Germany, 12/1993 { 9/1995. Cornell University, M.S. and Ph.D. in Applied Physics, 8/1990 and 1/1994. Stanford University, B.S. in Physics with Distinction and Honors, 6/1988. Academic Honors NASA Group Achievement Award (New Horizons Team) 2016. U. Maryland Board of Regent's Faculty Award for Scholarship 2010. Dean's Award for Excellence in Teaching 1997, 2008. U. Maryland Parents Association, Outstanding Faculty Nominee 2003. Certificate of Teaching Excellence 2003. Asteroid 12494 DH11 renamed Doughamilton 2000. Harold C. Urey Prize for Outstanding Research in Planetary Science 1999. NSF CAREER Award \Orbital Dynamics of Solar System Dust" 1998-2003. Professional Activities Co-Investigator with NASA's Juno mission to Jupiter. Collaborator with NASA's New Horizons mission to Pluto. Co-Investigator with the Galileo Dust Detection System (DDS) Team. Reviewer on over 100 occasions for 18 scientific journals and 6 book publishers. Reviewer for 6 domestic and 3 foreign funding agencies. Member of IAU C-A4 Organizing Committee (2015-Present); DDA Vice Chair, Chair, Past Chair (2011-2014); DDA Student Participation Committee (2005-2007); AAS Shapley Lecturer (2006-Present); DDA Committee (2003-2005); DPS Prize Committee (2000-2003); AAS Millennium Speaker (2000-2003); Planetary Data System Rings Node Advisory Council (1997-Present); Icarus editorial board (1999- 2002); AAS, AGU, DDA, DPS and IAU societies. Research Interests Solar System Dynamics: Orbital Evolution; Celestial Mechanics; Resonances; Numerical Methods; Rotational Dynamics; Charged Particle Motion. Origins: Satellite and Ring Systems; The Solar System; Extrasolar Planets.
    [Show full text]
  • New Horizons Pluto/KBO Mission Impact Hazard
    New Horizons Pluto/KBO Mission Impact Hazard Hal Weaver NH Project Scientist The Johns Hopkins University Applied Physics Laboratory Outline • Background on New Horizons mission • Description of Impact Hazard problem • Impact Hazard mitigation – Hubble Space Telescope plays a key role New Horizons: To Pluto and Beyond The Initial Reconnaissance of The Solar System’s “Third Zone” KBOs Pluto-Charon Jupiter System 2016-2020 July 2015 Feb-March 2007 Launch Jan 2006 PI: Alan Stern (SwRI) PM: JHU Applied Physics Lab New Horizons is NASA’s first New Frontiers Mission Frontier of Planetary Science Explore a whole new region of the Solar System we didn’t even know existed until the 1990s Pluto is no longer an outlier! Pluto System is prototype of KBOs New Horizons gives the first close-up view of these newly discovered worlds New Horizons Now (overhead view) NH Spacecraft & Instruments 2.1 meters Science Team: PI: Alan Stern Fran Bagenal Rick Binzel Bonnie Buratti Andy Cheng Dale Cruikshank Randy Gladstone Will Grundy Dave Hinson Mihaly Horanyi Don Jennings Ivan Linscott Jeff Moore Dave McComas Bill McKinnon Ralph McNutt Scott Murchie Cathy Olkin Carolyn Porco Harold Reitsema Dennis Reuter Dave Slater John Spencer Darrell Strobel Mike Summers Len Tyler Hal Weaver Leslie Young Pluto System Science Goals Specified by NASA or Added by New Horizons New Horizons Resolution on Pluto (Simulations of MVIC context imaging vs LORRI high-resolution "noodles”) 0.1 km/pix The Best We Can Do Now 0.6 km/pix HST/ACS-PC: 540 km/pix New Horizons Science Status •
    [Show full text]
  • A Deep Search for Additional Satellites Around the Dwarf Planet
    Search for Additional Satellites around Haumea A Preprint typeset using LTEX style emulateapj v. 01/23/15 A DEEP SEARCH FOR ADDITIONAL SATELLITES AROUND THE DWARF PLANET HAUMEA Luke D. Burkhart1,2, Darin Ragozzine1,3,4, Michael E. Brown5 Search for Additional Satellites around Haumea ABSTRACT Haumea is a dwarf planet with two known satellites, an unusually high spin rate, and a large collisional family, making it one of the most interesting objects in the outer solar system. A fully self-consistent formation scenario responsible for the satellite and family formation is still elusive, but some processes predict the initial formation of many small moons, similar to the small moons recently discovered around Pluto. Deep searches for regular satellites around KBOs are difficult due to observational limitations, but Haumea is one of the few for which sufficient data exist. We analyze Hubble Space Telescope (HST) observations, focusing on a ten-consecutive-orbit sequence obtained in July 2010, to search for new very small satellites. To maximize the search depth, we implement and validate a non-linear shift-and-stack method. No additional satellites of Haumea are found, but by implanting and recovering artificial sources, we characterize our sensitivity. At distances between 10,000 km and 350,000 km from Haumea, satellites with radii as small as 10 km are ruled out, assuming∼ an albedo∼ (p 0.7) similar to Haumea. We also rule out satellites larger∼ than &40 km in most of the Hill sphere using≃ other HST data. This search method rules out objects similar in size to the small moons of Pluto.
    [Show full text]
  • CHORUS: Let's Go Meet the Dwarf Planets There Are Five in Our Solar
    Meet the Dwarf Planet Lyrics: CHORUS: Let’s go meet the dwarf planets There are five in our solar system Let’s go meet the dwarf planets Now I’ll go ahead and list them I’ll name them again in case you missed one There’s Pluto, Ceres, Eris, Makemake and Haumea They haven’t broken free from all the space debris There’s Pluto, Ceres, Eris, Makemake and Haumea They’re smaller than Earth’s moon and they like to roam free I’m the famous Pluto – as many of you know My orbit’s on a different path in the shape of an oval I used to be planet number 9, But I break the rules; I’m one of a kind I take my time orbiting the sun It’s a long, long trip, but I’m having fun! Five moons keep me company On our epic journey Charon’s the biggest, and then there’s Nix Kerberos, Hydra and the last one’s Styx 248 years we travel out Beyond the other planet’s regular rout We hang out in the Kuiper Belt Where the ice debris will never melt CHORUS My name is Ceres, and I’m closest to the sun They found me in the Asteroid Belt in 1801 I’m the only known dwarf planet between Jupiter and Mars They thought I was an asteroid, but I’m too round and large! I’m Eris the biggest dwarf planet, and the slowest one… It takes me 557 years to travel around the sun I have one moon, Dysnomia, to orbit along with me We go way out past the Kuiper Belt, there’s so much more to see! CHORUS My name is Makemake, and everyone thought I was alone But my tiny moon, MK2, has been with me all along It takes 310 years for us to orbit ‘round the sun But out here in the Kuiper Belt… our adventures just begun Hello my name’s Haumea, I’m not round shaped like my friends I rotate fast, every 4 hours, which stretched out both my ends! Namaka and Hi’iaka are my moons, I have just 2 And we live way out past Neptune in the Kuiper Belt it’s true! CHORUS Now you’ve met the dwarf planets, there are 5 of them it’s true But the Solar System is a great big place, with more exploring left to do Keep watching the skies above us with a telescope you look through Because the next person to discover one… could be me or you… .
    [Show full text]
  • Anticipated Scientific Investigations at the Pluto System
    Space Sci Rev (2008) 140: 93–127 DOI 10.1007/s11214-008-9462-9 New Horizons: Anticipated Scientific Investigations at the Pluto System Leslie A. Young · S. Alan Stern · Harold A. Weaver · Fran Bagenal · Richard P. Binzel · Bonnie Buratti · Andrew F. Cheng · Dale Cruikshank · G. Randall Gladstone · William M. Grundy · David P. Hinson · Mihaly Horanyi · Donald E. Jennings · Ivan R. Linscott · David J. McComas · William B. McKinnon · Ralph McNutt · Jeffery M. Moore · Scott Murchie · Catherine B. Olkin · Carolyn C. Porco · Harold Reitsema · Dennis C. Reuter · John R. Spencer · David C. Slater · Darrell Strobel · Michael E. Summers · G. Leonard Tyler Received: 5 January 2007 / Accepted: 28 October 2008 / Published online: 3 December 2008 © Springer Science+Business Media B.V. 2008 L.A. Young () · S.A. Stern · C.B. Olkin · J.R. Spencer Southwest Research Institute, Boulder, CO, USA e-mail: [email protected] H.A. Weaver · A.F. Cheng · R. McNutt · S. Murchie Johns Hopkins University Applied Physics Lab., Laurel, MD, USA F. Bagenal · M. Horanyi University of Colorado, Boulder, CO, USA R.P. Binzel Massachusetts Institute of Technology, Cambridge, MA, USA B. Buratti Jet Propulsion Laboratory, Pasadena, CA, USA D. Cruikshank · J.M. Moore NASA Ames Research Center, Moffett Field, CA, USA G.R. Gladstone · D.J. McComas · D.C. Slater Southwest Research Institute, San Antonio, TX, USA W.M. Grundy Lowell Observatory, Flagstaff, AZ, USA D.P. Hinson · I.R. Linscott · G.L. Tyler Stanford University, Stanford, CA, USA D.E. Jennings · D.C. Reuter NASA Goddard Space Flight Center, Greenbelt, MD, USA 94 L.A. Young et al.
    [Show full text]
  • Pluto and Charon
    National Aeronautics and Space Administration 0 300,000,000 900,000,000 1,500,000,000 2,100,000,000 2,700,000,000 3,300,000,000 3,900,000,000 4,500,000,000 5,100,000,000 5,700,000,000 kilometers Pluto and Charon www.nasa.gov Pluto is classified as a dwarf planet and is also a member of a Charon’s orbit around Pluto takes 6.4 Earth days, and one Pluto SIGNIFICANT DATES group of objects that orbit in a disc-like zone beyond the orbit of rotation (a Pluto day) takes 6.4 Earth days. Charon neither rises 1930 — Clyde Tombaugh discovers Pluto. Neptune called the Kuiper Belt. This distant realm is populated nor sets but “hovers” over the same spot on Pluto’s surface, 1977–1999 — Pluto’s lopsided orbit brings it slightly closer to with thousands of miniature icy worlds, which formed early in the and the same side of Charon always faces Pluto — this is called the Sun than Neptune. It will be at least 230 years before Pluto history of the solar system. These icy, rocky bodies are called tidal locking. Compared with most of the planets and moons, the moves inward of Neptune’s orbit for 20 years. Kuiper Belt objects or transneptunian objects. Pluto–Charon system is tipped on its side, like Uranus. Pluto’s 1978 — American astronomers James Christy and Robert Har- rotation is retrograde: it rotates “backwards,” from east to west Pluto’s 248-year-long elliptical orbit can take it as far as 49.3 as- rington discover Pluto’s unusually large moon, Charon.
    [Show full text]
  • Study Points ⚫ Name a Dwarf Planet
    ⚫ What is the major difference between a planet and a dwarf planet? Study Points ⚫ Name a dwarf planet. ⚫ Where are the dwarf planets in our solar system? ⚫ Distinguish between a meteor, a meteorite, and a meteoroid. ⚫ What is a "shooting star"? Why do we see it? On average, how big is one? ⚫ Why do we study meteorites? ⚫ What is a comet? ⚫ Describe a comet including the nucleus, head and tail. Why do we see a comet? ⚫ Roughly, how big are comets? ⚫ What is the Asteroid Belt? the Oort Cloud? the Kuiper Belt? Where is each located? ⚫ Why study comets? ⚫ What is a meteor shower? What is the comet connection to a meteor shower? What’s in our solar system? Sun Planets Terrestrial Jovian Dwarf Small Solar System Bodies Meteoroids Comets Dust Sun (future lecture after Test 2 all about the Sun) a. Most of mass (>99%) of solar system b. Star – produces own energy by fusion c. Hot http://sohowww.nascom.nasa.gov/gallery/images/large/eit001_prev.jpg What’s in our solar system? Sun Planets Terrestrial Jovian http://www.techastronomy.com/UserFiles/2007/7/22/solar_system4(1).jpg From**KNOW Last THIS**Lecture: Terrestrial* Jovian* “Earth-like” “Jupiter-like” • Small, less massive • Large, massive • Close to Sun (warm) • Far from Sun (cold) • Rings • Big storms, turbulent atmosphere, belt rotation • Heavy elements • Hydrogen rich (light elements) • High density • Low density • Solid Surfaces • Gas and Liquid • Cratered • Few moons • Many moons • Thin atmospheres • Thick atmospheres • Weak magnetic fields • Large magnetic fields (some tilted) • Slow rotation
    [Show full text]
  • Results from the New Horizons Encounter with Pluto
    EPSC Abstracts Vol. 11, EPSC2017-140, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Results from the New Horizons encounter with Pluto C. B. Olkin (1), S. A. Stern (1), J. R. Spencer (1), H. A. Weaver (2), L. A. Young (1), K. Ennico (3) and the New Horizons Team (1) Southwest Research Institute, Colorado, USA, (2) Johns Hopkins University Applied Physics Laboratory, Maryland, USA (3) NASA Ames Research Center, California, USA ([email protected]) Abstract Hydra) and the various processes that would darken those surfaces over time [5]. In July 2015, the New Horizons spacecraft flew through the Pluto system providing high spatial resolution panchromatic and color visible light imaging, near-infrared composition mapping spectroscopy, UV airglow measurements, UV solar and radio uplink occultations for atmospheric sounding, and in situ plasma and dust measurements that have transformed our understanding of Pluto and its moons [1]. Results from the science investigations focusing on geology, surface composition and atmospheric studies of Pluto and its largest satellite Charon will be presented. We also describe the New Horizons extended mission. 1. Geology and Size Highlights from the geology investigation of Pluto Figure 1: The glacial ices of Sputnik Planitia. The include the discovery of a unexpected diversity of cellular pattern is a surface expression of mobile lid geomorpholgies across the surface, the discovery of a convection. The boundaries of the cells are troughs. deep basin (informally known as Sputnik Planitia) Despite it’s size of ~900,000 km2, there are no containing glacial ices undergoing mobile-lid identified craters across Sputnik Planitia.
    [Show full text]
  • 2015 October
    TTSIQ #13 page 1 OCTOBER 2015 www.nasa.gov/press-release/nasa-confirms-evidence-that-liquid-water-flows-on-today-s-mars Flash! Sept. 28, 2015: www.space.com/30674-flowing-water-on-mars-discovery-pictures.html www.space.com/30673-water-flows-on-mars-discovery.html - “boosting odds for life!” These dark, narrow, 100 meter~yards long streaks called “recurring slope lineae” flowing downhill on Mars are inferred to have been formed by contemporary flowing water www.space.com/30683-mars-liquid-water-astronaut-exploration.html INDEX 2 Co-sponsoring Organizations NEWS SECTION pp. 3-56 3-13 Earth Orbit and Mission to Planet Earth 13-14 Space Tourism 15-20 Cislunar Space and the Moon 20-28 Mars 29-33 Asteroids & Comets 34-47 Other Planets & their moons 48-56 Starbound ARTICLES & ESSAY SECTION pp 56-84 56 Replace "Pluto the Dwarf Planet" with "Pluto-Charon Binary Planet" 61 Kepler Shipyards: an Innovative force that could reshape the future 64 Moon Fans + Mars Fans => Collaboration on Joint Project Areas 65 Editor’s List of Needed Science Missions 66 Skyfields 68 Alan Bean: from “Moonwalker” to Artist 69 Economic Assessment and Systems Analysis of an Evolvable Lunar Architecture that Leverages Commercial Space Capabilities and Public-Private-Partnerships 71 An Evolved Commercialized International Space Station 74 Remembrance of Dr. APJ Abdul Kalam 75 The Problem of Rational Investment of Capital in Sustainable Futures on Earth and in Space 75 Recommendations to Overcome Non-Technical Challenges to Cleaning Up Orbital Debris STUDENTS & TEACHERS pp 85-96 Past TTSIQ issues are online at: www.moonsociety.org/international/ttsiq/ and at: www.nss.org/tothestarsOO TTSIQ #13 page 2 OCTOBER 2015 TTSIQ Sponsor Organizations 1.
    [Show full text]
  • 1 on the Origin of the Pluto System Robin M. Canup Southwest Research Institute Kaitlin M. Kratter University of Arizona Marc Ne
    On the Origin of the Pluto System Robin M. Canup Southwest Research Institute Kaitlin M. Kratter University of Arizona Marc Neveu NASA Goddard Space Flight Center / University of Maryland The goal of this chapter is to review hypotheses for the origin of the Pluto system in light of observational constraints that have been considerably refined over the 85-year interval between the discovery of Pluto and its exploration by spacecraft. We focus on the giant impact hypothesis currently understood as the likeliest origin for the Pluto-Charon binary, and devote particular attention to new models of planet formation and migration in the outer Solar System. We discuss the origins conundrum posed by the system’s four small moons. We also elaborate on implications of these scenarios for the dynamical environment of the early transneptunian disk, the likelihood of finding a Pluto collisional family, and the origin of other binary systems in the Kuiper belt. Finally, we highlight outstanding open issues regarding the origin of the Pluto system and suggest areas of future progress. 1. INTRODUCTION For six decades following its discovery, Pluto was the only known Sun-orbiting world in the dynamical vicinity of Neptune. An early origin concept postulated that Neptune originally had two large moons – Pluto and Neptune’s current moon, Triton – and that a dynamical event had both reversed the sense of Triton’s orbit relative to Neptune’s rotation and ejected Pluto onto its current heliocentric orbit (Lyttleton, 1936). This scenario remained in contention following the discovery of Charon, as it was then established that Pluto’s mass was similar to that of a large giant planet moon (Christy and Harrington, 1978).
    [Show full text]
  • New Horizons Explores the Pluto System 2015
    The Everest of Planetary Exploration: New Horizons Explores The Pluto System 2015 July 2015 Be There! New Horizons: Science At The Pluto System Total System Characterization • New satellites? Dust rings? • Measure satellite masses, orbits, colors, compositions Total System Characterization Outcome of Giant Impact • Goal: Understand formation of Pluto Pluto system and the Kuiper Belt – and transformation of icy debris early solar system Charon Model: R. Canup (SwRI) Distance (103 km) Global Geology Best “synthetic Pluto” from Hubble 2,300 km Resolution ~500 km Map: M. Buie (SwRI) • High-Res mapping of Pluto and satellites Charon, Nix and Hydra New Horizons: 90 meters/pixel • Search for changes on approach to Pluto, surface-atmosphere interactions, mobile frosts, clouds and hazes • Goal: Understand how dwarf planets evolve; compare and contrast with icy satellites Atmospheric Structure & Escape • Goal: Understand dwarf-planet atmospheres and climates Atmospheric Structure & Escape • Goal: Understand how planets lose their atmospheres Model: D McComas (SwRI) Composition & Temperature Maps • Surface-ice distribution; search for complex organic molecules • Relation of ices to sunlight, topography, atmosphere; evidence for cryovolcanism or geysers • Goal: understand Pluto and Charon as planet and major moon Archetype Kuiper Belt Planet • New Horizons will revolutionize our understanding of icy planets of the Kuiper belt and broader trans-Neptunian population • Pluto “saw” early cataclysmic events, including wholesale reorganization of the solar
    [Show full text]
  • Towards 6G Through Sdn and Nfv-Based Solutions for Terrestrial and Non-Terrestrial Networks
    TOWARDS 6G THROUGH SDN AND NFV-BASED SOLUTIONS FOR TERRESTRIAL AND NON-TERRESTRIAL NETWORKS A Dissertation Presented to The Academic Faculty By Ahan Kak In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the School of Electrical and Computer Engineering Georgia Institute of Technology May 2021 © Ahan Kak 2021 TOWARDS 6G THROUGH SDN AND NFV-BASED SOLUTIONS FOR TERRESTRIAL AND NON-TERRESTRIAL NETWORKS Thesis committee: Dr. Ian F. Akyildiz (Advisor) Dr. Chuanyi Ji School of Electrical and Computer School of Electrical and Computer Engineering (Formerly) Engineering Georgia Institute of Technology Georgia Institute of Technology Dr. Raghupathy Sivakumar (Chair) Dr. Henry L. Owen School of Electrical and Computer School of Electrical and Computer Engineering Engineering Georgia Institute of Technology Georgia Institute of Technology Dr. Mary Ann Weitnauer Dr. Andy Sun School of Electrical and Computer School of Industrial & Systems Engineering Engineering Georgia Institute of Technology Georgia Institute of Technology Date approved: April 6, 2021 To my family, for their endless love, support, and encouragement. ACKNOWLEDGMENTS I would like to begin by expressing my deepest gratitude to my advisor, Dr. Ian F. Aky- ildiz. I am extremely grateful to him for giving me the life-changing opportunity of joining his lab. His unparalleled vision and boundless passion have been integral in setting me on the path to academic success. Like a guiding light that shines through stormy seas, Prof. Akyildiz’s limitless wisdom has always led the way forward, even in the most difficult of times. His incredible work ethic has been a constant source of inspiration for me throughout this journey, one that has been greatly enriched by his immense knowledge and extensive experience.
    [Show full text]