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Juno Telecommunications
The cover The cover is an artist’s conception of Juno in orbit around Jupiter.1 The photovoltaic panels are extended and pointed within a few degrees of the Sun while the high-gain antenna is pointed at the Earth. 1 The picture is titled Juno Mission to Jupiter. See http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA13087 for the cover art and an accompanying mission overview. DESCANSO Design and Performance Summary Series Article 16 Juno Telecommunications Ryan Mukai David Hansen Anthony Mittskus Jim Taylor Monika Danos Jet Propulsion Laboratory California Institute of Technology Pasadena, California National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California October 2012 This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply endorsement by the United States Government or the Jet Propulsion Laboratory, California Institute of Technology. Copyright 2012 California Institute of Technology. Government sponsorship acknowledged. DESCANSO DESIGN AND PERFORMANCE SUMMARY SERIES Issued by the Deep Space Communications and Navigation Systems Center of Excellence Jet Propulsion Laboratory California Institute of Technology Joseph H. Yuen, Editor-in-Chief Published Articles in This Series Article 1—“Mars Global -
Spin-Orbit Coupling for Close-In Planets Alexandre C
A&A 630, A102 (2019) Astronomy https://doi.org/10.1051/0004-6361/201936336 & © ESO 2019 Astrophysics Spin-orbit coupling for close-in planets Alexandre C. M. Correia1,2 and Jean-Baptiste Delisle2,3 1 CFisUC, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal e-mail: [email protected] 2 ASD, IMCCE, Observatoire de Paris, PSL Université, 77 Av. Denfert-Rochereau, 75014 Paris, France 3 Observatoire de l’Université de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland Received 17 July 2019 / Accepted 20 August 2019 ABSTRACT We study the spin evolution of close-in planets in multi-body systems and present a very general formulation of the spin-orbit problem. This includes a simple way to probe the spin dynamics from the orbital perturbations, a new method for computing forced librations and tidal deformation, and general expressions for the tidal torque and capture probabilities in resonance. We show that planet–planet perturbations can drive the spin of Earth-size planets into asynchronous or chaotic states, even for nearly circular orbits. We apply our results to Mercury and to the KOI-1599 system of two super-Earths in a 3/2 mean motion resonance. Key words. celestial mechanics – planets and satellites: general – chaos 1. Introduction resonant rotation with the orbital libration frequency (Correia & Robutel 2013; Leleu et al. 2016; Delisle et al. 2017). The inner planets of the solar system, like the majority of the Despite the proximity of solar system bodies, the determi- main satellites, currently present a rotation state that is differ- nation of their rotational periods has only been achieved in ent from what is believed to have been the initial state (e.g., the second half of the 20th century. -
Mapping and Planetary Spatial Infrastructure Team
Mapping and Planetary Spatial Infrastructure Team INTRODUCTION SSB study on NASA PSD R&A Reorganization National Academy of Sciences, 13 May 2016 Jani Radebaugh, [email protected] Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise – Influence all phases of the mission lifecycle for science investigations and operations – Strategic needs must be anticipated and prioritized by the community – PSS recommended a “Cartography Research and Analysis Group” [CRAG] in Fall 2014. -
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. -
Motivation Sputnik Planitia Flexural Modeling Plans for GEOL
Motivation Sputnik Planitia Flexural modeling Sputnik Planitia Flexure model • Large teardrop-shaped basin The flexure of an elastic plate in two dimensions obeys Equation 1 located on Pluto at 20°N 180°E 푑4푤 퐷 + 푚 − 푐 푔푤 = 푉0 Equation 1. • Size: 1300 km by 900 km 푑푥4 4퐷 1/4 퐸∗ℎ3 • Depth: 3-4 km (basin) where 훼 = is the flexural parameter, 퐷 = is the flexural rigidity, is the 휌 −휌 12(1−푣2) 푚 • 푚 푐 Deposit of nitrogen ice density of the underlying layer of the ice shell, is the density of the ice shell. g is the gravity on • 푐 Water ice basement Pluto, E is the Young’s modulus of water ice, h is the elastic thickness, and 휈 is Poisson’s ratio 푑3푤 1 푑푤 For a single vertical load at 푥 = 0 , the boundary conditions are 퐷 = 푉 and = 0 Formation Hypotheses 푑푥3 2 0 푑푥 • An ancient impact basin created The deflection due to several line loads is found by superposition: 푉 훼3 푥−푥 푥−푥 푥−푥 by an impactor later filled with 푤 = σ 푖 sin 푖 + cos 푖 exp − 푖 Equation 2. 푖 8퐷 훼 훼 훼 N2 ice. The feature would have moved to the current location Where {푉푖} is the magnitude of the loads at position {푥푖} through polar wander. • Runaway deposition of N2 ice Inversion due to albedo feedback at the The load vector 퐕 that produces topography 퐰, is found by least squares optimization: ±30°. The depression is due to 퐕 = 퐌′퐌 + 퐂 −1 퐌′퐰 elastic flexure under the load of 풎 where M is the operator matrix that links a load at position 푥푗 to deflection at a point 푥푖 a thick N2 ice cap. -
The Chaotic Rotation of Hyperion*
ICARUS 58, 137-152 (1984) The Chaotic Rotation of Hyperion* JACK WISDOM AND STANTON J. PEALE Department of Physics, University of California, Santa Barbara, California 93106 AND FRANGOIS MIGNARD Centre d'Etudes et de Recherehes G~odynamique et Astronomique, Avenue Copernic, 06130 Grasse, France Received August 22, 1983; revised November 4, 1983 A plot of spin rate versus orientation when Hyperion is at the pericenter of its orbit (surface of section) reveals a large chaotic zone surrounding the synchronous spin-orbit state of Hyperion, if the satellite is assumed to be rotating about a principal axis which is normal to its orbit plane. This means that Hyperion's rotation in this zone exhibits large, essentially random variations on a short time scale. The chaotic zone is so large that it surrounds the 1/2 and 2 states, and libration in the 3/2 state is not possible. Stability analysis shows that for libration in the synchronous and 1/2 states, the orientation of the spin axis normal to the orbit plane is unstable, whereas rotation in the 2 state is attitude stable. Rotation in the chaotic zone is also attitude unstable. A small deviation of the principal axis from the orbit normal leads to motion through all angles in both the chaotic zone and the attitude unstable libration regions. Measures of the exponential rate of separation of nearby trajectories in phase space (Lyapunov characteristic exponents) for these three-dimensional mo- tions indicate the the tumbling is chaotic and not just a regular motion through large angles. As tidal dissipation drives Hyperion's spin toward a nearly synchronous value, Hyperion necessarily enters the large chaotic zone. -
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… . -
Survey of Juno Observations in Jupiter's Plasma Disk: Density
RESEARCH ARTICLE Survey of Juno Observations in Jupiter's Plasma Disk: 10.1029/2021JA029446 Density Key Points: E. Huscher1, F. Bagenal1 , R. J. Wilson1 , F. Allegrini2,3 , R. W. Ebert2,3 , P. W. Valek2 , • On most orbits, the densities exhibit J. R. Szalay4 , D. J. McComas4 , J. E. P. Connerney5,6 , S. Bolton2 , and S. M. Levin7 regular behavior mapping out a disk confined close to the centrifugal 1Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA, 2Southwest Research equator 3 • Small-scale ( minutes) variabilities Institute, San Antonio, TX, USA, Department of Physics and Astronomy, University of Texas at San Antonio, San 4 5 may indicate∼ radial transport via Antonio, TX, USA, Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA, Space Research local instabilities Corporation, Annapolis, MD, USA, 6Goddard Space Flight Center, Greenbelt, MD, USA, 7Jet Propulsion Laboratory/ • Occasionally a uniformly tenuous California Institute of Technology, Pasadena, CA, USA outer disk indicates enhanced losses, perhaps triggered by solar wind compression Abstract We explore the variation in plasma conditions through the middle magnetosphere of Jupiter with latitude and radial distance using Juno-JADE measurements of plasma density (electrons, protons, Supporting Information: sulfur, and oxygen ions) surveyed on Orbits 5–26 between March 2017 and April 2020. On most orbits, the Supporting Information may be found in the online version of this article. densities exhibit regular behavior, mapping out a disk between 10 and 50 RJ (Jovian radii). In the disk, the heavy ions are confined close to the centrifugal equator which oscillates relative to the spacecraft due to the 10° tilt of Jupiter's magnetic dipole. -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
ENGLISH HOME LANGUAGE GRADE 9 Reading a Myth: Persephone
ENGLISH HOME LANGUAGE GRADE 9 Reading a myth: Persephone MEMORANDUM 1. This myth explains the changing of the seasons. Which season is your favourite and why? Learners own response. Winter/Autumn/Spring/Summer✓ + reason.✓ 2. Myths are stories that explain natural occurrences and express beliefs about what is right and wrong. What natural occurrence does the bracketed paragraph explain? The paragraph relates to earthquakes and volcanos✓ that shake the earth’s core. It suggests that “fearful’ fire-breathing giants” presumably volcanos✓, heave and struggle to get free, which causes the earthquakes. ✓ 3. How do the Greeks explain how people fall in love? Eros (Cupid) the god of love✓, shoots people in the heart with a love-arrow✓ that makes them fall in love. 4. Who is Pluto? He is the “dark monarch” king of the underworld✓ otherwise known as hell. 5. A cause is an effect or action that produces a result. A result is called an effect. What effect does Eros’s arrow have on Pluto? Eros’s arrow fills Pluto’s heart with warm emotions. ✓He sees Persephone and immediately falls in love with her. ✓ 6. What is the result of Demeter’s anger at the land? The ground was no longer fertile. ✓ Nothing could grow anymore. Men and oxen worked to grow crops, but they could not. ✓ There was too much rain ✓ and too much sun✓, so the crops did not grow. The cattle died✓ due to starvation. All of mankind would die✓ of starvation. 7. How do the details that describe what happened to the earth explain natural occurrences? The paragraph suggests that drought✓ is caused by Demeter who is angry✓ with the land. -
Mapping and Planetary Spatial Infrastructure Team
Mapping and Planetary Spatial Infrastructure Team Report to the Planetary Science Subcommittee March 2016 Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products, and associated geospatial infrastructure are integral to the success of the planetary science enterprise – Influences all phases of the mission lifecycle for science investigations and operations – Strategic needs must be anticipated and prioritized by the community – PSS recommended a “Cartography Research and Analysis Group” [CRAG] in Fall 2014. • A team fulfilling this role now exists in the form of MAPSIT – MAPSIT succeeds former PCGMWG and assumes strategic planning role But wait, I thought we did this already? • No, we didn’t (really!) • From 1974 to 2012: – 1974: Lunar Photography and Cartography Committee (LPACC) – 1977: Lunar and Planetary Photography and Cartography Committee (LPPACC) – 1979: Planetary Cartography Working Group (PCWG) – Produced two 10-year plans and a supplement (at right) – 1994-2012: Planetary Cartography & Geologic Mapping Working Group (PCGMWG) • PCGMWG ceased “advisory” role in ~2011 • PCGMWG disbanded 2015 with end of PGG • Looming gap for NASA long-term strategic planning and prioritization activities until addressed by MAPSIT formation 3/9/2016 3 Enabling Planetary Science • Planetary Spatial Infrastructure is the technology, policies, standards, human resources, software tools, and related activities necessary to Geographic Information Science and Technology acquire, -
Westminsterresearch the Astrobiology Primer V2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., De La Rubia Leigh, A., Bond
WestminsterResearch http://www.westminster.ac.uk/westminsterresearch The Astrobiology Primer v2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., de la Rubia Leigh, A., Bond, J., Dartnell, L., Goldman, A.D., Lynch, K., Naud, M.-E., Paulino-Lima, I.G., Kelsi, S., Walter-Antonio, M., Abrevaya, X.C., Anderson, R., Arney, G., Atri, D., Azúa-Bustos, A., Bowman, J.S., Brazelton, W.J., Brennecka, G.A., Carns, R., Chopra, A., Colangelo-Lillis, J., Crockett, C.J., DeMarines, J., Frank, E.A., Frantz, C., de la Fuente, E., Galante, D., Glass, J., Gleeson, D., Glein, C.R., Goldblatt, C., Horak, R., Horodyskyj, L., Kaçar, B., Kereszturi, A., Knowles, E., Mayeur, P., McGlynn, S., Miguel, Y., Montgomery, M., Neish, C., Noack, L., Rugheimer, S., Stüeken, E.E., Tamez-Hidalgo, P., Walker, S.I. and Wong, T. This is a copy of the final version of an article published in Astrobiology. August 2016, 16(8): 561-653. doi:10.1089/ast.2015.1460. It is available from the publisher at: https://doi.org/10.1089/ast.2015.1460 © Shawn D. Domagal-Goldman and Katherine E. Wright, et al., 2016; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by- nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited. The WestminsterResearch online digital archive at the University of Westminster aims to make the research output of the University available to a wider audience.