Vibrant Pluto Seen in Historic Fly-By
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
The Geology of the Rocky Bodies Inside Enceladus, Europa, Titan, and Ganymede
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 2905.pdf THE GEOLOGY OF THE ROCKY BODIES INSIDE ENCELADUS, EUROPA, TITAN, AND GANYMEDE. Paul K. Byrne1, Paul V. Regensburger1, Christian Klimczak2, DelWayne R. Bohnenstiehl1, Steven A. Hauck, II3, Andrew J. Dombard4, and Douglas J. Hemingway5, 1Planetary Research Group, Department of Marine, Earth, and Atmospheric Sciences, North Carolina State University, Raleigh, NC 27695, USA ([email protected]), 2Department of Geology, University of Georgia, Athens, GA 30602, USA, 3Department of Earth, Environmental, and Planetary Sciences, Case Western Reserve University, Cleveland, OH 44106, USA, 4Department of Earth and Environmental Sciences, University of Illinois at Chicago, Chicago, IL 60607, USA, 5Department of Earth & Planetary Science, University of California Berkeley, Berkeley, CA 94720, USA. Introduction: The icy satellites of Jupiter and horizontal stresses, respectively, Pp is pore fluid Saturn have been the subjects of substantial geological pressure (found from (3)), and μ is the coefficient of study. Much of this work has focused on their outer friction [12]. Finally, because equations (4) and (5) shells [e.g., 1–3], because that is the part most readily assess failure in the brittle domain, we also considered amenable to analysis. Yet many of these satellites ductile deformation with the relation n –E/RT feature known or suspected subsurface oceans [e.g., 4– ε̇ = C1σ exp , (6) 6], likely situated atop rocky interiors [e.g., 7], and where ε̇ is strain rate, C1 is a constant, σ is deviatoric several are of considerable astrobiological significance. stress, n is the stress exponent, E is activation energy, R For example, chemical reactions at the rock–water is the universal gas constant, and T is temperature [13]. -
Pluto's Long, Strange History — in Pictures : Nature News & Comment
Pluto's long, strange history — in pictures Nature marks the 85th anniversary of the dwarf planet's discovery. Alexandra Witze 18 February 2015 Even at a distance of 5 billion kilometres, Pluto has entranced scientists and the public back on Earth. Nature looks at the history of this enigmatic world, which in July will get its first close-up visit by a spacecraft. First glimpse Lowell Observatory 18 February 1930: Farmer-turned-astronomer Clyde Tombaugh (pictured), aged 24, discovers Pluto while comparing photographic plates of the night sky at Lowell Observatory in Flagstaff, Arizona. The discovery, announced on 13 March 1930, is the culmination of observatory founder Percival Lowell’s obsessive quest to find a ‘Planet X’, the existence of which was suspected based on perturbations in Neptune’s orbit. Name game Galaxy Picture Library 1 May 1930: The Lowell Observatory announces that its favoured name for the discovery is Pluto, suggested by 11-year-old Venetia Burney (pictured) from Oxford, UK, after the Roman god of the underworld. Venetia later becomes the namesake of a student-built dust counter on NASA's New Horizons spacecraft, which is currently on its way to Pluto. Pair bond US Naval Observatory 22 June 1978: James Christy and Robert Harrington, of the US Naval Observatory's Flagstaff Station, discover Pluto’s largest moon, Charon. It is visible as a bulge (at top in left image) that regularly appears and disappears in observational images as the two bodies orbit their mutual centre of gravity1. The moon is so large relative to Pluto that the two are sometimes referred to as a binary planet. -
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… . -
Comparative Planetology Beyond Neptune Enabled by a Near-Term Interstellar Probe
51st Lunar and Planetary Science Conference (2020) 1464.pdf COMPARATIVE PLANETOLOGY BEYOND NEPTUNE ENABLED BY A NEAR-TERM INTERSTELLAR PROBE. K. D. Runyon ([email protected]), K. E. Mandt, P. Brandt, M. Paul, C. Lisse, R. McNutt, Jr. (Johns Hopkins APL, 11101 Johns Hopkins Rd., Laurel, MD, 20723, USA), C.B. Beddingfield (NASA/Ames), S.A. Stern (Southwest Research Institute) Summary: A properly instrumented Interstellar surprising differences despite water having played a Probe could enable flyby geoscience investigations of a substantial role in the surface and subsurface of each Kuiper belt dwarf planet, advancing comparative plan- planet (e.g., Prettyman et al., 2017; Prockter et al., 2005; etology in the trans-Neptunian region. Nimmo and Pappalardo, 2016; Beyer et al., 2019). With Introduction: Comparative planetology among the long time frames and relative difficulty in reaching KBO dwarf planets A) should be a priority for future trans-Neptunian planets, Interstellar Probe could ad- NASA missions; and B) could be partly addressed by a vance the field via in situ exploration of just one more targeted flyby of a dwarf planet by an interstellar probe planet, such as Quaoar, “Gonggong” (officially 2007 leaving the Solar System, such as described by McNutt OR10), or another. et al. (2019). This abstract is based on a near-term white A camera-instrumented Interstellar Probe could tar- paper to be submitted by mid-2020 to the National get high resolution images of a dwarf planet’s surface, Academies Planetary Science Decadal Survey Panel. similar to New Horizons’ flyby images of Pluto, Charon, Please contact the first author to be added to the white and Arrokoth (2014 MU69). -
What Is the Color of Pluto? - Universe Today
What is the Color of Pluto? - Universe Today space and astronomy news Universe Today Home Members Guide to Space Carnival Photos Videos Forum Contact Privacy Login NASA’s New Horizons spacecraft captured this high-resolution enhanced color view of http://www.universetoday.com/13866/color-of-pluto/[29-Mar-17 13:18:37] What is the Color of Pluto? - Universe Today Pluto on July 14, 2015. Credit: NASA/JHUAPL/SwRI WHAT IS THE COLOR OF PLUTO? Article Updated: 28 Mar , 2017 by Matt Williams When Pluto was first discovered by Clybe Tombaugh in 1930, astronomers believed that they had found the ninth and outermost planet of the Solar System. In the decades that followed, what little we were able to learn about this distant world was the product of surveys conducted using Earth-based telescopes. Throughout this period, astronomers believed that Pluto was a dirty brown color. In recent years, thanks to improved observations and the New Horizons mission, we have finally managed to obtain a clear picture of what Pluto looks like. In addition to information about its surface features, composition and tenuous atmosphere, much has been learned about Pluto’s appearance. Because of this, we now know that the one-time “ninth planet” of the Solar System is rich and varied in color. Composition: With a mean density of 1.87 g/cm3, Pluto’s composition is differentiated between an icy mantle and a rocky core. The surface is composed of more than 98% nitrogen ice, with traces of methane and carbon monoxide. Scientists also suspect that Pluto’s internal structure is differentiated, with the rocky material having settled into a dense core surrounded by a mantle of water ice. -
Jjmonl 1710.Pmd
alactic Observer John J. McCarthy Observatory G Volume 10, No. 10 October 2017 The Last Waltz Cassini’s final mission and dance of death with Saturn more on page 4 and 20 The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky Technical Support It is through their efforts that the McCarthy Observatory Bob Lambert has established itself as a significant educational and recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Route Mike Chiarella Roger Moore Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Doug Delisle Marc Polansky Cecilia Detrich Joe Privitera Dirk Feather Monty Robson Randy Fender Don Ross Louise Gagnon Gene Schilling John Gebauer Katie Shusdock Elaine Green Paul Woodell Tina Hartzell Amy Ziffer In This Issue INTERNATIONAL OBSERVE THE MOON NIGHT ...................... 4 SOLAR ACTIVITY ........................................................... 19 MONTE APENNINES AND APOLLO 15 .................................. 5 COMMONLY USED TERMS ............................................... 19 FAREWELL TO RING WORLD ............................................ 5 FRONT PAGE ............................................................... -
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. -
Deciphering Enceladus's Tectonic History: an Analog for the Pluto And
Deciphering Enceladus’s Tectonic History: An Analog for the Pluto and Charon System. E.S. Martin and S.A. Kattenhorn, Department of Geological Sciences, University of Idaho, Moscow, ID 83844-3022, [email protected], [email protected]. Introduction: Comparative planetology is a valu- stress fields. Detailed fracture mapping of a small re- able tool when data resolution hinders analysis. In the gion of the cratered terrains has been completed using case of Pluto and Charon, no detailed images of the crosscutting relationships to determine relative ages of surface exist; other icy bodies have been used to hint at fractures that belong to regionally extensive sets (Fig. what processes are or have occurred on the surface. 1). We have identified four distinct fracture sets with Triton has been speculated to be a good analog for different orientations showing a relative rotation of the Pluto and Charon, but [1] suggest that a heating event stress field through time, perhaps related to NSR. caused by the capture of Triton by Neptune would Small-Scale Tectonic Features: There are a vari- have altered the surface enough to render it too dis- ety of small-scale tectonic features found on Enceladus similar to Pluto and Charon. No icy satellite may ever that aid in identification of tectonic processes and may truly serve as a direct analog for another; however, the be relevant to the Pluto-Charon system. techniques used to construct an understanding of an icy Pit chains: Pit chains are linear troughs made up of body’s tectonic history are applicable to a variety of circular to elliptical depressions formed by the draining icy satellites. -
In the Czech Republic
EPSC Abstracts Vol. 12, EPSC2018-900, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 The planetary "Grand Tour" in the Czech Republic Tomas Petrasek (1), Julie Nekola Novakova (2), Kosmo Klub, z. s. (1) Faculty of Science, Charles University, Prague, Czech Republic, (2) Laboratory of Evolutionary Biology, Faculty of Science, Charles University, Prague, Czech Republic Abstract object (Sedna) is 13,5 km. As both the sizes and distances are in the same scale, and most of the Kosmo Klub is an association of space enthusiasts in bodies are within a direct line of sight, it is possible the Czech Republic, dedicated to popularization of to observe the correct apparent size of the model Sun astronautics and space science since 2004. Its most (or moons etc.) from any planet up to Saturn. Every recent project is the Planetary Trail in Prague. It is a single body is accompanied by a label summarizing model of the Solar System at 1:1 000 000 000 scale its important characteristics. located along a frequented trail for cyclists and pedestrians along the Vltava River. It will provide the 2. Figures visitors with basic information about our cosmic neighborhood, and provide a base for further outreach activities. 1. Introduction Blazing past the planets in the Solar System is a wonder for our imagination - and bringing the wonder of science to the general public is an important goal for both professional scientists and science popularizers. It educates and entertains at the same time, trains people in critical thinking, and explains the meaning and importance of scientific pursuit. -
PLUTO: a New Way to Explore the Planets
Q)mft version 4.1 ************************************** PLUTO: A New Way To Explore the Planets By Richard Shope and Jackie Giuliano ***** ********************************* he Pluto Fast Flyby Mission is an exciting adventure beginning (he next century with a new wuy to explore the planets, The Pluto Preproject Team at the Jet Propulsion 1,aboratory is leading the effort to design and build two spacecraft equipped with @ components atthe cutting edgeof advanced technology. ‘I’he proposed odyssey inthe first years of the ncw century will be achieved through the combined efforts of American and Russian project teams, and perhaps using Russian launch vehicles known as Protons. After seven to nine years in flight, these two innovative, cost-effective spacecraft will provide us the first ever view of the last unexplored planetary system: the mysterious planet Pluto and its enigmatic moon, Charon. The video “Ot(t of the Darkness: Mis- sion 7b Plu[o” (JPI. AVC-94- 164) provides an overview of this mission and an opportu- nity to involve your students in the challenges of such an ambitious endeavor. uL’k, vNk’k, uEu, N,k’LElkk L,uNk’Hk’L,&,k,kluE~NkL~ L’EURL, U kN vL Involve your students in ~k ku’ the thrill of discoveiy! ~ k u uk’k L,vk L’k, kQLl&kp Qlkk Llkkkl Qkklukk, ~x~, ~~ ~,~~~~~ The Pluto Fast Flyby video affords an opportunity for the teacher and student to ex- plore many concepts. These curriculum guides The cost-e ftlcient Pluto Fast Flyby spacecraft have been designed to provide the teacher at encountering Pluto and its moon Charon. -
A Tale of Two Sides: Pluto's Opposition Surge in 2018 and 2019
EPSC Abstracts Vol. 14, EPSC2020-546, 2020, updated on 27 Sep 2021 https://doi.org/10.5194/epsc2020-546 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. A Tale of Two Sides: Pluto's Opposition Surge in 2018 and 2019 Anne Verbiscer1, Paul Helfenstein2, Mark Showalter3, and Marc Buie4 1University of Virginia, Charlottesville, VA, USA ([email protected]) 2Cornell University, Ithaca, NY, USA ([email protected]) 3SETI Institute, Mountain View, CA, USA ([email protected]) 4Southwest Research Institute, Boulder, CO, USA ([email protected]) Near-opposition photometry employs remote sensing observations to reveal the microphysical properties of regolith-covered surfaces over a wide range of solar system bodies. When aligned directly opposite the Sun, objects exhibit an opposition effect, or surge, a dramatic, non-linear increase in reflectance seen with decreasing solar phase angle (the Sun-target-observer angle). This phenomenon is a consequence of both interparticle shadow hiding and a constructive interference phenomenon known as coherent backscatter [1-3]. While the size of the Earth’s orbit restricts observations of Pluto and its moons to solar phase angles no larger than α = 1.9°, the opposition surge, which occurs largely at α < 1°, can discriminate surface properties [4-6]. The smallest solar phase angles are attainable at node crossings when the Earth transits the solar disk as viewed from the object. In this configuration, a solar system body is at “true” opposition. When combined with observations acquired at larger phase angles, the resulting reflectance measurement can be related to the optical, structural, and thermal properties of the regolith and its inferred collisional history. -
Ice Ontnos: Focus on 136108 Haumea
Ice onTNOs: Focus on 136108 Haumea C. Dumas Collaborators: A. Alvarez, A. Barucci, C. deBergh, B. Carry, A. Guilbert, D. Hestroffer, P. Lacerda, F. deMeo, F. Merlin, C. Snodgrass, P. Vernazza, … Haumea Pluto (dwarf planets) DistribuTon of TNOs Largest TNOs Icy bodies in the OPSII context • Reservoir of volales in the solar system (H2O, N2, CH4, CO, CO2, C2H6, NH3OH, etc) • Small bodies populaon more hydrated than originally pictured – Main-belt comets (Hsieh and JewiZ 2006) – Themis asteroids family (Campins et al. 2010, Rivkin and Emery 2010) • Transport of water to the inner terrestrial planets (e.g. talk by Paul Hartogh) Paranal Observatory 6 SINFONI at UT4 7 SINFONI + NACO at UT4 8 SINFONI = MACAO + SPIFFI (SINFONI=Spectrograph for INtegral Field Observations in the Near Infrared) • AO SYSTEM: MACAO (Multi-Application Curvature Adaptive Optics): – Similar to UTs AO system for VLTI – 60 elements curvature sensing bimorph mirror – NGS or LGS – Developed by ESO • NEAR-IR SPECTRO: SPIFFI (SPectrometer for Infrared Faint Field Imaging): – 3-D spectrograph, 32 image slices, 1-2.5µm – Developed by MPE:Max Planck Institute for Extraterrestrial Physics + NOVA: Netherlands Research School for Astronomy SINFONI - Main characteristics • Location UT4 Cassegrain • Wavelength range 1-2.5µm • Detector 2048 x 2048 HAWAII array • Gratings J,H,K,H+K • Spectral resolution 1500 (H+K-filter) to 4000 (K-band) (outside OH lines) • Limiting magnitude (0.1”/spaxel) K~18.2, H+K~19.2 in hr, SNR~10 • FoV sampling 32 slices • Spatial resolution 0.25”/slice (no-AO), 0.1”(AO), 0.025” (AO) • Resulting FoV 8”x8”, 3”x3”, 0.8”x0.8” • Modes noAO, NGS-AO, LGS-AO SINFONI - IFS Principles SINFONI - IFS Principles (Cont’d) SINFONI - products Reconstructed image PSF spectrum H+K TNOs spectroscopy Orcus (Carry et al.