THE PLANETARY REPORT DECEMBER SOLSTICE 2013 VOLUME 33, NUMBER 4 Planetary.Org
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THE PLANETARY REPORT JUNE SOLSTICE 2016 VOLUME 36, NUMBER 2 Planetary.Org
THE PLANETARY REPORT JUNE SOLSTICE 2016 VOLUME 36, NUMBER 2 planetary.org ILLUMINATING CERES DAWN SHEDS NEW LIGHT ON AN ENIGMATIC WORLD BREAKTHROUGH STARSHOT C LIGHTSAIL 2 TEST C MEMBERSHIP UPGRADES SNAPSHOTS FROM SPACE EMILY STEWART LAKDAWALLA blogs at planetary.org/blog. Black Sands of Mars ON SOL 1192 (December 13, 2015), Curiosity approached the side of Namib, a Faccin and Marco Bonora Image: NASA/JPL/MSSS/Elisabetta massive barchan sand dune. Namib belongs to a field of currently active dark basaltic sand dunes that form a long barrier between the rover and the tantalizing rocks of Mount Sharp. This view, processed by Elisabetta Bonora and Marco Faccin, features wind-carved yardangs (crests or ridges ) of Mount Sharp in the background. After taking this set of photos, Curiosity went on to sample sand from the dune, and it is now working its way through a gap in the dune field on the way to the mountain. —Emily Stewart Lakdawalla SEE MORE AMATEUR-PROCESSED SPACE IMAGES planetary.org/amateur SEE MORE EVERY DAY! planetary.org/blogs 2 THE PLANETARY REPORT C JUNE SOLSTICE 2016 CONTENTS JUNE SOLSTICE 2016 COVER STORY Unveiling Ceres 6 Simone Marchi on why Ceres is a scientific treasure chest for Dawn. Pathway to the Stars Looking back at years of Society-led solar sail 10 development as Breakthrough Starshot is announced. Life, the Universe, and Everything 13 Planetary Radio in Death Valley. ADVOCATING FOR SPACE Partisan Peril 18 Casey Dreier looks at the U.S. President’s impact on space policy and legislation. DEVELOPMENTS IN SPACE SCIENCE Update on LightSail 2 20 Bruce Betts details the progress we’ve made in the year since LightSail 1 launched. -
DEGRADATION of ENDEAVOUR CRATER, MARS. J. A. Grant1, L. S. Crumpler2, T
46th Lunar and Planetary Science Conference (2015) 2017.pdf DEGRADATION OF ENDEAVOUR CRATER, MARS. J. A. Grant1, L. S. Crumpler2, T. J. Parker3, M. P. Golombek3, S. A. Wilson1, and D. W. Mittlefehldt4, Smithsonian Institution, NASM CEPS, 6th at Independence SW, Washington, DC, 20560 ([email protected]), 2New Mexico Museum of Natural History & Science, 1801 Mountain Rd NW, Albuquerque, NM, 87104, 3Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, 4NASA JSC, 2101 NASA Parkway, Houston, TX 77058. Introduction: The Opportunity rover has traversed icant degradation. A paucity of debris from the Shoe- portions of two western rim segments of Endeavour, a maker and Matijevic Formations relegates most erosion 22 km-diameter crater in Meridiani Planum (Fig. 1), to before the surrounding plains were emplaced, imply- for the past three years (e.g., [1]). The resultant data ing more efficient erosion in the past [7]. enables the evaluation of the geologic expression [2] Moreover, ejecta comprise ~50-60% of the relief and degradation state of the crater. Endeavour is Noa- around selected Mars complex craters [8] and only 20- chian-aged, complex in morphology [3], and originally 25% around selected lunar complex craters [6]. Hence, may have appeared broadly similar to the more pristine original rim relief at Endeavour may have been only 20.5 km-diameter Santa Fe complex crater in Lunae ~200-500 m or as much as ~400-800 m based on com- Palus (19.5°N, 312.0°E). By contrast, Endeavour is parison with complex Martian and lunar craters of considerably subdued and largely buried by younger broadly similar size [4, 5, 8]. -
NASA and Planetary Exploration
**EU5 Chap 2(263-300) 2/20/03 1:16 PM Page 263 Chapter Two NASA and Planetary Exploration by Amy Paige Snyder Prelude to NASA’s Planetary Exploration Program Four and a half billion years ago, a rotating cloud of gaseous and dusty material on the fringes of the Milky Way galaxy flattened into a disk, forming a star from the inner- most matter. Collisions among dust particles orbiting the newly-formed star, which humans call the Sun, formed kilometer-sized bodies called planetesimals which in turn aggregated to form the present-day planets.1 On the third planet from the Sun, several billions of years of evolution gave rise to a species of living beings equipped with the intel- lectual capacity to speculate about the nature of the heavens above them. Long before the era of interplanetary travel using robotic spacecraft, Greeks observing the night skies with their eyes alone noticed that five objects above failed to move with the other pinpoints of light, and thus named them planets, for “wan- derers.”2 For the next six thousand years, humans living in regions of the Mediterranean and Europe strove to make sense of the physical characteristics of the enigmatic planets.3 Building on the work of the Babylonians, Chaldeans, and Hellenistic Greeks who had developed mathematical methods to predict planetary motion, Claudius Ptolemy of Alexandria put forth a theory in the second century A.D. that the planets moved in small circles, or epicycles, around a larger circle centered on Earth.4 Only partially explaining the planets’ motions, this theory dominated until Nicolaus Copernicus of present-day Poland became dissatisfied with the inadequacies of epicycle theory in the mid-sixteenth century; a more logical explanation of the observed motions, he found, was to consider the Sun the pivot of planetary orbits.5 1. -
ISSUE 134, AUGUST 2013 2 Imperative: Venus Continued
Imperative: Venus — Virgil L. Sharpton, Lunar and Planetary Institute Venus and Earth began as twins. Their sizes and densities are nearly identical and they stand out as being considerably more massive than other terrestrial planetary bodies. Formed so close to Earth in the solar nebula, Venus likely has Earth-like proportions of volatiles, refractory elements, and heat-generating radionuclides. Yet the Venus that has been revealed through exploration missions to date is hellishly hot, devoid of oceans, lacking plate tectonics, and bathed in a thick, reactive atmosphere. A less Earth-like environment is hard to imagine. Venus, Earth, and Mars to scale. Which L of our planetary neighbors is most similar to Earth? Hint: It isn’t Mars. PWhy and when did Earth’s and Venus’ evolutionary paths diverge? This fundamental and unresolved question drives the need for vigorous new exploration of Venus. The answer is central to understanding Venus in the context of terrestrial planets and their evolutionary processes. In addition, however, and unlike virtually any other planetary body, Venus could hold important clues to understanding our own planet — how it has maintained a habitable environment for so long and how long it can continue to do so. Precisely because it began so like Earth, yet evolved to be so different, Venus is the planet most likely to cast new light on the conditions that determine whether or not a planet evolves habitable environments. NASA’s Kepler mission and other concurrent efforts to explore beyond our star system are likely to find Earth-sized planets around Sun-sized stars within a few years. -
Multispectral VNIR Evidence of Alteration Processes on Solander
Multispectral VNIR Evidence of Alteration Processes on W.H. Farrand1, J.F. Bell2, J.R. Johnson3, and D. W. Mittlefehldt4 1. Space Science Institute, Boulder, CO; [email protected] Solander Point, Endeavour Crater, Mars 2. Arizona State University, Tempe, AZ 3. Johns Hopkins University, Applied Physics Lab, Laurel, MD 1) Introduction: 4. NASA Johnson Space Center, Houston, TX The Mars Exploration Rover Opportunity has been exploring Noachian-aged rocks on the rim of Endeavour crater. This exploration began on the Cape York rim segment [1, 2] and has, from Sol 3393 of Opportunity’s mission to the present time, been over the rim segment known as Solander Point (Fig. 1). The visible and near infrared (VNIR) multispectral capability of the 4) Sulfates and oxide minerals in the sub- rover’s Pancam has been an important tool for use in selecting targets for in situ investigation and in it’s own right for surface? characterizing the VNIR reflectance of rock surfaces [3, 4]. Among the rock targets encountered on the Murray Ridge portion of Given the multispectral character of spectra collected by Pancam, a Solander Point were a set of outcrops that had the outward appearance of other occurrences of the Shoemaker formation impact unique identification of mineral phases is generally impractical. The drop breccia [1], but which had a distinct reflectance character. Also, the by chance overturning of the rocks Pinnacle and Stuart in reflectance from 934 to 1009 nm in the light-toned materials on Island revealed light-toned subsurface materials which were likely formed by subsurface aqueous alteration. -
High Concentrations of Manganese and Sulfur in Deposits on Murray Ridge, Endeavour Crater, Marsk
American Mineralogist, Volume 101, pages 1389–1405, 2016 High concentrations of manganese and sulfur in deposits on Murray Ridge, Endeavour Crater, Marsk RAYMOND E. ARVIDSON1,*, STEVEN W. SQUYreS2, RICHARD V. MOrrIS3, ANDrew H. KNOLL4, RALF GELLerT5, BENTON C. CLArk6, JEFFreY G. CATALANO1, BRAD L. JOLLIFF1, SCOTT M. MCLENNAN7, KENNETH E. HerkeNHOFF8, SCOTT VANBOMMEL5, DAVID W. MITTLEFEHLDT3, JOHN P. GROTZINger9, EDWARD A. GUINNESS1, JEFFreY R. JOHNSON10, JAMES F. BELL III11, WILLIAM H. FArrAND6, NATHAN STEIN1, VALerIE K. FOX1, MATTHew P. GOLOMbek12, MArgAreT A.G. HINKLE1, WENDY M. CALVIN13, AND PAULO A. DE SOUZA JR.14 1Department of Earth and Planetary Sciences, Washington University in Saint Louis, St. Louis, Missouri 63130, U.S.A. 2Department of Astronomy, Cornell University, Ithaca, New York 14853, U.S.A. 3Johnson Space Center, Houston, Texas 77058, U.S.A. 4Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts 02138, U.S.A. 5Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada 6Space Science Institute, Boulder, Colorado 80301, U.S.A. 7Department of Geosciences, Stony Brook University, Stony Brook, New York 11794, U.S.A. 8U.S. Geological Survey, Astrogeology Science Center, Flagstaff, Arizona 86001, U.S.A. 9Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, U.S.A. 10Johns Hopkins University, Applied Physics Laboratory, Laurel, Maryland 20723, U.S.A. 11School of Earth & Space Exploration, Arizona State University, Tempe, Arizona 85281, U.S.A. 12California Institute of Technology/Jet Propulsion Laboratory, Pasadena, California 91011 13Geological Sciences and Engineering, University of Nevada, Reno, Nevada 89503, U.S.A. 14CSIRO Digital Productivity Flagship, Hobart, Tasmania 7004, Australia ABSTRACT Mars Reconnaissance Orbiter HiRISE images and Opportunity rover observations of the ~22 km wide Noachian age Endeavour Crater on Mars show that the rim and surrounding terrains were densely fractured during the impact crater-forming event. -
Degradation of Endeavour Crater, Mars
LPSC (2015) Abstract #2017 At CY, present relief along the exposed Wdowiak ridge (WR) is located EROSIONAL FORM OF RIM rim segment is ~10 m and consists of ENIGMATIC WDOWIAK RIDGE immediately west of 6-7 m of Shoemaker Formation over at least several meters of Matijevic Formation. Endeavour’s rim and oriented NE-SW (Figs. 1 and 7). The ridge is capped by Degradation of Endeavour Crater, Mars By contrast, relief along the MR segment is considerably higher and the Shoemaker more resistant dark rocks that are not breccia and are chemically and texturally distinct from the overlying Shoemaker Formation [20]. Origin of the ridge is 1 2 3 3 Formation/Matijevic Formation contact is not visible and up to ~150 m section of J. A. Grant , L. S. Crumpler , T. J. Parker , M. P. Golombek , Shoemaker Formation is preserved at MR. Offset between rim segments is possible uncertain, but possibilities include exhumation of a local pre-impact high or 1 4 S. A. Wilson and D. W. Mittlefehldt and could relate to faulting during late stage crater formation and fractures are ejecta megablock [20] or impact melt and would support estimates of significant observed at MR (Fig. 4). Such fractures may be similar to those around smaller erosion. 1Smithsonian Institution, NASM CEPS, 6th at Independence SW, Washington, DC ([email protected]); terrestrial impacts [4]. 2New Mexico Museum of Natural History & Science, Albuquerque, NM 3Jet Propulsion Laboratory, Comparison to similar sized fresh, complex craters on Mars [5-8] suggests on Figure 7. False color mosaic of California Institute of Technology, Pasadena, CA 4NASA JSA, Houston, TX order of 300 m of ejecta was originally present at the rim of Endeavour crater. -
1 MEDIA ALERT Bill Nye the Science Guy™ and the Planetary Society To
MEDIA ALERT Bill Nye the Science Guy™ and The Planetary Society to Host Canadian Space Program Celebration Toronto gathering will highlight space exploration successes, future goals global community CONTACT: FOR IMMEDIATE RELEASE Mat Kaplan September 8, 2014 Email: [email protected] Mobile: 562-760-4152 The University of Toronto’s Convocation Hall will head for the final frontier on the evening of Wednesday, October 1, 2014, as Planetary Society CEO Bill Nye and very special guests arrive to celebrate Canadian space science and exploration. Titled “We See Thee Rise: The Canadian Space Program Today and Tomorrow,” the two-hour event will feature a special presentation by Mr. Nye, followed by a panel discussion for the Society’s weekly radio and podcast series, “Planetary Radio.” Bill Nye and the Planetary Society are also coming to Toronto to attend the annual meeting of the International Astronautical Congress. WHO: Moderated by Planetary Radio host Mat Kaplan, the panel will include: • Bill Nye, Planetary Society CEO • Canadian Space Agency astronaut Jeremy Hansen, who will have just returned from a week-long, underwater adventure as part of the 19th NASA Extreme Environment Mission Operations (NEEMO) mission • The University of Western Ontario’s Gordon Osinski, Associate Director of the Centre for Planetary Science and Exploration • Elizabeth Howell, space and science contributing writer for Universe Today, Space.com and other notable publications WHAT: Fans in the Hall and watching the live webcast will be entertained by the unique and very entertaining Ottawa-based band Dream World. The audience will also hear about the worldwide Planetary Society’s expanding, homegrown Canadian programs, offering a wide range of ways for space enthusiasts from BC to NS to become involved. -
Planetary Report Report
The PLANETARYPLANETARY REPORT REPORT Volume XXIV Number 4 July/August 2004 Saturn’s Allure Volume XXIV Table of Number 4 Contents July/August 2004 A PUBLICATION OF Features From Planetary Protection—Can’t Leave Home Without It The 6 When thinking about sending humans to Mars, it is in our nature to question: Editor could these organic explorers contaminate the Martian environment? Conversely, when they return to Earth, could astronauts inadvertently expose terrestrial life to very day, those who follow the adven- extraterrestrial biohazards? Margaret Race, an ecologist specializing in planetary tures of our robotic explorers among protection, ponders these questions and works to ensure that the environments of E both Mars and the Earth are protected. the planets have something new to see and learn. On the Internet, images from Mars, Cassini-Huygens’ New Home— Saturn, and other strange new worlds are 12 The First Days in Saturn’s Orbit posted regularly. At scientific conferences, Cassini-Huygens has begun its four-year tour of the spectacular ringed planet and its scientists jostle each other to give papers dozens of moons. Just hours after passing between two Saturnian rings and settling on their latest work, and journals are filled into orbit around the planet, Cassini began returning the best images ever taken of with papers announcing new results. Seldom the magnificent system. Here we showcase some of these first postcards from its have Earthly explorers seen such a trove of new home, some 934 million miles away. discoveries. When bringing these discoveries to Plan- The 2004 Shoemaker NEO Grants— etary Society members, it’s often hard to 18 Send in Those Applications! decide what is most important to include in It’s time for a new round of Shoemaker NEO Grants, funded entirely by donations this magazine. -
The Planetary Society
Public Involvement in International Lunar Exploration Bruce Betts Louis Friedman http://planetary.org The Planetary Society • Founded in 1980 by Carl Sagan, Bruce Murray, and Louis Friedman – Exploration of our solar system – Search for extraterrestrial life. • Largest space interest in the world • Membership open to all • Non-profit, nongovernmental – funded by dues, donations, – corporate sponsorships – No government money • Headquarters in Pasadena The Planetary Society •Projects – Involve and excite public – Fill otherwise unfilled niches – Test innovative technologies – Inspire future generations • Advocacy – Grass roots, Political, International • Publications – The Planetary Report – Planetary.org – Planetary Radio (planetary.org/radio) A Great Opportunity • The many international lunar missions planned for the next decade provide opportunities for powerful public involvement and engagement • The Planetary Society is working with several missions and seeks more opportunity • As an international NGO, the Society is interested in providing creative activities across all the missions. Planetary Society Mission Outreach Background • Providing of spacecraft hardware (e.g., MER DVD’s, Mars Microphone, Phoenix DVD) • Contests (e.g., Venus Express Art Contest, New Horizons Time Capsule, Naming contests (Magellan, Sojourner, MER rovers)) • Coverage of planetary activities via print, web, and radio Planetary Society Coverage of All Lunar Missions Will Include: • Planetary Report Magazine (authors usually the doers). – Special all lunar issue Jan/Feb 2007 • Web site (planetary.org) • Planetary Radio (planetary.org/radio, 110 radio stations, podcast, XM). Weekly. Planetary Society Activities • “Gateway” Web site covering all lunar missions and links to more info. One stop shopping. • With SMART-1, The Planetary Society organized events including live press events for insertion/impact, and has plans to do similar activities for many of the coming missions. -
The Planetary Report December Solstice 2011 Volume 31, Number 5
THE PLANETARY REPORT DECEMBER SOLSTICE 2011 VOLUME 31, NUMBER 5 www.planetary.org REMEMBERING THE YEAR IN PICTURES NEW (OLD) VENUS IMAGES C POLITICAL ACTION 2011 UPDATE C SHOEMAKER GRANT RECIPIENTS SNAPSHOTS FROM SPACE EMILY STEWART LAKDAWALLA blogs at planetary.org/blog. New images, old camera 1975 was a good-looking year for Venus VENERA 9 BECAME THE FIRST ARTIFICIAL satellite of Venus, and its lander was the first to photograph Venus’ surface, on October 20, 1975. One of its two cameras, a line-scanner that rotated in order to build a complete image, returned two views of a rock-strewn hillside. The scanner was angled from the spacecraft’s body, so this panorama shows the horizon at its edges and the Images: Russian Academy of Sciences/Don Mitchell Sciences/Don of Academy Russian Images: ground in front of the lander at its center. This view was reconstructed by Don Mitchell from data on tapes exchanged between the Soviet Union and Brown University. More recently, digital data have become available online, and Mitchell used those data to reconstruct a view of Venus (at right) captured by the Venera 9 orbiter on December 11, 1975. For more Venera photos, visit Mitchell’s website at MENTALLANDSCAPE.COM. —Emily Stewart Lakdawalla LEARN MORE ABOUT THIS IMAGE PLANETARY.ORG/SNAPSHOTS DIS COVER MORE ABOUT AMATEUR IMAGE PROCESSING PLANETARY.ORG/PROGRAMS/PROJECTS/AMATEUR SEE MORE EVERY DAY! PLANETARY.ORG/BLOG CONTACT US The Planetary Society 85 South Grand Avenue Pasadena, CA 91105-1602 General Calls: 626-793-5100 E-mail: [email protected] Internet: planetary.org 2 THE PLANETARY REPORT C DECEMBER SOLSTICE 2011 SNAPSHOTS FROM SPACE CONTENTS DECEMBER SOLSTICE 2011 The Year in Pictures Stunning photography of breakthroughs 6 in space science from the the past year. -
Mars Rover Opportunity Trekking Toward More Layers 7 June 2013, by Guy Webster
Mars rover Opportunity trekking toward more layers 7 June 2013, by Guy Webster for the mission. Solander Point also offers plenty of ground that is tilted toward the north, which is favorable for the solar-powered rover to stay active and mobile through the coming Martian southern-hemisphere winter. "We're heading to a 15-degree north-facing slope with a goal of getting there well before winter," said John Callas of NASA's Jet Propulsion Laboratory, Pasadena, Calif., project manager for the Mars Exploration Rover Project. The minimum-sunshine days of this sixth Martian winter for Opportunity will come in February 2014. NASA's Mars Exploration Rover Project launched twin rovers in 2003: Spirit on June 10 and Opportunity on July 7. Both rovers landed in NASA's Mars Exploration Rover Opportunity used its January 2004, completed three-month prime panoramic camera (Pancam) to acquire this view of missions and began years of bonus, extended "Solander Point" during the mission's 3,325th Martian day, or sol (June 1, 2013). Credit: NASA/JPL- missions. Both found evidence of wet environments Caltech/Cornell Univ./Arizona State Univ on ancient Mars. Spirit ceased operations during its fourth Martian winter, in 2010. Opportunity shows symptoms of aging, such as loss of motion in some joints, but continues to accomplish groundbreaking (Phys.org) —Approaching its 10th anniversary of exploration and science. leaving Earth, NASA's Mars Exploration Rover Opportunity is on the move again, trekking to a new study area still many weeks away. The destination, called "Solander Point," offers Opportunity access to a much taller stack of geological layering than the area where the rover has worked for the past 20 months, called "Cape York." Both areas are raised segments of the western rim of Endeavour Crater, which is about 14 miles (22 kilometers) in diameter.