Modelling Cometary Meteoroid Stream
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Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
The Leadership Issue
SUMMER 2017 NON PROFIT ORG. U.S. POSTAGE PAID ROLAND PARK COUNTRY SCHOOL connections BALTIMORE, MD 5204 Roland Avenue THE MAGAZINE OF ROLAND PARK COUNTRY SCHOOL Baltimore, MD 21210 PERMIT NO. 3621 connections THE ROLAND PARK COUNTRY SCHOOL COUNTRY PARK ROLAND SUMMER 2017 LEADERSHIP ISSUE connections ROLAND AVE. TO WALL ST. PAGE 6 INNOVATION MASTER PAGE 12 WE ARE THE ROSES PAGE 16 ADENA TESTA FRIEDMAN, 1987 FROM THE HEAD OF SCHOOL Dear Roland Park Country School Community, Leadership. A cornerstone of our programming here at Roland Park Country School. Since we feel so passionately about this topic we thought it was fitting to commence our first themed issue of Connections around this important facet of our connections teaching and learning environment. In all divisions and across all ages here at Roland Park Country School — and life beyond From Roland Avenue to Wall Street graduation — leadership is one of the connecting, lasting 06 President and CEO of Nasdaq, Adena Testa Friedman, 1987 themes that spans the past, present, and future lives of our (cover) reflects on her time at RPCS community members. Joe LePain, Innovation Master The range of leadership experiences reflected in this issue of Get to know our new Director of Information and Innovation Connections indicates a key understanding we have about the 12 education we provide at RPCS: we are intentional about how we create leadership opportunities for our students of today — and We Are The Roses for the ever-changing world of tomorrow. We want our students 16 20 years. 163 Roses. One Dance. to have the skills they need to be successful in the future. -
Mars Mapping, Data Mining, Change Detection, GIS Mapping, Time Series Analysis
ISPRS Technical Commission IV Symposium on Geospatial Databases and Location Based Services, 14 – 16 May 2014, Suzhou, China, MTSTC4-2014-172-2 TEMPORAL ANALYSIS OF ALL AVAILABLE HIGH-RESOLUTION MARS IMAGING PRODUCTS SINCE 1976 Panagiotis Sidiropoulos1 and Jan-Peter Muller Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey, RH56NT, UK [email protected], [email protected] Commission KEY WORDS: Mars mapping, data mining, change detection, GIS mapping, time series analysis ABSTRACT: Starting from Viking Orbiter 1, launched in August 1975, several mainly NASA orbiters have been sent to Mars to accomplish the robotic tasks of imaging its surface. Initial analyses of these early images indicated a planet with similar characteristics to the Moon pitted with craters and large volcanic and tectonic features but dead from a geological perspective. Recently, scientific interest has shifted towards high-resolution imaging, which allows the identification of previously undiscovered geological phenomena and surface features as well as the examination of surface composition and geological history. The increasing frequency of Mars orbiters, carrying high-resolution cameras, allows the dynamic analysis of Martian surface, i.e. the analysis of the temporal evolution of certain areas that reveal natural processes that happen over time. The latter can be roughly classified into two major categories; processes that happen periodically each and every Martian season (e.g. seasonal flows in high latitude areas (McEwen et al., 2011) and events that do not follow some iterative pattern but are rather sporadic (e.g. new impact craters (Byrne et al., 2009)). Consequently, it is beneficial to conduct a twin temporal grouping of Mars imaging products, the first examining product distribution through time, so as to point out areas that favor the search for sporadic events, and the second product distribution per season, to identify areas favouring the search for periodic events. -
Comet Section Observing Guide
Comet Section Observing Guide 1 The British Astronomical Association Comet Section www.britastro.org/comet BAA Comet Section Observing Guide Front cover image: C/1995 O1 (Hale-Bopp) by Geoffrey Johnstone on 1997 April 10. Back cover image: C/2011 W3 (Lovejoy) by Lester Barnes on 2011 December 23. © The British Astronomical Association 2018 2018 December (rev 4) 2 CONTENTS 1 Foreword .................................................................................................................................. 6 2 An introduction to comets ......................................................................................................... 7 2.1 Anatomy and origins ............................................................................................................................ 7 2.2 Naming .............................................................................................................................................. 12 2.3 Comet orbits ...................................................................................................................................... 13 2.4 Orbit evolution .................................................................................................................................... 15 2.5 Magnitudes ........................................................................................................................................ 18 3 Basic visual observation ........................................................................................................ -
USBC Approved Bowling Balls
USBC Approved Bowling Balls (See rulebook, Chapter VII, "USBC Equipment Specifications" for any balls manufactured prior to January 1991.) ** Bowling balls manufactured only under 13 pounds. 5/17/2011 Brand Ball Name Date Approved 900 Global Awakening Jul-08 900 Global BAM Aug-07 900 Global Bank Jun-10 900 Global Bank Pearl Jan-11 900 Global Bounty Oct-08 900 Global Bounty Hunter Jun-09 900 Global Bounty Hunter Black Jan-10 900 Global Bounty Hunter Black/Purple Feb-10 900 Global Bounty Hunter Pearl Oct-09 900 Global Break Out Dec-09 900 Global Break Pearl Jan-08 900 Global Break Point Feb-09 900 Global Break Point Pearl Jun-09 900 Global Creature Aug-07 900 Global Creature Pearl Feb-08 900 Global Day Break Jun-09 900 Global DVA Open Aug-07 900 Global Earth Ball Aug-07 900 Global Favorite May-10 900 Global Head Hunter Jul-09 900 Global Hook Dark Blue/Light Blue Feb-11 900 Global Hook Purple/Orange Pearl Feb-11 900 Global Hook Red/Yellow Solid Feb-11 900 Global Integral Break Black Nov-10 900 Global Integral Break Rose/Orange Nov-10 900 Global Integral Break Rose/Silver Nov-10 900 Global Link Jul-08 900 Global Link Black/Red Feb-09 900 Global Link Purple/Blue Pearl Dec-08 900 Global Link Rose/White Feb-09 900 Global Longshot Jul-10 900 Global Lunatic Jun-09 900 Global Mach One Blackberry Pearl Sep-10 900 Global Mach One Rose/Purple Pearl Sep-10 900 Global Maniac Oct-08 900 Global Mark Roth Ball Jan-10 900 Global Missing Link Black/Red Jul-10 900 Global Missing Link Blackberry/Silver Jul-10 900 Global Missing Link Blue/White Jul-10 900 Global -
Ancient Fluid Escape and Related Features in Equatorial Arabia Terra (Mars)
EPSC Abstracts Vol. 7 EPSC2012-132-3 2012 European Planetary Science Congress 2012 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2012 Ancient fluid escape and related features in equatorial Arabia Terra (Mars) F. Franchi(1), A. P. Rossi(2), M. Pondrelli(3), B. Cavalazzi(1), R. Barbieri(1), Dipartimento di Scienze della Terra e Geologico Ambientali, Università di Bologna, via Zamboni 67, 40129 Bologna, Italy ([email protected]). 2Jacobs University, Bremen, Germany. 3IRSPS, Università D’Annunzio, Pescara, Italy. Abstract Noachian [1]. The ELDs are composed by light rocks showing a polygonal pattern, described elsewhere on Arabia Terra, in the equatorial region of Mars, is Mars [4], and is characterized by a high sinuosity of long-time studied area especially for the abundance the strata that locally follows a concentric trend of fluid related features. Detailed stratigraphic and informally called “pool and rim” structures (Fig. morphological study of the succession exposed in the 1A). Crommelin and Firsoff craters evidenced the occurrences of flow structures and spring deposits that endorse the presence of fluids circulation in the Late Noachian. All the morphologies in these two proto-basins occur within the Equatorial Layered Deposits (ELDs). 1. Introduction Martian layered spring deposits are of considerable interest for their supposed relationship with water and high potential of microbial signatures preservation. Their supposed fluid-related origin [1] makes the Equatorial Layered Deposits attractive targets for future missions with astrobiological purposes. In this study we report the occurrence of mounds fields and flow structures in Firsoff and Crommelin craters and summarize the result of a detailed study of the remote-sensing data sets available in this region. -
The First Complete Genome Sequences of the Aci Lineage, the Most
www.nature.com/scientificreports OPEN The first complete genome sequences of the acI lineage, the most abundant freshwater Received: 10 June 2016 Accepted: 06 January 2017 Actinobacteria, obtained by whole- Published: 10 February 2017 genome-amplification of dilution- to-extinction cultures Ilnam Kang, Suhyun Kim, Md. Rashedul Islam & Jang-Cheon Cho The acI lineage of the phylum Actinobacteria is the most abundant bacterial group in most freshwater lakes. However, due to difficulties in laboratory cultivation, only two mixed cultures and some incomplete single-amplified or metagenome-derived genomes have been reported for the lineage. Here, we report the initial cultivation and complete genome sequences of four novel strains of the acI lineage from the tribes acI-A1, -A4, -A7, and -C1. The acI strains, initially isolated by dilution-to- extinction culturing, eventually failed to be maintained as axenic cultures. However, the first complete genomes of the acI lineage were successfully obtained from these initial cultures through whole genome amplification applied to more than hundreds of cultured acI cells. The genome sequences exhibited features of genome streamlining and showed that the strains are aerobic chemoheterotrophs sharing central metabolic pathways, with some differences among tribes that may underlie niche diversification within the acI lineage. Actinorhodopsin was found in all strains, but retinal biosynthesis was complete in only A1 and A4 tribes. Considering the influence of inland waters on global climate change1,2 and the essential roles of microbes in biogeochemical processes3, studies on major bacterial groups in freshwater environments are important. The acI lineage of the phylum Actinobacteria, comprised of ~13 tribes belonging to acI-A, -B, or -C sublineages, repre- sents one of the most widespread and abundant bacterial groups in freshwater environments4,5. -
Meteor- Scatter
Catch a Falling Star A beginner’s guide to meteor-scatter communication— just in time for “stormy” weather! By Kirk Kleinschmidt, NT0Z Newcomers to Amateur Radio usually have a few misconceptions about VHF propagation. The worst—which is often “propagated” by more experienced hams who should know better—suggests that VHF signals travel exclusively along line-of-sight paths and peter out after about 30 miles. That’s far from true, but if your VHF operation is limited to 2-meter FM it’s somehow practical, especially if you’re using a hand-held radio and a rubber ducky antenna. Once you cross the “30-mile barrier,” however, there are many exciting and interesting ways to propagate your VHF signal hundreds or even thousands of kilometers. Articles in the ARRL Operating Manual and QST detail E- and F-layer skip, tropospheric ducting and transequatorial field-aligned irregularities, moon-bounce, auroral propagation and others. These modes aren’t always casual. That is, many require robust stations, high power and more than a little patience. Meteor- scatter work—bouncing radio signals off the ionized trails produced by meteors burning through the ionosphere—doesn’t require an extraordinary station, but some patience is usually necessary unless you know exactly when conditions may be favorable! That’s precisely the case with the November Leonids meteor showers for the next few years. (Meteor showers are named for the constellations from which they seem to appear. Meteors produced during the recurring November 17 shower seem to “pour” from the constellation Leo.) As an added bonus, on one or more of those November days the short-duration, high-intensity Leonids have the potential to produce the best meteor-scatter propagation since November 1966 (and a spectacular light show if you’re on the night side of the planet!). -
Comet Prospects for 2017
Comet Prospects for 2017 February could be a busy month with the possibility of three periodic comets visible in binoculars. Three comets in parabolic orbits may also become visible in binoculars. These predictions focus on comets that are likely to be within range of visual observers, though comets often do not behave as expected and can spring surprises. Members are encouraged to make visual magnitude estimates, particularly of periodic comets, as long term monitoring over many returns helps understand their evolution. Please submit your magnitude estimates in ICQ format. Guidance on visual observation and how to submit estimates is given in the BAA Observing Guide to Comets. Drawings are also useful, as the human eye can sometimes discern features that initially elude electronic devices. Theories on the structure of comets suggest that any comet could fragment at any time, so it is worth keeping an eye on some of the fainter comets, which are often ignored. They would make useful targets for those making electronic observations, especially those with time on instruments such as the Faulkes telescopes. Such observers are encouraged to report electronic visual equivalent magnitude estimates via COBS. When possible use a waveband approximating to Visual or V magnitudes. These estimates can be used to extend the visual light curves, and hence derive more accurate absolute magnitudes. Such observations of periodic comets are particularly valuable as observations over many returns allow investigation into the evolution of comets. In addition to the information in the BAA Handbook and on the Section web pages, ephemerides for the brighter observable comets are published in the Circulars, and ephemerides for new and currently observable comets are on the JPL, CBAT and Seiichi Yoshida's web pages. -
Explanatory Supplement
The Herschel Catalogue of Solar System Object Observations - Explanatory Supplement Volume I The Herschel-PACS Solar System Object Observations Comet Catalogue HERSCHEL-HSC-DOC-2200 Version: 1.0 25th July 2018 The Herschel Catalogue of Solar System Object Observations - Explanatory Supplement Volume I: Herschel-PACS Solar System Object Observations Comet Catalogue Prepared by: Cristina Romero Calvo1, 2, Mark Kidger1, Miriam Rengel1, 3, 4 and Mircea Stoica5 1. Herschel Science Centre, European Space Agency, European Space Astronomy Centre 2. Technische Universität Berlin, Germany 3. Max-Planck-Institut für Sonnensystemforschung, Germany 4. European Organisation for the Exploitation of Meteorological Satellites, Germany 5. University Medical Center Hamburg-Eppendorf, Department of Neurophysiology and Pathophysiology, Hamburg, Germany HERSCHEL-HSC-DOC-2200, Version: 1.0, 25th July 2018 1. Abstract We present the first volume of the Herschel Catalogue of Solar System Object Observations (HCSSO). This has been prepared as a complement to the two catalogues of Herschel point source observations: The Herschel/SPIRE Point Source Catalogue (HSPSC) and the Herschel/PACS Point Source Catalogue (HPPSC), which filter and exclude moving targets. Although most of the solar system objects observed by Herschel were inactive, point sources, ten active comets were also observed, mainly at 70 and 160 μm, several of them at more than one epoch, although there were also a few observations at 100 μm. Both short period, Jupiter Family comets, mainly making close passes to Earth and non-periodic objects were observed by PACS. The resultant sample covers a variety of objects with a wide range of dynamical history and level of activity: five Jupiter family objects, and five non-periodic objects. -
1 Fluids Mobilization in Arabia Terra, Mars
Fluids mobilization in Arabia Terra, Mars: depth of pressurized reservoir from mounds self- similar clustering Riccardo Pozzobon1, Francesco Mazzarini2, Matteo Massironi1, Angelo Pio Rossi3, Monica Pondrelli4, Gabriele Cremonese5, Lucia Marinangeli6 1 Department of Geosciences, Università degli Studi di Padova, Via Gradenigo 6 - 35131, Padova, Italy 2 Istituto Nazionale di Geofisica e Vulcanologia (INGV), Via Della Faggiola, 32 - 56100 Pisa, Italy 3 Department of Physics and Earth Sciences, Jacobs University Bremen, Campus Ring 1 -28759 Bremen, Germany 4 International Research School of Planetary Sciences, Università d'Annunzio, viale Pindaro 42 – 65127, Pescara, Italy 5 INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5 - 35122, Padova, Italy 6 Laboratorio di Telerilevamento e Planetologia, DISPUTer, Universita' G. d'Annunzio, Via Vestini 31 - 66013 Chieti, Italy Abstract Arabia Terra is a region of Mars where signs of past-water occurrence are recorded in several landforms. Broad and local scale geomorphological, compositional and hydrological analyses point towards pervasive fluid circulation through time. In this work we focus on mound fields located in the interior of three casters larger than 40 km (Firsoff, Kotido and unnamed crater 20 km to the east) and showing strong morphological and textural resemblance to terrestrial mud volcanoes and spring-related features. We infer that these landforms likely testify the presence of a pressurized fluid reservoir at depth and past fluid upwelling. We have performed morphometric analyses to characterize the mound morphologies and consequently retrieve an accurate automated mapping of the mounds within the craters for spatial distribution and fractal clustering analysis. The outcome of the fractal clustering yields information about the possible extent of the percolating fracture network at depth below the craters. -
On the Materials Science of Nature's Arms Race
PROGRESS REPORT Natural Defense www.advmat.de On the Materials Science of Nature’s Arms Race Zengqian Liu, Zhefeng Zhang,* and Robert O. Ritchie* materials created by Nature, as opposed to Biological material systems have evolved unique combinations of mechanical “traditional” man-made solids. Extensive properties to fulfill their specific function through a series of ingenious research efforts have been directed to such designs. Seeking lessons from Nature by replicating the underlying principles materials, with emphasis on bamboo,[4,5] [6–8] [9–15] [16–21] of such biological materials offers new promise for creating unique combi- trees, mollusks, arthropods, birds,[22–27] fish,[28–34] mammals,[35–43] and nations of properties in man-made systems. One case in point is Nature’s human beings,[44–53] motivated not only means of attack and defense. During the long-term evolutionary “arms race,” by their unique structures and properties/ naturally evolved weapons have achieved exceptional mechanical efficiency functionalities, but also by the salient with a synergy of effective offense and persistence—two characteristics that mechanisms and underlying design prin- often tend to be mutually exclusive in many synthetic systems—which may ciples that account for their long-term perfection. present a notable source of new materials science knowledge and inspiration. Biological systems represent how a This review categorizes Nature’s weapons into ten distinct groups, and dis- wide diversity of generally composite cusses the unique structural and mechanical designs of each group by taking materials can be developed to best fulfill representative systems as examples. The approach described is to extract their specific demands using a fairly small the common principles underlying such designs that could be translated palette of chemical constituents, often into man-made materials.