Selection of Processing Tomato Genotypes Resistant to Two Spotted Spider Mite
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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. -
Low Resolution
No. 102 June 2021 IAMGIAMG NewsletterNewsletter Official Newsletter of the International Association for Mathematical Geosciences Contents ith the Covid-19 pandemic Wfar from over, most Announcement of the 2021 IAmG AwArds ......................... 1 scientific meetings have been PresIdent’s forum .............................................................. 3 postponed or converted to a member news ...................................................................... 3 digital format. While there are nomInAtIons for IAmG AwArds ........................................... 3 certainly benefits to online meetings (I definitely don’t miss multiple memorAndum wIth codA AssocIAtIon ................................ 3 flights each way and jetlag) they tend reseArch center for solId eArth bIG dAtA to lose the personal interactions. It founded At the chInA unIversIty of GeoscIences ........... 4 is difficult for an online conference rememberInG dr. Peter fox - A tItAn In the eArth to replicate the conversations in the scIence InformAtIcs communIty ........................................ 4 hallways between sessions or during a meal that can bring a community Ieee GeoscIence And remote sensInG socIety (Grss) dIs- together and build new connections and tInGuIshed lecturer (dl) ............................................. 4 ideas. If you have any ideas or examples Professor noel cressIe nAmed A fellow of the of how the IAMG could work to bring the royAl socIety of new south Wales................................... 4 community together, please -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
In Pdf Format
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Ceres: Astrobiological Target and Possible Ocean World
ASTROBIOLOGY Volume 20 Number 2, 2020 Research Article ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2018.1999 Ceres: Astrobiological Target and Possible Ocean World Julie C. Castillo-Rogez,1 Marc Neveu,2,3 Jennifer E.C. Scully,1 Christopher H. House,4 Lynnae C. Quick,2 Alexis Bouquet,5 Kelly Miller,6 Michael Bland,7 Maria Cristina De Sanctis,8 Anton Ermakov,1 Amanda R. Hendrix,9 Thomas H. Prettyman,9 Carol A. Raymond,1 Christopher T. Russell,10 Brent E. Sherwood,11 and Edward Young10 Abstract Ceres, the most water-rich body in the inner solar system after Earth, has recently been recognized to have astrobiological importance. Chemical and physical measurements obtained by the Dawn mission enabled the quantification of key parameters, which helped to constrain the habitability of the inner solar system’s only dwarf planet. The surface chemistry and internal structure of Ceres testify to a protracted history of reactions between liquid water, rock, and likely organic compounds. We review the clues on chemical composition, temperature, and prospects for long-term occurrence of liquid and chemical gradients. Comparisons with giant planet satellites indicate similarities both from a chemical evolution standpoint and in the physical mechanisms driving Ceres’ internal evolution. Key Words: Ceres—Ocean world—Astrobiology—Dawn mission. Astro- biology 20, xxx–xxx. 1. Introduction these bodies, that is, their potential to produce and maintain an environment favorable to life. The purpose of this article arge water-rich bodies, such as the icy moons, are is to assess Ceres’ habitability potential along the same lines Lbelieved to have hosted deep oceans for at least part of and use observational constraints returned by the Dawn their histories and possibly until present (e.g., Consolmagno mission and theoretical considerations. -
Ebook < Impact Craters on Mars # Download
7QJ1F2HIVR # Impact craters on Mars « Doc Impact craters on Mars By - Reference Series Books LLC Mrz 2012, 2012. Taschenbuch. Book Condition: Neu. 254x192x10 mm. This item is printed on demand - Print on Demand Neuware - Source: Wikipedia. Pages: 50. Chapters: List of craters on Mars: A-L, List of craters on Mars: M-Z, Ross Crater, Hellas Planitia, Victoria, Endurance, Eberswalde, Eagle, Endeavour, Gusev, Mariner, Hale, Tooting, Zunil, Yuty, Miyamoto, Holden, Oudemans, Lyot, Becquerel, Aram Chaos, Nicholson, Columbus, Henry, Erebus, Schiaparelli, Jezero, Bonneville, Gale, Rampart crater, Ptolemaeus, Nereus, Zumba, Huygens, Moreux, Galle, Antoniadi, Vostok, Wislicenus, Penticton, Russell, Tikhonravov, Newton, Dinorwic, Airy-0, Mojave, Virrat, Vernal, Koga, Secchi, Pedestal crater, Beagle, List of catenae on Mars, Santa Maria, Denning, Caxias, Sripur, Llanesco, Tugaske, Heimdal, Nhill, Beer, Brashear Crater, Cassini, Mädler, Terby, Vishniac, Asimov, Emma Dean, Iazu, Lomonosov, Fram, Lowell, Ritchey, Dawes, Atlantis basin, Bouguer Crater, Hutton, Reuyl, Porter, Molesworth, Cerulli, Heinlein, Lockyer, Kepler, Kunowsky, Milankovic, Korolev, Canso, Herschel, Escalante, Proctor, Davies, Boeddicker, Flaugergues, Persbo, Crivitz, Saheki, Crommlin, Sibu, Bernard, Gold, Kinkora, Trouvelot, Orson Welles, Dromore, Philips, Tractus Catena, Lod, Bok, Stokes, Pickering, Eddie, Curie, Bonestell, Hartwig, Schaeberle, Bond, Pettit, Fesenkov, Púnsk, Dejnev, Maunder, Mohawk, Green, Tycho Brahe, Arandas, Pangboche, Arago, Semeykin, Pasteur, Rabe, Sagan, Thira, Gilbert, Arkhangelsky, Burroughs, Kaiser, Spallanzani, Galdakao, Baltisk, Bacolor, Timbuktu,... READ ONLINE [ 7.66 MB ] Reviews If you need to adding benefit, a must buy book. Better then never, though i am quite late in start reading this one. I discovered this publication from my i and dad advised this pdf to find out. -- Mrs. Glenda Rodriguez A brand new e-book with a new viewpoint. -
Global Challenges
6–10 JANUARY 2020 | ORLANDO, FL DRIVING AEROSPACE SOLUTIONS FOR GLOBAL CHALLENGES What’s going on in Page 25 aiaa.org/scitech #aiaaSciTech From the forefront of innovation to the frontlines of the mission. No matter the mission, Lockheed Martin uses a proven approach: engineer with purpose, innovate with passion and define the future. We take time to understand our customer’s challenges and provide solutions that help them keep the world secure. Their mission defines our purpose. Learn more at lockheedmartin.com. © 2019 Lockheed Martin Corporation FG19-23960_002 AIAA sponsorship.indd 1 12/10/19 3:20 PM Live: n/a Trim: H: 8.5in W: 11in Job Number: FG18-23208_002 Bleed: .25 all around Designer: Kevin Gray Publication: AIAA Sponsorship Gutter: None Communicator: Ryan Alford Visual: Male and female in front of screens. Resolution: 300 DPI Due Date: 12/10/19 Country: USA Density: 300 Color Space: CMYK NETWORK NAME: SciTech ON-SITE Wi-Fi From the forefront of innovation › PASSWORD: 2020scitech to the frontlines of the mission. CONTENTS Technical Program Committee .................................................................4 Welcome ........................................................................................................5 Sponsors and Supporters ..........................................................................7 Forum Overview ...........................................................................................8 Pre-Forum Activities ................................................................................. -
Charted Lakes List
LAKE LIST United States and Canada Bull Shoals, Marion (AR), HD Powell, Coconino (AZ), HD Gull, Mono Baxter (AR), Taney (MO), Garfield (UT), Kane (UT), San H. V. Eastman, Madera Ozark (MO) Juan (UT) Harry L. Englebright, Yuba, Chanute, Sharp Saguaro, Maricopa HD Nevada Chicot, Chicot HD Soldier Annex, Coconino Havasu, Mohave (AZ), La Paz HD UNITED STATES Coronado, Saline St. Clair, Pinal (AZ), San Bernardino (CA) Cortez, Garland Sunrise, Apache Hell Hole Reservoir, Placer Cox Creek, Grant Theodore Roosevelt, Gila HD Henshaw, San Diego HD ALABAMA Crown, Izard Topock Marsh, Mohave Hensley, Madera Dardanelle, Pope HD Upper Mary, Coconino Huntington, Fresno De Gray, Clark HD Icehouse Reservior, El Dorado Bankhead, Tuscaloosa HD Indian Creek Reservoir, Barbour County, Barbour De Queen, Sevier CALIFORNIA Alpine Big Creek, Mobile HD DeSoto, Garland Diamond, Izard Indian Valley Reservoir, Lake Catoma, Cullman Isabella, Kern HD Cedar Creek, Franklin Erling, Lafayette Almaden Reservoir, Santa Jackson Meadows Reservoir, Clay County, Clay Fayetteville, Washington Clara Sierra, Nevada Demopolis, Marengo HD Gillham, Howard Almanor, Plumas HD Jenkinson, El Dorado Gantt, Covington HD Greers Ferry, Cleburne HD Amador, Amador HD Greeson, Pike HD Jennings, San Diego Guntersville, Marshall HD Antelope, Plumas Hamilton, Garland HD Kaweah, Tulare HD H. Neely Henry, Calhoun, St. HD Arrowhead, Crow Wing HD Lake of the Pines, Nevada Clair, Etowah Hinkle, Scott Barrett, San Diego Lewiston, Trinity Holt Reservoir, Tuscaloosa HD Maumelle, Pulaski HD Bear Reservoir, -
CITY MANAGER CITY of CAPE Co~
CITY MANAGER CITY OF CAPE co~. DEPARTMENT OF COMMUNITY D~~~aPMi=tfff 3: ftO MEMORANDUM TO: John Szerlag, City Manager FROM: Vincent A. Cautero, Community Develop~-n~.t Director{!t';)\__, Robert H. Pederson, Planning Manager~ Wyatt Daltry, Planning Team Coordinator vl> DATE: September 6, 2016 SUBJECT: Future Land Use Map Amendment Request-LU16-0012 The City has initiated a large scale future land use map amendment for a large area in Northern Cape Coral; the proposed area is 2,818.49 acres. This request is a follow-up to LU15-0004, which brought over 4,000-acres from the Urban Services Reserve Area into the Urban Services Transition Area. Once the amendment is adopted by Council, property owners could rezone their property for development to permit densities supported by centralized water and sewer utilities. The proposed amendment request includes the following: Current FLU Proposed FLU Acreage Single Family/Multi-Family by PDP (SM) SinQle-Family Residential (SF) 2,686.04 SM Multi-Family Residential (MF) 63.16 SM Parks and Recreation (PK) 10.24 Commercial Activity Center (CAC) SF 29.39 CAC MF 29.66 Thank you for your consideration of this future land use map amendment. Please contact Wyatt Daltry, Planning Team Coordinator, at 573-3160 if you have any questions. VAC/wad(North1 +2FLUMAmemoofintent) Attachment Planning Division Case Report LU 16-0012 Review Date: November 2, 2016 Applicant: City of Cape Coral, Department of Community Development Property Owners: See Attachment A Site Address: See Attachment A Authorized Representative: Wyatt Daltry, AICP Planning Team Coordinator City of Cape Coral Department of Community Development (239) 573-3160 Case Staff: Wyatt Daltry, AICP, Planning Team Coordinator Review Approved By: Robert Pederson, AICP, Planning Manager Purpose: The City has initiated this large-scale future land use map amendment for a large area in Northern Cape Coral. -
On the Chronostratigraphy of Planetary Satellites and Asteroids
On the Chronostratigraphy of Planetary Satellites and Asteroids Absolute Surface Age Determination of Small Planetary Bodies: Scaling the Lunar Crater Chronology System vorgelegt von Dipl.‐Geol. Nico Schmedemann Fachbereich Geowissenschaften Freie Universität Berlin Dissertation zur Erlangung des Grades Doktor der Naturwissenschaften (Dr. rer. nat.) Berlin, im Juli 2015 Hauptgutachter: Prof. Dr. R. Jaumann Freie Universität Berlin Institut für Geologische Wissenschaften Fachrichtung Planetologie und Fernerkundung und Deutsches Zentrum für Luft- und Raumfahrt Institut für Planetenforschung, Abt. Planetengeologie Zweitgutachter: Prof. Dr. S. v. Gasselt Freie Universität Berlin Institut für Geologische Wissenschaften Fachrichtung Planetologie und Fernerkundung Tag der Disputation: 1. Dezember 2015 Eidesstattliche Erklärung Hiermit versichere ich, die vorliegende Arbeit selbstständig angefertigt und keine anderen als die angegebenen Quellen und Hilfsmittel benutzt zu haben. Berlin, 2015 Danksagung Großer Dank gebührt dem zwischenzeitlich leider verstorbenen Herrn Prof. Dr. Gerhard Neukum (FU-Berlin) für die Vergabe des Themas und der damit verbundenen Einstellung als Wissenschaftlicher Mitarbeiter in der Fachrichtung Planetologie an der Freien Universität Berlin. Durch seine Beteiligung an zahlreichen aktiven Raumfahrtmissionen ergab sich für mich die Möglichkeit mit bisher unveröffentlichten Daten in den Projekten Cassini und Dawn zu arbeiten. Er hat mich oft dazu ermuntert neue Ideen im Detail an den vorhandenen Daten zu testen, mit früheren Ergebnissen zu vergleichen und dabei das große Bild nicht aus den Augen zu verlieren. Er bestand zudem auch auf starke Präsenz bei internationalen Konferenzen, die einen angeregten Gedankenaustausch mit anderen Fachkollegen ermöglichten, die oft auch grundsätzlich andere Ansichten vertreten haben. Da Herr Prof. Dr. Neukum meine Arbeit nicht mehr betreuen kann, möchte ich mich bei Herrn Prof. -
Astrobiology at APL—On the Path to Discovery
K. L. Craft et al. Astrobiology at APL—On the Path to Discovery Kathleen L. Craft, Jorge I. Núñez, Christopher E. Bradburne, Carolyn M. Ernst, Charles A. Hibbitts, Noam R. Izenberg, Jeffrey R. Johnson, Shannon M. MacKenzie, Kathleen E. Mandt, Scott L. Murchie, Korine A. Ohiri, Mark E. Perry, Leif E. Powers, Kirby D. Runyon, Abigal M. Rymer, Frank P. Seelos, Kristin S. Sotzen, Kevin B. Stevenson, Collin M. Timm, Christina E. Viviano, and Joseph H. Westlake ABSTRACT Astrobiology is an exciting field of science focused on understanding the origins, evolution, distri- bution, and future of life in the universe. NASA focuses much of its research and technology devel- opments on astrobiology, and the Johns Hopkins University Applied Physics Laboratory (APL) is a major contributor through research, technology, and missions. Astrobiology efforts at APL range from constraining when life first emerged on Earth and researching biosignature (i.e., signals of past or present life) preservation, to developing instruments and missions aiming to detect biosig- natures and characterize the capability of an extreme planetary environment to harbor and sup- port life. Beginning with APL’s Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on the Mars Reconnaissance Orbiter (MRO), which searches for past wet and potentially habit- able regions on Mars, APL has continued to develop cutting-edge techniques and instruments to search for biosignatures, remotely and in situ. Additionally, APL is leading and serving as a key partner in several exciting NASA missions that will occur in the coming decades with habitability and biosignature detection goals. In this article, we summarize current efforts and look forward, over the coming 25 years, to the potential astrobiology exploration and discoveries that await. -
Titan As Revealed by the Cassini Radar
Space Sci Rev (2019) 215:33 https://doi.org/10.1007/s11214-019-0598-6 Titan as Revealed by the Cassini Radar R.M.C. Lopes1 · S.D. Wall1 · C. Elachi2 · S.P.D. Birch3 · P. Corlies3 · A. Coustenis4 · A.G. Hayes3 · J.D. Hofgartner1 · M.A. Janssen1 · R.L. Kirk5 · A. LeGall6 · R.D. Lorenz7 · J.I. Lunine2,3 · M.J. Malaska1 · M. Mastroguiseppe8 · G. Mitri9 · C.D. Neish10 · C. Notarnicola11 · F. Paganelli12 · P. Paillou13 · V. Poggiali3 · J. Radebaugh14 · S. Rodriguez15 · A. Schoenfeld16 · J.M. Soderblom17 · A. Solomonidou18 · E.R. Stofan19 · B.W. Stiles1 · F. Tosi 20 · E.P. Turtle7 · R.D. West1 · C.A. Wood21 · H.A. Zebker22 · J.W. Barnes23 · D. Casarano24 · P. Encrenaz4 · T. Farr1 · C. Grima25 · D. Hemingway26 · O. Karatekin27 · A. Lucas28 · K.L. Mitchell1 · G. Ori9 · R. Orosei29 · P. Ries 1 · D. Riccio30 · L.A. Soderblom5 · Z. Zhang2 Received: 13 July 2018 / Accepted: 27 April 2019 / Published online: 21 May 2019 © Springer Nature B.V. 2019 Abstract Titan was a mostly unknown world prior to the Cassini spacecraft’s arrival in July 2004. We review the major scientific advances made by Cassini’s Titan Radar Map- per (RADAR) during 13 years of Cassini’s exploration of Saturn and its moons. RADAR measurements revealed Titan’s surface geology, observed lakes and seas of mostly liquid methane in the polar regions, measured the depth of several lakes and seas, detected tempo- ral changes on its surface, and provided key evidence that Titan contains an interior ocean. B R.M.C. Lopes 1 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 2 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA 3 Department of Astronomy, Cornell University, Ithaca, NY 14853, USA 4 LESIA – Observatoire de Paris, CNRS, UPMC Univ.