Mapping the Mars Canal Mania: Cartographic Projection and the Creation of a Popular Icon
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Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
The Search for Extraterrestrial Intelligence
THE SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE Are we alone in the universe? Is the search for extraterrestrial intelligence a waste of resources or a genuine contribution to scientific research? And how should we communicate with other life-forms if we make contact? The search for extraterrestrial intelligence (SETI) has been given fresh impetus in recent years following developments in space science which go beyond speculation. The evidence that many stars are accompanied by planets; the detection of organic material in the circumstellar disks of which planets are created; and claims regarding microfossils on Martian meteorites have all led to many new empirical searches. Against the background of these dramatic new developments in science, The Search for Extraterrestrial Intelligence: a philosophical inquiry critically evaluates claims concerning the status of SETI as a genuine scientific research programme and examines the attempts to establish contact with other intelligent life-forms of the past thirty years. David Lamb also assesses competing theories on the origin of life on Earth, discoveries of ex-solar planets and proposals for space colonies as well as the technical and ethical issues bound up with them. Most importantly, he considers the benefits and drawbacks of communication with new life-forms: how we should communicate and whether we could. The Search for Extraterrestrial Intelligence is an important contribution to a field which until now has not been critically examined by philosophers. David Lamb argues that current searches should continue and that space exploration and SETI are essential aspects of the transformative nature of science. David Lamb is honorary Reader in Philosophy and Bioethics at the University of Birmingham. -
Planet Mars & Its Inhabitants,The
THE PLANET MARS AND ITS INHABITANTS BY EROS URIDES (A MARTIAN) DEDICATION To the millions of God's children on this earth enthralled in darkness, for whom the solicitude of the Father is now in evidence, this book is dedicated. May it be a beacon to light the way of weary searchers after TRUTH. One hemisphere of Mars showing the North Polar Cap and the main Canal System covering the planet. The many thousands of small lateral canals, radiating from the larger waterways, and which form an important part of the general plan, have been purposely omitted from the above to avoid confusion. The circular spots and dots are the principal reservoirs used for impounding water for use during the long Martian summer. The dark areas shown in the drawing are Mars ancient sea bottoms now covered with vegetation. It will be observed that most of the canals are double, paralleling each other at a distance of about seventy-five miles. Centers of population are not shown for the reason that space is not available on so small a drawing. The City of Urid is situated adjacent to the reservoir in the center of drawing, just north of the equator. CONTENTS Chapter I.-EROS URIDES, of the City of Urid, planet Mars, the Author, introduces himself and his book THE PLANET MARS AND ITS INHABITANTS. Chapter II.-He describes the Population Centers, Temperatures and Climate. The whole Planet is gridironed with Canals. (See Diagram.) Chapter III.-He gives a full description of the marvelous Martian Canal System. Chapter IV.-Planetary Economy. -
Workshop on Mars Telescopic Observations
WORKSHCPON MARS TELESCOPIC OBSERVATIONS 90' 180'-;~~~~~~------------------..~~------------~~----..~o~,· 270' LPI Technical Report Number 95-04 Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPIITR--95-04 WORKSHOP ON MARS TELESCOPIC OBSERVATIONS Edited by J. F. Bell III and J. E. Moersch Held at Cornell University, Ithaca, New York August 14-15, 1995 Sponsored by Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 95-04 LPIITR--95-04 Compiled in 1995 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may be cited as Bell J. F.III and Moersch J. E., eds. (1995) Workshop on Mars Telescopic Observations. LPI Tech. Rpt. 95-04, Lunar and Planetary Institute, Houston. 33 pp. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Mail order requestors will be invoiced for the cost ofshipping and handling. Cover: Orbits of Mars (outer ellipse) and Earth (inner ellipse) showing oppositions of the planet from 1954to 1999. From C. Aammarion (1954) The Flammarion Book ofAstronomy, Simon and Schuster, New York. LPl Technical Report 95-04 iii Introduction The Mars Telescopic Observations Workshop, held August 14-15, 1995, at Cornell University in Ithaca, New York, was organized and planned with two primary goals in mind: The first goal was to facilitate discussions among and between amateur and professional observers and to create a workshop environment fostering collaborations and comparisons within the Mars ob serving community. -
Global Spectral Classification of Martian Low-Albedo Regions with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) Data A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, E02004, doi:10.1029/2006JE002726, 2007 Global spectral classification of Martian low-albedo regions with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) data A. Deanne Rogers,1 Joshua L. Bandfield,2 and Philip R. Christensen2 Received 4 April 2006; revised 12 August 2006; accepted 13 September 2006; published 14 February 2007. [1] Martian low-albedo surfaces (defined here as surfaces with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) albedo values 0.15) were reexamined for regional variations in spectral response. Low-albedo regions exhibit spatially coherent variations in spectral character, which in this work are grouped into 11 representative spectral shapes. The use of these spectral shapes in modeling global surface emissivity results in refined distributions of previously determined global spectral unit types (Surface Types 1 and 2). Pure Type 2 surfaces are less extensive than previously thought, and are mostly confined to the northern lowlands. Regional-scale spectral variations are present within areas previously mapped as Surface Type 1 or as a mixture of the two surface types, suggesting variations in mineral abundance among basaltic units. For example, Syrtis Major, which was the Surface Type 1 type locality, is spectrally distinct from terrains that were also previously mapped as Type 1. A spectral difference also exists between southern and northern Acidalia Planitia, which may be due in part to a small amount of dust cover in southern Acidalia. Groups of these spectral shapes can be averaged to produce spectra that are similar to Surface Types 1 and 2, indicating that the originally derived surface types are representative of the average of all low-albedo regions. -
Science and Technology Briefings – No
Mars: A New Frontier for Space December Briefing ___ ___ 2018 8 Exploration? Summary Despite the presence of water in the form of ice on the surface and liquid water underground, life on Mars appears unlikely under the current conditions and if it exists at all, it will confined to areas deep underground. After 43 missions to the Red Planet, the most recent of which – InSight (NASA) – landed on 26 November 2018 with a seismometer developed by the French National Centre for Space Studies (Centre national d’études spatiales - CNES), humankind’s age-old dream of exploring Mars has become a credible, albeit complex and costly project. Terra americana, with 8 American successes in 17 attempted landings, the priority should still be given to robotic missions to Mars. Our participation in the European Space Agency (ESA) and our international cooperation agreements should consolidate Source: CNES France’s role as a space power. Ms Catherine Procaccia, Senator Travelling to Mars, an age-old dream… and their increasing accuracy made it clear that these Mars, the subject of intense observation and curiosity rectilinear canals were nothing more than optical since ancient times, especially for the Mesopotamian, illusions. The theory of life on Mars was also challenged Babylonian, Egyptian, Chinese and Greek civilisations, by the first spectroscopic analyses over a century ago (7) continues to inspire the general public and fascinate which demonstrated that Mars was uninhabitable. These scientists.(1) It takes its name from the Roman god of war, discoveries, made before the Space Age began, were due to its erratic movement as seen from the Earth and its subsequently enhanced and updated by advances made red colour, caused by the dust particles containing high possible by space telescopes, of which Hubble is a prime levels of iron oxides found on the planet’s surface layers. -
Martian Enigmas a Closer Look
THE Martian Enigmas A Closer Look ELECTRONIC EDITION by Mark J. Carlotto i Copyright © 2008 by Mark J. Carlotto All rights reserved ii With love to my family, especially my children, who are living in interesting times. iii iv Acknowledgments Thanks to Vince DiPietro and Greg Molenaar for finding the original image of the Face on Mars and for taking the time to look for that second image which NASA claimed didn't exist, to Dick Hoagland for recognizing the importance of their discovery, for his many contributions, and for organizing, along with Randy Pozos, the Independent Mars Investigation group. Thanks to Tom Rautenberg, a member of that group, for coming to Boston in the winter of 1985 with two Viking data tapes. During the next few years I spent many hours analyzing the imagery on those tapes. I am indebted to my former employer, TASC, for allowing me to work on this project after hours, and owe a great deal to my colleagues there for many fruitful discussions on image processing, shape- from-shading, and fractals. Thanks to Brian O'Leary who collaborated with me on the shape-from-shading analysis of the Face, and to Dan Drasin, who has been involved in the Mars investigation from the beginning, for his many contributions to the first edition of The Martian Enigmas. I would also like to thank Erol Torun for his contributions to the first edition of this book, Jim Erjavec and Ron Nicks for allowing me to include their work in the revised edition, and Ananda Sirisena and Chris O'Kane for their recent work in the U.K. -
Observations of Mars and Its Satellites by the Mars Imaging Camera (MIC) on Planet-B
Earth Planets Space, 50, 183–188, 1998 Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B Tadashi Mukai1, Tokuhide Akabane2, Tatsuaki Hashimoto3, Hiroshi Ishimoto1, Sho Sasaki4, Ai Inada1, Anthony Toigo5, Masato Nakamura6, Yutaka Abe6, Kei Kurita6, and Takeshi Imamura6 1The Graduate School of Science and Technology, Kobe University, Kobe 657-8501, Japan 2Hida Observatory, Kyoto University, Kamitakara, Gifu 506-13, Japan 3Institute of Space and Astronautical Science, Kanagawa 229-8510, Japan 4Geological Institute, University of Tokyo, Tokyo 113, Japan 5Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, U.S.A. 6Space and Planetary Science, University of Tokyo, Tokyo 113, Japan (Received August 7, 1997; Revised December 16, 1997; Accepted January 30, 1998) We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. -
The Demon Haunted World
THE DEMON- HAUNTED WORLD Science as a Candle in the Dark CARL SAGAN BALLANTINE BOOKS • NEW YORK Preface MY TEACHERS It was a blustery fall day in 1939. In the streets outside the apartment building, fallen leaves were swirling in little whirlwinds, each with a life of its own. It was good to be inside and warm and safe, with my mother preparing dinner in the next room. In our apartment there were no older kids who picked on you for no reason. Just the week be- fore, I had been in a fight—I can't remember, after all these years, who it was with; maybe it was Snoony Agata from the third floor— and, after a wild swing, I found I had put my fist through the plate glass window of Schechter's drug store. Mr. Schechter was solicitous: "It's all right, I'm insured," he said as he put some unbelievably painful antiseptic on my wrist. My mother took me to the doctor whose office was on the ground floor of our building. With a pair of tweezers, he pulled out a fragment of glass. Using needle and thread, he sewed two stitches. "Two stitches!" my father had repeated later that night. He knew about stitches, because he was a cutter in the garment industry; his job was to use a very scary power saw to cut out patterns—backs, say, or sleeves for ladies' coats and suits—from an enormous stack of cloth. Then the patterns were conveyed to endless rows of women sitting at sewing machines. -
The Sand Ships of Mars By: Jeffrey D
The Sand Ships of Mars By: Jeffrey D. Beish (Rev. 12-19-2018) INTRODUCTION It was Ray Bradbury who wrote of the "Sand Ships of Mars" in his science fiction novel, The Martian Chronicles (Bradbury, 1950). One can imagine the fictional inhabitants of Mars trekking across its deserts in their floating machines stirring up huge dust devils. This great science fiction story set the stage for this author’s interest in Mars and who now writes about similar accounts of the real dusty whirlwinds on the Red Planet. [NOTE: see Mars Chart in Reference section for location names]. One of the most spectacular events to watch in our Solar System is the development of a major Martian dust storm. From Earth a Martian dust cloud may seem to be just a nuisance to any would-be telescopic explorer on that planet. However, if you consider the actual size of these clouds then you suddenly realize that many of them would cover entire western United States! Imagine if a Mars-sized planet-encircling dust storm would occur on Earth; it would blank out most of an entire Hemisphere! Some would-be Mars experts claim that after dust storms the dust settles quickly to the surface and reduces contrast of albedo features. This is contrary to the known facts; dust remains in the atmosphere of Mars for weeks -- at times months -- before settling to the surface [Pollack, 1989], [Kahn, 1992]. This dust is very fine particles of volcanic ash and when raised aloft during these storms they reach heights of several kilometers. -
The Opposition of Mars, 1999
The opposition of Mars, 1999 Richard McKim A report of the Mars Section (Director: R. J. McKim) The 1999 martian apparition was followed by BAA members while Mars Global Surveyor was monitoring the planet from martian orbit. The planet’s surface showed little change from 1997, indicating the absence of any great dust storm since solar conjunction. The long period of telescopic coverage enabled us to conclude that neither was there any planet-encircling storm in the southern martian spring or summer in 1999−2000. Three small telescopic storms were followed along the Valles Marineris, and two were seen at the edge of the summer N. polar cap. Dust storms commencing at the historically rarely-active Margaritifer Sinus emergence site (MGS data) point to ongoing changes in the fallout pattern of atmospheric dust. White cloud activity was high before and around opposition time − in northern midsummer − with morning and evening limb hazes, the equatorial cloud band (ECB) and orographic clouds. The ECB ‘season’ was identical to 1997, pointing to an equally low level of atmospheric dust-loading. Comparison with historical records suggests that the seasonal ‘wave of darkening’ may be partly attributable to the annual disappearance of the ECB. A ‘polar cyclone’ imaged by the Hubble Space Telescope between Mare Acidalium and the northern cap was followed over several days. The seasonal behaviour of the NPC, including its transition to the polar hood, was well observed. Its recession (observed from northern mid-spring) was a little slower than usual. The formation of the SPC from its winter hood, and its early recession, was also recorded. -
Planets Solar System Paper Contents
Planets Solar system paper Contents 1 Jupiter 1 1.1 Structure ............................................... 1 1.1.1 Composition ......................................... 1 1.1.2 Mass and size ......................................... 2 1.1.3 Internal structure ....................................... 2 1.2 Atmosphere .............................................. 3 1.2.1 Cloud layers ......................................... 3 1.2.2 Great Red Spot and other vortices .............................. 4 1.3 Planetary rings ............................................ 4 1.4 Magnetosphere ............................................ 5 1.5 Orbit and rotation ........................................... 5 1.6 Observation .............................................. 6 1.7 Research and exploration ....................................... 6 1.7.1 Pre-telescopic research .................................... 6 1.7.2 Ground-based telescope research ............................... 7 1.7.3 Radiotelescope research ................................... 8 1.7.4 Exploration with space probes ................................ 8 1.8 Moons ................................................. 9 1.8.1 Galilean moons ........................................ 10 1.8.2 Classification of moons .................................... 10 1.9 Interaction with the Solar System ................................... 10 1.9.1 Impacts ............................................ 11 1.10 Possibility of life ........................................... 12 1.11 Mythology .............................................