We Can't Get Enough of the Red Planet
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VI FORSKER PÅ MARS Kort Om Aktiviteten I Mange Tiår Har Mars Vært Et Yndet Objekt for Forskere Verden Over
VI FORSKER PÅ MARS Kort om aktiviteten I mange tiår har Mars vært et yndet objekt for forskere verden over. Men hvorfor det? Hva er det med den røde planeten som er så interessant? Her forsøker vi å gi en oversikt over hvorfor vi er så opptatt av Mars. Hva har vi oppdaget, og hva er det vi tenker å gjøre? Det finnes en planet i solsystemet vårt som bare er bebodd av roboter -MARS- Læringsmål Elevene skal kunne - gi eksempler på dagsaktuell forskning og drøfte hvordan ny kunnskap genereres gjennom samarbeid og kritisk tilnærming til eksisterende kunnskap - utforske, forstå og lage teknologiske systemer som består av en sender og en mottaker - gjøre rede for energibevaring og energikvalitet og utforske ulike måter å omdanne, transportere og lagre energi på VI FORSKER PÅ MARS side 1 Innhold Kort om aktiviteten ................................................................................................................................ 1 Læringsmål ................................................................................................................................................ 1 Mars gjennom historien ...................................................................................................................... 3 Romkappløp mot Mars ................................................................................................................... 3 2000-tallet gir rovere i fleng ....................................................................................................... 4 Hva nå? ...................................................................................................................................................... -
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. -
Generate Viewsheds of Mastcam Images from the Curiosity Rover, Using Arcgis® and Public Datasets
TECHNICAL Coupling Mars Ground and Orbital Views: Generate REPORTS: METHODS Viewsheds of Mastcam Images From the Curiosity 10.1029/2020EA001247 Rover, Using ArcGIS® and Public Datasets Key Points: 1 2 1 3 4 • Mastcam images from the Curiosity M. Nachon , S. Borges , R. C. Ewing , F. Rivera‐Hernández , N. Stein , and rover are available online but lack a J. K. Van Beek5 public method to be placed back in the Mars orbital context 1Department of Geology and Geophysics, Texas A&M University, College Station, TX, USA, 2Department of Astronomy • This procedure allows users to and Planetary Sciences—College of Engineering, Forestry, and Natural Sciences, Northern Arizona University, Flagstaff, generate Mastcam image viewsheds: 3 4 locate in a map view the Mars AZ, USA, Department of Earth Sciences, Dartmouth College, Hanover, NH, USA, Division of Geological and Planetary 5 terrains visible in Mastcam images Sciences, California Institute of Technology, Pasadena, CA, USA, Malin Space Science Systems, San Diego, CA, USA • This procedure uses ArcGIS® and publicly available Mars datasets Abstract The Mastcam (Mast Camera) instrument onboard the NASA Curiosity rover provides an Supporting Information: exclusive view of Mars: High‐resolution color images from Mastcam allow users to study Gale crater's • Dataset S1 geologic terrains along Curiosity's path. These ground observations complement the spatially broader • Dataset S2 • Dataset S3 views of Gale crater provided by spacecrafts from orbit. However, for a given Mastcam image, it can be • Table S1 challenging to locate the corresponding terrains on the orbital view. No method for locating Mastcam images • Table S2 onto orbital images had been made publicly available. -
U.S. Postal Service Salutes Legendary Author Celebrating 100Th Anniversary of Edgar Rice Burroughs’ Creation of Tarzan
FOR IMMEDIATE RELEASE National Contact: Roy Betts August 16, 2012 [email protected] 202-268-3207 Local Contact: Richard Maher [email protected] 714-662-6350 usps.com/news Release No. 12-094 U.S. Postal Service Salutes Legendary Author Celebrating 100th anniversary of Edgar Rice Burroughs’ Creation of Tarzan To obtain a high-resolution image of the stamp for media use only, email [email protected]. TARZANA, CA — The U.S. Postal Service will honor tomorrow one of the most prolific authors of the early 20th century and inventor of the iconic character Tarzan with the issuance of the Edgar Rice Burroughs Forever Stamp. The stamp issuance coincides with the 100th anniversary of the publication of Burroughs’ first story, Under the Moons of Mars, and his first Tarzan story, Tarzan of the Apes, in 1912. The Edgar Rice Burroughs Forever Stamp will be dedicated tomorrow at 11:30 a.m. PT at the Tarzana Community and Cultural Center in Tarzana, CA, and will go on sale tomorrow at Post Offices nationwide, online at usps.com and by phone at 800-782-6724. Best known for inventing the legendary character Tarzan, Burroughs wrote more than 70 books, including historical fiction and several popular series of science fiction tales. “At the Postal Service, we’re proud to honor wonderful writers like Mr. Burroughs,” said Giselle Valera, vice president and managing director, Global Business. “These creative geniuses make lasting contributions to our cultural heritage, and we want more Americans to learn about them. Our stamp featuring Mr. -
General Vertical Files Anderson Reading Room Center for Southwest Research Zimmerman Library
“A” – biographical Abiquiu, NM GUIDE TO THE GENERAL VERTICAL FILES ANDERSON READING ROOM CENTER FOR SOUTHWEST RESEARCH ZIMMERMAN LIBRARY (See UNM Archives Vertical Files http://rmoa.unm.edu/docviewer.php?docId=nmuunmverticalfiles.xml) FOLDER HEADINGS “A” – biographical Alpha folders contain clippings about various misc. individuals, artists, writers, etc, whose names begin with “A.” Alpha folders exist for most letters of the alphabet. Abbey, Edward – author Abeita, Jim – artist – Navajo Abell, Bertha M. – first Anglo born near Albuquerque Abeyta / Abeita – biographical information of people with this surname Abeyta, Tony – painter - Navajo Abiquiu, NM – General – Catholic – Christ in the Desert Monastery – Dam and Reservoir Abo Pass - history. See also Salinas National Monument Abousleman – biographical information of people with this surname Afghanistan War – NM – See also Iraq War Abousleman – biographical information of people with this surname Abrams, Jonathan – art collector Abreu, Margaret Silva – author: Hispanic, folklore, foods Abruzzo, Ben – balloonist. See also Ballooning, Albuquerque Balloon Fiesta Acequias – ditches (canoas, ground wáter, surface wáter, puming, water rights (See also Land Grants; Rio Grande Valley; Water; and Santa Fe - Acequia Madre) Acequias – Albuquerque, map 2005-2006 – ditch system in city Acequias – Colorado (San Luis) Ackerman, Mae N. – Masonic leader Acoma Pueblo - Sky City. See also Indian gaming. See also Pueblos – General; and Onate, Juan de Acuff, Mark – newspaper editor – NM Independent and -
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. -
Habitability of Mars: How Welcoming Are the Surface and Subsurface to Life on the Red Planet?
geosciences Review Habitability of Mars: How Welcoming Are the Surface and Subsurface to Life on the Red Planet? Aleksandra Checinska Sielaff and Stephanie A. Smith * Youth and Families Program Unit, Washington State University, Pullman, WA 99163, USA * Correspondence: [email protected] Received: 31 July 2019; Accepted: 20 August 2019; Published: 22 August 2019 Abstract: Mars is a planet of great interest in the search for signatures of past or present life beyond Earth. The years of research, and more advanced instrumentation, have yielded a lot of evidence which may be considered by the scientific community as proof of past or present habitability of Mars. Recent discoveries including seasonal methane releases and a subglacial lake are exciting, yet challenging findings. Concurrently, laboratory and environmental studies on the limits of microbial life in extreme environments on Earth broaden our knowledge of the possibility of Mars habitability. In this review, we aim to: (1) Discuss the characteristics of the Martian surface and subsurface that may be conducive to habitability either in the past or at present; (2) discuss laboratory-based studies on Earth that provide us with discoveries on the limits of life; and (3) summarize the current state of knowledge in terms of direction for future research. Keywords: Mars; habitability; surface; subsurface; water; organics; methane; life; microorganisms; lichens; bryophytes 1. Introduction “The Earth remains the only inhabited world known so far, but scientists are finding that the universe -
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. -
ROVING ACROSS MARS: SEARCHING for EVIDENCE of FORMER HABITABLE ENVIRONMENTS Michael H
PERSPECTIVE ROVING ACROSS MARS: SEARCHING FOR EVIDENCE OF FORMER HABITABLE ENVIRONMENTS Michael H. Carr* My love affair with Mars started in the late 1960s when I was appointed a member of the Mariner 9 and Viking Orbiter imaging teams. The global surveys of these two missions revealed a geological wonderland in which many of the geological processes that operate here on Earth operate also on Mars, but on a grander scale. I was subsequently involved in almost every Mars mission, both US and non- US, through the early 2000s, and wrote several books on Mars, most recently The Surface of Mars (Carr 2006). I also participated extensively in NASA’s long-range strategic planning for Mars exploration, including assessment of the merits of various techniques, such as penetrators, Mars rovers showing their evolution from 1996 to the present day. FIGURE 1 balloons, airplanes, and rovers. I am, therefore, following the results In the foreground is the tethered rover, Sojourner, launched in 1996. On the left is a model of the rovers Spirit and Opportunity, launched in 2004. from Curiosity with considerable interest. On the right is Curiosity, launched in 2011. IMAGE CREDIT: NASA/JPL-CALTECH The six papers in this issue outline some of the fi ndings of the Mars rover Curiosity, which has spent the last two years on the Martian surface looking for evidence of past habitable conditions. It is not the fi rst rover to explore Mars, but it is by far the most capable (FIG. 1). modest-sized landed vehicles. Advances in guidance enabled landing Included on the vehicle are a number of cameras, an alpha particle at more interesting and promising places, and advances in robotics led X-ray spectrometer (APXS) for contact elemental composition, a spec- to vehicles with more independent capabilities. -
Mariner to Mercury, Venus and Mars
NASA Facts National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 Mariner to Mercury, Venus and Mars Between 1962 and late 1973, NASA’s Jet carry a host of scientific instruments. Some of the Propulsion Laboratory designed and built 10 space- instruments, such as cameras, would need to be point- craft named Mariner to explore the inner solar system ed at the target body it was studying. Other instru- -- visiting the planets Venus, Mars and Mercury for ments were non-directional and studied phenomena the first time, and returning to Venus and Mars for such as magnetic fields and charged particles. JPL additional close observations. The final mission in the engineers proposed to make the Mariners “three-axis- series, Mariner 10, flew past Venus before going on to stabilized,” meaning that unlike other space probes encounter Mercury, after which it returned to Mercury they would not spin. for a total of three flybys. The next-to-last, Mariner Each of the Mariner projects was designed to have 9, became the first ever to orbit another planet when two spacecraft launched on separate rockets, in case it rached Mars for about a year of mapping and mea- of difficulties with the nearly untried launch vehicles. surement. Mariner 1, Mariner 3, and Mariner 8 were in fact lost The Mariners were all relatively small robotic during launch, but their backups were successful. No explorers, each launched on an Atlas rocket with Mariners were lost in later flight to their destination either an Agena or Centaur upper-stage booster, and planets or before completing their scientific missions. -
Combinatorics in Space
Combinatorics in Space The Mariner 9 Telemetry System Mariner 9 Mission Launched: May 30, 1971 Arrived: Nov. 14, 1971 Turned Off: Oct. 27, 1972 Mission Objectives: (Mariner 8): Map 70% of Martian surface. (Mariner 9): Study temporal changes in Martian atmosphere and surface features. Live TV A black and white TV camera was used to broadcast “live” pictures of the Martian surface. Each photo-receptor in the camera measures the brightness of a section of the Martian surface about 4-5 km square, and outputs a grayness value in the range 0-63. This value is represented as a binary 6-tuple. The TV image is thus digitalized by the photo-receptor bank and is output as a stream of thousands of binary 6-tuples. Coding Needed Without coding and a failure probability p = 0.05, 26% of the image would be in error ... unacceptably poor quality for the nature of the mission. Any coding will increase the length of the transmitted message. Due to power constraints on board the probe and equipment constraints at the receiving stations on Earth, the coded message could not be much more than 5 times as long as the data. Thus, a 6-tuple of data could be coded as a codeword of about 30 bits in length. Other concerns A second concern involves the coding procedure. Storage of data requires shielding of the storage media – this is dead weight aboard the probe and economics require that there be little dead weight. Coding should therefore be done “on the fly”, without permanent memory requirements. -
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.