1 the Martian Near Surface

Total Page:16

File Type:pdf, Size:1020Kb

1 the Martian Near Surface The Martian Near Surface Environment: Analysis of Antarctic Soils and Laboratory Experiments on Putative Martian Organics Item Type text; Electronic Dissertation Authors Archer, Paul Douglas Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 07/10/2021 13:24:53 Link to Item http://hdl.handle.net/10150/195892 1 THE MARTIAN NEAR SURFACE ENVIRONMENT: ANALYSIS OF ANTARCTIC SOILS AND LABORATORY EXPERIMENTS ON PUTATIVE MARTIAN ORGANICS by Paul Douglas Archer, Jr. _____________________ A Dissertation Submitted to the Faculty of the DEPARTMENT OF PLANETARY SCIENCES In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 2010 2 THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE As members of the Dissertation Committee, we certify that we have read the dissertation prepared by Paul Douglas Archer, Jr. entitled The Martian Near Surface Environment: Analysis of Antarctic Soils and Laboratory Experiments on Putative Martian Organics and recommend that it be accepted as fulfilling the dissertation requirement for the Degree of Doctor of Philosophy _______________________________________________________________________ Date: April 22, 2010 Peter H. Smith _______________________________________________________________________ Date: April 22, 2010 Mark A. Smith _______________________________________________________________________ Date: April 22, 2010 William V. Boynton _______________________________________________________________________ Date: April 22, 2010 Victor R. Baker _______________________________________________________________________ Date: April 22, 2010 Shane Byrne Final approval and acceptance of this dissertation is contingent upon the candidate‘s submission of the final copies of the dissertation to the Graduate College. I hereby certify that I have read this dissertation prepared under my direction and recommend that it be accepted as fulfilling the dissertation requirement. ________________________________________________ Date: April 22, 2010 Dissertation Director: Peter H. Smith 3 STATEMENT BY AUTHOR This dissertation has been submitted in partial fulfillment of requirements for an advanced degree at the University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library. Brief quotations from this dissertation are allowable without special permission, provided that accurate acknowledgment of source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his or her judgment the proposed use of the material is in the interests of scholarship. In all other instances, however, permission must be obtained from the author. SIGNED: Paul Douglas Archer, Jr. 4 Acknowledgements I‘d first like to thank the many people who helped me complete the actual work in this dissertation. To my advisor, Peter Smith, who allowed me to find my own path but gave me direction when it was needed. And for letting me participate as a team member on the Phoenix Mission, one of the best experiences of my life. To Hiroshi Imanaka and Mark Smith, to whom I owe almost all of the experimental knowledge I gained in completing this dissertation. Without the help that they willingly gave, there is no way I would ever have completed this work. To the guys down in the LPL machine shop who helped me design my varied experimental apparatus and then were able to actually build the things based on my specifications. To Mercer Medding in the Soil, Water, and Environmental Science Department at the University of Arizona who gave me a crash course in soil properties and analytical techniques. To the IPY team whose combined expertise and frequent telecons helped me understand the Dry Valleys of Antarctica as if I had been there myself. And lastly, to my dissertation committee whose feedback was instrumental in producing this final product and who, certainly, will be some of the few people who will ever read this work in its entirety! Second, I‘d like to thank my friends and coworkers who kept me sane the past six years and helped me to become the scientist and person I am today. Particularly, to my fellow classmates with whom I went through many classes, traveled across the western United States on various fieldtrips, and who all became lifelong friends: I couldn‘t have done it without you. Third, I‘d like to thank my family for everything you‘ve done for me. To my dad, who for the past six years constantly asked me how I was doing on my dissertation. Now that I‘m done, you actually have to read this thing! And to my mom, who always asked me how I was doing on my ―book‖. You both gave me my love of learning and exploration and made me who I am today. To my siblings who constantly encouraged me and told me how cool they thought my research was. I appreciate your support and your friendship and everything else you guys do for me. Lastly, I‘d like to thank my wife Dana and my son Wesley. We did it Dana! My life is so much better with you in it. You constantly motivate me to do my best and to be a better person. Your daily encouragement and constant support gave me the confidence I needed to get this work done. And Wesley, who introduced me to the world of fatherhood and who just yesterday learned how to say ―Jupiter‖. You have made my life so much more rewarding; watching you learn and grow is amazing. I love you both and can‘t imagine my life without you. 5 Dedication To my wife, Dana, and my son, Wesley, who motivated me to go to work every morning and gave me a reason to hurry home every night. 6 Table of Contents Chapter 1 – Introduction .................................................................................................. 13 1.1 Astrobiology ....................................................................................................... 13 1.2 Astrobiology and Mars ....................................................................................... 15 1.3 The Phoenix Mission .......................................................................................... 19 1.4 Antarctica and Mars ........................................................................................... 20 1.5 From Antarctica to the lab .................................................................................. 23 1.6 This Work ........................................................................................................... 23 1.6.1 Antarctic Soil Analysis ............................................................................... 24 1.6.2 Irradiation of Organic Material ................................................................... 25 1.6.3 Pyrolysis of Organic Material ..................................................................... 26 Chapter 2 – Physical Properties of Arid Soils ................................................................. 28 2.1 Introduction ........................................................................................................ 28 2.2 The Antarctic Dry Valleys as a Martian analogue ............................................. 31 2.3 Antarctic Soil Regimes....................................................................................... 34 2.4 Sample Locations ............................................................................................... 36 2.5 Experimental Methods ....................................................................................... 47 2.6 Results and Discussion ....................................................................................... 52 2.6.1 Taylor Valley Physical Properties. ............................................................. 53 2.6.2 Taylor Valley Mineralogy and Specific Surface Area ................................ 59 2.6.3 University Valley Physical Properties ........................................................ 64 2.6.4 University Valley Mineralogy and Specific Surface Area ......................... 65 2.6.5 University Valley Salts ............................................................................... 66 2.6.6 University Valley Synthesis ........................................................................ 70 2.6.7 Particle Size and Color Ratio ...................................................................... 70 2.7 Implications for Mars ......................................................................................... 78 2.7.1 Ancient Mars ............................................................................................... 81 2.7.2 Modern Mars ............................................................................................... 82 2.7.3 The Phoenix Landing Site ........................................................................... 87 2.7.4 Viking ......................................................................................................... 90 2.8 Connection to Work on Putative Martian Organics ........................................... 90 Chapter 3 – UV Irradiation of Putative Martian Organics ............................................... 95 3.1 Introduction .......................................................................................................
Recommended publications
  • DISR) on the Huygens Probe
    Data Archive Users’ Guide for the Descent Imager and Spectral Radiometer (DISR) on the Huygens Probe By: The DISR Team 29 January 2013 Version 2.0 International Traffic in Arms Regulations (ITAR) disclosure... Evaluation by the Export Officer of the University of Arizona's Office for the Responsible Conduct of Research (ORCR) has deemed that this document is not subject to International Traffic in Arms Regulations (ITAR) control, and is not restricted by the Arms Export Control Act. It is suitable for public release, and its distribution is unlimited. DISR - C. See 29 January 2013 Index 1.0 Introduction & Science Objectives .................................................................................. 3 2.0 Instrument Description.................................................................................................... 4 3.0 Titan Descent Sequence & Divergences ...................................................................... 11 4.0 Archive Description....................................................................................................... 15 5.0 Data Calibration............................................................................................................ 19 5.1 General Information.................................................................................................. 19 5.2 Descent Cycles......................................................................................................... 20 5.3 Lamp Datasets ........................................................................................................
    [Show full text]
  • Astrobiology and the Search for Life on Mars Edited by Sarah Kember
    Astrobiology and The Search for Life on Mars edited by Sarah Kember Introduction: What Is Life? I’m not going to answer this question. In fact, I doubt if it will ever be possible to give a full answer. (Haldane, 1949: 58) What Is Life? J. B. S. Haldane (1949) and Erwin Schrödinger (1944), two of the twentieth century’s most influential scientists, posed the direct question, ‘what is life?’ and declared that it was a question unlikely to find an answer. Life, they suggested, might exceed the ability of science to represent it and even though the sciences of biology, physics and chemistry might usefully describe life’s structures, systems and processes, those sciences should not seek to reduce it to the sum of its parts. While Schrödinger drew attention to the physical structure of living matter, including especially the cell, Haldane asserted that ‘what is common to life is the chemical events’ (1949: 59) and so therefore life might be defined, though not reduced, to ‘a pattern of chemical processes’ (62) involving the use of oxygen, enzymes and so on. Following Schrödinger and Haldane, Chris McKay’s article, published in 2004 and included in this collection, asks again ‘What is Life – and How Do We Search For It in Other Worlds?’. For him, the still open and unresolved question of life is intrinsically linked to the problem of how to find it (here, or elsewhere) since, he queries, how can we search for something that we cannot adequately define? It should be noted that this dilemma did not deter the founders of Artificial Life, a project that succeeded Artificial Intelligence and that sought to both simulate ‘life-as-we-know-it’ and synthesise ‘life-as-it-could-be’ by reducing life to the informational and therefore computational criteria of self-organisation, self-replication, evolution, autonomy and emergence (Langton, 1996: 40; Kember, 2003).
    [Show full text]
  • Fungal Physiology and the Origins of Molecular Biology
    Microbiology (2009), 155, 3799–3809 DOI 10.1099/mic.0.035238-0 Review Fungal physiology and the origins of molecular biology Robert Brambl Correspondence Department of Plant Biology, The University of Minnesota, 250 Biological Sciences Center, Saint Robert Brambl Paul, MN 55108, USA [email protected] Molecular biology has several distinct origins, but especially important are those contributed by fungal and yeast physiology, biochemistry and genetics. From the first gene action studies that became the basis of our understanding of the relationship between genes and proteins, through chromosome structure, mitochondrial genetics and membrane biogenesis, gene silencing and circadian clocks, studies with these organisms have yielded basic insight into these processes applicable to all eukaryotes. Examples are cited of pioneering studies with fungi that have stimulated new research in clinical medicine and agriculture; these studies include sexual interactions, cell stress responses, the cytoskeleton and pathogenesis. Studies with the yeasts and fungi have been effective in applying the techniques and insights gained from other types of experimental systems to research in fungal cell signalling, cell development and hyphal morphogenesis. The early years of biochemical genetics Neurospora crassa, as Norman Horowitz reminded us, this experimental approach and its reductionist interpretation In the late 1940s Jackson W. Foster published a treatise on were not widely accepted at the time (Horowitz, 1991). fungal physiology in which he marvelled at the progress Geneticists and biologists in general were uncomfortable that had been made in the most recent years, in the decade with simple interpretations of complex phenomena; the following his graduate study in S. A. Waksman’s labor- idea that a mutant phenotype was anything more than a atory.
    [Show full text]
  • Phoenix Mission to Mars Will Search for Climate Clues 22 May 2008
    Phoenix mission to Mars will search for climate clues 22 May 2008 On May 25, 2008, approaching 5 p.m. PDT, NASA Phoenix will touch down in Green Valley with the scientists will be wondering: Just how green is their aid of a parachute, retro rockets and three strong valley? That's because at that time the Phoenix legs with shock absorbing footpads to slow it Mars Mission space vehicle will be touching down down. on its three legs to make a soft landing onto the northern Mars terrain called Green Valley. That's sol (a Martian day) zero. Of course, no valley is actually green on the Red "We'll know within two hours of landing if Phoenix Planet. The place got its name after analysis of landed nominally," said Arvidson. "It will land, images from Mars Reconnaissance Orbiter's deploy its solar panels, take a picture and then go HiRISE instrument. HiRISE can image rocks on to bed." Mars as small as roughly a yard and a half across. Green is the color that that landing site selection The next day, Sol 1, begins a crucial period of team used to represent the fewest number of rocks operations for the mission. Arvidson said, "We'll be in an area, corresponding to a desirable place to checking out the instruments and begin robotic arm land. Thus, "green valley," a relatively rock-less operations within about a week, if everything goes region, is a "sweet spot" where the Phoenix well, and collect soil and ice samples over the spacecraft will land.
    [Show full text]
  • Phoenix–Thefirst Marsscout Mission
    Phoenix – The First Mars Scout Mission Barry Goldstein Jet Propulsion Laboratory, California Institute of Technology Pasadena CA [email protected] Robert Shotwell Jet Propulsion Laboratory, California Institute of Technology [email protected] Abstract —1 2As the first of the new Mars Scouts missions, 4) Characterize the history of water, ice, and the polar the Phoenix project was select ed by NASA in August of climate. Determine the past and present biological potential 2003. Four years later, almost to the day, Phoenix was of the surface and subsurface environments. launched from Cape Canaveral Air Station and successfully injected into an interplanetary trajectory on its way to Mars. TABLE OF CONTENTS On May 25, 2008 Phoenix conducted the first successful 1. INTRODUCTION ..................................................... 1 powered decent on Mars in over 30 years. This paper will 2. DEVELOPMENT PHASE ACTIVITIES ..................... 3 highlight some of the key changes since the 2008 IEEE 3. ENTRY DESCENT & LANDING MATURITY .......... 11 paper of the same name, as well as performance through 4. CONCLUSION ....................................................... 18 cruise, landing at the north pole of Mars and some of the REFERENCES ........................................................... 19 preliminary results of the surface mission. BIOGRAPHIES .......................................................... 20 Phoenix “Follows the water” responding directly to the recently published data from Dr. William Boynton, PI (and 1. INTRODUCTION Phoenix co-I) of the Mars Odyssey Gamma Ray Spectrometer (GRS). GRS data indicate extremely large The first of a new series of highly ambitious missions to quantities of water ice (up to 50% by mass) within the upper explore Mars, Phoenix was selected in August 2003 to 50 cm of the northern polar regolith.
    [Show full text]
  • Robert Lee Metzenberg Jr. 1930—2007
    NATIONAL ACADEMY OF SCIENCES ROBE R T LEE METZENBE R G J R . 1 9 3 0 — 2 0 0 7 A Biographical Memoir by ROWLAND H. DAVIS AND E R IC U. SELKE R Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2008 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. ROBERT LEE METZENBERG JR. June 11, 1930–July 15, 2007 ROWLAND H . DAVIS AND E RIC U. SELKE R N PERFORMING OVER A half century of work on the genetics, Ibiochemistry, and molecular biology of the fungus Neuros- pora crassa, Robert Metzenberg distinguished himself as an exceptionally broad and creative investigator. Neurospora was established as a model organism in the 1930s and 1940s as a result of B. O. Dodge’s study of its life cycle and Beadle’s and Tatum’s Nobel-prize-winning work dissecting biochemical pathways (Davis and Perkins, 2002). Metzenberg was one of a few researchers who stimulated the popularity of the organ- ism for the rest of the 20th century, making contributions that extended into many areas of modern biology. His early studies of the pathways of sulfur and phosphate acquisition in Neurospora concentrated on mechanisms of positive control of gene activity and resulted in the discovery of complex cascade regulatory systems. Metzenberg and his colleagues also showed that the 5S rRNA genes of Neurospora are dispersed among its chromosomes rather than being clustered, as in previously described eukaryotes. He then used the dispersed 5S genes to construct molecular maps of the N.
    [Show full text]
  • The Search for the Elusive Link Between Genome Structure and Gene Function Michel Morange
    Pseudoalleles and gene complexes: the search for the elusive link between genome structure and gene function Michel Morange To cite this version: Michel Morange. Pseudoalleles and gene complexes: the search for the elusive link between genome structure and gene function. Perspectives in Biology and Medicine, Johns Hopkins University Press, 2016, 58 (2), pp.196-204. 10.1353/pbm.2015.0027. hal-01347725 HAL Id: hal-01347725 https://hal.archives-ouvertes.fr/hal-01347725 Submitted on 21 Jul 2016 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution - NonCommercial - NoDerivatives| 4.0 International License 1 Pseudoalleles and gene complexes: the search for the elusive link between genome structure and gene function Michel Morange, Centre Cavaillès, République des savoirs: Lettres, sciences, philosophie USR3608, Ecole normale supérieure, 29 rue d’Ulm, 75230 Paris Cedex 05, France E-mail: [email protected] ABSTRACT After their discovery in the first decades of the XXth century, pseudoalleles generated much interest among geneticists: they apparently violated the conception of the genome as a collection of independent genes elaborated by Thomas Morgan’s group. Their history is rich, complex, and deserves more than one short contribution.
    [Show full text]
  • James Bonner Papers
    http://oac.cdlib.org/findaid/ark:/13030/kt30003586 No online items Finding Aid for the James Bonner Papers 1940-1996 Processed by Mariella Soprano, Elisa Piccio, and Ruth Sustaita. Caltech Archives Archives California Institute of Technology 1200 East California Blvd. Mail Code 015A-74 Pasadena, CA 91125 Phone: (626) 395-2704 Fax: (626) 395-4073 Email: [email protected] URL: http://archives.caltech.edu/ ©2011 California Institute of Technology. All rights reserved. Finding Aid for the James Bonner 10155-MS 1 Papers 1940-1996 Descriptive Summary Title: James Bonner Papers, Date (inclusive): 1940-1996 Collection number: 10155-MS Creator: Bonner, James Frederick 1910-1996 Extent: 34 linear feet Repository: California Institute of Technology. Caltech Archives Pasadena, California 91125 Abstract: The papers of James Frederick Bonner (1910 – 1996), Caltech alumnus (PhD, 1934) and professor of biology, 1938-1981. His papers include a large correspondence section with colleagues and organizations worldwide, as well as writings and talks, papers about his consultancy activities, scientific and technical files and biographical material. Physical location: Archives, California Institute of Technology. Languages represented in the collection: English Access The collection is open for research. Researchers must apply in writing for access. Some files are confidential and will remain closed for an indefinite period. Researchers may request information about closed files from the Caltech Archivist. Publication Rights Copyright may not have been assigned to the California Institute of Technology Archives. All requests for permission to publish or quote from manuscripts must be submitted in writing to the Caltech Archivist. Permission for publication is given on behalf of the California Institute of Technology Archives as the owner of the physical items and, unless explicitly stated otherwise, is not intended to include or imply permission of the copyright holder, which must also be obtained by the reader.
    [Show full text]
  • Camera on Mars Orbiter Snaps Phoenix During Landing 27 May 2008
    Camera on Mars Orbiter Snaps Phoenix During Landing 27 May 2008 information that it was in good health after its first night on Mars, and the Phoenix team sent the spacecraft its to-do list for the day. "We can see cracks in the troughs that make us think the ice is still modifying the surface," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson. "We see fresh cracks. Cracks can't be old. They would fill in." Camera pointing for the image from HiRISE used navigational information about Phoenix updated on landing day. The camera team and Phoenix team would not know until the image was sent to Earth whether it had actually caught Phoenix. "We saw a few other bright spots in the image first, but when we saw the parachute and the lander with the cords connecting them, there was no question," said HiRISE Principal Investigator Alfred McEwen, also of the University of Arizona. NASA's Mars Phoenix Lander can be seen parachuting "I'm floored. I'm absolutely floored," said Phoenix down to Mars, in this image captured by the High Project Manager Barry Goldstein of NASA's Jet Resolution Imaging Science Experiment camera on Propulsion Laboratory, Pasadena, Calif. A team NASA's Mars Reconnaissance Orbiter. Image credit: analyzing what can be learned from the Phoenix NASA/JPL-Calech/University of Arizona descent through the Martian atmosphere will use the image to reconstruct events. HiRISE usually points downward. For this image, A telescopic camera in orbit around Mars caught a the pointing was at 62 degrees, nearly two-thirds of view of NASA's Phoenix Mars Lander suspended the way from straight down to horizontal.
    [Show full text]
  • Space Optics Contributions by the College of Optical Sciences Over the Past 50 Years
    Invited Paper Space optics contributions by the College of Optical Sciences over the past 50 years James B. Breckinridge*a and Peter Smithb aGraduate Aeronautical Laboratory, M/S 150-50 Firestone, Caltech, 1200 E. California Blvd. , Pasadena, CA., 91125; bLunar and Planetary Laboratory, University of Arizona, Tucson, AZ. 85721 ABSTRACT We present a review of the contributions by students, staff, faculty and alumni to the Nation’s space program over the past 50 years. The balloon polariscope led the way to future space optics missions. The missions Pioneer Venus (large probe solar flux radiometer), Pioneer 10/11 (imaging photopolarimeter) to Jupiter and Saturn, Hubble Space Telescope (HST), and next generation large aperture space telescopes are discussed. Keywords: Pioneer 10/11, Imaging, Photopolarimetry, Pioneer Venus, Jupiter, Saturn, Venus, Radiometry, balloon polariscope and space telescopes 1. INTRODUCTION The successful development of rocket engines during WW2 inspired the image of space telescopes and the exploration of the solar system. The May 29, 1944 issue of Life Magazine (p. 78) shows the first science based drawings of what a man walking on a planetary surface might see. Made by Chesley Bonestell these images inspired generations of astronomers, geologists and the general public. In 1946 Professor Lyman Spitzer of Princeton University proposed the construction of a space telescope for astrophysics. Thus were planted the seeds of modern space telescopes for planetary science and astrophysics. The Optical Science Center was founded only 6 years after the Russians orbited Sputnik. In the fall of 1958 President Eisenhower established the civilian space agency: National Aeronautics and Space Agency (NASA).
    [Show full text]
  • Elder Statesmen of Science Unite for Mars Mission - Metro - the Boston Globe 2/8/15, 10:54 AM
    Elder statesmen of science unite for Mars mission - Metro - The Boston Globe 2/8/15, 10:54 AM Elder scientists work to send humans to Mars SEAN PROCTOR/GLOBE STAFF Gerald Voecks (left), Michael Hecht (second from left), and Jeff Hoffman (right) are working on technology to turn carbon dioxide into oxygen on Mars. By Carolyn Y. Johnson GLOBE STAFF FEBRUARY 08, 2015 http://www.bostonglobe.com/metro/2015/02/08/elder-statesmen-scienc…ZQqOEuhKC56rdtE4uPN/story.html?s_campaign=email_BG_TodaysHeadline Page 1 of 6 Elder statesmen of science unite for Mars mission - Metro - The Boston Globe 2/8/15, 10:54 AM CAMBRIDGE — They are graybeards still going boldly: the retired astronaut; the researcher whose career began before the first Viking craft touched down on the red planet nearly 40 years ago; the octogenarian just now updating his 520-page tome, “Human Missions to Mars.” At an age when most are retired or thinking hard about it, they’ve put their minds together to help solve one of the great puzzles of human interplanetary travel. And NASA has awarded them $30 million to press on. CONTINUE READING BELOW ▼ To be clear, these elder statesmen of science don’t plan to pay a visit themselves. They are building an oxygen-generating machine to ride aboard the unmanned Mars 2020 rover, an early version of a technology that could enable the next generation to breathe and burn fuel on Mars — and power their way home. Perhaps it’s no coincidence that the abbreviated acronym for their instrument — the Mars Oxygen In-Situ Resources Utilization Experiment — is MOXIE.
    [Show full text]
  • Issue 111, August 2007
    Phoenix Rises NASA’s Phoenix Mars Lander mission blasted off on August 4, aiming for a May 25, 2008, arrival at the Red Planet and a close-up examination of the surface of the northern polar region. Perched atop a Delta II rocket, the spacecraft left Cape Canaveral Air Force Base at 5:26 a.m. Eastern Time into the predawn sky above Florida’s Atlantic coast. “[The] launch is the fi rst step in the long journey to the surface of Mars. We certainly are excited about launching, but we still are concerned about our actual landing, the most diffi cult step of this mission,” said Phoenix Principal Investigator Peter Smith. The spacecraft established communications with its ground team via the Goldstone, California, antenna station of NASA’s Deep Space Network at 7:02 a.m. Eastern Time, after separating from the third stage of the launch vehicle. “The launch team did a spectacular job getting us on the way,” The Phoenix Mars Lander mission said Barry Goldstein, Phoenix project manager at NASA’s Jet Propulsion roared into space on August 4 and Laboratory. “Our trajectory is still being evaluated in detail; however, we began its journey to seek evidence Lare well within expected limits for a successful journey to the Red Planet. of water on our neighboring planet. Photo courtesy of NASA. We are all thrilled!” The Phoenix Mars mission is the fi rst of NASA’s competitively proposed and selected Mars Scout missions, an initiative for lower-cost, competed spacecraft. Named for the resilient mythological bird, the Phoenix mission fi ts perfectly with the agency’s core Mars Exploration Program, whose theme is “follow the water.” The University of Arizona was selected to lead the mission in August 2003 and is the fi rst public university to lead a Mars exploration P mission.
    [Show full text]