2020 Crew Health & Performance EVA Roadmap
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The IRM the Iron That Binds: the Unexpectedly Strong Magnetism Of
ISSN: 2152-1972 The IRM Inside... Visiting Fellows' Reports 2 Current Articles 4 QuarterlySummer 2014, Vol. 24 No.2 The iron that binds: The unexpectedly strong magnetism of high-temperature ceramic cements commonly used in rock magnetic experiments. Evgeniya Khakhalova and Josh M. Feinberg IRM The main goal of many IRM visitors is to better understand the composition of the mag- netic remanence carriers in their samples. Typically, a material’s Curie or Néel temperature serves as the primary means for estimat- ing its mineralogical composi- tion. However, many of the most commonly used techniques, such as high temperature susceptibil- ity and thermal demagnetization experiments, have to be inter- preted carefully due to the com- plicating effects of grain size. For example, single-domain grains contribute less signal to suscep- tibility experiments than super- Fig 1. RT SIRM curves on cooling from 300 K to 10 K and warming from 10 K to 300 K and SIRM warming curves from paramagnetic and multidomain 10 K to 300 K after field-cooling (FC) and zero-field-cooling (ZFC) of samples (a) Omega700_3, (b) Omega600, and (c) grains of the same material, and OmegaCC. SIRM was imparted using a field of 2.5 T. thermal demagnetization experi- ments are insensitive to superparamagnetic grains. Fur- ples dominated by hematite, goethite, and ferrihydrite). ther, the unblocking temperatures observed in a thermal In these instances, any source of magnetic contamination demagnetization experiment will typically be lower than in a strong-field thermomagnetic experiment can lead to the Curie or Néel temperature of the material. an incorrect interpretation of a sample’s magnetic miner- In this context, strong-field thermomagnetic ex- alogy. -
A Retrospective Snapshot of the Planning Processes in MER Operations After 5 Years
A Retrospective Snapshot of the Planning Processes in MER Operations After 5 Years Anthony Barrett, Deborah Bass, Sharon Laubach, and Andrew Mishkin Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive M/S 301-260 {firstname.lastname}@jpl.nasa.gov Abstract Over the past five years on Mars, the Mars Exploration Rovers have traveled over 20 kilometers to climb tall hills and descend into craters. Over that period the operations process has continued to evolve as deep introspection by the MER uplink team suggests streamlining improvements and lessons learned adds complexity to handle new problems. As such, the operations process and its supporting tools automate enough of the drudgery to circumvent staff burnout issues while being nimble and safe enough to let an operations staff respond to the problems that Mars throws up on a daily basis. This paper describes the currently used integrated set of planning processes that support rover operations on a daily basis after five years of evolution. Figure 1. Mars Exploration Rover For communications, each rover has a high gain antenna Introduction for receiving instructions from Earth, and a low gain On January 3 & 24, 2004 Spirit and Opportunity, the twin antenna for transmitting data to the Odyssey or Mars Mars Exploration Rovers (MER), landed on opposite sides Reconnaissance orbiters with subsequent relay to Earth. of Mars at Gusev Crater and Meridiani Planum Given that it takes between 6 and 44 minutes for a signal to respectively. Each rover was originally expected to last 90 travel to and from the rovers, simple joystick operations Sols (Martian days) due to dust accumulation on the solar are not feasible. -
This Preview Includes the Entire Resource. the Teacher Information
This preview includes the entire resource. The teacher information pages and two of the student pages are unmarked so that you can try before you buy! I I Literacy is a challenging, quick, and fun way to reinforce ELA and reading skills. Each page features a different theme, so not only will your students be practicing skills, they will also be learning about curriculum-based, high-interest topics. Each page has its own unique design, so students will never get bored seeing the same old thing over and over. While each page is different, they do have some elements in common. Each page features: • 6 standards-based ELA/Reading activities, each in its own space. Activities are numbered for easy reference. • An open-ended bonus activity, marked by a star, at the bottom of the page to be completed on the backside. Perfect for fast finishers, as homework, or extra credit. • A short reading passage with one or two text-dependent questions. Most of the passages are informational text (written by a published author of over 100 nonfiction books for children), but a few are fictional – just to shake things up. The questions are more closely aligned to close reading than simple comprehension. • A theme-based joke or fun fact (joke answers can be found upside down in the bottom right hand corner). • A list of the skills addressed at the bottom (indicated by a picture of a nail – which stands for “nailed it!”) This list repeats in the table of contents for easy reference. • A picture of a whale in the upper right corner simply because it is so adorable. -
Of Curiosity in Gale Crater, and Other Landed Mars Missions
44th Lunar and Planetary Science Conference (2013) 2534.pdf LOCALIZATION AND ‘CONTEXTUALIZATION’ OF CURIOSITY IN GALE CRATER, AND OTHER LANDED MARS MISSIONS. T. J. Parker1, M. C. Malin2, F. J. Calef1, R. G. Deen1, H. E. Gengl1, M. P. Golombek1, J. R. Hall1, O. Pariser1, M. Powell1, R. S. Sletten3, and the MSL Science Team. 1Jet Propulsion Labora- tory, California Inst of Technology ([email protected]), 2Malin Space Science Systems, San Diego, CA ([email protected] ), 3University of Washington, Seattle. Introduction: Localization is a process by which tactical updates are made to a mobile lander’s position on a planetary surface, and is used to aid in traverse and science investigation planning and very high- resolution map compilation. “Contextualization” is hereby defined as placement of localization infor- mation into a local, regional, and global context, by accurately localizing a landed vehicle, then placing the data acquired by that lander into context with orbiter data so that its geologic context can be better charac- terized and understood. Curiosity Landing Site Localization: The Curi- osity landing was the first Mars mission to benefit from the selection of a science-driven descent camera (both MER rovers employed engineering descent im- agers). Initial data downlinked after the landing fo- Fig 1: Portion of mosaic of MARDI EDL images. cused on rover health and Entry-Descent-Landing MARDI imaged the landing site and science target (EDL) performance. Front and rear Hazcam images regions in color. were also downloaded, along with a number of When is localization done? MARDI thumbnail images. The Hazcam images were After each drive for which Navcam stereo da- used primarily to determine the rover’s orientation by ta has been acquired post-drive and terrain meshes triangulation to the horizon. -
Complex Garment Systems to Survive in Outer Space
Volume 7, Issue 2, Fall 2011 Complex Garment Systems to Survive in Outer Space Debi Prasad Gon, Assistant Professor, Textile Technology, Panipat Institute of Engineering & Technology, Pattikalyana, Samalkha, Panipat, Haryana, INDIA [email protected] Palash Paul, Assistant Professor, Textile Technology, Panipat Institute of Engineering & Technology, Pattikalyana, Samalkha, Panipat, Haryana, INDIA ABSTRACT The success of astronauts in performing Extra-Vehicular Activity (EVA) is highly dependent on the performance of the spacesuit they are wearing. Since the beginning of the Space Shuttle Program, one basic suit design has been evolving. The Space Shuttle Extravehicular Mobility Unit (EMU) is a waist entry suit consisting of a hard upper torso (HUT) and soft fabric mobility joints. The EMU was designed specifically for zero gravity operations. With a new emphasis on planetary exploration, a new EVA spacesuit design is required. Now the research scientists are working hard and striving for the new, lightweight and modular designs. Thus they have reached to the Red surface of Mars. And sooner or later the astronauts will reach the other planets too. This paper is a review of various types of spacesuits and the different fabrics required for the manufacturing of the same. The detailed construction of EMU and space suit for Mars is discussed here, along with certain concepts of Biosuit- Mechanical Counter pressure Suit. Keywords: Extra-Vehicular Activity (EVA), spacesuits, Biosuit-Mechanical Counter pressure Suit Tissues (skin, heart, -
Mars One Applicant Study Material Booklet
COMPILED BY MICHAEL GRUNDLING Index: PAGE WHAT ’S THE HISTORIC SUCCESS RATE OF MISSIONS TO MARS ............................................................... 3 THE ROADMAP ..................................................................................................................................... 5 WHAT HAPPENS AFTER THE FIRST HUMANS ’ ARRIVAL ON MARS ? ............................................................. 11 WILL THE MISSION BE HARMFUL TO MARS ’ ENVIRONMENT ? ..................................................................... 12 IS THIS A SUSTAINABLE MISSION ?........................................................................................................... 13 WHAT GOVERNMENTAL SYSTEM AND SOCIAL STRUCTURE WILL BE IMPLEMENTED ON MARS ? .................... 14 WHAT WILL THE ASTRONAUTS DO ON MARS ? ......................................................................................... 15 WHAT ARE THE RISKS OF DUST AND SAND ON MARS ? ............................................................................. 17 IS IT SAFE TO LIVE ON MARS ? ................................................................................................................ 19 HOW SAFE IS THE JOURNEY ? ................................................................................................................. 20 HOW LONG DOES IT TAKE TO TRAVEL TO MARS ? .................................................................................... 21 WHY MARS , AND NOT ANOTHER PLANET ? ............................................................................................. -
Copyright © 2006 by Douglas W. Gage. Published by the Mars Society with Permission
Copyright © 2006 by Douglas W. Gage. Published by The Mars Society with permission BEGIN HIGH FIDELITY MARS SIMULATIONS NOW! Douglas W. Gage XPM Technologies - [email protected] ABSTRACT While analog environments (e.g., Antarctica) and mission experiments (e.g., FMARS, MDRS) are useful, a long term, logically sequenced series of experiments and evaluations in faithfully simulated Mars (outdoor) and Mars habitat (indoor) environments is an absolute prerequisite for manned missions to Mars. Mars suit pressure should be minimized in order to simplify suit design, and habitat pressure should also be minimized, to eliminate "EVA" prebreathing and to reduce structural stress. But we need to experimentally establish the long-term health implications of living in such an atmosphere before we make irrevocable design decisions. This will require a habitat simulation facility that operates continuously for years. Coupling the habitat simulation with a Martian surface simulation (Martian atmospheric pressure and composition, temperature, lighting, wind, dust, and analog-regolith) will support the long term evolutionary development cycle of all types of systems and processes: equipment reliability testing, development of techniques and procedures (e.g., repair, emergency survival), mission plan development and validation, and then later crew training and mission rehearsal. Finally, after launch, the facility will be used to "shadow" actual mission operations. For these purposes we need high fidelity simulation facilities, not just rough analogs. Apart from reduced gravity and radiation, we can provide very high fidelity right here on earth, at costs much lower than in space or on the moon. The time to start is now! INTRODUCTION Sending humans to Mars is the capstone specific goal identified for the “Vision for Space Exploration” promulgated by President Bush [1]. -
Concepts and Approaches for Mars Exploration 6132.Pdf
Concepts and Approaches for Mars Exploration 6132.pdf EXPLORATION STRATEGIES FOR HUMAN MISSIONS: MARS FIELD GEOLOGY, BIOLOGY AND PALEONTOLOGY WORKSHOP. Patricia Wood Dickerson, Lockheed Martin, NASA - Johnson Space Center, C 23, Houston, TX 77058. [email protected]. Introduction: Field exploration strategy, crew Analytical Capabilities & Instruments: Robotic skills and training, analytical capabilities, and Earth-Mars reconnaissance of the Martian surface, human field explo- communications were themes of the Mars Field Geology, rations, and preliminary laboratory research will focus both Biology and Paleontology workshop [1] convened by Mi- on fundamental scientific questions and on site and resource chael B. Duke, David S. McKay, and William R. Muehlber- assessment. Both endeavors will require observations, ger (November, 1998). The intent was to expand the explo- measurements, sampling, and analysis of Martian material, ration culture within NASA: one which captures the experi- and geophysical studies. The team framed their recommen- ence and insight of the scientists, mission operations per- dations of candidate instruments in terms of six specific sonnel, and crews of the Apollo and Skylab explorations; objectives in the human exploration of Mars: field observa- one which applies and develops new technology appropriate tion, sample acquisition, maintenance of crew health and to the quest; one which clearly articulates the scientific safety, search for evidence of past or present life, geological questions and scrupulously reports both data and interpreta- and geophysical field investigation, sample selection and tion. preparation. The convenors charged the thirty-one veteran field Recommendations. 1) The need for specific obser- scientists and space explorers to frame specific recommen- vations and analyses should be the primary driver for the dations, which would build upon mission architecture de- development of compact, integrated field instruments. -
Moon-Miners-Manifesto-Mars.Pdf
http://www.moonsociety.org/mars/ Let’s make the right choice - Mars and the Moon! Advantages of a low profile for shielding Mars looks like Arizona but feels like Antarctica Rover Opportunity at edge of Endeavor Crater Designing railroads and trains for Mars Designing planes that can fly in Mars’ thin air Breeding plants to be “Mars-hardy” Outposts between dunes, pulling sand over them These are just a few of the Mars-related topics covered in the past 25+ years. Read on for much more! Why Mars? The lunar and Martian frontiers will thrive much better as trading partners than either could on it own. Mars has little to trade to Earth, but a lot it can trade with the Moon. Both can/will thrive together! CHRONOLOGICAL INDEX MMM THEMES: MARS MMM #6 - "M" is for Missing Volatiles: Methane and 'Mmonia; Mars, PHOBOS, Deimos; Mars as I see it; MMM #16 Frontiers Have Rough Edges MMM #18 Importance of the M.U.S.-c.l.e.Plan for the Opening of Mars; Pavonis Mons MMM #19 Seizing the Reins of the Mars Bandwagon; Mars: Option to Stay; Mars Calendar MMM #30 NIMF: Nuclear rocket using Indigenous Martian Fuel; Wanted: Split personality types for Mars Expedition; Mars Calendar Postscript; Are there Meteor Showers on Mars? MMM #41 Imagineering Mars Rovers; Rethink Mars Sample Return; Lunar Development & Mars; Temptations to Eco-carelessness; The Romantic Touch of Old Barsoom MMM #42 Igloos: Atmosphere-derived shielding for lo-rem Martian Shelters MMM #54 Mars of Lore vs. Mars of Yore; vendors wanted for wheeled and walking Mars Rovers; Transforming Mars; Xities -
2005 Astronomy Magazine Index
2005 Astronomy Magazine Index Subject index flyby of Titan, 2:72–77 Einstein, Albert, 2:30–53 Cassiopeia (constellation), 11:20 See also relativity, theory of Numbers Cassiopeia A (supernova), stellar handwritten manuscript found, 3C 58 (star remnant), pulsar in, 3:24 remains inside, 9:22 12:26 3-inch telescopes, 12:84–89 Cat's Eye Nebula, dying star in, 1:24 Einstein rings, 11:27 87 Sylvia (asteroid), two moons of, Celestron's ExploraScope telescope, Elysium Planitia (on Mars), 5:30 12:33 2:92–94 Enceladus (Saturn's moon), 11:32 2003 UB313, 10:27, 11:68–69 Cepheid luminosities, 1:72 atmosphere of water vapor, 6:22 2004, review of, 1:31–40 Chasma Boreale (on Mars), 7:28 Cassini flyby, 7:62–65, 10:32 25143 (asteroid), 11:27 chonrites, and gamma-ray bursts, 5:30 Eros (asteroid), 11:28 coins, celestial images on, 3:72–73 Eso Chasma (on Mars), 7:28 color filters, 6:67 Espenak, Fred, 2:86–89 A Comet Hale-Bopp, 7:76–79 extrasolar comets, 9:30 Aeolis (on Mars), 3:28 comets extrasolar planets Alba Patera (Martian volcano), 2:28 from beyond solar system, 12:82 first image of, 4:20, 8:26 Aldrin, Buzz, 5:40–45 dust trails of, 12:72–73 first light from, who captured, 7:30 Altair (star), 9:20 evolution of, 9:46–51 newly discovered low-mass planets, Amalthea (Jupiter's moon), 9:28 extrasolar, 9:30 1:68–71 amateur telescopes. See telescopes, Conselice, Christopher, 1:20 smallest, 9:26 amateur constellations whether have diamond layers, 5:26 Andromeda Galaxy (M31), 10:84–89 See also names of specific extraterrestrial life, 4:28–34 disk of stars surrounding, 7:28 constellations eyepieces, telescope. -
MMM #273 Since December 1986 March 2014 P1
MMM #273 Since December 1986 March 2014 p1 A Desert Castle in Ancient Khorezm in the arid, sandy plains of central Uzbekistan: A model for the (Mars dust) retaining walls hiding a modern Martian hotel? Why not be playful? MMM’s Annual Mars-Theme Issue (March is for Mars) Feature Articles: 2 In Focus: Mars - Do we go to explore? - or to make it a 2nd Earth? 3 “Desert Castle Architectures” for Hotels in rural Mars 4 We may all be Martians! “Life likely came to Earth on a Martian Meteorite” 6 MMM Platform for Mars, V.3 6 Chronological Index To MMM THEMES Issue: MARS Coming Up. Yuri’s Night and Earthday For past articles, Visit http://www.moonsociety.org/publications/mmm_classics/ or /mmm_themes/ MMM #273 Since December 1986 March 2014 p2 About Moon Miners’ Manifesto - “The Moon - it’s not Earth, but it’s Earth’s!” • MMM’s VISION: “expanding the human economy through of-planet resources”; early heavy reliance on Lunar materials; early use of Mars system and asteroid resources; and permanent settlements supporting this economy. • MMM’s MISSION: to encourage “spin-up” entrepreneurial development of the novel technologies needed and promote the economic-environmental rationale of space and lunar settlement. • Moon Miners’ Manifesto CLASSICS: The non-time-sensitive articles and editorials of MMM’s first twenty years plus have been re-edited, reillustrated, and republished in 23 PDF format volumes, for free downloading from this location: http://www.MoonSociety.org/publications/mmm_classics/ • MMM THEME Issues: 14 collections of articles according to themes: ..../publications/mmm_themes/ • MMM Glossary: new terms, old terms/new meanings: www.moonsociety.org/publications/m3glossary.html • MMM retains its editorial independence and serves many groups, each with its own philosophy, agenda, and programs. -
Mars Exploration Rover Mobility and IDD Downlink Analysis Tools
To appear in i-SAIRAS Conference Proceedings, Feb 2008, Los Angeles, CA, USA Mars Exploration Rover Mobility and IDD Downlink Analysis Tools Jeffrey J. Biesiadecki and Robert Liebersbach and Mark W. Maimone Jet Propulsion Laboratory, California Institute of Technology Pasadena, CA USA [email protected] Abstract— Driving and manipulation activities on the Mars various flight software (FSW) subsystems [13] (e.g., the Exploration Rovers often must be planned from scratch Mobility software module [2]), and are typically stored in each day, making this a fast-paced activity by typical space Flash memory prior to transmission [15]. Data are usually mission standards. Such a schedule requires rapid turnaround in understanding what happened during activities on the relayed through UHF frequencies to an orbiter at Mars previous Martian Solar Day (Sol). In addition to obvious (e.g., Mars Odyssey) or can be transmitted directly to faults, subtle changes in expected behavior must be detected Earth at lower bandwidth using X-band frequencies. The and understood rapidly, to prevent the next day's plan from Deep Space Network receives the raw data and forwards exacerbating any imminent problem. it to the Jet Propulsion Laboratory (JPL), where processes We developed an advanced set of tools to help speed up the understanding of previous Sols' activities. Plots of detailed en- controlled by the Ground Data Systems [19] and Mission gineering data are generated automatically and incorporated Data Operations Teams automatically archive the raw data, into HTML pages, allowing quick visual inspection of each generate preliminary reports [18], and populate an archived activity. Data from different sources are grouped together filesystem with individual Data Product files.