Robotic Lunar Ecopoiesis Test Bed
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
Calculating the Potato Radius of Asteroids Using the Height of Mt. Everest
Calculating the Potato Radius of Asteroids using the Height of Mt. Everest M. E. Caplan∗ Center for the Exploration of Energy and Matter, Indiana University, Bloomington, IN 47408 (Dated: November 16, 2015) Abstract At approximate radii of 200-300 km, asteroids transition from oblong `potato' shapes to spheres. This limit is known as the Potato Radius, and has been proposed as a classification for separating asteroids from dwarf planets. The Potato Radius can be calculated from first principles based on the elastic properties and gravity of the asteroid. Similarly, the tallest mountain that a planet can support is also known to be based on the elastic properties and gravity. In this work, a simple novel method of calculating the Potato Radius is presented using what is known about the maximum height of mountains and Newtonian gravity for a spherical body. This method does not assume any knowledge beyond high school level mechanics, and may be appropriate for students interested in applications of physics to astronomy. arXiv:1511.04297v1 [physics.ed-ph] 7 Nov 2015 1 I. INTRODUCTION Spacecraft are currently exploring asteroids and dwarf planets, such as the Near Earth Asteroid Rendezvous mission (NEAR) landing on Eros,1 the Dawn mission orbiting Ceres and Vesta,2 and the New Horizons flyby of Pluto and Charon.3 Additionally, the Mars Re- connaissance Orbiter (MRO) has observed the Martian moons Phobos and Deimos.4 These missions observe a remarkable variety of shapes for these bodies, shown in Fig. 1. Smaller asteroids have irregular shapes while dwarf planets (large asteroids) are nearly spherical. -
NCKRI: 2012-2013 Annual Report
The National Cave and Karst Research Institute (NCKRI) will be the world’s premier cave and karst research organization. NCKRI promotes and performs projects of national and international application, of the highest quality and integrity, through dedicated staff and partners. NCKRI is a non-profit 501(c)(3) corporation. It was created by the US Congress in 1998 in partnership with the National Park Service, State of New Mexico, and the City of Carlsbad. Federal and state funding for NCKRI is adminis- tered by the New Mexico Institute of Mining and Technolo- gy (aka New Mexico Tech or NMT). Funds not produced by agreements through NMT are accepted directly by NCKRI. NCKRI’s enabling legislation, the National Cave and Karst Research Institute Act of 1998, 16 U.S.C. §4310, iden- tifies NCKRI’s mission as to: 1) further the science of speleology; 2) centralize and standardize speleological information; 3) foster interdisciplinary cooperation in cave and karst research programs; 4) promote public education; 5) promote national and international cooperation in pro- tecting the environment for the benefit of cave and karst landforms; and 6) promote and develop environmentally sound and sus- tainable resource management practices. NCKRI produced this publication as part of its annual Our 2011-12 Annual Report cover showed a speleothem reporting of activities. The reporting period covers NCKRI’s reported as destroyed. It still exists; a similar nearby speleo- fiscal year, from 1 July to 30 June of the following year. them had been destroyed. For reasons like this, NCKRI ar- Digital copies of this and previous reports are available for chives cave photos as historical and scientific records. -
Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report
NASA Technical Memorandum 84414 Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report Infrared Experiments Working Group NOVEMBER 1981 NASA NASA Technical Memorandum 84414 Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report Infrared Experiments Working Group Jet Propulsion Laboratory Pasadena, California NASA National Aeronautics and Space Administration Scientific and Technical Information Branch 1981 TABLE OF CONTENTS Preface Summary of Principal Conclusions and Recommendations Chapter I The Role of Infrared Sensing in Atmospheric Science Chapter II Review of Existing Infrared Measurement Techniques Chapter III Critical Comparison of Proposed Measurement Techniques Chapter IV Conclusions and Recommended Instrument Developments Appendices: A Critical Technologies B Applicability of Atmospheric Infrared Instrumentation to Surface Science C Supporting Studies in Data Analysis and Numerical Modeling D Description of Planned Earth Orbital Platforms ii PREFACE Experiments conducted in the infrared spectral region provide a powerful tool for the study of the composition, structure and dynamics of planetary atmospheres. However, the field has become highly complex, especially that part associated with spacecraft sensing, and the range of technologies used so diverse that it is difficult to determine which of the available methods for making a particular measurement is to be preferred, even for those deeply involved in the field. Unfortunately, the realities of the age demand that some selectivity be employed; not all approaches can be supported. Furthermore, the chosen methods are generally sufficiently untried that long pre-flight developments are neces- sary if viable proposals are to be written for future flight opportunities. These considerations clearly lead to a program of developments which must be coordinated on a national scale. -
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. -
A Brief Discussion from the Epistemological, Religious and Societal Dimension
International Journal of Astrobioethics: a brief discussion from Astrobiology the epistemological, religious and cambridge.org/ija societal dimension Octavio A. Chon-Torres1 Research Article Programa de Estudios Generales, Universidad de Lima, Lima, Peru Cite this article: Chon-Torres OA (2019). Astrobioethics: a brief discussion from Abstract the epistemological, religious and As astrobiology progresses in its quest to discover life on other planets or to put ourselves in societal dimension. International Journal of another one, so does its moral problematic. Astrobiology is not only part of natural sciences, Astrobiology 1–7. https://doi.org/10.1017/ S147355041900017X but also deals with direct aspects of humanities. For this reason, this paper aims to briefly examine astrobioethics from the epistemological, religious and societal dimension. It also Received: 31 January 2019 deals with different researches in this regard, in order to better understand the state of the Revised: 24 June 2019 art on this topic and that astrobioethics can help us not only on how we should relate with Accepted: 25 June 2019 extraterrestrial lifeforms, but even with terrestrials. Key words: Astrobiocentrism; astrobioethics; astrobiology; transdisciplinarity Astrobioethics is the discipline inside astrobiology that studies not only the morality of all activities related to the presence of life on other worlds, but also studies our attitude towards Author for correspondence: the expansion of terrestrial life in the Universe. The discipline that focuses on moral problems Octavio A. Chon-Torres, E-mail: ochon@ulima. edu.pe is ethics; however, as ethics is not an exact science but rather a branch of philosophy, its prob- lematic nature makes its content always updated according to the social context in which it operates. -
Perceptions of Female High School Students on Engineering
Journal of Education and Practice www.iiste.org ISSN 2222-1735 (Paper) ISSN 2222-288X (Online) Vol.7, No.25, 2016 Perceptions of Female High School Students on Engineering Diana Starovoytova Madara* Sitati Namango School of Engineering, Moi University P. O .Box 3900, Eldoret, Kenya Abstract There is overwhelming evidence that females are underrepresented in engineering worldwide, and Kenya is not an exception. Recent study at School of Engineering (SOE), Moi University (MU) established that engineering parity ration was found to be 1.68 %, meaning that for every 59 students admitted to MU there was only one student admitted to SOE. Engineering female parity index was found to be 0.0038, meaning that, on average, for 260 female students admitted to MU, only 1(one) female student was admitted to SOE. Humankind depends on engineers to create new technologies, to find solutions to practical problems and to shape the world that people live in and the future they rely on. Yet young people have little or no perception of engineering and the understanding they do have is all too often confused with other careers, such as science. The perception of engineering as “masculine” and “too hard” is a contributing factor for the female minority in engineering. On the other hand there are very few studies on what high school students think about engineering. In view of the above, this paper will try to fill this gap of information, by exploring teenage girls’ perceptions of engineering as a subject for study and as a potential career choice. Furthermore, it will attempt to raise awareness about and improve the image of engineering, by providing fused notion of engineering to the potential broad audience of this paper. -
Radar Sounder Evidence of Thick, Porous Sediments in Meridiani
PUBLICATIONS Geophysical Research Letters RESEARCH LETTER Radar sounder evidence of thick, porous sediments 10.1002/2017GL074431 in Meridiani Planum and implications Key Points: for ice-filled deposits on Mars • The MARSIS radar sounder has detected subsurface echoes deep Thomas R. Watters1 , Carl J. Leuschen2, Bruce A. Campbell1 , Gareth A. Morgan1 , within the Meridiani Planum deposits 3 1 4 5 • The time delay between surface and Andrea Cicchetti , John A. Grant , Roger J. Phillips , and Jeffrey J. Plaut subsurface echoes is consistent with 1 2 deposits having a low bulk value of Center for Earth and Planetary Studies, Smithsonian Institution, Washington, District of Columbia, USA, Center for Remote the real dielectric constant Sensing of Ice Sheets, University of Kansas, Lawrence, Kansas, USA, 3Infocom Department, La Sapienza University of Rome, • New compaction relationships for Rome, Italy, 4Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington Mars indicate that a low dielectric University, St. Louis, Missouri, USA, 5Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA constant can be accounted for without invoking pore-filling water ice Abstract Meridiani Planum is one of the most intensely studied regions on Mars, yet little is known about Supporting Information: the physical properties of the deposits below those examined by the Opportunity rover. We report the • Supporting Information S1 detection of subsurface echoes within the Meridiani Planum deposits from data obtained by the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument. The delay time between the Correspondence to: T. R. Watters, surface and subsurface returns is indicative of materials with a real dielectric constant of 3.6 ± 0.6. -
Complete List of Contents
Complete List of Contents Volume 1 Cape Canaveral and the Kennedy Space Center ......213 Publisher’s Note ......................................................... vii Chandra X-Ray Observatory ....................................223 Introduction ................................................................. ix Clementine Mission to the Moon .............................229 Preface to the Third Edition ..................................... xiii Commercial Crewed vehicles ..................................235 Contributors ............................................................. xvii Compton Gamma Ray Observatory .........................240 List of Abbreviations ................................................. xxi Cooperation in Space: U.S. and Russian .................247 Complete List of Contents .................................... xxxiii Dawn Mission ..........................................................254 Deep Impact .............................................................259 Air Traffic Control Satellites ........................................1 Deep Space Network ................................................264 Amateur Radio Satellites .............................................6 Delta Launch Vehicles .............................................271 Ames Research Center ...............................................12 Dynamics Explorers .................................................279 Ansari X Prize ............................................................19 Early-Warning Satellites ..........................................284 -
A Lunar Micro Rover System Overview for Aiding Science and ISRU Missions Virtual Conference 19–23 October 2020 R
i-SAIRAS2020-Papers (2020) 5051.pdf A lunar Micro Rover System Overview for Aiding Science and ISRU Missions Virtual Conference 19–23 October 2020 R. Smith1, S. George1, D. Jonckers1 1STFC RAL Space, R100 Harwell Campus, OX11 0DE, United Kingdom, E-mail: [email protected] ABSTRACT the form of rovers and landers of various size [4]. Due to the costly nature of these missions, and the pressure Current science missions to the surface of other plan- for a guaranteed science return, they have been de- etary bodies tend to be very large with upwards of ten signed to minimise risk by using redundant and high instruments on board. This is due to high reliability re- reliability systems. This further increases mission cost quirements, and the desire to get the maximum science as components and subsystems are expected to be ex- return per mission. Missions to the lunar surface in the tensively qualified. next few years are key in the journey to returning hu- mans to the lunar surface [1]. The introduction of the As an example, the Mars Science Laboratory, nick- Commercial lunar Payload Services (CLPS) delivery named the Curiosity rover, one of the most successful architecture for science instruments and technology interplanetary rovers to date, has 10 main scientific in- demonstrators has lowered the barrier to entry of get- struments, requires a large team of people to control ting science to the surface [2]. Many instruments, and and cost over $2.5 billion to build and fly [5]. Curios- In Situ Surface Utilisation (ISRU) experiments have ity had 4 main science goals, with the instruments and been funded, and are being built with the intention of the design of the rover specifically tailored to those flying on already awarded CLPS missions. -
Human Exploration of Mars Design Reference Architecture 5.0
July 2009 “We are all . children of this universe. Not just Earth, or Mars, or this System, but the whole grand fireworks. And if we are interested in Mars at all, it is only because we wonder over our past and worry terribly about our possible future.” — Ray Bradbury, 'Mars and the Mind of Man,' 1973 Cover Art: An artist’s concept depicting one of many potential Mars exploration strategies. In this approach, the strengths of combining a central habitat with small pressurized rovers that could extend the exploration range of the crew from the outpost are assessed. Rawlings 2007. NASA/SP–2009–566 Human Exploration of Mars Design Reference Architecture 5.0 Mars Architecture Steering Group NASA Headquarters Bret G. Drake, editor NASA Johnson Space Center, Houston, Texas July 2009 ACKNOWLEDGEMENTS The individuals listed in the appendix assisted in the generation of the concepts as well as the descriptions, images, and data described in this report. Specific contributions to this document were provided by Dave Beaty, Stan Borowski, Bob Cataldo, John Charles, Cassie Conley, Doug Craig, Bret Drake, John Elliot, Chad Edwards, Walt Engelund, Dean Eppler, Stewart Feldman, Jim Garvin, Steve Hoffman, Jeff Jones, Frank Jordan, Sheri Klug, Joel Levine, Jack Mulqueen, Gary Noreen, Hoppy Price, Shawn Quinn, Jerry Sanders, Jim Schier, Lisa Simonsen, George Tahu, and Abhi Tripathi. Available from: NASA Center for AeroSpace Information National Technical Information Service 7115 Standard Drive 5285 Port Royal Road Hanover, MD 21076-1320 Springfield, VA 22161 Phone: 301-621-0390 or 703-605-6000 Fax: 301-621-0134 This report is also available in electronic form at http://ston.jsc.nasa.gov/collections/TRS/ CONTENTS 1 Introduction ...................................................................................................................... -
CO2 Glaciers on the South Polar Layered Deposits of Mars
Sixth Mars Polar Science Conference (2016) 6072.pdf 1† 2 1 3 CO2 Glaciers on the South Polar Layered Deposits of Mars. I. B. Smith ; E. Larour ; N. E. Putzig ; R. Greve ; N. Schlegel2. 1Planetary Science Institute, Denver, Co; 2Jet Propulsion Laboratory, Pasadena, Ca; 3Hokkaido !University, Sapporo, Japan †Contact: [email protected]. Introduction: A thin unit of CO2 ice, called the south polar residual cap (SPRC), overlies the south polar layered deposits (SPLD) of Mars. This unit, cap- ping a domed-shaped ice cap, has inspired several studies concerning the glacial-like flow of CO2 ice under martian conditions [1-3]. Furthermore, evidence of moraines at the north pole have led to interpretations that CO2 ice was once prevalent there and that it flowed [4]. Laboratory experiments determined that CO2 ice is much less viscous than water ice at similar temperatures (~150 K), by up to two orders of magni- tude [1,2], and therefore it may flow much more readi- ly. Based on those rheological studies, [3] determined that the bulk of the SPLD could not be CO2 because the cap would have insufficient strength to maintain its current shape over the long periods of time implied by crater dating [5]. Thus, CO2 could not be abundant in the SPLD. That was the state of knowledge until 2011, when data from the Shallow Radar (SHARAD) instrument on Mars Reconnaissance Orbiter were used to deter- mine that massive CO2 deposits are buried beneath the surface of the SPRC [6]. Using geophysical arguments and layer geometry, [6] and then [7] determined that CO2 ice up to 1000 m thick had been deposited in the spiral depressions of the SPLD before being buried.