Feasibility of Using Lunar Magnetic Fields to Control Cubesat Attitude
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New Views of the Moon Enabled by Combined Remotely Sensed and Lunar Sample Data Sets, a Lunar Initiative
New Views of the Moon Enabled by Combined Remotely Sensed and Lunar Sample Data Sets, A Lunar Initiative Using the hand tool on your Reader, click on the links below to view that particular section of the proposal. Proposal Summary Scientific/Technical/Management Objectives and Expected Significance Background and Impact Approach and Methodology: The Role of Integration in Fundamental Problems of Lunar Geoscience Workshop 2: New Views of the Moon II: Understanding the Moon Through the Integration of Diverse Datasets. Abstract Volume and Subsequent Publications Statement of Relevance Work Plan Potential Workshop (2000): Thermal and Magmatic Evolution of the Moon Potential Workshop (2001): Early Lunar Differentiation, Core Formation, Effects of Early Planetesimal Impacts, and the Origin of the Moon’s Global Asymmetry Potential Workshop (2002): Selection of Sites for Future Sample Return Capstone Publication Timeline for the New Views of the Moon Initiative Personnel: Initiative Management and Proposal Management References Facilities: The LPI Appendix 1. Workshop on New Views of the Moon: Integrated Remotely Sensed, Geophysical, and Sample Datasets. List of presentations Appendix 2. LPSC 30 (1999) special sessions related to the Lunar Initiative. List of presentations (oral and poster) Appendix 3. Lunar Initiative Steering Committee Web Note: This is the text of a proposal submitted on behalf of the Lunar Science Community to support ongoing workshops and activities associated with the CAPTEM Lunar Initiative. It was submitted in May, 1999, in response to the ROSS 99 NRA, which solicits such proposals to be submitted to the relevant research programs. This proposal was submitted jointly to Cosmo- chemistry and Planetary Geology and Geophysics. -
Atlas V Launches LRO/LCROSS Mission Overview
Atlas V Launches LRO/LCROSS Mission Overview Atlas V 401 Cape Canaveral Air Force Station, FL Space Launch Complex-41 AV-020/LRO/LCROSS United Launch Alliance is proud to be a part of the Lunar Reconnaissance Orbiter (LRO) and the Lunar Crater Observation and Sensing Satellite (LCROSS) mission with the National Aeronautics and Space Administration (NASA). The LRO/LCROSS mission marks the sixteenth Atlas V launch and the seventh flight of an Atlas V 401 configuration. LRO/LCROSS is a dual-spacecraft (SC) launch. LRO is a lunar orbiter that will investigate resources, landing sites, and the lunar radiation environment in preparation for future human missions to the Moon. LCROSS will search for the presence of water ice that may exist on the permanently shadowed floors of lunar polar craters. The LCROSS mission will use two Lunar Kinetic Impactors, the inert Centaur upper stage and the LCROSS SC itself, to produce debris plumes that may reveal the presence of water ice under spectroscopic analysis. My thanks to the entire Atlas team for its dedication in bringing LRO/LCROSS to launch, and to NASA for selecting Atlas for this ground-breaking mission. Go Atlas, Go Centaur, Go LRO/LCROSS! Mark Wilkins Vice President, Atlas Product Line Atlas V Launch History Flight Config. Mission Mission Date AV-001 401 Eutelsat Hotbird 6 21 Aug 2002 AV-002 401 HellasSat 13 May 2003 AV-003 521 Rainbow 1 17 Jul 2003 AV-005 521 AMC-16 17 Dec 2004 AV-004 431 Inmarsat 4-F1 11 Mar 2005 AV-007 401 Mars Reconnaissance Orbiter 12 Aug 2005 AV-010 551 Pluto New Horizons 19 Jan 2006 AV-008 411 Astra 1KR 20 Apr 2006 AV-013 401 STP-1 08 Mar 2007 AV-009 401 NROL-30 15 Jun 2007 AV-011 421 WGS SV-1 10 Oct 2007 AV-015 401 NROL-24 10 Dec 2007 AV-006 411 NROL-28 13 Mar 2008 AV-014 421 ICO G1 14 Apr 2008 AV-016 421 WGS-2 03 Apr 2009 Payload Fairing Number of Solid Atlas V Size (meters) Rocket Boosters Flight/Configuration Key AV-XXX ### Number of Centaur Engines 3-digit Tail Number 3-digit Configuration Number LRO Overview LRO is the first mission in NASA’s planned return to the Moon. -
Protons in the Near Lunar Wake Observed by the SARA Instrument on Board Chandrayaan-1
FUTAANA ET AL. PROTONS IN DEEP WAKE NEAR MOON 1 Protons in the Near Lunar Wake Observed by the SARA 2 Instrument on Board Chandrayaan-1 3 Y. Futaana, 1 S. Barabash, 1 M. Wieser, 1 M. Holmström, 1 A. Bhardwaj, 2 M. B. Dhanya, 2 R. 4 Sridharan, 2 P. Wurz, 3 A. Schaufelberger, 3 K. Asamura 4 5 --- 6 Y. Futaana, Swedish Institute of Space Physics, Box 812, Kiruna, SE-98128, Sweden. 7 ([email protected]) 8 9 10 1 Swedish Institute of Space Physics, Box 812, Kiruna, SE-98128, Sweden 11 2 Space Physics Laboratory, Vikram Sarabhai Space Center, Trivandrum 695 022, India 12 3 Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland 13 4 Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Japan 14 Index Terms 15 6250 Moon 16 5421 Interactions with particles and fields 17 2780 Magnetospheric Physics: Solar wind interactions with unmagnetized bodies 18 7807 Space Plasma Physics: Charged particle motion and acceleration 19 Abstract 20 Significant proton fluxes were detected in the near wake region of the Moon by an ion mass 21 spectrometer on board Chandrayaan-1. The energy of these nightside protons is slightly higher than 22 the energy of the solar wind protons. The protons are detected close to the lunar equatorial plane at 23 a 140˚ solar zenith angle, i.e., ~50˚ behind the terminator at a height of 100 km. The protons come 24 from just above the local horizon, and move along the magnetic field in the solar wind reference 25 frame. -
Global Mapping of Elemental Abundance on Lunar Surface by SELENE Gamma-Ray Spectrometer
Lunar and Planetary Science XXXVI (2005) 2092.pdf Global Mapping of elemental abundance on lunar surface by SELENE gamma-ray spectrometer. 1M. -N. Kobayashi, 1A. A. Berezhnoy, 6C. d’Uston, 1M. Fujii, 1N. Hasebe, 3T. Hiroishi, 4H. Kaneko, 1T. Miyachi, 5K. Mori, 6S. Maurice, 4M. Nakazawa, 3K. Narasaki, 1O. Okudaira, 1E. Shibamura, 2T. Takashima, 1N. Yamashita, 1Advanced Research Institute of Sci.& Eng., Waseda Univ., 3-4-1, Okubo, Shinjuku-ku, Tokyo, 169-8555, Japan, (masa- [email protected]), 2Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, 3Niihama Works, Sumitomo Heavy Industry Ltd., Niihama, Ehime, Japan, Moriya Works, 4Meisei Electric Co., Ltd., 3-249-1, Yuri-ga-oka, Moriya-shi, Ibaraki, 302-0192, 5Clear Pulse Co., 6-25-17, Chuo, Ohta-ku, Tokyo, Japan, 143-0024, 6Centre d’Etude Spatiale des Rayonnements, CNRS/UPS, Colonel Roche, B.P 4346, France. Introduction: Elemental composition on the sur- face of a planet is very important information for solv- ing the origin and the evolution of the planet and also very necessary for understanding the origin and the evolution of solar system. Planetary gamma-ray spec- troscopy is extremely powerful approach for the ele- mental composition measurement. Gamma-ray spec- trometer (GRS) will be on board SELENE, advanced lunar polar orbiter, and employ a large-volume Ge detector of 252cc as the main detector [1]. SELENE GRS is, therefore, approximately twice more sensitiv- ity than Lunar Prospector GRS, four times more sensi- Figure 1: The schematic drawing of SELENE Gamma- tive than APOLLO GRS. -
Mission Design for the Lunar Reconnaissance Orbiter
AAS 07-057 Mission Design for the Lunar Reconnaissance Orbiter Mark Beckman Goddard Space Flight Center, Code 595 29th ANNUAL AAS GUIDANCE AND CONTROL CONFERENCE February 4-8, 2006 Sponsored by Breckenridge, Colorado Rocky Mountain Section AAS Publications Office, P.O. Box 28130 - San Diego, California 92198 AAS-07-057 MISSION DESIGN FOR THE LUNAR RECONNAISSANCE ORBITER † Mark Beckman The Lunar Reconnaissance Orbiter (LRO) will be the first mission under NASA’s Vision for Space Exploration. LRO will fly in a low 50 km mean altitude lunar polar orbit. LRO will utilize a direct minimum energy lunar transfer and have a launch window of three days every two weeks. The launch window is defined by lunar orbit beta angle at times of extreme lighting conditions. This paper will define the LRO launch window and the science and engineering constraints that drive it. After lunar orbit insertion, LRO will be placed into a commissioning orbit for up to 60 days. This commissioning orbit will be a low altitude quasi-frozen orbit that minimizes stationkeeping costs during commissioning phase. LRO will use a repeating stationkeeping cycle with a pair of maneuvers every lunar sidereal period. The stationkeeping algorithm will bound LRO altitude, maintain ground station contact during maneuvers, and equally distribute periselene between northern and southern hemispheres. Orbit determination for LRO will be at the 50 m level with updated lunar gravity models. This paper will address the quasi-frozen orbit design, stationkeeping algorithms and low lunar orbit determination. INTRODUCTION The Lunar Reconnaissance Orbiter (LRO) is the first of the Lunar Precursor Robotic Program’s (LPRP) missions to the moon. -
Analysis and Design of Integrated Magnetorquer Coils for Attitude Control of Nanosatellites
Analysis and Design of Integrated Magnetorquer Coils for Attitude Control of Nanosatellites Hassan Ali*, M. Rizwan Mughal*†, Jaan Praks †, Leonardo M. Reyneri+, Qamar ul Islam* * †Department of Electrical Engineering, Institute of Space Technology, Islamabad, Pakistan, †Department of Electronic and Nano Engineering, Aalto University, Espoo, Finland +Department of Electronics and Telecommunications, Politecnico di Torino, Torino, Italy Abstract—The nanosatellites typically use either magnetic rods or become a challenge. In order to stabilize the tumbling satellite, coil to generate magnetic moment which consequently interacts the attitude control system is very necessary. There are two with the earth magnetic field to generate torque. In this research, types of attitude control systems i.e. passive and active [1-6]. we present a novel design which integrates printed embedded The permanent magnetics and the gravity gradients are passive coils, compact coils and magnetic rods in a single package which type. They being cost effective, consume no power but no is also complaint with 1U CubeSat. These options provide maximum flexibility, redundancy and scalability in the design. pointing accuracy is achieved using these types of actuators. The printed coils consume no extra space because the copper The majority of the missions these days require better pointing traces are printed in the internal layers of the printed circuit accuracies. The active control systems are typically used for in board (PCB). Moreover, they can be made reconfigurable by missions where better pointing accuracy is desired. The printing them into certain layers of the PCB, allowing the user to magnetorquer is a good option to control the attitude of select any combination of series and parallel coils for optimized nanosatellite. -
Research and Educational Space Activities at AAU
Research and Educational Space Activities at AAU Jens Dalsgaard Nielsen Axel Michelsen Martin Kragelund August 08 1 O 1997 Champ ACS study Danish Satellite Program (cont.) - Intelligent Autonomous O 2000 Rømer Detailed Design Systems (IAS) specialization CubeSat Def. Phase - TEAM AAU CubeSat 2001 O BEST summer school (25 sts.) 2002 O Advanced ACS+GPS -AAU CubeSat launched (75 sts. 2003 O - AAUSAT-II (+45 sts.) SSETI-Express (ESA) 2004 O Baumanetz (Russia) Baumanetz Launch STEC05 Conference 2005 O SSETI-Express Launch AAUSAT-II 2008 AAUSAT3 2 Ørsted – the first danish satellite 3 Satellites at Aalborg University – Ørsted •Danish National Satellite Project • •Started: 1993 •Launch: February 1999 •Dimension: 34 cm x 45 cm x 68 cm •Mass: 62 kg •Payload: Magnetometers •AAU main delivery: ACS 4 Ørsted purpose High precision measurement of earth magnetic field over place and time Coil based attitude Control 100% danish project 20 millionUS$ Launched 1999 Still in full operation • AAU ADCS – attitude determination and control 5 ACS control structure 6 AAU achievement Responsibility for analysis, design, implementation, verification of the ACDS system First proven control algorithm design based on use of only magnetorquer concept. Use of modular and hierarchical approach to facilitate easy verification and test. Several related Ph.D. work was conducted (ACS , ADS, Fault Diagnosis, Supervisory control) Has been complete success, In operation more than 7 years IT WAS HER IT ALL STARTED ! 7 ! 8 The Aalborg way of making Engineers • Problem and Project Based Learning: • Solve a engineering problem within semester theme • Receive lectures for learning new theory and technology • Mantra: Best Learning is by “Just Doing” • Math, Theory etc lectures them selves dont give anything • Same goes for Control, Realtime Systems, Power Eng,.. -
Comparison of Magnetorquer Performance
Comparison of Magnetorquer Performance Max Pastena, James Barrington-Brown Presentation to CubeSat Workshop 8th August 2010 Background • Focused on the development and marketing of products for the Space Segment • Focus is on satellite sub-system design and manufacture • Growing number of license agreements with small satellite and sub-system manufactures • Worldwide customer base Magnetorquer Function Magnetorquers produce a torque on the spacecraft by interacting with the Earth’s Magnetic field: T=MxB Advantages: Disadvantages: •Low power consumption •Low Torque •Low volume •No Torque along Earth’s magnetic field •Simplicity and reliability •Difficult beyond LEO •Simple operation Suitable for: •Initial De tumbling due to the low power consumption and very low power availability during the phase •Reaction Wheel (if any) unloading •Two axes control of momentum stabilized satellites (Momentum wheel) But also............ •Three axis control when low power and volume is available on board the spacecraft •High efficiency manoeuvres Attitude Manoeuvres Necessary Dipole Moment to perform a 90deg manoeuvre @400km vs requested time in the best case i.e. Earth’s magnetic field perpendicular to the rotation axis •0.2 Am2 Dipole Moment Magnetic Torquer is a good compromise to have good agility for 1U, 2U and 3U cubesat •Magnetic Torquer with dipole moment <0.06Am2 are not suitable for attitude maneuvers De-tumbling Necessary Dipole Moment to perform the detumbling @ 400km vs requested time •0.2 Am2 Dipole Moment Magnetic Torquer is a good compromise -
Planetary Science
Mission Directorate: Science Theme: Planetary Science Theme Overview Planetary Science is a grand human enterprise that seeks to discover the nature and origin of the celestial bodies among which we live, and to explore whether life exists beyond Earth. The scientific imperative for Planetary Science, the quest to understand our origins, is universal. How did we get here? Are we alone? What does the future hold? These overarching questions lead to more focused, fundamental science questions about our solar system: How did the Sun's family of planets, satellites, and minor bodies originate and evolve? What are the characteristics of the solar system that lead to habitable environments? How and where could life begin and evolve in the solar system? What are the characteristics of small bodies and planetary environments and what potential hazards or resources do they hold? To address these science questions, NASA relies on various flight missions, research and analysis (R&A) and technology development. There are seven programs within the Planetary Science Theme: R&A, Lunar Quest, Discovery, New Frontiers, Mars Exploration, Outer Planets, and Technology. R&A supports two operating missions with international partners (Rosetta and Hayabusa), as well as sample curation, data archiving, dissemination and analysis, and Near Earth Object Observations. The Lunar Quest Program consists of small robotic spacecraft missions, Missions of Opportunity, Lunar Science Institute, and R&A. Discovery has two spacecraft in prime mission operations (MESSENGER and Dawn), an instrument operating on an ESA Mars Express mission (ASPERA-3), a mission in its development phase (GRAIL), three Missions of Opportunities (M3, Strofio, and LaRa), and three investigations using re-purposed spacecraft: EPOCh and DIXI hosted on the Deep Impact spacecraft and NExT hosted on the Stardust spacecraft. -
The Lunar Dust-Plasma Environment Is Crucial
TheThe LunarLunar DustDust --PlasmaPlasma EnvironmentEnvironment Timothy J. Stubbs 1,2 , William M. Farrell 2, Jasper S. Halekas 3, Michael R. Collier 2, Richard R. Vondrak 2, & Gregory T. Delory 3 [email protected] Lunar X-ray Observatory(LXO)/ Magnetosheath Explorer (MagEX) meeting, Hilton Garden Inn, October 25, 2007. 1 University of Maryland, Baltimore County 2 NASA Goddard Space Flight Center 3 University of California, Berkeley TheThe ApolloApollo AstronautAstronaut ExperienceExperience ofof thethe LunarLunar DustDust --PlasmaPlasma EnvironmentEnvironment “… one of the most aggravating, restricting facets of lunar surface exploration is the dust and its adherence to everything no matter what kind of material, whether it be skin, suit material, metal, no matter what it be and it’s restrictive friction-like action to everything it gets on. ” Eugene Cernan, Commander Apollo 17. EvidenceEvidence forfor DustDust AboveAbove thethe LunarLunar SurfaceSurface Horizon glow from forward scattered sunlight • Dust grains with radius of 5 – 6 m at about 10 to 30 cm from the surface, where electrostatic and gravitational forces balance. • Horizon glow ~10 7 too bright to be explained by micro-meteoroid- generated ejecta [Zook et al., 1995]. Composite image of morning and evening of local western horizon [Criswell, 1973]. DustDust ObservedObserved atat HighHigh AltitudesAltitudes fromfrom OrbitOrbit Schematic of situation consistent with Apollo 17 observations [McCoy, 1976]. Lunar dust at high altitudes (up to ~100 km). 0.1 m-scale dust present Gene Cernan sketches sporadically (~minutes). [McCoy and Criswell, 1974]. InIn --SituSitu EvidenceEvidence forfor DustDust TransportTransport Terminators Berg et al. [1976] Apollo 17 Lunar Ejecta and Meteorites (LEAM) experiment. PossiblePossible DustyDusty HorizonHorizon GlowGlow seenseen byby ClementineClementine StarStar Tracker?Tracker? Above: image of possible horizon glow above the lunar surface. -
The Moon and Eclipses
Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole. -
Prototype Design and Mission Analysis for a Small Satellite Exploiting Environmental Disturbances for Attitude Stabilization
Calhoun: The NPS Institutional Archive Theses and Dissertations Thesis and Dissertation Collection 2016-03 Prototype design and mission analysis for a small satellite exploiting environmental disturbances for attitude stabilization Polat, Halis C. Monterey, California: Naval Postgraduate School http://hdl.handle.net/10945/48578 NAVAL POSTGRADUATE SCHOOL MONTEREY, CALIFORNIA THESIS PROTOTYPE DESIGN AND MISSION ANALYSIS FOR A SMALL SATELLITE EXPLOITING ENVIRONMENTAL DISTURBANCES FOR ATTITUDE STABILIZATION by Halis C. Polat March 2016 Thesis Advisor: Marcello Romano Co-Advisor: Stephen Tackett Approved for public release; distribution is unlimited THIS PAGE INTENTIONALLY LEFT BLANK REPORT DOCUMENTATION PAGE Form Approved OMB No. 0704–0188 Public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instruction, searching existing data sources, gathering and maintaining the data needed, and completing and reviewing the collection of information. Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing this burden, to Washington headquarters Services, Directorate for Information Operations and Reports, 1215 Jefferson Davis Highway, Suite 1204, Arlington, VA 22202-4302, and to the Office of Management and Budget, Paperwork Reduction Project (0704-0188) Washington, DC 20503. 1. AGENCY USE ONLY 2. REPORT DATE 3. REPORT TYPE AND DATES COVERED (Leave blank) March 2016 Master’s thesis 4. TITLE AND SUBTITLE 5. FUNDING NUMBERS PROTOTYPE DESIGN AND MISSION ANALYSIS FOR A SMALL SATELLITE EXPLOITING ENVIRONMENTAL DISTURBANCES FOR ATTITUDE STABILIZATION 6. AUTHOR(S) Halis C. Polat 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) 8. PERFORMING Naval Postgraduate School ORGANIZATION REPORT Monterey, CA 93943-5000 NUMBER 9.