Interlaced Optimal-REQUEST and Unscented Kalman Filtering For

Total Page:16

File Type:pdf, Size:1020Kb

Interlaced Optimal-REQUEST and Unscented Kalman Filtering For Chinese Journal of Aeronautics, 2013,26(2): 449–455 Chinese Society of Aeronautics and Astronautics & Beihang University Chinese Journal of Aeronautics [email protected] www.sciencedirect.com Interlaced optimal-REQUEST and unscented Kalman filtering for attitude determination Quan Wei *, Xu Liang, Zhang Huijuan, Fang Jiancheng Science and Technology on Inertial Laboratory, Key Laboratory of Fundamental Science for National Defense-Novel Inertial Instrument & Navigation System Technology, Beihang University, Beijing 100191, China Received 25 November 2011; revised 13 February 2012; accepted 22 May 2012 Available online 7 March 2013 KEYWORDS Abstract Aimed at low accuracy of attitude determination because of using low-cost components Attitude determination; which may result in non-linearity in integrated attitude determination systems, a novel attitude Hybrid simulation; determination algorithm using vector observations and gyro measurements is presented. The Interlaced filtering; various features of the unscented Kalman filter (UKF) and optimal-REQUEST (quaternion estima- Optimal-REQUEST; tor) algorithms are introduced for attitude determination. An interlaced filtering method is pre- Unscented Kalman filter sented for the attitude determination of nano-spacecraft by setting the quaternion as the attitude representation, using the UKF and optimal-REQUEST to estimate the gyro drifts and the quaternion, respectively. The optimal-REQUEST and UKF are not isolated from each other. When the optimal-REQUEST algorithm estimates the attitude quaternion, the gyro drifts are estimated by the UKF algorithm synchronously by using the estimated attitude quaternion. Furthermore, the speed of attitude determination is improved by setting the state dimension to three. Experimen- tal results show that the presented method has higher performance in attitude determination compared to the UKF algorithm and the traditional interlaced filtering method and can estimate the gyro drifts quickly. ª 2013 Production and hosting by Elsevier Ltd. on behalf of CSAA & BUAA. 1. Introduction including accuracy and speed, not only depends on the capa- bility of inboard sensors, but also relies on the performance High-accuracy attitude determination is required to achieve of attitude determination algorithms. Besides the accuracy, high-accuracy attitude control and attitude stability for the better the observation ability is, the quicker the speed of nano-spacecraft. As such, attitude determination is important attitude determination is, especially, for the new-generation to any spacecraft. The performance of attitude determination, smart small satellites. A typical system for attitude determina- tion of nano-spacecraft comprises several gyroscopes and a vector-sensor. The development of new sensor technology * Corresponding author. Tel.: +86 10 82339013. promotes the integration of micro-electro-mechanical system E-mail address: [email protected] (W. Quan). (MEMS) gyroscopes and a complementary metal oxide Peer review under responsibility of Editorial Committe of CJA. semiconductor (CMOS) transistor active pixel sensor (APS) as a star sensor, and the quick development of a high performance strapdown stellar-inertial integrated attitude Production and hosting by Elsevier determination system,1 which is especially suitable for the high 1000-9361 ª 2013 Production and hosting by Elsevier Ltd. on behalf of CSAA & BUAA. http://dx.doi.org/10.1016/j.cja.2013.02.023 450 W. Quan et al. performance attitude determination of nano-spacecraft.2,3 The UKF and optimal-REQUEST, an interlaced filtering method attitude determination algorithms based on state estimation is presented by setting the quaternion as the attitude represen- and vector observation are most effective because of their high tation, using the UKF and optimal-REQUEST to estimate the accuracy and efficiency.4,5 gyro drifts and the quaternion respectively. When the optimal- At present, there are many real-time attitude estimation REQUEST algorithm is used to estimate the attitude quater- algorithms for spacecraft based on state estimation. The ex- nion, the gyro drifts are estimated by the UKF algorithm only tended Kalman filter (EKF) method is widely used in nonlin- using the three-dimensional state variable which is much ear systems.6–10 However, it needs to calculate the Jacobian quicker than in the case of six dimensions.18 Meanwhile, the matrix for the linearization of nonlinear systems, which results attitude quaternion derived from the optimal-REQUEST, is in low accuracy and output frequency. The unscented Kalman adopted when the UKF estimates the gyro drifts. Further- filter (UKF) method was presented by Juliear and Uhlman in more, the state dimension is only set to three to improve the 1995, in which they used special sample points to fit the non- speed of attitude determination. This method not only has linear state and let the mean and variance of sampling points higher performance of attitude determination, but also quickly equal to those of the states at the sampling moment. Based estimates gyro drifts. on such sampling points in the nonlinear system, the corre- sponding transformation sampling points were obtained, dur- 2. System model ing which the corresponding mean and variance were calculated. For non-linearized systems, this method can 2.1. Gyro measurement model achieve higher accuracy of filtering than the EKF method.11,12 Among attitude determination methods based on vector Supposing that the three sensitive axes of three MEMS gyro- observation, the quaternion estimator (QUEST) method13 is scopes are respectively parallel to the three body-axes of a a very popular algorithm for single frame. However, it shows spacecraft, a general gyroscope model is given by two disadvantages. One is that at least two simultaneous mea- x~ k ¼ xk þ bk þ gv;k ð1Þ surements are needed to estimate attitude completely. The other is that the information of previous measurements is lost bkþ1 ¼ bk þ gu;k ð2Þ entirely. To solve the above problems, the recursive quaternion where x~ is the gyroscope measurement, x the attitude angu- estimator (REQUEST) method was presented by Bar-Itzhack k k lar rate of the gyro input axis, b the gyro drift vector; g and in 1996,14 which was actually a recursive QUEST method. k v;k gu;k are independent zero-mean Gaussian white-noise pro- The K-matrix is sequentially propagated and updated as state 2 2 cesses, and the variance of gv;k and gu;k are rv 1 and ru1 respec- variables. The REQUEST method is suboptimal since the T tively, 1 ¼½111 . propagation noise is suppressed using a fading memory factor. In 2004, the optimal-REQUEST method was presented by 2.2. Star sensor measurement model Choukroun et al.15, in which the REQUEST algorithm was embedded in the framework of a Kalman filter. For that pur- As a high-accuracy vector sensor, the measurement model of pose, the K-matrix elements are modeled as state variables and the star sensor is defined by model equations for the process and the measurement of the K-matrix are developed. The attitude quaternion is then iso- bk ¼ AðqkÞrk þ dbk ð3Þ lated from the estimated K-matrix. The optimal-REQUEST where rk is the stellar reference vector in inertial coordinates, method has the advantage of sequentially processing the mea- which can be obtained from the astronomical ephemeris; bk sured information. It can estimate the attitude even when the measurement vector containing noise in the star sensor acquiring a single vector measurement at each observation coordinates, which are supposed to be the same as the body time, but under the condition of non-collinearity between at coordinates of the spacecraft; dbk the noise of the measurement least two observed lines-of-sight. This method cannot estimate and satisfied by parameters other than attitude, and even then it cannot esti- EðdbÞ¼0 mate and compensate for gyroscope drifts, which results in ð4Þ Eðdb Á dbTÞ¼r2ðI À bbTÞ the divergence of the optimal-REQUEST. 3 2 The EKF and UKF methods can estimate not only attitude where I3 is the third-order identity matrix and r the variance parameters, but also gyro drifts. However, these methods re- of the measurement noise. quire measurements from the star sensor that are disposed AðqkÞ is the attitude matrix from the inertial coordinates to sequentially. Therefore, a traditional interlaced filtering meth- the spacecraft body coordinates, and can be described as a T T od based on the EKF, QUEST, and optimal-REQUEST for function of the quaternion qk ¼½qk q4k : 16 micro-spacecraft was presented by Yu and Fang in 2005 2 T T AðqkÞ¼ððq4kÞ À qk qkÞI3 þ 2qkqk À 2q4k½qk ð5Þ and an adaptive interlaced filtering method for attitude deter- T mination of nano-spacecraft was presented by Quan et al. in where qk ¼½q1k q2k q3k and q4k are the vector and scale 17 2008. However, the optimal-REQUEST algorithm is only part of the quaternion, respectively; ½qk denotes the cross- an approximate algorithm and contains errors beyond those product matrix associated with the vector qk . of the EKF and UKF for attitude information. There is six- 2.3. Spacecraft attitude kinematical model dimensional state variable for filtering models in Refs. 16,17, which leads to low speed of attitude determination. However, using the EKF and UKF directly with the Spacecraft attitude is described using the quaternion qk in the 14 quaternion attitude parameterization yields a non-unit norm body coordinates relative to the inertial coordinates , and the quaternion estimate. According to the various features
Recommended publications
  • Deep Space Craft an Overview of Interplanetary Flight Dave Doody Deep Space Craft an Overview of Interplanetary Flight
    Deep Space Craft An Overview of Interplanetary Flight Dave Doody Deep Space Craft An Overview of Interplanetary Flight Published in association with PPraxisraxis PPublishiublishingng Chichester, UK Dave Doody NASA Jet Propulsion Laboratory (Caltech) Pasadena California USA Front cover illustrations: (Upper) Artist's rendition of the Dawn spacecraft operating its ion propulsion system upon arrival at the main-belt asteroid Vesta in 2011. Image courtesy McRel, Mid-continent Research for Education and Learning. (Next lower) Artist's concept of the Phoenix lander operating in the Martian Arctic, as it did from May to November 2008. Image courtesy University of Arizona. (Lower left) Artist's concept of the Cassini spacecraft as it operates in Saturn orbit July 2004 through the present day. Back cover illustrations: (Left) A near-duplicate of the Mars Phoenix lander used in developing command sequences before being sent to the spacecraft. Here, members of the Robotic Arm Engineering Team test the arm's motorized raft in the Payload Interoperability Testbed at the University of Arizona, Tucson in July 2008. Image courtesy University of Arizona. (Right) Rob Manning, Chief Engineer of NASA's Mars Exploration Program, cheers along with other team members as the ®rst images from rover Spirit come back from Mars. Courtesy NASA/Bill Ingalls. SPRINGER±PRAXIS BOOKS IN ASTRONAUTICAL ENGINEERING SUBJECT ADVISORY EDITOR: John Mason M.B.E., B.Sc., M.Sc., Ph.D. ISBN 978-3-540-89509-1 Springer Berlin Heidelberg New York Springer is part of Springer-Science + Business Media (springer.com) Library of Congress Control Number: 2008943657 Apart from any fair dealing for the purposes of research or private study, or criticism or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be reproduced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licences issued by the Copyright Licensing Agency.
    [Show full text]
  • Mp-Avt-171-09
    UNCLASSIFIED/UNLIMITED Attitude Determination and Control of Future Small Satellites H. Ersin Soken, A. Rustem Aslan and Chingiz Hajiyev Aeronautics and Astronautics Faculty Istanbul Technical University Istanbul, TURKEY [email protected]/[email protected]/[email protected] ABSTRACT As well as other subsystems, Attitude Determination and Control System (ADCS) development is a challenging process for small satellites because of design limitations, such as size, weight and the power consumption. Besides, if they are thought in a concept with military missions, then the requirement for a high attitude pointing accuracy is something certain. Works on the effective attitude determination and control methods for small satellites can be accepted as a part of this struggle. In this paper, problems that are met during ADCS development phase for future small satellites are stated and possible solutions are suggested. 1.0 INTRODUCTION Since their first appearance, small satellites have begun to play a more and more important role in space researches and today, they have a certain share in astronautic applications, especially about new technology demonstration. Because of many advantages such as low investment and operational costs, enabling COTS (commercial of the shell) technology in space, short system development periods etc. they have been highly preferred to their larger competitors. More than 400 micro satellites launched in the last 20 years is a good proof for that [1]. Mini Satellite 100-500 kg Micro Satellite 10-100 kg Nano Satellite 1-10 kg Pico Satellite 0.1-1 kg Table 1: Small satellite classification. Although they have been investigated in depth, there are still many steps to be taken in the development phase of these types of satellites and an important field to be examined is their attitude determination and control systems (ADCS).
    [Show full text]
  • JPL Has Once Again Closed out the Year in Style. Less Than a Month
    Jet DECEMBER Propulsion 2006 Laboratory VOLUME 36 NUMBER 17 2006 INREVIEW By Mark Whalen JPL has once again closed out the year in style. Less than a month after the announcement that Mars Global Surveyor has likely finished its operat- ing career, the most productive Mars mission in history came through with the explosive news in December that its photographs have revealed bright new deposits in two gullies on Mars that suggest water carried sediment A gully as imaged by Mars Global Surveyor liquid water was involved in its genesis. through them sometime during the is shown at left in August 1999 and at right However, this observation and a similar in September 2005. The images show the light-toned flow in Terra Sirenum to- past seven years. southeast wall of an unnamed crater in the gether show that some gully sites are Centauri Montes region. No light-toned indeed changing today, providing tanta- In the meantime, the Laboratory con- deposit was present in August 1999, but lizing evidence there might be sources of appeared by February 2004. The new light- liquid water beneath the surface of Mars tinues its studies of the solar system toned flow, by itself, does not prove that right now. and beyond, with 15 spacecraft, two rovers, seven science instruments and three Earth observatories all meeting or exceeding their require- ments. Following are some highlights, chronologically, from 2006. Continued on page 2 2 niverse CONT'D U 2006INREVIEW A new image from the Galaxy Evolution Explorer completed MARCH a multi-wavelength, neon-col- Cassini found what may be evidence ored portrait of the enormous of liquid water reservoirs that erupt in Cartwheel galaxy after a smaller Yellowstone-like geysers on Saturn’s galaxy plunged through it, trigger- moon Enceladus.
    [Show full text]
  • CONSTELLATION an Official Publication of the Bucks-Mont Astronomical Association, Inc
    CONSTELLATION An Official Publication of the Bucks-Mont Astronomical Association, Inc. April/May/June Chris Sommers and VOLUME 23, Issue No. 2 2008 Scott Petersen, Editors © BMAA, Inc. 2008 BMAA News BMAA has had a busy spring, despite almost all of our StarWatches being clouded out. In April we attended an open house at Montgomery County Community College’s Observatory, and Dwight Dulsky and Lou Vittorio made presentations at Upper Moreland Middle School. In May we had our Astronomy Day exhibit set up in Peddler’s Village in New Hope and Dwight Dulsky led the effort at the Bucks County Science Teachers Association’s semi- annual meeting in Doylestown. We have a lot to look forward to this summer, including the summer triangle, summer globular clusters (see Orum Stringer’s List in this Issue) including M56 as described by Alan Pasicznyk, jovial Jupiter and its parade of double shadow transits, and multiple occultations of Antares by the Moon. Happy observing BMAAers!!! Summer Planetary Jewel: Jovial Jupiter Courtesy of Steve Olson BMAA Gophers Position Name President Dwight Dulsky Vice President Bernie Kosher Treasurer Ed Radomski Secretary Herb Borteck Star Watch Coordinator George Reagan Constellation Editors Chris Sommers and Scott Petersen Webmaster Jim Moyer For More Information About BMAA Go to www.bma2.org. 1 ****** Alan's Collection of Excellent Deep Sky Objects Through a 4.5 Inch Newtonian. Raisins in a Pie", M56 ¾ Alan Pasicznyk When I finally located the dim glow of M56 for the first time on July 15, 1991, I was expecting to find nothing more than "just another globular cluster" to log into my list of Messier objects.
    [Show full text]
  • FY 2002 Performance and Accountability Report FY 2002 Was the Second Year of Continuous, Permanent Human Habitation of the International Space Station
    National Aeronautics and Space Administration Fiscal Year 2002 Performance and Accountability Report Contents NASAVision and Mission Part I: Management’s Discussion and Analysis Transmittal Letter 6Message From the Administrator 8Reliability and Completeness of Financial and Performance Data 9Federal Managers’ Financial Integrity Act Statement of Assurance Overview 13Mission 13Organizational Structure 15Highlights of Performance Goals and Results 53Actions Planned to Achieve Key Unmet Goals 53Looking Forward 55Analysis of Financial Statements 55Systems, Controls, and Legal Compliance 56Integrity Act Material Weaknesses and Non-Conformances 58Additional Key Management Information 58The President’s Management Agenda 71Management Challenges and High-Risk Areas Part II: Performance 84Summary of Annual Performance by Strategic Goals Performance Discussion 87Space Science 99Earth Science 109Biological and Physical Research 117Human Exploration and Development of Space 123Aerospace Technology Supporting Data 133Space Science 145Earth Science 173Biological and Physical Research 185Human Exploration and Development of Space 193Aerospace Technology 209Manage Strategically Crosscutting Process 219Provide Aerospace Products and Capabilities Crosscutting Process 223Generate Knowledge Crosscutting Process 225Communicate Knowledge Crosscutting Process Part III: Financial 233Letter From the Chief Financial Officer Financial Statements and Related Auditor’s Reports 236Financial Overview 238Financial Statements 267Auditor’s Reports NASA Office of Inspector
    [Show full text]
  • Mars Earth Return Vehicle (MERV) Propulsion Options
    Mars Earth Return Vehicle (MERV) Propulsion Options Steven R. Oleson,1 Melissa L. McGuire,2 Laura Burke,3 James Fincannon,4 Joe Warner,5 Glenn Williams,6 and Thomas Parkey7 NASA Glenn Research Center, Cleveland, Ohio 44135 Tony Colozza,8 Jim Fittje,9 Mike Martini,10 and Tom Packard11 Analex Corporation, Cleveland, Ohio 44135 Joseph Hemminger12 N&R Engineering, Cleveland, Ohio 44135 John Gyekenyesi13 ASRC Engineering, Cleveland, Ohio 44135 The COMPASS Team was tasked with the design of a Mars Sample Return Vehicle. The current Mars sample return mission is a joint National Aeronautics and Space Administration (NASA) and European Space Agency (ESA) mission, with ESA contributing the launch vehicle for the Mars Sample Return Vehicle. The COMPASS Team ran a series of design trades for this Mars sample return vehicle. Four design options were investigated: Chemical Return /solar electric propulsion (SEP) stage outbound, all-SEP, all chemical and chemical with aerobraking. The all-SEP and Chemical with aerobraking were deemed the best choices for comparison. SEP can eliminate both the Earth flyby and the aerobraking maneuver (both considered high risk by the Mars Sample Return Project) required by the chemical propulsion option but also require long low thrust spiral times. However this is offset somewhat by the chemical/aerobrake missions use of an Earth flyby and aerobraking which also take many months. Cost and risk analyses are used to further differentiate the all-SEP and Chemical/Aerobrake options. 1COMPASS Lead, DSB0, 21000 Brookpark Road, and AIAA Senior Member. 2COMPASS Integration Lead, DSB0, 21000 Brookpark Road, non-member. 3Mission Designer, DSB0, 21000 Brookpark Road, and Non-Member.
    [Show full text]
  • Status of Solar Sail Propulsion: Moving Toward an Interstellar Probe
    https://ntrs.nasa.gov/search.jsp?R=20070037462 2019-08-30T01:59:41+00:00Z Status of Solar Sail Propulsion: Moving Toward an Interstellar Probe Les Johnson, Roy M. Young, and Edward E. Montgomery IV NASA George C. Marshall Space Flight Center, Huntsville. AL 35812 Abstract. NASA's In-Space Propulsion Technology Program has developed the first- generation of solar sail propulsion systems sufficient to accomplish inner solar system science and exploration missions. These first-generation solar sails, when operational, will range in size from 40 meters to well over 100 meters in diameter and have an areal density of less than 13 grams-per-square meter. A rigorous, multiyear technology development effort culminated last year in the testing of two different 20-meter solar sail systems under thermal vacuum conditions. This effort provided a number of significant insights into the optimal design and expected performance of solar sails as well as an understanding of the methods and costs of building and using them. In a separate effort, solar sail orbital analysis tools for mission design were developed and tested. Laboratory simulations of the effects of long-term space radiation exposure were also conducted on two candidate solar sail materials. Detailed radia- tion and charging environments were defined for mission trajectories outside the protection of the earth's magnetosphere, in the solar wind environment. These were used in other analytical tools to prove the adequacy of sail design features for accommodating the harsh space environment. Preceding, and in conjunction with these technology efforts, NASA sponsored several mission application studies for solar sails, including one that would use an evolved sail capa- bility to support humanity's first mission into nearby interstellar space.
    [Show full text]
  • Volume 134Preliminary3.Indd
    CONTENTS Page FOREWORD vii PREFACE ix Part I SESSION 1: ORBIT DETERMINATION 1 1 Algorithm of Automatic Detection and Analysis of Non-Evolutionary Changes in Orbital Motion of Geocentric Objects (AAS 09-103) Sergey Kamensky, Andrey Tuchin, Victor Stepanyants and Kyle T. Alfriend . 3 Deriving Density Estimates Using CHAMP Precision Orbit Data for Periods of High Solar Activity (AAS 09-104) Andrew Hiatt, Craig A. McLaughlin and Travis Lechtenberg ......23 Geosat Follow-on Precision Orbit Improvement through Drag Model Update (AAS 09-105) Stephen R. Mance, Craig A. McLaughlin, Frank G. Lemoine, David D. Rowlands, and Paul J. Cefola ............43 On Preliminary Orbit Determination: A New Approach (AAS 09-106) Reza Raymond Karimi and Daniele Mortari...........63 Comparision of Different Methods of LEO Satellite Orbit Determination for a Single Pass Through a Radar (AAS 09-107) Zakhary N. Khutorovsky, Sergey Yu. Kamensky, Nickolay N. Sbytov and Kyle T. Alfriend .................71 Passive Multi-Target Tracking with Application to Orbit Determination for Geosynchronous Objects (AAS 09-108) Kyle J. DeMars and Moriba Jah ..............89 SESSION 2: RENDEZVOUS, RELATIVE MOTION, FORMATION FLIGHT AND SATELLITE CONSTELLATIONS 1 101 A Cooperative Egalitarian Peer-to-Peer Strategy for Refueling Satellites in Circular Constellations (AAS 09-109) Atri Dutta and Panagiotis Tsiotras .............103 An Investigation of Teardrop Relative Orbits for Circular and Elliptical Chief Satellites (AAS 09-110) David J. Irvin Jr., Richard G. Cobb and T. Alan Lovell .......121 xiii Page Control System Design and Simulation of Spacecraft Formations Via Leader-Follower Approach (AAS 09-111) Mahmut Reyhanoglu.................141 Decentralized Optimization for Control of Satellite Imaging Formations in Complex Regimes (AAS 09-112) Lindsay D.
    [Show full text]
  • Aas 03-003 the Inertial Stellar Compass: a Multifunction
    AAS 03-003 THE INERTIAL STELLAR COMPASS: A MULTIFUNCTION, LOW POWER, ATTITUDE DETERMINATION TECHNOLOGY BREAKTHROUGH T. Brady, S. Buckley Charles Stark Draper Laboratory, Inc. Systems Engineering and Evaluation Directorate Cambridge, MA 02139 C. J. Dennehy, J. Gambino, A. Maynard NASA Goddard Space Flight Center (GSFC) Guidance, Navigation, and Control Division Greenbelt, MD 20771 The Inertial Stellar Compass (ISC) is a miniature, low power, stellar inertial attitude determination system with an accuracy of better than 0.1º (1 sigma) in three axes. The ISC consumes only 3.5 Watts of power and is contained in a 2.5 kg package. With its embedded on- board processor, the ISC provides attitude quaternion information and has Lost-in-Space (LIS) initialization capability. The attitude accuracy and LIS capability are provided by combining a wide field of view Active Pixel Sensor (APS) star camera and Micro- ElectroMechanical System (MEMS) inertial sensor information in an integrated sensor system. The performance and small form factor make the ISC a useful sensor for a wide range of missions. In particular, the ISC represents an enabling, fully integrated, micro- satellite attitude determination system. Other applications include using the ISC as a “single sensor” solution for attitude determination on medium performance spacecraft and as a “bolt on” independent safe-hold sensor or coarse acquisition sensor for many other spacecraft. NASA's New Millennium Program (NMP) has selected the ISC technology for a Space Technology 6 (ST6) flight validation experiment scheduled for 2004. NMP missions, such as ST6, are intended to validate advanced technologies that have not flown in space in order to reduce the risk associated with their infusion into future NASA missions.
    [Show full text]
  • Autonav Mark3
    AutoNav Mark3: Engineering the Next Generation of Autonomous Onboard Navigation and Guidance J. Ed Riedel, Shyam Bhaskaran, Dan B. Eldred, Robert A. Gaskell, Christopher A. Grasso, Brian Kennedy, Daniel Kubitscheck, Nickolaos Mastrodemos, Stephen. P. Synnott, Andrew Vaughan, Robert A. Werner Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA. 91101, USA, [email protected] The success of JPL's AutoNav system at comet Tempel-1 on July 4, 2005, demonstrated the power of autonomous navigation technology for the Deep Impact Mission. This software is being planned for use as the onboard navigation, tracking and rendezvous system for a Mars Sample Return Mission technology demonstration, and several mission proposals are evaluating its use for rendezvous with, and landing on asteroids. Before this however, extensive re-engineering of AutoNav will take place. This paper describes the AutoNav systems-engineering effort in several areas: extending the capabilities, improving operability, utilizing new hardware elements, and demonstrating the new possibilities of AutoNav in simulations. I. Introduction Autonomous onboard deep-space navigation is an inevitable progression of robotic, and undoubtedly manned, space exploration technology. The success of JPL’s AutoNav system during the Comet Temple impact and flyby on July 4 (Fig. 1, Ref. 1) 2005, following the equally successful encounters at the comets Borrelly (Fig. 2, Ref. 2, Ref. 3) and Wild-2 (Fig. 3, Ref. 4), also utilizing this system, demonstrates the power of this technology. Indeed, plans have been made to use the AutoNav system as the onboard navigation, tracking and rendezvous system for an at-Mars demonstration of autonomous rendezvous for purposes of proving technologies for Mars Sample Return Mission (MSR).
    [Show full text]
  • Prime Focus (05-08)
    Highlights of the May Sky. -- -- -- 1st -- -- -- Dusk: Mercury passes less than 3º fromfrom thethe PleiadesPleiades Prime Focus rdrd P s (continues until the 33 ). A Publication of the Kalamazoo Astronomical Society -- -- -- 5th -- -- -- New Moon 8:18 am EDT May 2008 AM: Eta Aquarid meteor shower (10 per hour). -- -- -- 6th -- -- -- ThisThis MonthsMonths KAS EventsEvents Dusk: The Moon passes 2º above Mercury. General Meeting: Friday, May 2 @ 7:00 pm thth -- -- -- 8 -- -- -- PM: Asteroid 5 Astraea Kalamazoo Math & Science Center - See Page 10 for Details lessless thanthan 55´ southsouth ofof 6th-- magnitude 37 Virginis. Observing Session: Saturday, May 3 @ 8:30 pm -- -- -- 10thth -- -- -- Galaxies of Virgo Cluster - Kalamazoo Nature Center PM: The Moon skims the southern edge of M44, the Beehive Cluster. Astrophoto Workshop: Saturday, May 10 @ 8:00 pm Beehive Cluster. Kalamazoo Nature Center - See Page 3 for Details PM: The Moon near Mars. -- -- -- 11th -- -- -- Observing Session: Saturday, May 24 @ 8:30 pm First Quarter Moon 11:47 pm EDT Moon, Jupiter, & Saturn - Kalamazoo Nature Center -- -- -- 12th -- -- -- PM: Saturn and Regulus a few degrees north ofof the Moon. Inside the Newsletter. Inside the Newsletter. -- -- -- 19th -- -- -- PM: Mars passes a few April Meeting Minutes........................... p. 2 arcminutes north of 5.3 magnitude Eta Cancri. Board Meeting Minutes......................... p. 2 Full Moon Worthwhile Web Sites......................... p. 3 10:11 pm EDT Astrophotography Workshop............. p. 3 -- -- -- 22nd -- -- -- Astronomy Day 2008 Report.............. p. 4 PM: Mars passes through M44, the Beehive Cluster. Phobos in 3D........................................... p. 6 NASA Space Place.................................. p. 7 -- -- -- 24th -- -- -- Dawn: The Moon is a few May Night Sky......................................... p. 8 degrees below Jupiter -- KAS Officers & Announcements.......
    [Show full text]
  • Event Horizon Event Horizon Archives 18 April Meeting Roundup by Mike Spicer (Continued from Front Page)
    Volume 15, Issue 5 John Gauvreau on Things We Never Think May 2008 About Photo and Story by Mike Spicer There were very few From The Editor’s Desk seats empty for the Hamil- ton Amateur Astronomers' Every year in the spring we celebrate April meeting at the Spec- Astronomy Day as an opportunity to tator Auditorium Friday do outreach to the community. All we evening, 11 April 2008. need do is look around the club and see all of Fifty members and almost the grey hairs to realize that we need to do a a dozen guests were in better job of getting young people interested in attendance for our line-up astronomy. Photographs of HAA meetings of excellent speakers! from many years ago show a lot of young peo- ple. How do we get them interested in our Club Observing Director hobby? One thing is certain, if we don’t get Prof. Greg Emery gave a new people interested, there are going to be a very detailed run-down of lot of telescopes sitting idle when we are all the Sky for April to aug- too old to lift them anymore. (Continued on page 2) Tim Philp, Editor Inside this issue: NOTICE Chair Report 3 Astronomy Day at Bayfront Park Image Stacking 4-5 in Hamiltion. Saturday May 10th Taking Care of Your Telescopes 7-8 @ 20:00 hrs. The Sky this Month 9—11 WEATHER AND CLOUDS PER- Knowns and Unknowns 13 MITTING! 4-D Ionosphere 16-17 Check the web site for directions. Event Horizon Event Horizon Archives 18 April Meeting Roundup By Mike Spicer (Continued from Front Page) ment his very informative arti- tions, pick up free magazines our 15th anniversary dinner cle in last month's newsletter, and copies of our club news- venue this fall.
    [Show full text]