The Pioneer Anomaly: an Inconvenient Reality Or NASA‟S 12 Year Misconception?
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Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
The Quest to Understand the Pioneer Anomaly
The quest to understand the Pioneer anomaly I Michael Martin Nieto, Theoretical Division (MS-8285) Los Alamos National Laboratory Los Alarnos, New Mexico 87545 USA E-mail: [email protected] +a l1 l I l uring the 1960's, when the Jet Propulsion Laboratory (JPL) Pioneer 10 was launched on 2 March 1972 local time, aboard D first started thinking about what eventually became the an Atlas/Centaur/TE364-4launch vehicle (see Fig. l).It was the "Grand Tours" of the outer planets (the Voyager missions of the first craft launched into deep space and was the first to reach an 1970's and 1980's),the use of planetary flybys for gravity assists of outer giant planet, Jupiter,on 4 Dec. 1973 [l, 21. Later it was the first spacecraft became of great interest. The concept was to use flybys to leave the "solar system" (past the orbit of Pluto or, should we now of the major planets to both mowthe direction of the spacecraft say, Neptune). The Pioneer project, eventually extending over and also to add to its heliocentric velocity in a manner that was decades, was managed at NASAIAMES Research Center under the unfeasible using only chemical fuels. The first time these ideas were hands of four successive project managers, the legendary Charlie put into practice in deep space was with the Pioneers. Hall, Richard Fimrnel, Fred Wirth, and the current Larry Lasher. While in its Earth-Jupiter cruise, Pioneer 10 was still bound to the solar system. By 9 January 1973 Pjoneer l0 was at a distance of 3.40 AU (Astronomical Units'), beyond the asteroid belt. -
Pioneer Anomaly: What Can We Learn from Future Planetary Exploration Missions?
56th International Astronautical Congress, Paper IAC-05-A3.4.02 PIONEER ANOMALY: WHAT CAN WE LEARN FROM FUTURE PLANETARY EXPLORATION MISSIONS? Andreas Rathke EADS Astrium GmbH, Dept. AED41, 88039 Friedrichshafen, Germany. Email: [email protected] Dario Izzo ESA Advanced Concepts Team, ESTEC, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands. Email: [email protected] The Doppler-tracking data of the Pioneer 10 and 11 spacecraft show an unmodelled constant acceleration in the direction of the inner Solar System. Serious efforts have been undertaken to find a conventional explanation for this effect, all without success at the time of writing. Hence the effect, commonly dubbed the Pioneer anomaly, is attracting considerable attention. Unfortunately, no other space mission has reached the long-term navigation accuracy to yield an independent test of the effect. To fill this gap we discuss strategies for an experimental verification of the anomaly via an upcoming space mission. Emphasis is put on two plausible scenarios: non-dedicated concepts employing either a planetary exploration mission to the outer Solar System or a piggybacked micro- spacecraft to be launched from an exploration spacecraft travelling to Saturn or Jupiter. The study analyses the impact of a Pioneer anomaly test on the system and trajectory design for these two paradigms. Both paradigms are capable of verifying the Pioneer anomaly and determine its magnitude at 10% level. Moreover they can discriminate between the most plausible classes of models of the anomaly. The necessary adaptions of the system and mission design do not impair the planetary exploration goals of the missions. I. -
Max-Planck-Institut Für Sonnensystemforschung Max Planck Institute for Solar System Research Tätigkeitsbericht 2011 Activit
Max-Planck-Institut für Sonnensystemforschung Max Planck Institute for Solar System Research Tätigkeitsbericht 2011 Activity Report 2011 Inhalt Contents 1 Inhalt Contents 1 Wissenschaftliche Zusammenarbeit 2 Scientific collaborations 1.1 Wissenschaftliche Gäste 2 Scientific guests 1.2 Aufenthalt von MPS-Wissenschaftlern an anderen Instituten 4 Stay of MPS scientists at other institutes 1.3 Projekte in Zusammenarbeit mit anderen Institutionen 5 Projects in collaboration with other institutions 2 Vorschläge und Anträge 22 Proposals 2.1 Projektvorschläge 22 Project proposals 2.2 Anträge auf Beobachtungszeit 23 Observing time proposals 3 Publikationen 25 Publications 3.1 Referierte Publikationen 25 Refereed publications 3.2 Doktorarbeiten 45 PhD theses 4 Vorträge und Poster 46 Talks and posters 5 Seminare 69 Seminars 6 Lehrtätigkeit 73 Lectures 7 Tagungen und Workshops 74 Conferences and workshops 7.1 Organisation von Tagungen und Workshops 74 Organization of conferences and workshops 7.2 Convener bei wissenschaftlichen Tagungen 74 Convener during scientific meetings 8 Gutachtertätigkeit für wissenschaftliche Zeitschriften 75 Reviews for scientific journals 9 Herausgebertätigkeit 76 Editorship 10 Mitgliedschaft in wissenschaftlichen Gremien 76 Membership in scientific councils 11 Auszeichnungen 77 Awards Wissenschaftliche Zusammenarbeit / Scientific collaborations 2 1. Wissenschaftliche Zusammenarbeit / Scientific collaborations 1.1 Wissenschaftlich Gäste (mit Aufenthalt ≥1 Woche) Scientific guests (with stay ≥1 week) Jaime Araneda (University of Concepcion, Chile), 1 Jul - 15 Aug (host: E. Marsch) Ankit Barik (Indian Institute of Technology, Kharagpour, India), 19 May - 15 Jul (host: U. Christensen) Alexander Bazilevsky (Vernadsky Institute, Russian Academy of Sciences, Moscow, Russia), 1 Aug - 26 Aug (host: W. Markiewicz) Jishnu Bhattacharya (Indian Institute of Technology, Kanpur, India), 10 May – 18 Jul (host: L. -
Estimating the Thermally Induced Acceleration of the New Horizons Spacecraft
Estimating the thermally induced acceleration of the New Horizons spacecraft André G. C. Guerra,1, ∗ Frederico Francisco,1, y Paulo J. S. Gil,2, z and Orfeu Bertolami1, x 1Departamento de Física e Astronomia and Centro de Física do Porto, Faculdade de Ciências, Universidade do Porto, Portugal 2CCTAE, IDMEC, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais, 1049-001 Lisboa, Portugal (Dated: November 3, 2017) Residual accelerations due to thermal effects are estimated through a model of the New Horizons spacecraft and a Monte Carlo simulation. We also discuss and estimate the thermal effects on the attitude of the spacecraft. The work is based on a method previously used for the Pioneer and Cassini probes, which solve the Pioneer anomaly problem. The results indicate that after the encounter with Pluto there is a residual acceleration of the order of 10−9 m=s2, and that rotational effects should be difficult, although not impossible, to detect. I. INTRODUCTION mination of the γ parameter of the parametrised post- Newtonian (PPN) formalism so far [9], but also led to The first probes aimed at the planets beyond the aster- the detection of a similar anomalous acceleration of ther- oid belt were launched in the 1970s, starting with the ap- mal origin, just like the Pioneer spacecraft [10]. propriately named Pioneer 10 and 11. These two space- The New Horizons mission has undergone some “hiber- craft visited Jupiter and Saturn and paved the way for nation” periods, where no thruster was fired. Therefore, the two much heavier and more sophisticated Voyager 1 it is very likely that a similar thermal origin accelera- and 2, which completed the round through all four gas gi- tion might show up in the radiometric data. -
A Route to Understanding of the Pioneer Anomaly
The XXII Texas Symposium on Relativistic Astrophysics, Stanford University, December 13-17, 2004 1 A Route to Understanding of the Pioneer Anomaly aSlava G. Turyshev, bMichael Martin Nieto, and cJohn D. Anderson∗ a,cJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA bTheoretical Division (MS-B285), Los Alamos National Laboratory, University of California, Los Alamos, NM 87545 The Pioneer 10 and 11 spacecraft yielded the most precise navigation in deep space to date. However, while at heliocentric distance of ∼ 20–70 AU, the accuracies of their orbit reconstructions were limited by a small, anomalous, Doppler frequency drift. This drift can be interpreted as a −8 2 sunward constant acceleration of aP =(8.74 ± 1.33) × 10 cm/s which is now commonly known as the Pioneer anomaly. Here we discuss the Pioneer anomaly and present the next steps towards understanding of its origin. They are: 1) Analysis of the entire set of existing Pioneer 10 and 11 data, obtained from launch to the last telemetry received from Pioneer 10, on 27 April 2002, when it was at a heliocentric distance of 80 AU. This data could yield critical new information about the anomaly. If the anomaly is confirmed, 2) Development of an instrumental package to be operated on a deep space mission to provide an independent confirmation on the anomaly. If further confirmed, 3) Development of a deep-space experiment to explore the Pioneer anomaly in a dedicated mission with an accuracy for acceleration resolution at the level of 10−10 cm/s2 in the extremely low frequency range. -
PURE MILK. >1 Daily Messenger
• \ - - y ' .. ..,,...... •»..?<i (.'• ., .... 1 . > - ' - ' - • - • —•-• w-- -"'•t*^ -"•*+ r^ <~?rU-r^<, r'r^Vt" ?-£.'!: •3^*?; dJL' ^J< „ : <•>£> _ 'V: • ' :-' •'. ".-.-•v.-. ••- :.,.'i,'...-' -.:'r • •.--- ' — - '.' • ••'••'. " • . •• -.•r-rrr-'t ••V.»Vjl-fJW.-i'-':t". - SM -<>?:"•: ": A' '.>'•:* • li'. ' .,t;r- A^.'W iSjtt'.iU A. .,, , ; ;-•<".p. * , *;.^^,;5.-r^ ^st&wji* • V. -v.; .Vr- A 4 .... ^jKk '•' ^w^s-v* ixstikjtm, .'s ?• .;"- "'i - '• ;;v<? ; i •-. ;. ;4.;.-^ :'* "(".i •' • - - ^ l : .»...' • -.>'•/•'} '"<• .:.':W.-;V^; . i :••' ! NORWALK, CONNECTICUT, TUESDAY, FEBRUARY 1, 1881.«,1. V,?"-' .i.v-vs.' W-rH-iv,.,;...ifi-W' v. -•*"•—* < VOL. LXIY.-vNUMBl!Ei WHOLE NUMBER 1726 At 7 a. m. a sharp cannonade was opened ** My Godly Man. rifle-pits had been thrown up with epaul- lorsville toward the Rappahannock, passed NORWALK GAZETTE, REAL^ESTATE. Tlie Harbor Bar. on our left, followed by infantry demonstra J. M. POTTER, i * (From tbe Utica Observer*) • vu it:'i•' -1 mcnts for artillery. Especially was this the along Banks' Ford, six miles distant, and tions of no paiticular earnestness. Two houis PUBLISHED EVERY TUESQ^.MORRiRS, 5 DEALER IN You ask me if I think a godly man ^ CIIAELE8 BUEE TODD. case at what is called Banks'Ford and the continued to Fredericksburg. That wing For Sale or to Rent. a l^ter the enemy was observed moving a mile —35 Doses Can be built up Christ-like, on naturea plan, A ship has crossed the harbor bar, United .States Ford, each of which was held was ready for the advance at an early hour WO HOUSES, one of Six Booms, on Fair St.; or so to the south and front of the centre, '35 cents. -
The Non-Gravitational Accelerations of the Cassini Spacecraft and the Nature of the “Pioneer Anomaly”
Dipartimento di Ingegneria Astronautica e Aerospaziale Dottorato di ricerca in Ingegneria Aerospaziale Ciclo XXIII The non-gravitational accelerations of the Cassini spacecraft and the nature of the “Pioneer anomaly” Dottorando: Relatore: Mauro Di Benedetto Ch.mo Prof. Luciano Iess Anno Accademico 2010-2011 Table of Contents Introduction vi 1 The Pioneer anomaly 1 1.1 Pioneer 10 & 11 mission . 2 1.2 Spacecraft design . 3 1.3 Discovery of the anomalous acceleration . 4 1.4 Status of current investigations . 8 1.5 Contribution from this work . 9 2 CassiniteststhePioneeranomaly 10 2.1 Cassinimission .......................... 11 2.1.1 The interplanetary cruise phase . 11 2.1.2 The Saturnian phase . 12 2.2 Spacecraft design . 13 2.2.1 Cassini coordinate system . 16 2.3 Experimental method to test the Pioneer anomaly . 17 2.3.1 Inner cruise phase . 18 2.3.2 Radio science experiments in the outer cruise phase . 18 2.3.3 Multi arc method on the Saturnian phase . 20 2.3.4 Disentangling RTG and Pioneer like acceleration . 22 3 Theorbitdeterminationmethod 24 3.1 The orbit determination problem . 25 3.2 Method of differential correction . 26 3.2.1 Linearization procedure . 28 3.2.2 The weighted least squares solution . 29 3.2.3 A priori information . 31 3.3 TheODPfilter:SIGMA .. .. .. .. .. .. .. .. .. 34 3.3.1 Householder transformations . 36 3.4 Consider parameters: definition . 38 3.4.1 Mathematical formulation . 38 3.5 The multi arc method . 42 i TABLE OF CONTENTS ii 4 Radio metric observables 44 4.1 Range and range-rate observables . 45 4.1.1 Data information content . -
The Study of the Anomalous Acceleration of Pioneer 10 and 11
The Study of the Anomalous Acceleration of Pioneer 10 and 11 SlavaSlava G.G. Turyshev,Turyshev, JohnJohn D.D. AndersonAnderson ((JetJet PropulsionPropulsion Laboratory,Laboratory, CaltechCaltech)) MichaelMichael MartinMartin NietoNieto ((LosLos AlamosAlamos NationalNational Laboratory,Laboratory, UU ofof CaliforniaCalifornia)) Journées du GREX 2004 Nice, France, 29 October 2004 THETHE STUDYSTUDY OFOF THETHE PIONEERPIONEER ANOMALYANOMALY Conclusions & Outline: The Pioneer 10/11 anomalous acceleration: −82 aP =±(8.74 1.33) ×10 cm/s A line-of-sight constant acceleration towards the Sun: –We find no mechanism or theory that explains the anomaly – Most plausible cause is systematics, yet to be demonstrated Phys. Rev. D 65 (2002) 082004, gr-qc/0104064 Possible Origin? Conventional Physics [not yet understood]: – Gas leaks, heat reflection, drag force, etc… New Physics [many proposals exist, some interesting] Both are important − a “win-win” situation: – CONVENTIONAL explanation: improvement of spacecraft engineering for precise navigation & attitude control – NEW physics: would be truly remarkable… THETHE STUDYSTUDY OFOF THETHE PIONEERPIONEER ANOMALYANOMALY Pioneer 10/11 Mission – Built: TRW (Northrop-Grumman Space Technology) – Navigation: Jet Propulsion Laboratory, Caltech – Project management: NASA Ames Research Center Position of Pioneer 10 on 29 October 2004: Last successful precession maneuver to point the spacecraft to Earth was accomplished on 11 Feb 2000 (distance from the Sun of 75 AU) THETHE STUDYSTUDY OFOF THETHE PIONEERPIONEER -
Radioisotope Power Systems: an Imperative for Maintaining U.S
Radioisotope Power Systems: An Imperative for Maintaining U.S. Leadership in Space Exploration Radioisotope Power Systems Committee, National Research Council ISBN: 0-309-13858-2, 68 pages, 8 1/2 x 11, (2009) This free PDF was downloaded from: http://www.nap.edu/catalog/12653.html Visit the National Academies Press online, the authoritative source for all books from the National Academy of Sciences, the National Academy of Engineering, the Institute of Medicine, and the National Research Council: • Download hundreds of free books in PDF • Read thousands of books online, free • Sign up to be notified when new books are published • Purchase printed books • Purchase PDFs • Explore with our innovative research tools Thank you for downloading this free PDF. If you have comments, questions or just want more information about the books published by the National Academies Press, you may contact our customer service department toll-free at 888-624-8373, visit us online, or send an email to [email protected]. This free book plus thousands more books are available at http://www.nap.edu. Copyright © National Academy of Sciences. Permission is granted for this material to be shared for noncommercial, educational purposes, provided that this notice appears on the reproduced materials, the Web address of the online, full authoritative version is retained, and copies are not altered. To disseminate otherwise or to republish requires written permission from the National Academies Press. Radioisotope Power Systems: An Imperative for Maintaining U.S. Leadership in Space Exploration http://www.nap.edu/catalog/12653.html Radioisotope Power Systems Committee Space Studies Board Aeronautics and Space Engineering Board Division on Engineering and Physical Sciences Copyright © National Academy of Sciences. -
FINAL REPORT SYSTEM DESIGN of the PIONEER VENUS SPACECRAFT VOLUME 2 SCIENCE U a by L.K
FINAL REPORT SYSTEM DESIGN OF THE PIONEER VENUS SPACECRAFT VOLUME 2 SCIENCE U a By L.K. ACHESON NET AL. P 0 JUL1974 E-4 (d U ,L) July 1973 R ECFIvJ_ o w 0 (v Prepared Under Contract No.. i a - 750 W0 By 'PPli HUGHES AIRCRAFT COMPANY me o EL SEGUNDO, CALIFORNIA AME S For I AMES RESEARCH CENTER NATIONAL AERONAUTICS AND SPACE ADMINISTRATION . ErZ4 C) IS~ PREFACE The Hughes Aircraft Company Pioneer Venus final report is based on study task reports prepared during performance of the "System Design Study of the Pioneer Spacecraft. " These task reports were forwarded to Ames Research Center as they were completed during the nine months study phase. The significant results from these task reports, along with study results developed after task report publication dates, are reviewed in this final report to provide complete study documentation. Wherever appropriate, the task reports are cited by referencing a task number and Hughes report refer- ence number. The task reports can be made available to the reader specific- ally interested in the details omitted in the final report for the sake of brevity. This Pioneer Venus Study final report describes the following baseline configurations: * "Thor/Delta Spacecraft Baseline" is the baseline presented at the midterm review on 26 February 1973. * "Atlas/Centaur Spacecraft Baseline" is the baseline resulting from studies conducted since the midterm, but prior to receipt of the NASA execution phase RFP, and subsequent to decisions to launch both the multiprobe and orbiter missions in 1978 and use the Atlas/Centaur launch vehicle. * "Atlas/Centaur Spacecraft Midterm Baseline" is the baseline presented at the 26 February 1973 review and is only used in the launch vehicle utilization trade study. -
A Study of Anomalous Acceleration of the Pioneer 10 and 11
The Study of the Anomalous Acceleration of the Pioneer 10 and 11 SlavaSlava G.G. Turyshev,Turyshev, JohnJohn D.D. AndersonAnderson ((JetJet PropulsionPropulsion Laboratory,Laboratory, CaltechCaltech)) MichaelMichael MartinMartin NietoNieto ((LosLos AlamosAlamos NationalNational Laboratory,Laboratory, UU ofof CaliforniaCalifornia)) The XXII Texas Symposium on Relativistic Astrophysics Stanford University, December 13-17, 2004 THETHE STUDYSTUDY OFOF THETHE PIONEERPIONEER ANOMALYANOMALY Conclusions and Outline: The Pioneer 10 and 11 anomalous acceleration: −82 aP =±×(8.74 1.33) 10 cm/s A line-of-sight constant acceleration towards the Sun: –We find no mechanism or theory that explains the anomaly – Most plausible cause is systematics, yet to be demonstrated Phys. Rev. D 65 (2002) 082004, gr-qc/0104064 Possible Origin? Conventional Physics [not yet understood]: – Gas leaks, heat reflection, drag force, etc… New Physics [many proposals exist, some interesting] A “win-win” situation, as both are important: – CONVENTIONAL explanation: improvement of spacecraft engineering for precise navigation & attitude control – NEW physics: would be truly remarkable… THETHE STUDYSTUDY OFOF THETHE PIONEERPIONEER ANOMALYANOMALY Pioneer 10/11 Mission – Built: TRW (Northrop-Grumman Space Technology) – Navigation: Jet Propulsion Laboratory, Caltech – Project management: NASA Ames Research Center Position of Pioneer 10 on 15 December 2004: Last successful precession maneuver to point the spacecraft to Earth was accomplished on 11 Feb 2000 (distance from the