Anomalous Accelerations in Spacecraft Flybys of the Earth
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Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
Document Downloaded From: This Paper Must Be Cited As: the Final
Document downloaded from: http://hdl.handle.net/10251/122856 This paper must be cited as: Acedo Rodríguez, L.; Piqueras, P.; Moraño Fernández, JA. (2018). A possible flyby anomaly for Juno at Jupiter. Advances in Space Research. 61(10):2697-2706. https://doi.org/10.1016/j.asr.2018.02.037 The final publication is available at http://doi.org/10.1016/j.asr.2018.02.037 Copyright Elsevier Additional Information See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/321306820 A possible flyby anomaly for Juno at Jupiter Article in Advances in Space Research · November 2017 DOI: 10.1016/j.asr.2018.02.037 CITATION READS 1 149 3 authors, including: Luis Acedo José Antonio Moraño Universitat Politècnica de València Universitat Politècnica de València 93 PUBLICATIONS 1,145 CITATIONS 55 PUBLICATIONS 162 CITATIONS SEE PROFILE SEE PROFILE Some of the authors of this publication are also working on these related projects: Call for Papers Complexity: Discrete Models in Epidemiology, Social Sciences, and Population Dynamics View project Call for Papers: Journal "Symmetry" (MDPI) Special Issue "Mathematical Epidemiology in Medicine & Social Sciences" View project All content following this page was uploaded by Luis Acedo on 28 February 2018. The user has requested enhancement of the downloaded file. A possible flyby anomaly for Juno at Jupiter L. Acedo,∗ P. Piqueras and J. A. Mora˜no Instituto Universitario de Matem´atica Multidisciplinar, Building 8G, 2o Floor, Camino de Vera, Universitat Polit`ecnica de Val`encia, Valencia, Spain December 14, 2017 Abstract In the last decades there have been an increasing interest in im- proving the accuracy of spacecraft navigation and trajectory data. -
What Is Gravity Probe B? a Quest for Experimental Truth the GP-B Flight
What is Gravity Probe B? than Gravity Probe B. It’s just a star, a telescope, and a spinning sphere.” However, it took the exceptional collaboration of Stanford, Gravity Probe B (GP-B) is a NASA physics mission to experimentally MSFC, Lockheed Martin and a host of others more than four decades investigate Einstein’s 1916 general theory of relativity—his theory of gravity. to develop the ultra-precise gyroscopes and the other cutting- GP-B uses four spherical gyroscopes and a telescope, housed in a satellite edge technologies necessary to carry out this “simple” experiment. orbiting 642 km (400 mi) above the Earth, to measure, with unprecedented accuracy, two extraordinary effects predicted by the general theory of rela- The GP-B Flight Mission & Data Analysis tivity: 1) the geodetic effect—the amount by which the Earth warps the local spacetime in which it resides; and 2) the frame-dragging effect—the amount On April 20, 2004 at 9:57:24 AM PDT, a crowd of over 2,000 current and by which the rotating Earth drags its local spacetime around with it. GP-B former GP-B team members and supporters watched and cheered as the tests these two effects by precisely measuring the precession (displacement) GP-B spacecraft lifted off from Vandenberg Air Force Base. That emotionally angles of the spin axes of the four gyros over the course of a year and com- overwhelming day, culminating with the extraordinary live video of paring these experimental results with predictions from Einstein’s theory. the spacecraft separating from the second stage booster meant, as GP-B Program Manager Gaylord Green put it, “that 10,000 things went right.” A Quest for Experimental Truth Once in orbit, the spacecraft first underwent a four-month Initialization The idea of testing general relativity with orbiting gyroscopes was sug- and Orbit Checkout (IOC), in which all systems and instruments were gested independently by two physicists, George Pugh and Leonard Schiff, initialized, tested, and optimized for the data collection to follow. -
SEER for Hardware's Cost Model for Future Orbital Concepts (“FAR OUT”)
Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com SEER for Hardware’s Cost Model for Future Orbital Concepts (“FAR OUT”) Lee Fischman ISPA/SCEA Industry Hills 2008 Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Introduction A model for predicting the cost of long term unmanned orbital spacecraft (Far Out) has been developed at the request of AFRL. Far Out has been integrated into SEER for Hardware. This presentation discusses the Far Out project and resulting model. © 2008 Galorath Incorporated Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Goals • Estimate space satellites in any earth orbit. Deep space exploration missions may be considered as data is available, or may be an area for further research in Phase 3. • Estimate concepts to be launched 10-20 years into the future. • Cost missions ranging from exploratory to strategic, with a specific range decided based on estimating reliability. The most reliable estimates are likely to be in the middle of this range. • Estimates will include hardware, software, systems engineering, and production. • Handle either government or commercial missions, either “one-of-a-kind” or constellations. • Be used in a “top-down” manner using relatively less specific mission resumes, similar to those available from sources such as the Earth Observation Portal or Janes Space Directory. © 2008 Galorath Incorporated Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Challenge: Technology Change Over Time Evolution in bus technologies Evolution in payload technologies and performance 1. -
Arxiv:0907.4184V1 [Gr-Qc] 23 Jul 2009 Keywords Anomalous Puzzle
Space Science Reviews manuscript No. (will be inserted by the editor) The Puzzle of the Flyby Anomaly Slava G. Turyshev · Viktor T. Toth Received: date / Accepted: date Abstract Close planetary flybys are frequently employed as a technique to place space- craft on extreme solar system trajectories that would otherwise require much larger booster vehicles or may not even be feasible when relying solely on chemical propulsion. The theo- retical description of the flybys, referred to as gravity assists, is well established. However, there seems to be a lack of understanding of the physical processes occurring during these dynamical events. Radio-metric tracking data received from a number of spacecraft that experienced an Earth gravity assist indicate the presence of an unexpected energy change that happened during the flyby and cannot be explained by the standard methods of mod- ern astrodynamics. This puzzling behavior of several spacecraft has become known as the flyby anomaly. We present the summary of the recent anomalous observations and discuss possible ways to resolve this puzzle. Keywords Flyby anomaly · gravitational experiments · spacecraft navigation. 1 Introduction Significant changes to a spacecraft’s trajectory require a substantial mass of propellant. In particular, placing a spacecraft on a highly elliptical or hyperbolic orbit, such as the orbit required for an encounter with another planet, requires the use of a large booster vehicle, substantially increasing mission costs. An alternative approach is to utilize a gravitational assist from an intermediate planet that can change the direction of the velocity vector. Al- arXiv:0907.4184v1 [gr-qc] 23 Jul 2009 though such an indirect trajectory can increase the duration of the cruise phase of a mission, the technique nevertheless allowed several interplanetary spacecraft to reach their target destinations economically (Anderson 1997; Van Allen 2003). -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
Stardust Sample Return
National Aeronautics and Space Administration Stardust Sample Return Press Kit January 2006 www.nasa.gov Contacts Merrilee Fellows Policy/Program Management (818) 393-0754 NASA Headquarters, Washington DC Agle Stardust Mission (818) 393-9011 Jet Propulsion Laboratory, Pasadena, Calif. Vince Stricherz Science Investigation (206) 543-2580 University of Washington, Seattle, Wash. Contents General Release ............................................................................................................... 3 Media Services Information ……………………….................…………….................……. 5 Quick Facts …………………………………………..................………....…........…....….. 6 Mission Overview …………………………………….................……….....……............…… 7 Recovery Timeline ................................................................................................ 18 Spacecraft ………………………………………………..................…..……...........……… 20 Science Objectives …………………………………..................……………...…..........….. 28 Why Stardust?..................…………………………..................………….....………............... 31 Other Comet Missions .......................................................................................... 33 NASA's Discovery Program .................................................................................. 36 Program/Project Management …………………………........................…..…..………...... 40 1 2 GENERAL RELEASE: NASA PREPARES FOR RETURN OF INTERSTELLAR CARGO NASA’s Stardust mission is nearing Earth after a 2.88 billion mile round-trip journey -
High Precision Modelling of Thermal Perturbations with Application to Pioneer 10 and Rosetta
High precision modelling of thermal perturbations with application to Pioneer 10 and Rosetta Vom Fachbereich Produktionstechnik der UNIVERSITAT¨ BREMEN zur Erlangung des Grades Doktor-Ingenieur genehmigte Dissertation von Dipl.-Ing. Benny Rievers Gutachter: Prof. Dr.-Ing. Hans J. Rath Prof. Dr. rer. nat. Hansj¨org Dittus Fachbereich Produktionstechnik Fachbereich Produktionstechnik Universit¨at Bremen Universit¨at Bremen Tag der m¨undlichen Pr¨ufung: 13. Januar 2012 i Kurzzusammenfassung in Deutscher Sprache Das Hauptthema dieser Doktorarbeit ist die pr¨azise numerische Bestimmung von Thermaldruck (TRP) und Solardruck (SRP) f¨ur Satelliten mit komplexer Geome- trie. F¨ur beide Effekte werden analytische Modelle entwickelt und als generischen numerischen Methoden zur Anwendung auf komplexe Modellgeometrien umgesetzt. Die Analysemethode f¨ur TRP wird zur Untersuchung des Thermaldrucks f¨ur den Pio- neer 10 Satelliten f¨ur den kompletten Zeitraum seiner 30-j¨ahrigen Mission verwendet. Hierf¨ur wird ein komplexes dreidimensionales Finite-Elemente Modell des Satelliten einschließlich detaillierter Materialmodelle sowie dem detailliertem ¨außerem und in- nerem Aufbau entwickelt. Durch die Spezifizierung von gemessenen Temperaturen, der beobachteten Trajektorie sowie detaillierten Modellen f¨ur die W¨armeabgabe der verschiedenen Komponenten, wird eine genaue Verteilung der Temperaturen auf der Oberfl¨ache von Pioneer 10 f¨ur jeden Zeitpunkt der Mission bestimmt. Basierend auf den Ergebnissen der Temperaturberechnung wird der resultierende Thermaldruck mit Hilfe einer Raytracing-Methode unter Ber¨ucksichtigung des Strahlungsaustauschs zwischen den verschiedenen Oberf¨achen sowie der Mehrfachreflexion, berechnet. Der Verlauf des berechneten TRPs wird mit den von der NASA ver¨offentlichten Pioneer 10 Residuen verglichen, und es wird aufgezeigt, dass TRP die so genannte Pioneer Anomalie inner- halb einer Modellierungsgenauigkeit von 11.5 % vollst¨andig erkl¨aren kann. -
A Test of General Relativity Using the LARES and LAGEOS Satellites And
A Test of General Relativity Using the LARES and LAGEOS Satellites and a GRACE Earth’s Gravity Model Measurement of Earth’s Dragging of Inertial Frames Ignazio Ciufolini∗1,2, Antonio Paolozzi2,3, Erricos C. Pavlis4, Rolf Koenig5, John Ries6, Vahe Gurzadyan7, Richard Matzner8, Roger Penrose9, Giampiero Sindoni10, Claudio Paris2,3, Harutyun Khachatryan7 and Sergey Mirzoyan7 1 Dip. Ingegneria dell’Innovazione, Universit`adel Salento, Lecce, Italy 2Museo della fisica e Centro studi e ricerche Enrico Fermi, Rome, Italy 3Scuola di Ingegneria Aerospaziale, Sapienza Universit`adi Roma, Italy 4Joint Center for Earth Systems Technology (JCET), University of Maryland, Baltimore County, USA 5Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Potsdam, Germany 6Center for Space Research, University of Texas at Austin, Austin, USA 7Center for Cosmology and Astrophysics, Alikhanian National Laboratory and Yerevan State University, Yerevan, Armenia 8Theory Center, University of Texas at Austin, Austin, USA 9Mathematical Institute, University of Oxford, Oxford, UK 10DIAEE, Sapienza Universit`adi Roma, Rome, Italy April 1, 2016 We present a test of General Relativity, the measurement of the Earth’s dragging of inertial frames. Our result is obtained using about 3.5 years of laser-ranged observations of the LARES, LAGEOS and LAGEOS 2 laser- ranged satellites together with the Earth’s gravity field model GGM05S pro- arXiv:1603.09674v1 [gr-qc] 29 Mar 2016 duced by the space geodesy mission GRACE. We measure µ = (0.994 ± 0.002) ± 0.05, where µ is the Earth’s dragging of inertial frames normalized to its General Relativity value, 0.002 is the 1-sigma formal error and 0.05 is the estimated systematic error mainly due to the uncertainties in the Earth’s gravity model GGM05S. -
Conclusive Analysis & Cause of the Flyby Anomaly
Introduction Theory Analysis Conclusion Conclusive analysis & cause of the flyby anomaly Range proportional spectral shifts for general communication V. Guruprasad Inspired Research, New York http://www.inspiredresearch.com 2019-07-17 c 2019 V. Guruprasad IEEE NAECON 2019 1/20 Introduction Theory Analysis Conclusion Summary • Popular context: Astrometric solar-system anomalies[1] Pioneer: ∆V r_ H r at r 5 AU (blueshift) { SOLVED[2] • 0 Flyby: ∆V trajectory∼ ≈ − discontinuity≥ at satellite range • [3] Lunar orbit eccentricity growth: also H0 • ∼ Earth orbit radius growth: also H0 • ∼ • Present work: conclusive solution of the flyby anomaly All NASA-tracked flybys checked, fit to 1%, more issues found • Fit presence and absence, correlated to transponder • • Real motivation and result: wave theory+practice correction Rewrite communication and radar: source range in all signals • Rewrites physics and astrophysics since Kepler • Computation overlooked since Euler and d'Alembert • Needed extremely robust empirical validation • [1] Anderson and Nieto 2009. [2] Turyshev et al. 2012. [3] The terrestrial reference frame is uncertain to about same order..Altamimi et al. 2016 c 2019 V. Guruprasad IEEE NAECON 2019 2/20 Introduction Theory Analysis Conclusion Faithful led by the blind • Fourier transform presumes clock rate stability Clock rate stability requires design and procedures • But even HST calibration cycles only correct cumulative errors • No awareness of range proportional or scale drift rate errors • Best Allan deviations in any observations -
Working at the Jet Propulsion Laboratory (JPL)
Working at the Jet Propulsion Laboratory (JPL), Anderson, Campbell, Ekelund, Ellis, and Jordan reported on and characterized orbital‐energy changes during six Earth flybys by the Galileo, NEAR, Cassini, Rosetta, and MESSENGER spacecraft; the JPL researchers found an empirical prediction formula consistent with the anomalous energy changes. http://virgo.lal.in2p3.fr/NPAC/relativite_fichiers/anderson_2.pdf “Anomalous Orbital‐Energy Changes Observed during Spacecraft Flybys of Earth” (2008) According to Wikipedia, “The flyby anomaly is an unexpected energy increase during Earth‐flybys of spacecraft. This anomaly has been observed as a shift in the S‐ Band and X‐Band Doppler and ranging telemetry. Taken together it causes a significant unaccounted velocity increase of over 13 mm/sec during flybys.” http://en.wikipedia.org/wiki/Flyby_anomaly What might the flyby anomaly have to do with the Pioneer anomaly and Milgrom’s Modified Newtonian Dynamics (MOND)? Define modified general relativity theory (GRT) with the Rañada‐Milgrom effect to be the heuristic model obtained by replacing the ‐1/2 in the standard form of Einstein’s field equations by ‐1/2 + dark‐ matter‐compensation‐constant, where this constant might be approximately sqrt((60±10)/4) * 10^‐5, based upon the Rañada effect for the Pioneer anomaly combined with the empirical validity of MOND. http://en.wikipedia.org/wiki/Pioneer_anomaly http://en.wikipedia.org/wiki/Modified_Newtonian_dynamics http://vixra.org/pdf/1203.0016v1.pdf “Anomalous Gravitational Acceleration and the OPERA Neutrino Anomaly (Updated)”. The slingshot effect in orbital mechanics uses the orbital angular momentum from a large body like a planet to increase the orbital velocity of a small body like a spacecraft. -
+ Gravity Probe B
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Gravity Probe B Experiment “Testing Einstein’s Universe” Press Kit April 2004 2- Media Contacts Donald Savage Policy/Program Management 202/358-1547 Headquarters [email protected] Washington, D.C. Steve Roy Program Management/Science 256/544-6535 Marshall Space Flight Center steve.roy @msfc.nasa.gov Huntsville, AL Bob Kahn Science/Technology & Mission 650/723-2540 Stanford University Operations [email protected] Stanford, CA Tom Langenstein Science/Technology & Mission 650/725-4108 Stanford University Operations [email protected] Stanford, CA Buddy Nelson Space Vehicle & Payload 510/797-0349 Lockheed Martin [email protected] Palo Alto, CA George Diller Launch Operations 321/867-2468 Kennedy Space Center [email protected] Cape Canaveral, FL Contents GENERAL RELEASE & MEDIA SERVICES INFORMATION .............................5 GRAVITY PROBE B IN A NUTSHELL ................................................................9 GENERAL RELATIVITY — A BRIEF INTRODUCTION ....................................17 THE GP-B EXPERIMENT ..................................................................................27 THE SPACE VEHICLE.......................................................................................31 THE MISSION.....................................................................................................39 THE AMAZING TECHNOLOGY OF GP-B.........................................................49 SEVEN NEAR ZEROES.....................................................................................58