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Copyright Copyright © © 2006 Viktor T. 2006 Viktor T. Toth Toth http:// http:// www.vttoth.com www.vttoth.com / / 1 1 First Year Seminar in Science First Year Seminar in Science Carleton University, October 16, 2006 Carleton University, October 16, 2006 The Pioneer The Pioneer Anomaly Anomaly Seeking an Explanation in Seeking an Explanation in Telemetry Records Telemetry Records

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Page 1: The Pioneer Anomaly - Viktor TothzSupernovae, microwave background show accelerated expansion Dark matter? Dark energy? ... z3m High Gain Antenna zTransmitter: 8W zData rate: 16-2048

Copyright Copyright ©© 2006 Viktor T. 2006 Viktor T. TothTothhttp://http://www.vttoth.comwww.vttoth.com/ / 11

First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

The PioneerThe PioneerAnomalyAnomaly

Seeking an Explanation in Seeking an Explanation in Telemetry RecordsTelemetry Records

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Copyright Copyright ©© 2006 Viktor T. 2006 Viktor T. TothTothhttp://http://www.vttoth.comwww.vttoth.com/ / 22

First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

The Pioneer AnomalyThe Pioneer Anomaly

Anomalous acceleration of the Pioneer Anomalous acceleration of the Pioneer 10/11 spacecraft was detected in the 10/11 spacecraft was detected in the 1980s, confirmed by several research 1980s, confirmed by several research teamsteamsMay be mechanical in origin, may be May be mechanical in origin, may be ““new physicsnew physics””In the past, short stretches of data were In the past, short stretches of data were studied; new effort under way with studied; new effort under way with complete data set, including oncomplete data set, including on--board board telemetry.telemetry.

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Copyright Copyright ©© 2006 Viktor T. 2006 Viktor T. TothTothhttp://http://www.vttoth.comwww.vttoth.com/ / 33

First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

Science of the AnomalyScience of the Anomaly

Astronomy (planetary orbits)Astronomy (planetary orbits)Relativity theory / fundamental physicsRelativity theory / fundamental physicsRadio scienceRadio scienceThermal physicsThermal physicsEngineeringEngineeringData processingData processingNumerical analysisNumerical analysis

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First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

The Pioneer 10/11 MissionsThe Pioneer 10/11 Missions

Launched in 1972 and 1973Launched in 1972 and 1973First to explore beyond MarsFirst to explore beyond MarsFirst to visit Jupiter and SaturnFirst to visit Jupiter and SaturnPlanned duration: 600Planned duration: 600--900 days900 days

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First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

Mission ObjectivesMission Objectives

Primary ObjectivesPrimary ObjectivesExplore the asteroid beltExplore the asteroid beltExplore beyond MarsExplore beyond MarsExplore JupiterExplore Jupiter

Secondary ObjectivesSecondary ObjectivesExplore the outer solar systemExplore the outer solar systemSearch for gravity wavesSearch for gravity wavesSearch for Search for ““Planet XPlanet X””

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First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

Experimental General RelativityExperimental General Relativity

Non-linearity

Un

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re

1

0.998 10.999 1.001 1.002

1.002

1.001

0.999

0.998

β

γ

Cassini ‘03

Mercury Ranging ‘93

LLR ’04

γ −− ≤ ± × 51 (2.1 2.3) 10

General Relativity

Mars Ranging ‘76 γ −− ≤ × 31 2 10

Astrometric VLBI ‘04γ −− ≤ × 41 4 10

( ) ∑∑∑

∑ ∑∑

≠≠≠

≠ ≠≠

∂−

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⎞⎜⎜⎝

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+==

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34334

34224

34114

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1122

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µµµβ

µγµβµ

µγ

µγ

µγ

µγ

Parameterized Post-Newtonian (PPN) formalismFrom Moyer (JPL Publication 00-7)

Albert Einstein(1879-1955)

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May not work at large distancesMay not work at large distances

Galaxies do not rotate as expectedGalaxies do not rotate as expectedSupernovae, microwave background Supernovae, microwave background show accelerated expansionshow accelerated expansion

Dark matter?Dark matter? Dark energy?Dark energy?

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First Year Seminar in ScienceFirst Year Seminar in ScienceCarleton University, October 16, 2006Carleton University, October 16, 2006

Pioneer Orbits Pioneer Orbits –– Early YearsEarly Years

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Pioneer and Voyager Orbits Pioneer and Voyager Orbits through the Outer Solar Systemthrough the Outer Solar System

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The Pioneer SpacecraftThe Pioneer Spacecraft

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Science InstrumentsScience Instruments1.1. JPL Helium Vector MagnetometerJPL Helium Vector Magnetometer2.2. ARC Plasma AnalyzerARC Plasma Analyzer3.3. U/Chicago Charged Particle ExperimentU/Chicago Charged Particle Experiment4.4. U/Iowa Geiger Tube TelescopeU/Iowa Geiger Tube Telescope5.5. GSFC Cosmic Ray TelescopeGSFC Cosmic Ray Telescope6.6. UCSD Trapped Radiation DetectorUCSD Trapped Radiation Detector7.7. UCS Ultraviolet PhotometerUCS Ultraviolet Photometer8.8. U/Arizona Imaging U/Arizona Imaging PhotopolarimeterPhotopolarimeter9.9. CIT Jovian Infrared RadiometerCIT Jovian Infrared Radiometer10.10. GE Asteroid/Meteoroid DetectorGE Asteroid/Meteoroid Detector11.11. LaRCLaRC Meteoroid DetectorMeteoroid Detector12.12. FluxFlux--Gate Magnetometer (PioneerGate Magnetometer (Pioneer--11 only)11 only)

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The Pioneer SpacecraftThe Pioneer Spacecraft

Mass: ~250 kgMass: ~250 kgRadioisotope Thermoelectric GeneratorsRadioisotope Thermoelectric GeneratorsElectrical Power: ~160W (at launch)Electrical Power: ~160W (at launch)11 Scientific Instruments11 Scientific Instruments3m High Gain Antenna3m High Gain AntennaTransmitter: 8WTransmitter: 8WData rate: 16Data rate: 16--2048 bps2048 bpsSpin stabilized (4.8 rpm nominal)Spin stabilized (4.8 rpm nominal)

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Orientation ManeuversOrientation Maneuvers

Few maneuvers needed for spinning Few maneuvers needed for spinning spacecraftspacecraftFew maneuvers Few maneuvers →→ clean dataclean dataIngenious Ingenious ““Closed loopClosed loop”” CONSCAN CONSCAN maneuver lets the spacecraft maneuver lets the spacecraft ““home inhome in””on DSN signalon DSN signalLate in the mission, ~2 Late in the mission, ~2 CONSCANsCONSCANs a a year were performedyear were performed

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Pioneer Power SourcePioneer Power SourceRTG Thermal Power: ~650WRTG Thermal Power: ~650W

Electrical Power: ~40WElectrical Power: ~40W

4 4 RTGsRTGs per spacecraftper spacecraft

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Passive Thermal ControlPassive Thermal Control

Louver systemLouver systemThermally activated bimetallic springsThermally activated bimetallic springsLouvers are fully closed <40Louvers are fully closed <40°°F*F*

*When the Pioneer 10/11 spacecraft were designed, NASA was not y*When the Pioneer 10/11 spacecraft were designed, NASA was not yet using the metric system.et using the metric system.

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Pioneer Louver ArrangementPioneer Louver Arrangement

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Pioneer 10 After 30 YearsPioneer 10 After 30 Years

Distance from Sun: ~80 AUDistance from Sun: ~80 AURoundRound--trip light time: ~21 hourstrip light time: ~21 hoursSpeed relative to the Sun: ~12 km/sSpeed relative to the Sun: ~12 km/s

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Pioneer 10 After 30 YearsPioneer 10 After 30 Years

One instrument (GTT) still operating (powerOne instrument (GTT) still operating (power--down command sent last track, but never down command sent last track, but never confirmed)confirmed)Bus voltage ~ 26VDC instead of nominal 28VDCBus voltage ~ 26VDC instead of nominal 28VDCTransmitter XCO failed (probably due to cold)Transmitter XCO failed (probably due to cold)Transmitter still operating in coherent modeTransmitter still operating in coherent modeMany temperature readings Many temperature readings ““off the scaleoff the scale”” or or outside calibrated rangesoutside calibrated rangesPropellant lines frozen (no maneuvers possible)Propellant lines frozen (no maneuvers possible)

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Pioneer 10/11 are the Pioneer 10/11 are the most precisely most precisely

navigated deep space navigated deep space craft to date.craft to date.

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Deep Space Deep Space NetworkNetwork

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Downlink Power BudgetDownlink Power Budget

Received power was Received power was ––181 dBm at EOM!181 dBm at EOM!That is <0.000000000000000000001 W!That is <0.000000000000000000001 W!

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Communications SubsystemCommunications SubsystemTransmitter Block DiagramTransmitter Block Diagram

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Doppler MeasurementsDoppler Measurements

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Doppler MeasurementsDoppler Measurements

One-way Doppler

TwoTwo--way Dopplerway Doppler

ThreeThree--way Dopplerway Doppler

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Terrestrial EffectsTerrestrial EffectsObserved Polar Motion 1996-2000

Variation in Length of Day since 1990

Tectonic Plate Motion

Earth Rotation

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Solar EffectsSolar Effects

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Doppler FitsDoppler FitsModel predicts spacecraft motion and DopplerModel predicts spacecraft motion and DopplerAntenna measures actual DopplerAntenna measures actual DopplerDifference is called the Difference is called the ““Doppler ResidualDoppler Residual””““BadBad”” fit:fit:

““GoodGood”” fit:fit:

Accuracy is measured in Accuracy is measured in mHzmHz!!

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Doppler ResidualsDoppler Residuals

catftftf 2)()( 0modelobs −=−

Phys. Rev. D 65 (2002) 082004, gr-qc/0104064

1 Hz ≈ 65 mm/s

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Discovery of the AnomalyDiscovery of the Anomaly

Search began in 1979 (for Search began in 1979 (for ““Planet XPlanet X””))Anomaly first detected in 1980Anomaly first detected in 1980Initial JPL ODP analysis in 1990Initial JPL ODP analysis in 1990--9595Aerospace Corporation confirms: 1996Aerospace Corporation confirms: 1996--9898Another confirmation by Another confirmation by MarkwardtMarkwardt (2002)(2002)Also confirmed by Olsen (2005)Also confirmed by Olsen (2005)

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Interpreting the ResidualInterpreting the Residual

Frequency shift: Frequency shift: (5.99 (5.99 ±± 0.01)0.01)××1010––99 Hz/sHz/sVelocity change: Velocity change: (8.74 (8.74 ±± 1.33)1.33)××1010––1010 m/sm/s22

Clock acceleration: Clock acceleration: (2.92 (2.92 ±± 0.44)0.44)××1010––1818 s/ss/s22

Velocity change (acceleration) is the Velocity change (acceleration) is the ““conventionalconventional”” interpretationinterpretationEffect small by engineering standards, but Effect small by engineering standards, but huge by the standards of gravity physicshuge by the standards of gravity physics

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Unknown directionUnknown direction

1

2

3

4

Opposite the direction of motion: Drag force?Opposite the direction of motion: Drag force?4. 4. Towards the Sun: Gravity?Towards the Sun: Gravity?3.3.Along the spin axis: OnAlong the spin axis: On--board systematics?board systematics?2.2.Towards the Earth: Effect on radio beam?Towards the Earth: Effect on radio beam?1.1.

v

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Consensus as of 2006Consensus as of 2006

The Pioneer Anomaly is realThe Pioneer Anomaly is realConventional physics Conventional physics failsfails to explain itto explain itAlternatives proposed includeAlternatives proposed include

Modified Newtonian Dynamics (MOND)Modified Newtonian Dynamics (MOND)Nonsymmetric gravitational theoryNonsymmetric gravitational theoryDark matterDark matterYukawa potential (Yukawa potential (VVgravgrav = = ––GeGe––mrmr//rr))

aaPP ≈≈ cHcH00 –– coincidence?coincidence?

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Thermal RadiationThermal Radiation

Only ~65W of directed heat neededOnly ~65W of directed heat needed~2500W heat available on board~2500W heat available on boardHeat sources includeHeat sources include

Radioisotope thermoelectric generators (Radioisotope thermoelectric generators (RTGsRTGs))Electrically generated heatElectrically generated heatSmall radioisotope heater units (Small radioisotope heater units (RHUsRHUs))

Previous estimates: insufficient directed Previous estimates: insufficient directed heat to explain the anomalyheat to explain the anomalyConclusions based on rough estimatesConclusions based on rough estimates

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TelemetryTelemetry

Precise and detailed information onPrecise and detailed information onElectrical powerElectrical powerTemperaturesTemperatures

All information from spacecraft was All information from spacecraft was packaged in Master Data Records (packaged in Master Data Records (MDRsMDRs))Once science data was extracted and Once science data was extracted and spacecraft operations no longer needed the spacecraft operations no longer needed the data, data, MDRsMDRs were thought to be expendablewere thought to be expendable

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BUTBUT……

The Pioneer 10/11 The Pioneer 10/11 MDRsMDRs were saved!were saved!First, on tapeFirst, on tapeLater, Later, ‘‘flopticalfloptical’’ disksdisksTotal amount of Total amount of data: 40 gigabytesdata: 40 gigabytes

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WhatWhat’’s in the Telemetry?s in the Telemetry?

MDRsMDRs containcontainReception characteristicsReception characteristicsScience dataScience dataEngineering telemetryEngineering telemetry

Types of readingsTypes of readingsThermalThermalElectrical (voltages, currents)Electrical (voltages, currents)Propellant pressurePropellant pressureSwitches and sensorsSwitches and sensorsCommand and logic statesCommand and logic statesCountersCounters

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Analog ReadingsAnalog Readings

Analog data is lowAnalog data is low--resolution (6 bits, 64 levels)resolution (6 bits, 64 levels)Calibration is importantCalibration is important

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What do we see?What do we see?

Individual events (e.g., thruster firings)Individual events (e.g., thruster firings)Long term trends (e.g., propellant temp.)Long term trends (e.g., propellant temp.)

VPT1 temperature on board Pioneer 11 on April 19-20, 1974 (major course correction maneuver)

Nitrogen tank temperature on board Pioneer 10, entire mission.

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Design InformationDesign Information

RTGRTG Spacecraft BodySpacecraft Body

HGAHGA

GeometryGeometry

Infrared ReflectivityInfrared Reflectivity

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New AnalysisNew Analysis

Design details +Design details +Telemetry record =Telemetry record =New estimates on accelerationNew estimates on accelerationand its temporal profile!and its temporal profile!

Better yet: Incorporate thermal Better yet: Incorporate thermal model into orbit estimationmodel into orbit estimation

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FocusFocus

RTG heat: Radiation reflected off the RTG heat: Radiation reflected off the back of the HGA, which is highly back of the HGA, which is highly reflectivereflectiveElectrical heat: most heat generated Electrical heat: most heat generated inside main spacecraft body, emitted inside main spacecraft body, emitted preferentially through the backpreferentially through the back

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New AnalysisNew Analysis

Complete Doppler data set has been Complete Doppler data set has been collected and assembledcollected and assembledTelemetry is availableTelemetry is availableIt is possible to It is possible to ““reflyrefly”” both missions, both missions, analyzing any anomalous behavioranalyzing any anomalous behaviorUsing telemetry in orbital analysis is new Using telemetry in orbital analysis is new technique; never done beforetechnique; never done beforeWe hope to find an unambiguous answerWe hope to find an unambiguous answer

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ConclusionsConclusions

Wikipedia lists the Pioneer Anomaly as Wikipedia lists the Pioneer Anomaly as one of the great one of the great ‘‘unresolved problemsunresolved problems’’ in in physicsphysicsNew Scientist calls it one of New Scientist calls it one of ““13 things 13 things that do not make sensethat do not make sense””But, the explanation may be mundaneBut, the explanation may be mundaneEither way, itEither way, it’’s wins win--win: new physics is win: new physics is great, but improved spacecraft navigation great, but improved spacecraft navigation is also a valuable resultis also a valuable result

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Questions?Questions?