Pioneer Anomaly: Evaluating Newly Recovered Data
Viktor T. Toth, Slava G. Turyshev

TL;DR
This paper analyzes newly recovered Pioneer spacecraft data and telemetry to investigate the Pioneer anomaly, aiming to determine if thermal recoil forces could explain the observed small sunward acceleration.
Contribution
It introduces a comprehensive approach combining new Doppler data, telemetry, and thermal modeling to reassess the Pioneer anomaly and explore thermal recoil as a potential cause.
Findings
Extended Doppler data set analyzed
Telemetry data used for detailed spacecraft history
Thermal recoil force considered as possible explanation
Abstract
The Pioneer 10/11 spacecraft yielded the most precise navigation in deep space to date. However, their radio-metric tracking data received from the distances between 20--70 astronomical units from the Sun consistently indicated the presence of a small, anomalous, Doppler frequency drift. The drift is a blue frequency shift that can be interpreted as a sunward acceleration of a_P = (8.74 +/- 1.33) x 10^(-10) m/s^2 for each particular spacecraft. This signal has become known as the Pioneer anomaly; the nature of this anomaly remains unexplained. New Pioneer 10 and 11 radio-metric Doppler data recently became available. The much extended set of Pioneer Doppler data is the primary source for new upcoming investigation of the anomaly. We also have almost entire records of flight telemetry files received from the the Pioneers. Together with original project documentation and newly developed…
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