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Pioneer 10 search for gravitational waves - No evidence for coherent radiation from GemingaAttempts to identify a periodic gravitational wave signal from the binary Geminga in the reduced Doppler data from the Pioneer 10 spacecraft are reported. The study was performed to examine the possibility that the observed 160 min solar oscillation is driven by a gravitational wave from the binary, which has a period exactly one cycle different from the solar oscillation. Three 12 hr passes of Doppler data from Pioneer 10, now beyond the orbit of Neptune, were subjected to FFT analysis to detect a spectral gravitational wave signature. None was found. Least squares analysis of all low noise data from 1981 to characterize the amplitude and phase of a signal from Geminga also produced a null result. Finally, an upper bound was calculated for the polarization component of the potentially observable gravitational strain.
Document ID
19840053947
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Anderson, J. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Armstrong, J. W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Estabrook, F. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Hellings, R. W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lau, E. K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Wahlquist, H. D.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 12, 2013
Publication Date
March 8, 1984
Publication Information
Publication: Nature
Volume: 308
ISSN: 0028-0836
Subject Category
Astrophysics
Accession Number
84A36734
Funding Number(s)
PROJECT: PROJECT PIONEER
Distribution Limits
Public
Copyright
Other

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