Pioneer anomaly: What can we learn from future pla...

2005 ◽  
Author(s):  
Andreas Rathke ◽  
Dario Izzo
Keyword(s):  
2005 ◽  
Vol 20 (11) ◽  
pp. 2304-2308 ◽  
Author(s):  
J. P. MBELEK

Results from an almost twenty years study of radiometric data from Pioneer 10/11, Galileo and Ulysses spacecraft indicate an anomalous time depending blueshift1, 2 which bares hardly prosaic explanations. Local manifestation of the expansion of the universe or new force terms are not favored either by the observational data. So, we explore the possibility that the reported anomaly, referred to as the "Pioneer anomaly", does not result from a real change in velocity. It turns out that the main Pioneer anomaly may be looked at as a new validation of general relativity (GR) in the weak field and low velocity limit on account of the "machian" behavior of quintessence like dark energy.


Nature ◽  
2011 ◽  
Vol 477 (7362) ◽  
pp. 9-9
Keyword(s):  

2008 ◽  
Vol 23 (02) ◽  
pp. 109-114 ◽  
Author(s):  
CHRISTIAN CORDA

In the general picture of high order theories of gravity, recently, the R-1 theory has been analyzed in two different frameworks. In this letter a third context is added, considering an explicit coupling between the R-1 function of the Ricci scalar and the matter Lagrangian. The result is a non-geodesic motion of test particles which, in principle, could be connected with Dark Matter and Pioneer anomaly problems.


2009 ◽  
Vol 5 (S261) ◽  
pp. 159-169 ◽  
Author(s):  
A. Fienga ◽  
J. Laskar ◽  
P. Kuchynka ◽  
C. Leponcin-Lafitte ◽  
H. Manche ◽  
...  

AbstractWe present here several gravity tests made with the latest INPOP08 planetary ephemerides. We first propose two methods to estimate the PPN parameter β and its correlated value, the Sun J2, and we discuss the correlation between the Sun J2 and the mass of the asteroid ring. We estimate a possible advance in the planet perihelia. We also show that no constant acceleration larger than 1/4 of the Pioneer anomaly is compatible with the observed motion of the planets in our Solar System.


2007 ◽  
Vol 646 (1) ◽  
pp. 1-5 ◽  
Author(s):  
William F. Hall
Keyword(s):  

2002 ◽  
Vol 17 (14) ◽  
pp. 875-885 ◽  
Author(s):  
JOHN D. ANDERSON ◽  
EUNICE L. LAU ◽  
SLAVA G. TURYSHEV ◽  
PHILIP A. LAING ◽  
MICHAEL MARTIN NIETO

The data from Pioneer 10 and 11 shows an anomalous, constant, Doppler frequency drift that can be interpreted as an acceleration directed towards the Sun of aP = (8.74 ± 1.33) × 10-8 cm / s 2. Although one can consider a new physical origin for the anomaly, one must first investigate the contributions of the prime candidates, which are systematics generated on board. Here we expand upon previous analyses of thermal systematics. We demonstrate that thermal models put forth so far are not supported by the analyzed data. Possible ways to further investigate the nature of the anomaly are proposed.


Focus ◽  
2011 ◽  
Vol 28 ◽  
Author(s):  
David Lindley
Keyword(s):  

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