Measurement of the solar system acceleration using the Earth scale factor

Abstract

We propose an alternative method to detect the secular aberration drift induced by the solar system acceleration due to the attraction to the Galaxy centre. This method is free of the individual radio source proper motion caused by intrinsic structure variation. We developed a procedure to estimate the scale factor directly from very long baseline interferometry (VLBI) data analysis in a source-wise mode within a global solution. The scale factor is estimated for each reference radio source individually as a function of astrometric coordinates (right ascension and declination). This approach splits the systematic dipole effect and uncorrelated motions on the level of observational parameters. We processed VLBI observations from 1979.7 to 2016.5 to obtain the scale factor estimates for more than 4,000 reference radio sources. We show that the estimates highlight a dipole systematics aligned with the direction to the centre of the Galaxy. With this method we obtained a Galactocentric acceleration vector with an amplitude of 5.2 $\pm$ 0.2 μas/yr and direction ${\alpha }_G=281°\pm 3°$ and ${\delta }_G=-35°\pm 3°$.

arXiv commentaccepted to A&A

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• The ACCELERATION programme: I. Cosmology with the redshift drift
• A purely acceleration-based measurement of the fundamental Galactic parameters
• Toward a direct measurement of the cosmic acceleration: the first preparation with FAST
• The Science of Fundamental Catalogs
• Statistical distribution of HI 21cm intervening absorbers as potential cosmic acceleration probes
• Resolving VLBI correlator ambiguity in the time delay model improves precision of geodetic measurements