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Newtonian gravitation is non-radiative but is extremely pervasive andpenetrates equally into every media because it cannot be shielded. The extraterrestrial fgravity is responsible for earth's trajectory. However itscorrelation or geodesic deviation is manifested as semi-diurnal and diurnaltides. Tidal signals, A(t) are temporal modulations in the field differentialwhich can be observed in a wide variety of natural and laboratory situations.A(t) is a quasi-static, low frequency signal which arises from the relativechanges in positions of the detector and source and is not part of theelectromagnetic spectrum. Isaac Newton was the first to recognize theimportance of tides in astrometry and attempetd to estimate lunar mass fromocean tides. By a case study we show, how the systematics of the gravitationalcorrelation can be used for calibration and de-trending which can significantlyincrease the confidence level of high precision experiments. A(t) can also beused to determine the distribution of celestial masses independently of the"1-2-3" law. Guided by modern advances in gravity wave detectors we argue thatit is important to develop high precision accelerometry. With a resolution ofabout a nano-m it will be possible to determine solar system masses and detectthe SMBH at the center of our galaxy. Observations of the gravitationalcorrelation can potentially open up yet to be explored vistas of the cosmos.

Tidal Accelerometry: Exploring the Cosmos Via Gravitational Correlations