  Dynamical effects in general relativity have been finally, relatively
recently observed by LIGO\cite{2016LRR....19....1A}. To be able to measure
these signals, great care has to be taken to minimize all sources of noise in
the detector. One of the sources of noise is called Newtonian noise. In this
article we present an analysis of the dynamical (time dependent) nature of the
Newtonian noise. In that respect, it is a misnomer to call it Newtonian noise,
the Newtonian theory does not afford any dynamical notion of the gravitational
field. The dynamical aspects of the nature of the Newtonian noise have
heretofore been disregarded as they were considered negligible. However, we
demonstrate that they are indeed not far from the realm of being measurable.
They could be used to validate Einsteinian general relativity or to give
valuable information on the true dynamical nature of gravity. One fundamental
question, for example, is a direct measurement the speed of propagation of
gravitational effects and the verification that it is indeed the same as the
speed of light. We propose a simple laboratory experiment that could affirm or
deny this proposition. We also analyze the possibility of the detection of
large geophysical events, such as earthquakes. We find that large seismic
events seem to be easily observable with the present ensemble of gravitational
wave detectors,. The ensemble of gravitational wave detectors could easily
serve as a system of early warning for otherwise catastrophic seismic events.
