  We propose to formulate a theory for Classical Stochastic Gravity for certain
applications in Astrophysics and Cosmology.This involves the Langevin approach
in curved spacetime, which is introduced here, in the form of a classical
Einstein-Langevin equation.The domain of applications of such an approach and
possible outcomes of this formulation which are quite different than its
semiclassical counterpart (which is an active area of research), are
discussed.This field of study can be seen to emerge out of well established
ideas and results in Brownian motion theory as well as the Stochastic
Semiclassical Gravity and related issues in Thermodynamics. A brief
calculation, to demonstrate the contribution of stochasticty and induce
fluctuations to the background spacetime via heuristic solution of the Einstein
Langevin equation is given .The applicability of the proposed theme can have a
wider expanse than is mentioned in this article.
