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A Symmetry Principle has been shown to augment unambiguously the EinsteinField Equations, promoting the whole closed-string massless NS-NS sector tostringy graviton fields. Here we consider its weak field approximation, take anon-relativistic limit, and derive the stringy augmentation of Newton Gravity:\[ \begin{array}{lll} {\bf{\nabla}^{2}\Phi}=4\pi G\rho+\bf{H}{\bf{\cdot}}\bf{H}\,, \quad&\qquad\bf{\nabla}\bf{\cdot}\bf{H}=0\,,\quad&\qquad {\bf{\nabla}\bf{\times}\bf{H}}=4\pi G\, \bf{K}\,. \end{array} \]Not only the mass density $\rho$ but also the current density $\mathbf{K}$ isintrinsic to matter. Sourcing $\mathbf{H}$ which is of NS-NS $H$-flux origin,$\mathbf{K}$ is nontrivial if the matter is `stringy'. $\mathbf{H}$ contributesquadratically to the Newton potential, but otherwise is decoupled from thepoint particle dynamics, i.e. $\bf{\ddot{x}}=-\bf{\nabla}\Phi$. We define`stringization' analogous to magnetization and discuss regular as well asmonopole-like singular solutions.

Stringy Newton Gravity with $H$-flux