Stringy Newton Gravity with $H$-flux
  A Symmetry Principle has been shown to augment unambiguously the Einstein
Field Equations, promoting the whole closed-string massless NS-NS sector to
stringy graviton fields. Here we consider its weak field approximation, take a
non-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 $\mathbf{K}$ is
intrinsic to matter. Sourcing $\mathbf{H}$ which is of NS-NS $H$-flux origin,
$\mathbf{K}$ is nontrivial if the matter is `stringy'. $\mathbf{H}$ contributes
quadratically to the Newton potential, but otherwise is decoupled from the
point particle dynamics, i.e. $\bf{\ddot{x}}=-\bf{\nabla}\Phi$. We define
`stringization' analogous to magnetization and discuss regular as well as
monopole-like singular solutions.
