In non-relativistic quantum theories with short-range Hamiltonians, a velocity v can be chosen such that the influence of any local perturbation is approximately confined to within a distance r until a time t ∼ r/v, thereby defining a linear light cone and giving rise to an emergent notion of locality. In systems with power-law (1/r α ) interactions, when α exceeds the dimension D, an analogous bound confines influences to within a distance r only until a time t ∼ (α/v) log r, suggesting that the velocity, as calculated from the slope of the light cone, may grow exponentially in time. We rule out this possibility; light cones of power-law interacting systems are algebraic for α > 2D, becoming linear as α → ∞. Our results impose strong new constraints on the growth of correlations and the production of entangled states in a variety of rapidly emerging, long-range interacting atomic, molecular, and optical systems. Though non-relativistic quantum theories are not explicitly causal, Lieb and Robinson [1] proved that an effective speed limit emerges dynamically in systems with short-ranged interactions, thereby extending the notion of causality into the fields of condensed matter physics, quantum chemistry, and quantum information science. Specifically, they proved that when interactions have a finite range or decay exponentially in space, the influence of a local perturbation decays exponentially outside of a space-time region bounded by the line t = r/v, which therefore plays the role of a light cone [ Fig. 1(a)]. However, many of the systems to which non-relativistic quantum theory is routinely applied-ranging from frustrated magnets and spin glasses [2,3] The results of Lieb and Robinson were first generalized to power-law (1/r α ) interacting systems by Hastings and Koma [17], with the following picture emerging. For α > D, the influence of a local perturbation is bounded by a function ∝ e vt /r α , and while a light cone can still be defined as the boundary outside of which this function falls below some threshold value, yielding t ∼ log r, that boundary is logarithmic rather than linear [ Fig. 1(b)]. Improvements upon these results exist, revealing, e.g., that the light-cone remains linear at intermediate distance scales [12], but all existing bounds consistently predict an asymptotically logarithmic light cone. An immediate and striking consequence is that the maximum group velocity, defined by the slope of the light cone, grows exponentially with time, thus suggesting that the aforementioned processes -thermalization, entanglement growth after a quench, etc. -may in principle be sped up exponentially by the presence of long-range interactions. In this manuscript, we show that this scenario is not possible. While light cones can potentially be sub-linear for any finite α, thus allowing a velocity that grows with time, for α > 2D they remain bounded by a polynomial t ∼ r ζ , and ζ ≤ 1 approaches unity for increasing α [ Fig. 3(c)].Model and formalism.-We assume a generic spin model with time-independent Ham...