A new preprint quantifies the upcoming GJ 710 passage at 0.0621 pc (~10,000 AU) in 1.3 Myr using linear motion approximations on a volume-complete sample of stars within 25 pc, after correcting radial velocities for gravitational redshift and convective blueshift biases. The study reports an encounter rate of 10.6 ± 4.5 per Myr within 1 pc, or one every ~95 kyr on average, rendering the GJ 710 event statistically rare at roughly one per 50 Myr. While the linear approximation and binary corrections improve statistics over prior Gaia DR2 analyses, they understate long-term gravitational focusing and galactic tide synergies that could amplify Oort cloud perturbations beyond the paper's immediate 0.47-Myr window. Earlier work such as Dybczyński & Berski (2018) already flagged similar minimum distances, yet this update sharpens the kinematics and highlights how such a flyby can raise inner-solar-system comet flux by factors of several on Myr timescales, potentially elevating impact probabilities centuries to millennia after closest approach. Limitations include edge incompleteness in the time window and the assumption that most encounters are single stars rather than unresolved multiples.