Using precession of orbits due to non-Newtonian interaction between two celestial bodies and modern tracking data of satellites, planets and a pulsar we obtain new more precise limits on possible Yukawa-type deviations from the Newton law in planets (satellites)radii ranges.
@article{arxiv.gr-qc/0302048,
title = {Test of inverse square law through precession of orbits},
author = {N. I. Kolosnitsyn and V. N. Melnikov},
journal= {arXiv preprint arXiv:gr-qc/0302048},
year = {2009}
}