  We present measures for 10 pairs in the constellation of Scorpius using a C14
telescope, Lucky Imaging, and the Reduc software. The separations of Alpha
Centauri AB, as determined from the orbital elements of Pourbaix and Boffin
(2016), were used as an image scale and position angle calibrator. Our internal
uncertainties are ~0.06 arcsec in rho and ~0.06 degree in PA. There is
excellent agreement with historic data extrapolated to epoch of observation
(~2018.53), and micro-arcsecond positions from the GAIA database where the
differences are ~0.05 arcsec in rho and ~0.15 degrees in PA. In addition, we
present rectilinear elements for the 10 Sco pairs and orbital elements for two
of them. Ephemera are given for these pairs based on both the rectilinear
elements and the orbital elements.
