  The orbits of 8 systems with low-mass components (HIP 14524, HIP 16025, HIP
28671, HIP 46199, HIP 47791, HIP 60444, HIP 61100 and HIP 73085) are presented.
Speckle interferometric data were obtained at the 6 m Big Alt-azimuth Special
Astrophysical Observatory of the Russian Academy of Sciences (BTA SAO RAS) from
2007 to 2019. New data, together with measures already in the literature, made
it possible to improve upon previous orbital solutions in six cases and to
construct orbits for the first time in the two remaining cases (HIP 14524 and
HIP 60444). Mass sums are obtained using both Hipparcos and Gaia parallaxes,
and a comparison with previously published values is made. Using the Worley &
Heintz criteria, the classiffcation of the orbits constructed is carried out.
