  We present here a quantitative, accurate estimate of the impact of
uncertainties of astrophysical nature on the determination of the dark matter
distribution within our Galaxy, the Milky Way. Based on an update of a previous
analysis, this work is motivated by recent new determinations of astrophysical
quantities of relevance -- such as the Galactic parameters (R0,V0) -- from the
GRAVITY collaboration and the GAIA satellite, respectively. We find that even
with these state-of-the-art determination and a range of uncertainties -- both
statistical and systematic -- much narrowed with respect to previous work, the
uncertainties on the dark matter distribution and their impact on searches of
physics beyond the standard model stays sizable.
