The MACRO underground detector at Gran Sasso has recorded about 30 mil
lion muon events in the period 1989-1995. We have analyzed these data
to look for time variations and to study the pointing capabilities of
the apparatus in the search for astrophysical point sources. We have o
bserved a 3% seasonal variation of the high energy muon rate, due to a
tmospheric temperature variations, in agreement with theoretical predi
ctions. We report also the detection of the moon shadowing effect with
a statistical significance of 3.7 sigma. The results obtained straigh
ten the possibility that a ''muon astronomy'' using underground experi
ments is possible.