  It is generally accepted that the lifetime of molecular clouds does not
exceed $3\cdot 10^7$ yr due to disruption by stellar feedback. We put together
some arguments giving evidence that a substantial fraction of molecular clouds
(primarily in the outer regions of a disc) may avoid destruction process for at
least $10^8$ yr or even longer. A molecular cloud can live long if massive
stars are rare or absent. Massive stars capable to destroy a cloud may not form
for a long time if a cloud is low massive, or stellar initial mass function is
top-light, or if there is a delay of the beginning of active star formation. A
long duration of the inactive phase of clouds may be reconciled with the low
amount of the observed starless giant molecular clouds if to propose that they
were preceded by slowly contraction phase of the magnetized dark gas,
non-detected in CO-lines.

Astrophysics of Galaxies;Cosmology and Nongalactic Astrophysics