  We present observations of the High Mass X-ray Binary GX 301-2 taken during
the Galactic Plane Scan (GPS) with Integral following our RXTE observations
(Kreykenbohm et al. 2004). The optical companion of GX 301-2 is the B1Ia+
hypergiant Wray 977 with a luminosity of 1.3 x 10^6 Lsun and a mass of ~48 Msun
making the system one of the most massive X-ray binaries known. The system was
observed 24 times during the GPS thus covering many orbital phases including
the pre-periastron flare. The source is clearly detected in all Integral
instruments in most pointings. The derived X-ray light curves show strong
variability on all timescales. Depending on the orbital phase of the pointings,
the luminosity changes by factor of more than 10 during the pre-periastron
flare compared to other pointings. Furthermore, broad band spectra using all
instruments available on Integral are compared with data taken by the RXTE
instruments PCA and HEXTE (using the same data as in Kreykenbohm et al. 2004).
