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We report on the diffuse X-ray emissions from the Galactic center (GCDX)observed with the X-ray Imaging Spectrometer (XIS) on board the Suzakusatellite. The highly accurate energy calibrations and extremely low backgroundof the XIS provide many new facts on the GCDX. These are (1) the origin of the6.7/7.0keV lines is collisional excitation in hot plasma, (2) new SNR andsuper-bubble candidates are found, (3) most of the 6.4keV line is fluorescenceby X-rays, and (4) time variability of the 6.4keV line is found from the SgrB2complex.

X-Ray Observations of the Galactic Center with Suzaku