We investigate the umbral oscillation at multi-height solar atmospheres above a sunspot in the active region National Oceanic and Atmospheric Administration (NOAA) 12680 on 2017 September 15. In this study, the extreme ultraviolet images were measured by the Atmospheric Imaging Assembly (AIA), while the ultraviolet spectral lines and images were observed by the Interface Region Imaging Spectrograph. At the sunspot umbra, the AIA 1700 Å intensity curve shows the primary oscillation with a long period of ~(4.2士0.8) minutes, while the intensity curves in AIA 1600 Å, 171 Å and 193 Å exhibit an，apparent oscillation with a short period of ~(2.8士0.3) minutes. Meanwhile, a short period of ~(3. 1土0.5)minutes is found in the MgIIh & k lines and the slit-jaw image at 2796 Å, a short period of ~(2.9土0.4)minutes is detected in the Si IV 1393.76 Å line. Our observations suggest that the oscillatory periods at the sunspot umbra decrease with the height of solar outer atmospheres. The short period is roughly equal to 3 minutes, which could be interpreted as the propagating slow magnetoacoustic wave above the sunspot umbra, and it might originate from the temperature minimum region and then propagate up to the corona.While the long period is close to 5 minutes oscillation in the photosphere, which might be regarded as the solar P-mode wave.