The polar mesopause in summer is the coldest region of the Earth because gravity wave-driven mean meridional circulation results in upwelling and adiabatic cooling in the summer polar mesopause region (see e.g., Fritts et al., 2003). Accurate observations of mesopause temperature are essential for studying the short-term dynamics and long-term climate of the middle and upper atmosphere. However, the specific environment of the mesosphere makes obtaining continuous measurements of mesopause temperature quite difficult. Ground-based radio radars, such as MF (medium frequency) and VHF (very high frequency) radars, are widely used to measure the neutral horizontal wind in the mesosphere, but they are not capable of measuring temperature. Ground-based optical instruments, such as lidars and airglow spectrometers, can provide high temporal resolution and accurate temperature measurements but are limited to clear sky and often to nighttime conditions. Sounding rockets can provide a good in situ soundings of neutral mesospheric temperatures, but the high cost and complicated logistics of launching rockets generally make them impractical for routine observations. Meteor radars have been widely employed for investigating the mesosphere and lower thermosphere (MLT) region for decades, especially for the neutral wind of the MLT region. Because of the advantages Abstract We present the climatology of mesopause temperatures using high-latitude and middlelatitude meteor radars. The daily mesopause temperatures are estimated using ambipolar diffusion coefficient data from the meteor radars at Davis Station (68.6°S, 77.9°E), in Antarctica, Svalbard (78.3°N, 16°E), Tromsø (69.6°N, 19.2°E) in the Arctic, and Mohe (53.5°N, 122.3°E) and Beijing (40.3°N, 116.2°E) in the northern middle latitudes. The seasonal variations in the meteor radar-derived temperatures are in good agreement with the temperatures from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument onboard the TIMED satellite. Interhemispheric observations indicate that the mesopause temperatures over the southern and northern polar regions show a clear seasonal asymmetry. The seasonal variations in the Davis Station meteor radar temperatures in the southern polar mesopause are dominated by an annual oscillation (AO) with a relatively weak semiannual oscillation (SAO), which show a clear minimum during summer and a maximum during winter. The mesopause temperatures in the northern high and middle latitudes observed by the Svalbard, Tromsø, Mohe, and Beijing meteor radars mainly show an AO, with a maximum during winter and a minimum during summer. The AO in the northern polar regions is stronger than that in the southern polar regions, while the SAO in the southern polar regions is relatively strong compared to that in the northern polar regions. YI ET AL.