Author/Authors :
Yamashita، نويسنده , , N. and Gasnault، نويسنده , , O. and Forni، نويسنده , , O. and dʹUston، نويسنده , , C. and Reedy، نويسنده , , R.C. and Karouji، نويسنده , , Y. and Kobayashi، نويسنده , , S. and Hareyama، نويسنده , , M. and Nagaoka، نويسنده , , H. and Hasebe، نويسنده , , N. and Kim، نويسنده , , K.J.، نويسنده ,
Abstract :
The first unambiguous global distribution of Ca on the Moon has been revealed by the Kaguya Gamma-Ray Spectrometer. The observation of the 3737 keV gamma rays from 40Ca with a high energy resolution Ge detector, corrected for fast neutrons, improved greatly our confidence in these remote sensing data. While the derived Ca abundance generally confirms the mare-highland dichotomy, we found that the eastern mare regions such as Crisium, Nectaris, and Fecunditatis exhibit unexpected high Ca abundances. This may be explained by regional concentrations of high-Ca clinopyroxene. Our Ca map also shows that the lowest CaO abundance found in the returned samples (∼8 wt%) may actually be common in Oceanus Procellarum, suggesting the possible sampling bias of Apollo and Luna missions. These observational results on Ca serve as a complementary criterion for better characterization of mare regions on the Moon.
Keywords :
Calcium , high-Ca pyroxene , Kaguya , SELENE , Gamma-ray spectroscopy , moon