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["Table 1 Lunar regolith samples imaged by microtomography in the present study."]
[]
["sample","mission","sampling site","grain size (mm)","maturity","energy (keV)","voxel size (mm)","N"]
[10084,"Apollo 11","Mare Tranquillitatis","75-105","mature2)","20. 24.9","1.73, 1.74",199]
["L1613-1","Luna 16","Mare Fecunditatis","<83","mature or submature",25,1.3,107]
["L1613-3",null,null,"127-200",null,"20, 24.9","1.73, 1.74",389]
["L24130.3-1","Luna 24","Mare Crisium","<74","immature",25,1.3,65]
["L24130.3-2",null,null,"74-95",null,"20, 24.9","1.73, 1.74",1108]
["L24130.3-3",null,null,"95-200",null,"20, 24.9","1.73, 1.74",318]
["L24130.3-4",null,null,"200-370",null,20,1.73,102]
["605011)","Apollo 16","Descartes Highlands","75-105","mature3)",20,1.73,104]
["L2001-1","Luna 20","Apollonius Highlands ","<83","mature or submature",25,1.3,143]
["L2001-4",null,null,"200-450",null,"17.9, 18.1, 24","1.73, 1.74",103]
[]
["1) Particles of 105-250 mm in size also examined with microtomography by Katagiri et  al. (2014)"]
["2) Is/FeO = 78 (Morris et al. 1978)"]
["3) Is/FeO = 80 (Morris et al. 1978)"]