Giant impact was an energetic process Deep magma ocean or total melting of the Earth is compatible with the giant impact model A. G. W. Cameron 2011/12/21 ここまで
How deep was the terrestrial magma ocean ? What is the condition of the metal-silicate equilibrium, low pressure or high pressure ?
図17 Sm Eu Gd
図 5 難揮発性の親石元素 Sc Ti Y La Eu Tb Lu Th. U V Sm Mg Si Ca Ba Ce. Nd Sr Yb Ta Li Zr Nb Al (Mantle+Crust)/C 1 1. 0 低 高 Cr 難揮発性の元素 揮発性・やや揮発性の元 素 < 1300 K 親鉄元素 Fe 揮発性の程度 Cu Mn Ga Na Sn Co K 揮発性 元素 Rb 0. 1 Ni 親 鉄 元 素 0. 01 Zn P 強親鉄元素 In Re Cd Ge Ag 0. 01 0. 001 Tl Pb Ir Os Cs Au Bi
(Mantle composition/(CI-chondrite+Mg) Depletion factor 親鉄元素の枯渇 枯渇の理由 核に分配された (+揮発性) Al Mg Ca Ti 分配係数, D C(CI chondrite) C(mantle) = ━━━━━━ F(core)・D + F(mantle) Si C (M) in metal D = ━━━━━━ C (M) in silicate, oxide Fe Co Ni F (core)=0. 325 F(mantle)=0. 675(wt. fraction) C: abundance(wt. %) Mc. Donough and Sun (1995) 低圧での平衡に比べてマントルに Niが多すぎる。 3
Asuka 881757 (lunar meteorite) No. 9 No. 7 F d No. 11 Grain 2 the mean age of the glass and the maskelynite, 3798+/ -12 Ma of the 39 Ar-40 Ar ages Grain 3 Grain 1 No. 4 No. 12 F d F d No. 9 No. 1 No. 21 No. 5 16 No. 8 No. 6 3 No. 4 No. 11 No. 25 -26 No. 23 No. 22
http: //www. haberer-meteorite. de/english/Asteroid%202008%20 tc 3/Asteroid%202008%20 TC. html Meteorongs in large number (basalt) Almahata Sitta The main mass (in private hands) of 155, 57 g Coarse-grained Ureilite MS-170 Slices & fragments