Blbliography-2 Pellenberger, Th.v., Mitt- Bebensra, Hyg. 18, 149 (1927). Pellenberger, Th.v., Biochem. 2. I87, 1 (1927). Pellenberger, Th.v. and Lunde, G., Norsk. Geol. Tids. 9, 48 (1926). Pellenberger, Th.v. and Lunde, Q., Biochem. Zeit. I87, 15, (I926). Glendenin, L.E., Steinberg, E.F., Inghram, M.Q., and Hess, D.C., Phys. Rev. 84, 860 (1951). Qoldberg, E. and Brown, H., Anal. Chem. 22, 508 (195O). Goldberg, S., Uchiyama, A. and Brown, H., Geochim. et Cosmoehim. Acta 2, 1 (1951). Qoldschmidt, V.M,, Geochemistry, Oxford University Press (1954). Qoldschmidt, V.M., Qeochemische Verteilungsgesetze der Elemente, IX, Shrifter Norshe Vidensskaps Akad. 1, Oslo I, Nat-naturv, Klasse No. 4 (1957) or (1938). Qoldschmidt, V.M. and Peters, C, Nachr. Ges., Wiss. GSttlngen, Math.-physlk. Klasse, IV, l4l (1935 a). Qoldschmidt, V.M. and Peters, C, Nachr. Ges., Wiss. GSttingen, Math.-physik. Klasse, III, 56; IV, 57 and 278 (1953 b). Greenstein, J. and Richardson, R.S., Astrophys. J. :L15, 556 (1951). Harklns, W«D., J. Am. Chem. Soc. 59,, 856 (1917). Haxel, 0., Jensen, J.H.D„, Suess, H.E., Phys. Rev. 75, I766 (1949). ""• Herzog, L. and Pinson, W.H., Private Communication (1955). Hess, H., Private Communication (1955)* Hevesey, G.v., Kgl. Danske Videnskab. Selskab., Nat. fys. Medd. VI, 7 (1925). Hevesey, G.v. and Hobbies R., Z. anorg^ allgem. Chera. 212, 154 (1955). Hevesey, G.v. and WUrstlin, K., Z. physlk. allgem. Chera. 216, 505 (1954). Ifevesey, G.v. and WUrstlin, K.^ z. physik. Chem., A^, Haber-Bajid 605 {1928)»
Blbliography-5 Hughes, D.J. and Sherman, D., Phys. Rev. 78, 632 (195O). Hunnaerts, J., Trans. Int. Astron. Union 7, 462 (195O). Kopferman, H. and Wessel, C, Zeit. f. Phys. 150, 100 (1951). Koritnig, S., Qeochim. et Cosmoehim. Acta 1, 89 (1951). Kuroda, P.K., and Sandell, E.B,, Geochim. et Cosmoehim. Acta 6, 59 (1954). Landergren, S., Arkiv. Kemi, Mineral, Geol. I9A, Ko. 25, 7 (1948); No. 26, 51 (1948). Mattauch, J,, Physik. Z. 91^ 36I (1954). Mayer, M.Goeppert, Phys. Rev. 74, 255 (1948). Mayer, M.Goeppert, Phys. Rev. 7^, 1969 (1949). Mayer, M.Goeppert and Jensen, H., Elementary Theory of Nuclear Shell Structure, Wiley and. Sons, New York (1955). Mlnaral, E., Nachr. Ges. Wiss. C^ttingen IV, N.P., 1, No. 14, p. 155 (1935). Mlnnaert, M., The Sun, Ed. by G.P, Kulper, University of Chicago Press (1953). Mueller^ Q.^ Gteochlm. et Cosmoehim. Acta 4, 1 (1952). Nevin, L. and de Jager, C, B.A.N. 12. 105 (1954). Noddack, I., Zeit. anorg. allgem. Chem, 225, 537 (1935). Noddack, I. and Noddack, W., Naturwlss. 33,, 59 (1930). Noddack, I. and Noddack, W., Zeit. physik. Chem. A 154, 207 (1951). Noddack, I. and Noddack, W., Svensk. Kemisk Tidskrlft 46, 175 (1934). "~ Onishi, H, and Sandell, E.B«, Qeochim. et Cosmoehim. Acta 7? 1 (1955). Patterson, C, Qeochim. et Cosmoehim. Acta, In Press (1955)* Patterson, C, Brown, H., Tilton, G., and Inghram, M., Phys. Rev. 92, 1254 (1955).
- Page 1 and 2:
05" 9003'9 ,^ r.V- ou 15 -^ CBNTiJA
- Page 3 and 4:
DISCLAIMER Portions of this documen
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o which states that the elements wi
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inattention will be drawn to any ev
- Page 9 and 10:
6 the proportions 10:1:2- The Nodda
- Page 11 and 12:
8 Just in the case of these element
- Page 13 and 14:
10 spectral lines on the temperatur
- Page 15 and 16:
12 have studied the iron sulfide fr
- Page 17 and 18:
14 the proportion of the three phas
- Page 19 and 20:
16 by more than a factor of 10, e.g
- Page 21 and 22:
18 million times smaller than that
- Page 23 and 24:
20 as occurs at other points in the
- Page 25 and 26:
22 220 ppm relative to silicon equa
- Page 27 and 28:
24 abundances, R, and column three
- Page 29 and 30:
26o The heavier rare gases^ Bie rar
- Page 31 and 32:
28, the amount is very constant nea
- Page 33 and 34:
30o valueso This ratio is 300 hy we
- Page 35 and 36: greater constancy in the copper dat
- Page 37 and 38: 33 o mass curve we natst assun® ab
- Page 39 and 40: 35. Noddack*s value of 1.86 for the
- Page 41 and 42: 37 value. Undoubtedly a marked decr
- Page 43 and 44: 3Bo meteorites. We have selected a
- Page 45 and 46: 40 than that given by Noddack (1955
- Page 47 and 48: 42 The average is secured by assumi
- Page 49 and 50: 44 these data all appear to be doub
- Page 51 and 52: 46 ppm are not presented with great
- Page 53 and 54: 48 We adopt values for u235, u^^°
- Page 55 and 56: 50 the elements were formed at leas
- Page 57 and 58: i»2o for the sum of isobaric abund
- Page 59 and 60: 5u« This means that the In^^^ in n
- Page 61 and 62: :>6„ of the neutron excess number
- Page 63 and 64: dance values fitting into the trend
- Page 65 and 66: OUo 56 56 The hjalf life of m , whi
- Page 67 and 68: TABLE II 6 Atomic Abundances of the
- Page 69 and 70: TABLE II continued 3 45 Rh 1.3 3,5
- Page 71 and 72: TABLE III Element A N I Log H H 1 H
- Page 73 and 74: 21 22 23 24 25 26 27 28 29 Sc Ti V
- Page 75 and 76: TABLE III Continued 5 37 Rb p- 37.
- Page 77 and 78: 52 55 5^ 55 56 57 58 Te I Xe Cs Bn
- Page 79 and 80: 67 Ho 68 Er 71 Lu 72 Hf 73 Ta 74 W
- Page 81: TABLE III Continued 11 122 124 40 4
- Page 88 and 89: Pinson, W.H., Ahrens, L.H. and Fran