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TABLE II continued 4 70 71 Yb Lu 1.5 o,m 1.5 0,48 1.5 0.48 0.110 0.0251 72 Hf 1.5 0,7 O0555 0,219 73 74 Ta W 0,^40 14,5 0.51 17.0 0.26 13.0 ? 0.0363 0.352 75 Re 0.12 0.41 - 0
TABLE III Element A N I Log H H 1 H 2 iL 1 -1 0 10,56 10.56 6.72 3.62 X 10^^ 3.62 X W'^ 5.2 X 10^ 2 He 4 1 2 -1 0 9»^5 9.45 2o8 X 10- 2,8 X 109 3 Li 6 3 4_ 0 1 2.00 0.87 1-97 100 7.4 92,6 4 Be 9_ 3__ 1 lj!i30 20 5 B 10 11. i 0 1- 1.38 0.65 1.29 24 ^,5 19.5 6 C 12 6 X 0 6.83 6.82 4.87 6.75 X 10^ 6,67 X 10^ 7.4 X 10^ 7 N 14 15 i 0 7.15 7.15 4,71 1,41 X lOj 1.41 X 10*; 5.1 X 10^ 8 0 16 8 if 0 1 2 7.40 7.40 3.97 4.71 2,5 X lOj 2.5 X 104 9.3 X jof 5,1 X 10^ 9 P Li 10 1^ 3.20 1600 10 Ne 20 21 22 10 11 12 0 1 2 7.00 6.95 4.48 5,99 1,0 X lOl 9.0 X 10° 3.0 X 107 9.7 X 10^
Page 1 and 2:
05" 9003'9 ,^ r.V- ou 15 -^ CBNTiJA
Page 3 and 4:
DISCLAIMER Portions of this documen
Page 5 and 6:
o which states that the elements wi
Page 7 and 8:
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: TABLE II continued 3 45 Rh 1.3 3,5
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 86 and 87: Blbliography-2 Pellenberger, Th.v.,
Page 88 and 89: Pinson, W.H., Ahrens, L.H. and Fran
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