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TABLE III Continued 2 11 Na 23 12 1 4.60 4,0 x lO'^ 12 Mg 24 i 12 li 0 1 6,15 6,04 5-15. 5,19 1.41 X 10§ 1.11 X 10? 1,41 X 10? 1755 X 10-^ 13 Al 27 14 1 4.80 6,3 X 10^ 14 Si 28 29 W 14 i5> 16^ 0 1 2 6.00 5,96 4.67 4,49 1,0 X 10? 9o2 X 10^ ft- 4.7 X 10,^ »••••• .ill .———«) 15 P .3L 16 1 ?
21 22 23 24 25 26 27 28 29 Sc Ti V Cr m. Pe Co Hi Cu i£5 46 50 51 50 52 ?5. 54 56 Ik 51 60 61 62 64 63 65- 24 24 25 '26 27 W 27 28 26 28 30. 28 30 ^1 3"? 12 30 32 33 W 36 34 35- TABLE III Continued 3 1 2 3 •If 4 5 2 4 i 5. 2 4 i 2 4 1 8 5 T 1,68 3,01 1,91 1.90 1?78T 1:74 2.58 0.00 2,58 4,26 2,90 4ol8 3,24 sTsar 3.90 5-78 4,55 5,75 4.14 3,30 3,24 4,44 4.27 3.87 2«>5? 3.65 2.50 2,36 2.20 48 1020 81 56,2 §4,5' 380 1 379 18170 800 15200 1730 7900 6.084 X 105 3,59 X loj 5.57 X 105 1,34 X Kr 2000 1730. 27400 18570 7170 340 lOM" 518 228 7tr.5
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 and 70: TABLE II continued 3 45 Rh 1.3 3,5
Page 71: TABLE III Element A N I Log H H 1 H
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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