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220px-HEUraniumC

Uranium, U, is the name of element 92. Wikipedia has an article which provides a lot of information about the element.  This article will focus on things Wikipedia does not stress:

Nuclear properties[]

Information sources[]

Japan Atomic Energy Agency (JAEA) maintains an on-line chart of nuclides which includes decay properties of many predicted nuclides[1] - unlike charts published by Korea Atomic Energy Research Institute (KAERI) or the (U.S.) National Nuclear Data Center (NNDC). This chart gives separate numerical values for partial half-lives against fission, beta emission (both β- and β+), and alpha emission. This reference provides the most focused look at the most significant predicted Pu isotopes. Other references used are cited.

Predicted and observed properties[]

Isotopes from the neutron dripline down to 239U, plus 237U are predicted or observed to decay primarily by beta emission. Half lives are predicted to increase, as A declines, from around 0.001 sec at the dripline to 8 sec at 247U and predicted to reach 3/4 hr in 241U. 240U has an observed half-life of 14.1 hr, and 237U has a half-life of 6.75 days, making those the longest-lived beta-emitting isotopes.

238U, plus isotopes in the band 236U to 232U decay by alpha emission, Of these, only 232U has a half-life less than 105 yr. They are, to say the least, well-studied.

Positive beta decay sets in at 231U, which is almost entirely free of alpha decay (branch ratio = 0.0001). As A declines, alpha decay becomes increasingly important until positive beta decay disappears (below BR = 0.0001) at 227U. Only alpha decay has been observed in the 12 lightest isotopes, down to 215U[2].

Neutron count in 218U is 126, Half-lives for alpha emitting isotopes with N < 126 are in the millisecond range, which is longer than half-lives for isotopes with N slightly above 126. This is to be expected below a neutron shell closure.

211U has been predicted ([3]) to decay by fission, and for half-lives to drop below 10-09 level for isotopes down to 198U. Isotopes in the band 197U to 192U are predicted to have half-lives in the 10-09 - 0.001 sec range.

Occurrence[]

Formation[]

a) Outside Earth

U isotopes from the neutron dripline down to 233U can form during supernovae and neutron star mergers. Rapid capture of electrons occurs in both, and some material ejected from a disintegrating neutron star has A high enough to beta-decay directly to U. Decay chains to lighter isotopes are blocked by 232Th, 231Pa, and 230Th to 226Th[2]. Below that, lower Z elements block decay chains.

b) On Earth

238U does not form on earth. Molar concentration ratio between 234U and 235U is 0.0075 and that of lighter isotopes is effectively 0. Neutrons from 238U spontaneous fission, produce small amounts of 235U and 236U (at 0.20 branch ration). Neutron capture by 236U produces the 6.75 day isotope 237U, so fresh 238U is the result of two neutron captures by the same nucleus within a few days of each other. With neutrons as rare as they are even in rich uranium ore, the chances of that happening are tiny.

It should be noted that the 0.8 branch ratio for fission in 235U is one of two cases of induced nuclear fission contributing to earth's energy sources. The other is 239Pu (0.64 branch ratio for fission)[4].

Persistence[]

As is true of the other elements, most U isotopes are short lived. Only 9 have half-lives over a day. Of these, 5 have half-lives exceeding 105 yr, and 3 have half-lives exceeding 2×106 yr. Considering only material evolving from an initial supernova or kilonova, 233U (1.59×105 yr) and 234U (246×105 yr) can be expected to survive long enough to be incorporated into forming planetesimals. In the case of 234U, those primordial nuclei will eventually fall below the equilibrium concentration between 234U and 238U. By the time fully mature planets form, only 234U will remain. The half-life of 236U is 2.34×107 yr which is roughly the span of time required for a mature terrestrial (rocky) planet to form. 236U would have been a part of the early earth, and its decay energy one of its heat sources. Eventually, the primordial nuclei decayed, and were replaced by those produced by the slow formation by neutron capture which continues to this day.

Atomic properties[]

Wikipedia's article "Uranium" discusses the element's properties in detail. Among those details is the presence of the element on earth. One thing that article did not touch on is the chemical activity of uranium in this context. The element reduces many metals, including iron. Earth's core is depleted in U, which means its mantle is enriched proportionately. Its crustal concentration is higher still.

References[]

2. "Nuclear Properties for Astrophysical Applications"; P. Moller & J. R. Nix; Los Alamos National Laboratory website; search by "LANL, T2", then "Nuclear Properties for Astrophysical Applications".

  1. "Chart of the Nuclides, 2014", Japan Atomic Energy Agency; website available using "chart of nuclides" and "JAEA" as internet search terms.
  2. 2.0 2.1 "Isotopes of uranium", Wikipedia article.
  3. "Decay Modes and a Limit of Existence of Nuclei"; H. Koura; 4th Int. Conf. on the Chemistry and Physics of Transactinide Elements; Sept. 2011.
  4. "Curium", sect. 2.3; "Wikipedia.
9-Period Periodic Table of Elements
1 1
H
2
He
2 3
Li
4
Be
5
B
6
C
7
N
8
O
9
F
10
Ne
3 11
Na
12
Mg
13
Al
14
Si
15
P
16
S
17
Cl
18
Ar
4 19
K
20
Ca
21
Sc
22
Ti
23
V
24
Cr
25
Mn
26
Fe
27
Co
28
Ni
29
Cu
30
Zn
31
Ga
32
Ge
33
As
34
Se
35
Br
36
Kr
5 37
Rb
38
Sr
39
Y
40
Zr
41
Nb
42
Mo
43
Tc
44
Ru
45
Rh
46
Pd
47
Ag
48
Cd
49
In
50
Sn
51
Sb
52
Te
53
I
54
Xe
6 55
Cs
56
Ba
57
La
58
Ce
59
Pr
60
Nd
61
Pm
62
Sm
63
Eu
64
Gd
65
Tb
66
Dy
67
Ho
68
Er
69
Tm
70
Yb
71
Lu
72
Hf
73
Ta
74
W
75
Re
76
Os
77
Ir
78
Pt
79
Au
80
Hg
81
Tl
82
Pb
83
Bi
84
Po
85
At
86
Rn
7 87
Fr
88
Ra
89
Ac
90
Th
91
Pa
92
U
93
Np
94
Pu
95
Am
96
Cm
97
Bk
98
Cf
99
Es
100
Fm
101
Md
102
No
103
Lr
104
Rf
105
Db
106
Sg
107
Bh
108
Hs
109
Mt
110
Ds
111
Rg
112
Cn
113
Nh
114
Fl
115
Mc
116
Lv
117
Ts
118
Og
8 119
Uue
120
Ubn
121
Ubu
122
Ubb
123
Ubt
124
Ubq
125
Ubp
126
Ubh
127
Ubs
128
Ubo
129
Ube
130
Utn
131
Utu
132
Utb
133
Utt
134
Utq
135
Utp
136
Uth
137
Uts
138
Uto
139
Ute
140
Uqn
141
Uqu
142
Uqb
143
Uqt
144
Uqq
145
Uqp
146
Uqh
147
Uqs
148
Uqo
149
Uqe
150
Upn
151
Upu
152
Upb
153
Upt
154
Upq
155
Upp
156
Uph
157
Ups
158
Upo
159
Upe
160
Uhn
161
Uhu
162
Uhb
163
Uht
164
Uhq
165
Uhp
166
Uhh
167
Uhs
168
Uho
169
Uhe
170
Usn
171
Usu
172
Usb
9 173
Ust
174
Usq
Alkali metal Alkaline earth metal Lanthanide Actinide Superactinide Transition metal Post-transition metal Metalloid Other nonmetal Halogen Noble gas
predicted predicted predicted predicted predicted predicted predicted predicted predicted

(12-05-20)