Stable isotope

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Periodic table colored according to the number of stable isotopes. It can be seen that odd-atomic number elements have fewer stable isotopes than their even neighbours.
Periodic table colored according to the number of stable isotopes. It can be seen that odd-atomic number elements have fewer stable isotopes than their even neighbours.

Stable isotopes are chemical isotopes that are not radioactive (to current knowledge). Stable isotopes of the same element have the same chemical characteristics and therefore behave almost identically. The mass differences, due to a difference in the number of neutrons, result in partial separation of the light isotopes from the heavy isotopes during chemical reactions (isotope fractionation). For example, the difference in mass between the two stable isotopes of hydrogen, 1H (1 proton, no neutron, also known as protium) and 2H (1 proton, 1 neutron, also known as deuterium) is almost 100%. Therefore, a significant fractionation will occur.

Commonly analysed stable isotopes include oxygen, carbon, nitrogen, hydrogen and sulfur. These isotope systems have been under investigation for many years as they are relatively simple to measure. Recent advances in mass spectrometry (ie. multiple-collector inductively coupled plasma mass spectrometry) now enable the measurement of heavier stable isotopes, such as iron, copper, zinc, molybdenum, etc.

Stable isotopes have been used in botanical and plant biological investigations for many years, and more and more ecological and biological studies are finding stable isotopes (mostly carbon, nitrogen and oxygen) to be extremely useful. Other workers have used oxygen isotopes to reconstruct historical atmospheric temperatures, making them important tools for climate research.

Most of naturally occurring isotopes are stable; however, a few tens of them are radioactive with very long half-lives. If the half life of a nuclide is comparable to or greater than the Earth's age (4.5 billions years), a significant amount will have survived since the formation of the Solar System, and will contribute to the natural isotopic composition of a chemical element. The lowest half lives of such isotopes are around 700 million years (e.g., 235U). Many isotopes that are presumed to be stable (i.e. no radioactivity has been observed for them) are predicted to be radioactive with extremely long half-lives (sometimes as high as 1018 years or more). If the predicted half life falls into an experimentally accessible range, such isotopes have a chance to move from the list of stable nuclides to the radioactive category, once their activity is observed. Good examples are bismuth-209 and tungsten-180 which have been recently (2003) found to be alpha-active.

Contents

[edit] Research areas

The Island of Stability may reveal a number of stable atoms that are heavier (and with more protons) than lead.

[edit] Stable isotope fractionation

There are three types of isotope fractionation:

[edit] List of stable isotopes

See also: List of elements by nuclear stability

There are 81 known elements which have at least one stable isotope. As of September 2007, there were 250 known stable isotopes. Tin has 10 stable isotopes, more than any other element. Xenon is the only element which has 9 stable isotopes. There is no element with exactly 8 stable isotopes. Mononuclidic elements are those that have a single isotope (stable or very long-lived) in their natural abundance. Every element from hydrogen to lead has at least one stable isotope with the exceptions of technetium and promethium; elements with more than 82 protons only have radioactive isotopes, although they can still occur naturally because their half-lives are of an order of magnitude not much less than that of the time since the death of a nearby star, or because they occur in a decay chain of another radioactive isotope with such a half-life. It wasn't until 2003 that bismuth-209 was shown to be radioactive.[1] All stable isotopes are the ground states of nuclei, excluding tantalum-180m, which is the excited level (the ground state of this nucleus is radioactive), but its decay is extremely strongly forbidden by spin-parity selection rules.

  1. Hydrogen-1
  2. Hydrogen-2
  3. Helium-3
  4. Helium-4
  5. Lithium-6
  6. Lithium-7
  7. Beryllium-9
  8. Boron-10
  9. Boron-11
  10. Carbon-12
  11. Carbon-13
  12. Nitrogen-14
  13. Nitrogen-15
  14. Oxygen-16
  15. Oxygen-17
  16. Oxygen-18
  17. Fluorine-19
  18. Neon-20
  19. Neon-21
  20. Neon-22
  21. Sodium-23
  22. Magnesium-24
  23. Magnesium-25
  24. Magnesium-26
  25. Aluminium-27
  26. Silicon-28
  27. Silicon-29
  28. Silicon-30
  29. Phosphorus-31
  30. Sulfur-32
  31. Sulfur-33
  32. Sulfur-34
  33. Sulfur-36
  34. Chlorine-35
  35. Chlorine-37
  36. Argon-36
  37. Argon-38
  38. Argon-40
  39. Potassium-39
  40. Potassium-41
  41. Calcium-40
  42. Calcium-42
  43. Calcium-43
  44. Calcium-44
  45. Scandium-45
  46. Titanium-46
  47. Titanium-47
  48. Titanium-48
  49. Titanium-49
  50. Titanium-50
  51. Vanadium-51
  52. Chromium-50
  53. Chromium-52
  54. Chromium-53
  55. Chromium-54
  56. Manganese-55
  57. Iron-54
  58. Iron-56
  59. Iron-57
  60. Iron-58
  61. Cobalt-59
  62. Nickel-58
  63. Nickel-60
  64. Nickel-61
  65. Nickel-62
  66. Nickel-64
  67. Copper-63
  68. Copper-65
  69. Zinc-64
  70. Zinc-66
  71. Zinc-67
  72. Zinc-68
  73. Zinc-70
  74. Gallium-69
  75. Gallium-71
  76. Germanium-70
  77. Germanium-72
  78. Germanium-73
  79. Germanium-74
  80. Arsenic-75
  81. Selenium-74
  82. Selenium-76
  83. Selenium-77
  84. Selenium-78
  85. Selenium-80
  86. Bromine-79
  87. Bromine-81
  88. Krypton-78
  89. Krypton-80
  90. Krypton-82
  91. Krypton-83
  92. Krypton-84
  93. Krypton-86
  94. Rubidium-85
  95. Strontium-84
  96. Strontium-86
  97. Strontium-87
  98. Strontium-88
  99. Yttrium-89
  100. Zirconium-90
  101. Zirconium-91
  102. Zirconium-92
  103. Zirconium-94
  104. Niobium-93
  105. Molybdenum-92
  106. Molybdenum-94
  107. Molybdenum-95
  108. Molybdenum-96
  109. Molybdenum-97
  110. Molybdenum-98
    Technetium - No stable isotopes
  111. Ruthenium-96
  112. Ruthenium-98
  113. Ruthenium-99
  114. Ruthenium-100
  115. Ruthenium-101
  116. Ruthenium-102
  117. Ruthenium-104
  118. Rhodium-103
  119. Palladium-102
  120. Palladium-104
  121. Palladium-105
  122. Palladium-106
  123. Palladium-108
  124. Palladium-110
  125. Silver-107
  126. Silver-109
  127. Cadmium-106
  128. Cadmium-108
  129. Cadmium-110
  130. Cadmium-111
  131. Cadmium-112
  132. Cadmium-114
  133. Indium-113
  134. Tin-112
  135. Tin-114
  136. Tin-115
  137. Tin-116
  138. Tin-117
  139. Tin-118
  140. Tin-119
  141. Tin-120
  142. Tin-122
  143. Tin-124
  144. Antimony-121
  145. Antimony-123
  146. Tellurium-122
  147. Tellurium-123
  148. Tellurium-124
  149. Tellurium-126
  150. Iodine-127
  151. Xenon-124
  152. Xenon-126
  153. Xenon-128
  154. Xenon-129
  155. Xenon-130
  156. Xenon-131
  157. Xenon-132
  158. Xenon-134
  159. Xenon-136
  160. Caesium-133
  161. Barium-132
  162. Barium-134
  163. Barium-135
  164. Barium-136
  165. Barium-137
  166. Barium-138
  167. Lanthanum-139
  168. Cerium-136
  169. Cerium-138
  170. Cerium-140
  171. Cerium-142
  172. Praseodymium-141
  173. Neodymium-142
  174. Neodymium-143
  175. Neodymium-145
  176. Neodymium-146
  177. Neodymium-148
    Promethium - No stable isotopes
  178. Samarium-144
  179. Samarium-150
  180. Samarium-152
  181. Samarium-154
  182. Europium-153
  183. Gadolinium-154
  184. Gadolinium-155
  185. Gadolinium-156
  186. Gadolinium-157
  187. Gadolinium-158
  188. Gadolinium-160
  189. Terbium-159
  190. Dysprosium-156
  191. Dysprosium-158
  192. Dysprosium-160
  193. Dysprosium-161
  194. Dysprosium-162
  195. Dysprosium-163
  196. Dysprosium-164
  197. Holmium-165
  198. Erbium-162
  199. Erbium-164
  200. Erbium-166
  201. Erbium-167
  202. Erbium-168
  203. Erbium-170
  204. Thulium-169
  205. Ytterbium-168
  206. Ytterbium-170
  207. Ytterbium-171
  208. Ytterbium-172
  209. Ytterbium-173
  210. Ytterbium-174
  211. Ytterbium-176
  212. Lutetium-175
  213. Hafnium-176
  214. Hafnium-177
  215. Hafnium-178
  216. Hafnium-179
  217. Hafnium-180
  218. Tantalum-180m
  219. Tantalum-181
  220. Tungsten-182
  221. Tungsten-183
  222. Tungsten-184
  223. Tungsten-186
  224. Rhenium-185
  225. Osmium-187
  226. Osmium-188
  227. Osmium-189
  228. Osmium-190
  229. Osmium-192
  230. Iridium-191
  231. Iridium-193
  232. Platinum-192
  233. Platinum-194
  234. Platinum-195
  235. Platinum-196
  236. Platinum-198
  237. Gold-197
  238. Mercury-196
  239. Mercury-198
  240. Mercury-199
  241. Mercury-200
  242. Mercury-201
  243. Mercury-202
  244. Mercury-204
  245. Thallium-203
  246. Thallium-205
  247. Lead-206
  248. Lead-207
  249. Lead-208

[edit] See also

[edit] References

  1. ^ WWW Table of Radioactive Isotopes.