Stable isotope
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Stable_isotope"
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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.

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Contents

Research areas

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

Unibidium or something close to it has been discovered inside thorium . The exact element has yet to be determined, but the atomic_number is around 122 and the atomic_mass is around 292.



Stable isotope fractionation

There are three types of isotope fractionation:

List of stable isotopes

There are 81 known elements which have at least 1 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. Calcium-46
  46. Scandium-45
  47. Titanium-46
  48. Titanium-47
  49. Titanium-48
  50. Titanium-49
  51. Titanium-50
  52. Vanadium-51
  53. Chromium-50
  54. Chromium-52
  55. Chromium-53
  56. Chromium-54
  57. Manganese-55
  58. Iron-54
  59. Iron-56
  60. Iron-57
  61. Iron-58
  62. Cobalt-59
  63. Nickel-58
  64. Nickel-60
  65. Nickel-61
  66. Nickel-62
  67. Nickel-64
  68. Copper-63
  69. Copper-65
  70. Zinc-64
  71. Zinc-66
  72. Zinc-67
  73. Zinc-68
  74. Zinc-70
  75. Gallium-69
  76. Gallium-71
  77. Germanium-70
  78. Germanium-72
  79. Germanium-73
  80. Germanium-74
  81. Arsenic-75
  82. Selenium-74
  83. Selenium-76
  84. Selenium-77
  85. Selenium-78
  86. Selenium-80
  87. Bromine-79
  88. Bromine-81
  89. Krypton-78
  90. Krypton-80
  91. Krypton-82
  92. Krypton-83
  93. Krypton-84
  94. Krypton-86
  95. Rubidium-85
  96. Strontium-84
  97. Strontium-86
  98. Strontium-87
  99. Strontium-88
  100. Yttrium-89
  101. Zirconium-90
  102. Zirconium-91
  103. Zirconium-92
  104. Zirconium-94
  105. Niobium-93
  106. Molybdenum-92
  107. Molybdenum-94
  108. Molybdenum-95
  109. Molybdenum-96
  110. Molybdenum-97
  111. Molybdenum-98
    Technetium - No stable isotopes
  112. Ruthenium-96
  113. Ruthenium-98
  114. Ruthenium-99
  115. Ruthenium-100
  116. Ruthenium-101
  117. Ruthenium-102
  118. Ruthenium-104
  119. Rhodium-103
  120. Palladium-102
  121. Palladium-104
  122. Palladium-105
  123. Palladium-106
  124. Palladium-108
  125. Palladium-110
  126. Silver-107
  127. Silver-109
  128. Cadmium-106
  129. Cadmium-108
  130. Cadmium-110
  131. Cadmium-111
  132. Cadmium-112
  133. Cadmium-114
  134. Indium-113
  135. Tin-112
  136. Tin-114
  137. Tin-115
  138. Tin-116
  139. Tin-117
  140. Tin-118
  141. Tin-119
  142. Tin-120
  143. Tin-122
  144. Tin-124
  145. Antimony-121
  146. Antimony-123
  147. Tellurium-122
  148. Tellurium-123
  149. Tellurium-124
  150. Tellurium-126
  151. Iodine-127
  152. Xenon-124
  153. Xenon-126
  154. Xenon-128
  155. Xenon-129
  156. Xenon-130
  157. Xenon-131
  158. Xenon-132
  159. Xenon-134
  160. Xenon-136
  161. Caesium-133
  162. Barium-132
  163. Barium-134
  164. Barium-135
  165. Barium-136
  166. Barium-137
  167. Barium-138
  168. Lanthanum-139
  169. Cerium-136
  170. Cerium-138
  171. Cerium-140
  172. Cerium-142
  173. Praseodymium-141
  174. Neodymium-142
  175. Neodymium-143
  176. Neodymium-145
  177. Neodymium-146
  178. Neodymium-148
    Promethium - No stable isotopes
  179. Samarium-144
  180. Samarium-150
  181. Samarium-152
  182. Samarium-154
  183. Europium-153
  184. Gadolinium-154
  185. Gadolinium-155
  186. Gadolinium-156
  187. Gadolinium-157
  188. Gadolinium-158
  189. Gadolinium-160
  190. Terbium-159
  191. Dysprosium-156
  192. Dysprosium-158
  193. Dysprosium-160
  194. Dysprosium-161
  195. Dysprosium-162
  196. Dysprosium-163
  197. Dysprosium-164
  198. Holmium-165
  199. Erbium-162
  200. Erbium-164
  201. Erbium-166
  202. Erbium-167
  203. Erbium-168
  204. Erbium-170
  205. Thulium-169
  206. Ytterbium-168
  207. Ytterbium-170
  208. Ytterbium-171
  209. Ytterbium-172
  210. Ytterbium-173
  211. Ytterbium-174
  212. Ytterbium-176
  213. Lutetium-175
  214. Hafnium-176
  215. Hafnium-177
  216. Hafnium-178
  217. Hafnium-179
  218. Hafnium-180
  219. Tantalum-180m
  220. Tantalum-181
  221. Tungsten-182
  222. Tungsten-183
  223. Tungsten-184
  224. Tungsten-186
  225. Rhenium-185
  226. Osmium-187
  227. Osmium-188
  228. Osmium-189
  229. Osmium-190
  230. Osmium-192
  231. Iridium-191
  232. Iridium-193
  233. Platinum-192
  234. Platinum-194
  235. Platinum-195
  236. Platinum-196
  237. Platinum-198
  238. Gold-197
  239. Mercury-196
  240. Mercury-198
  241. Mercury-199
  242. Mercury-200
  243. Mercury-201
  244. Mercury-202
  245. Mercury-204
  246. Thallium-203
  247. Thallium-205
  248. Lead-206
  249. Lead-207
  250. Lead-208
  251. Unbibium-292 ??? Uncertain in both atomic number (element) and weight.

See also

References

  1. ^ WWW Table of Radioactive Isotopes.
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