碲的同位素

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主要的碲同位素
同位素 衰變
丰度 半衰期 (t1/2) 方式 能量
MeV
產物

Template:Infobox tellurium isotopes

標準原子質量英语Standard atomic weight (Ar, 標準)
←Sb51 I53

原子量:127.60(3))有39种同位素与17种同核异构体原子量介于104至142。其中,有八种同位素(120Te、122Te、123Te、124Te、125Te、126Te、128Te、130Te)存在于自然界。128Te和130Te有放射性,但半衰期都极长,分别为2.25×1024年和7.91×1020年。[2]碲最长寿的人造同位素则是半衰期19.31天的121Te,但诸如121mTe(半衰期164.7天)的同核异构体有更长的半衰期。

放射性同位素128Te和130Te是碲最常见的两种同位素。碲与一样都是放射性同位素的丰度比稳定同位素的丰度大的例子。

有团队报告称已发现123Te的电子捕获,但他们之后的测量结果否认了这点。[3]123Te的半衰期至少为9.2×1016年。[3]

圖表[编辑]

Template:Isotopes table |- | 104Te[4] | style="text-align:right" | 52 | style="text-align:right" | 52 | | <18 ns | α | 100Sn | 0+ | | |- | 105Te | style="text-align:right" | 52 | style="text-align:right" | 53 | 104.94364(54)# | 620(70) ns | α | 101Sn | 5/2+# | | |- | 106Te | style="text-align:right" | 52 | style="text-align:right" | 54 | 105.93750(14) | 70(20) µs
[70(+20-10) µs] | α | 102Sn | 0+ | | |- | rowspan=2|107Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 55 | rowspan=2|106.93501(32)# | rowspan=2|3.1(1) ms | α (70%) | 103Sn | rowspan=2|5/2+# | rowspan=2| | rowspan=2| |- | β+ (30%) | 107Sb |- | rowspan=4|108Te | rowspan=4 style="text-align:right" | 52 | rowspan=4 style="text-align:right" | 56 | rowspan=4|107.92944(11) | rowspan=4|2.1(1) s | β+ (51%) | 108Sb | rowspan=4|0+ | rowspan=4| | rowspan=4| |- | α (49%) | 104Sn |- | β+, p (2.4%) | 107Sn |- | β+, α (.065%) | 104In |- | rowspan=4|109Te | rowspan=4 style="text-align:right" | 52 | rowspan=4 style="text-align:right" | 57 | rowspan=4|108.92742(7) | rowspan=4|4.6(3) s | β+ (86.99%) | 109Sb | rowspan=4|(5/2+) | rowspan=4| | rowspan=4| |- | β+, p (9.4%) | 108Sn |- | α (7.9%) | 105Sn |- | β+, α (.005%) | 105In |- | rowspan=2|110Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 58 | rowspan=2|109.92241(6) | rowspan=2|18.6(8) s | β+ (99.99%) | 110Sb | rowspan=2|0+ | rowspan=2| | rowspan=2| |- | β+, p (.003%) | 109Sn |- | rowspan=2|111Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 59 | rowspan=2|110.92111(8) | rowspan=2|19.3(4) s | β+ | 111Sb | rowspan=2|(5/2)+# | rowspan=2| | rowspan=2| |- | β+, p (不常見) | 110Sn |- | 112Te | style="text-align:right" | 52 | style="text-align:right" | 60 | 111.91701(18) | 2.0(2) min | β+ | 112Sb | 0+ | | |- | 113Te | style="text-align:right" | 52 | style="text-align:right" | 61 | 112.91589(3) | 1.7(2) min | β+ | 113Sb | (7/2+) | | |- | 114Te | style="text-align:right" | 52 | style="text-align:right" | 62 | 113.91209(3) | 15.2(7) min | β+ | 114Sb | 0+ | | |- | 115Te | style="text-align:right" | 52 | style="text-align:right" | 63 | 114.91190(3) | 5.8(2) min | β+ | 115Sb | 7/2+ | | |- | rowspan=2 style="text-indent:1em" | 115m1Te | rowspan=2 colspan="3" style="text-indent:2em" | 10(7) keV | rowspan=2|6.7(4) min | β+ | 115Sb | rowspan=2|(1/2)+ | rowspan=2| | rowspan=2| |- | IT | 115Te |- | style="text-indent:1em" | 115m2Te | colspan="3" style="text-indent:2em" | 280.05(20) keV | 7.5(2) µs | | | 11/2- | | |- | 116Te | style="text-align:right" | 52 | style="text-align:right" | 64 | 115.90846(3) | 2.49(4) h | β+ | 116Sb | 0+ | | |- | 117Te | style="text-align:right" | 52 | style="text-align:right" | 65 | 116.908645(14) | 62(2) min | β+ | 117Sb | 1/2+ | | |- | style="text-indent:1em" | 117mTe | colspan="3" style="text-indent:2em" | 296.1(5) keV | 103(3) ms | IT | 117Te | (11/2-) | | |- | 118Te | style="text-align:right" | 52 | style="text-align:right" | 66 | 117.905828(16) | 6.00(2) d | ε | 118Sb | 0+ | | |- | 119Te | style="text-align:right" | 52 | style="text-align:right" | 67 | 118.906404(9) | 16.05(5) h | β+ | 119Sb | 1/2+ | | |- | rowspan=2 style="text-indent:1em" | 119mTe | rowspan=2 colspan="3" style="text-indent:2em" | 260.96(5) keV | rowspan=2|4.70(4) d | β+ (99.99%) | 119Sb | rowspan=2|11/2- | rowspan=2| | rowspan=2| |- | IT (.008%) | 119Te |- | 120Te | style="text-align:right" | 52 | style="text-align:right" | 68 | 119.90402(1) | colspan=3 align=center|觀測上穩定[n 1] | 0+ | 9(1)×10−4 | |- | 121Te | style="text-align:right" | 52 | style="text-align:right" | 69 | 120.904936(28) | 19.16(5) d | β+ | 121Sb | 1/2+ | | |- | rowspan=2 style="text-indent:1em" | 121mTe | rowspan=2 colspan="3" style="text-indent:2em" | 293.991(22) keV | rowspan=2|154(7) d | IT (88.6%) | 121Te | rowspan=2|11/2- | rowspan=2| | rowspan=2| |- | β+ (11.4%) | 121Sb |- | 122Te | style="text-align:right" | 52 | style="text-align:right" | 70 | 121.9030439(16) | colspan=3 align=center|稳定 | 0+ | 0.0255(12) | |- | 123Te | style="text-align:right" | 52 | style="text-align:right" | 71 | 122.9042700(16) | colspan=3 align=center|觀測上穩定[n 2] | 1/2+ | 0.0089(3) | |- | style="text-indent:1em" | 123mTe | colspan="3" style="text-indent:2em" | 247.47(4) keV | 119.2(1) d | IT | 123Te | 11/2- | | |- | 124Te | style="text-align:right" | 52 | style="text-align:right" | 72 | 123.9028179(16) | colspan=3 align=center|稳定 | 0+ | 0.0474(14) | |- | 125Te[n 3] | style="text-align:right" | 52 | style="text-align:right" | 73 | 124.9044307(16) | colspan=3 align=center|稳定 | 1/2+ | 0.0707(15) | |- | style="text-indent:1em" | 125mTe | colspan="3" style="text-indent:2em" | 144.772(9) keV | 57.40(15) d | IT | 125Te | 11/2- | | |- | 126Te | style="text-align:right" | 52 | style="text-align:right" | 74 | 125.9033117(16) | colspan=3 align=center|稳定 | 0+ | 0.1884(25) | |- | 127Te[n 3] | style="text-align:right" | 52 | style="text-align:right" | 75 | 126.9052263(16) | 9.35(7) h | β | 127I | 3/2+ | | |- | rowspan=2 style="text-indent:1em" | 127mTe | rowspan=2 colspan="3" style="text-indent:2em" | 88.26(8) keV | rowspan=2|109(2) d | IT (97.6%) | 127Te | rowspan=2|11/2- | rowspan=2| | rowspan=2| |- | β (2.4%) | 127I |- | 128Te[n 3][n 4] | style="text-align:right" | 52 | style="text-align:right" | 76 | 127.9044631(19) | 2.2(3)×1024 a[n 5] | ββ | 128Xe | 0+ | 0.3174(8) | |- | style="text-indent:1em" | 128mTe | colspan="3" style="text-indent:2em" | 2790.7(4) keV | 370(30) ns | | | 10+ | | |- | 129Te[n 3] | style="text-align:right" | 52 | style="text-align:right" | 77 | 128.9065982(19) | 69.6(3) min | β | 129I | 3/2+ | | |- | style="text-indent:1em" | 129mTe | colspan="3" style="text-indent:2em" | 105.50(5) keV | 33.6(1) d | | | 11/2- | | |- | 130Te[n 3][n 4] | style="text-align:right" | 52 | style="text-align:right" | 78 | 129.9062244(21) | 790(100)×1018 a | ββ | 130Xe | 0+ | 0.3408(62) | |- | style="text-indent:1em" | 130m1Te | colspan="3" style="text-indent:2em" | 2146.41(4) keV | 115(8) ns | | | (7)- | | |- | style="text-indent:1em" | 130m2Te | colspan="3" style="text-indent:2em" | 2661(7) keV | 1.90(8) µs | | | (10+) | | |- | style="text-indent:1em" | 130m3Te | colspan="3" style="text-indent:2em" | 4375.4(18) keV | 261(33) ns | | | | | |- | 131Te[n 3] | style="text-align:right" | 52 | style="text-align:right" | 79 | 130.9085239(21) | 25.0(1) min | β | 131I | 3/2+ | | |- | rowspan=2 style="text-indent:1em" | 131mTe | rowspan=2 colspan="3" style="text-indent:2em" | 182.250(20) keV | rowspan=2|30(2) h | β (77.8%) | 131I | rowspan=2|11/2- | rowspan=2| | rowspan=2| |- | IT (22.2%) | 131Te |- | 132Te[n 3] | style="text-align:right" | 52 | style="text-align:right" | 80 | 131.908553(7) | 3.204(13) d | β | 132I | 0+ | | |- | 133Te | style="text-align:right" | 52 | style="text-align:right" | 81 | 132.910955(26) | 12.5(3) min | β | 133I | (3/2+) | | |- | rowspan=2 style="text-indent:1em" | 133mTe | rowspan=2 colspan="3" style="text-indent:2em" | 334.26(4) keV | rowspan=2|55.4(4) min | β (82.5%) | 133I | rowspan=2|(11/2-) | rowspan=2| | rowspan=2| |- | IT (17.5%) | 133Te |- | 134Te | style="text-align:right" | 52 | style="text-align:right" | 82 | 133.911369(11) | 41.8(8) min | β | 134I | 0+ | | |- | style="text-indent:1em" | 134mTe | colspan="3" style="text-indent:2em" | 1691.34(16) keV | 164.1(9) ns | | | 6+ | | |- | 135Te[n 6] | style="text-align:right" | 52 | style="text-align:right" | 83 | 134.91645(10) | 19.0(2) s | β | 135I | (7/2-) | | |- | style="text-indent:1em" | 135mTe | colspan="3" style="text-indent:2em" | 1554.88(17) keV | 510(20) ns | | | (19/2-) | | |- | rowspan=2|136Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 84 | rowspan=2|135.92010(5) | rowspan=2|17.63(8) s | β (98.7%) | 136I | rowspan=2|0+ | rowspan=2| | rowspan=2| |- | β, n (1.3%) | 135I |- | rowspan=2|137Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 85 | rowspan=2|136.92532(13) | rowspan=2|2.49(5) s | β (97.01%) | 137I | rowspan=2|3/2-# | rowspan=2| | rowspan=2| |- | β, n (2.99%) | 136I |- | rowspan=2|138Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 86 | rowspan=2|137.92922(22)# | rowspan=2|1.4(4) s | β (93.7%) | 138I | rowspan=2|0+ | rowspan=2| | rowspan=2| |- | β, n (6.3%) | 137I |- | rowspan=2|139Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 87 | rowspan=2|138.93473(43)# | rowspan=2|500 ms
[>300 ns]# | β | 139I | rowspan=2|5/2-# | rowspan=2| | rowspan=2| |- | β, n | 138I |- | rowspan=2|140Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 88 | rowspan=2|139.93885(32)# | rowspan=2|300 ms
[>300 ns]# | β | 140I | rowspan=2|0+ | rowspan=2| | rowspan=2| |- | β, n | 139I |- | rowspan=2|141Te | rowspan=2 style="text-align:right" | 52 | rowspan=2 style="text-align:right" | 89 | rowspan=2|140.94465(43)# | rowspan=2|100 ms
[>300 ns]# | β | 141I | rowspan=2|5/2-# | rowspan=2| | rowspan=2| |- | β, n | 140I |- | 142Te | style="text-align:right" | 52 | style="text-align:right" | 90 | 141.94908(64)# | 50 ms
[>300 ns]# | β | 142I | 0+ | | |}

  1. Believed to undergo β+β+ decay to 120Sn with a half-life over 2.2×1016 years
  2. Believed to undergo β+ decay to 123Sb with a half-life over 9.2×1016 years
  3. 3.0 3.1 3.2 3.3 3.4 3.5 3.6 Fission product
  4. 4.0 4.1 Primordial radionuclide
  5. Longest measured half-life of any nuclide
  6. Very short-lived fission product, responsible for the iodine pit as precursor of 135Xe via 135I
同位素列表
銻的同位素 碲的同位素 碘的同位素

参考文獻[编辑]

  1. Meija, Juris; et al. Atomic weights of the elements 2013 (IUPAC Technical Report). Pure and Applied Chemistry. 2016, 88 (3): 265–91. doi:10.1515/pac-2015-0305. 
  2. Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. The NUBASE2020 evaluation of nuclear properties (PDF). Chinese Physics C. 2021, 45 (3): 030001. doi:10.1088/1674-1137/abddae (English). 
  3. 3.0 3.1 A. Alessandrello; et al. New Limits on Naturally Occurring Electron Capture of 123Te. Physical Review C. January 2003, 67 (1): 014323. Bibcode:2003PhRvC..67a4323A. S2CID 119523039. arXiv:hep-ex/0211015可免费查阅. doi:10.1103/PhysRevC.67.014323. 
  4. Auranen, K.; et al. Superallowed α decay to doubly magic 100Sn (PDF). Physical Review Letters. 2018, 121 (18): 182501 [2021-05-22]. Bibcode:2018PhRvL.121r2501A. PMID 30444390. doi:10.1103/PhysRevLett.121.182501可免费查阅. (原始内容存档 (PDF)于2021-11-03).