釤的同位素

釤的同位素

釤(原子量:150.36(2))在自然界中存在5种稳定同位素(144Sm、149Sm、150Sm、152Sm、154Sm)和2种长寿命放射性同位素(半衰期1.06×1011年的147Sm和半衰期7×1015年的148Sm),其中152Sm的丰度最高,达26.74%。146Sm的半衰期也很长,但不足以在今天大量存在,现为绝种核素(英语:extinct radionuclide)。它可用于太阳系的测年。[3][4]2012年一篇把146Sm的半衰期从10.3(5)×107年更新到6.8(7)×107年的论文已于2023年撤稿。[4][5]它是不确定是不是原生核素(英语:primordial nuclide)的核素中半衰期最长的。

主要的釤同位素

同位素

衰變

丰度

半衰期 (t1/2)

方式

能量(MeV)

產物

144Sm

3.08%

穩定,帶82粒中子

146Sm

痕量

9.20×107 年[1]

α

2.529

142Nd

147Sm

15.00%

1.06×1011 年

α

2.311

143Nd

148Sm

11.25%

7×1015 年

α

1.987

144Nd

149Sm

13.82%

穩定,帶87粒中子

150Sm

7.37%

穩定,帶88粒中子

151Sm

人造

94.6 年

β−

0.077

151Eu

152Sm

26.74%

穩定,帶90粒中子

153Sm

人造

46.2846 小時

β−

0.808

153Eu

154Sm

22.74%

穩定,帶92粒中子

標準原子質量(英语:Standard atomic weight) (Ar, 標準)150.36(2)[2]

←Pm(61)

Eu(63)→

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除了以上8种同位素以外,钐最长寿的放射性同位素是半衰期94.6年的151Sm[6]以及半衰期340天的145Sm。剩下的同位素原子量介于129至168,半衰期都短于两天。

圖表

编辑

符號

Z

N

同位素質量(u)[n 1][n 2]

半衰期[n 1][n 2][n 3]

衰變方式[7]

衰變產物[n 4][n 5]

原子核自旋[n 1]

相對豐度(莫耳分率)[n 2]

相對豐度的變化量(莫耳分率)

激發能量[n 1][n 2]

129Sm

62

67

128.95464(54)#

550(100) ms

5/2+#

130Sm

62

68

129.94892(43)#

1# s

β+

130Pm

0+

131Sm

62

69

130.94611(32)#

1.2(2) s

β+

131Pm

5/2+#

β+, p (不常見)

130Nd

132Sm

62

70

131.94069(32)#

4.0(3) s

β+

132Pm

0+

β+, p

131Nd

133Sm

62

71

132.93867(21)#

2.90(17) s

β+

133Pm

(5/2+)

β+, p

132Nd

134Sm

62

72

133.93397(21)#

10(1) s

β+

134Pm

0+

135Sm

62

73

134.93252(17)

10.3(5) s

β+ (99.98%)

135Pm

(7/2+)

β+, p (.02%)

134Nd

135mSm

0(300)# keV

2.4(9) s

β+

135Pm

(3/2+,5/2+)

136Sm

62

74

135.928276(13)

47(2) s

β+

136Pm

0+

136mSm

2264.7(11) keV

15(1) µs

(8-)

137Sm

62

75

136.92697(5)

45(1) s

β+

137Pm

(9/2-)

137mSm

180(50)# keV

20# s

β+

137Pm

1/2+#

138Sm

62

76

137.923244(13)

3.1(2) min

β+

138Pm

0+

139Sm

62

77

138.922297(12)

2.57(10) min

β+

139Pm

1/2+

139mSm

457.40(22) keV

10.7(6) s

IT (93.7%)

139Sm

11/2-

β+ (6.3%)

139Pm

140Sm

62

78

139.918995(13)

14.82(12) min

β+

140Pm

0+

141Sm

62

79

140.918476(9)

10.2(2) min

β+

141Pm

1/2+

141mSm

176.0(3) keV

22.6(2) min

β+ (99.69%)

141Pm

11/2-

IT (.31%)

141Sm

142Sm

62

80

141.915198(6)

72.49(5) min

β+

142Pm

0+

143Sm

62

81

142.914628(4)

8.75(8) min

β+

143Pm

3/2+

143m1Sm

753.99(16) keV

66(2) s

IT (99.76%)

143Sm

11/2-

β+ (.24%)

143Pm

143m2Sm

2793.8(13) keV

30(3) ms

23/2(-)

144Sm

62

82

143.911999(3)

觀測上穩定[n 6]

0+

0.0307(7)

144mSm

2323.60(8) keV

880(25) ns

6+

145Sm

62

83

144.913410(3)

340(3) d

ε

145Pm

7/2-

145mSm

8786.2(7) keV

990(170) ns[0.96(+19-15) µs]

(49/2+)

146Sm[n 7]

62

84

145.913041(4)

9.20(26)×107 a[1]

α

142Nd

0+

痕量

147Sm[n 7][n 8][n 9]

62

85

146.9148979(26)

1.06(2)×1011 a

α

143Nd

7/2-

0.1499(18)

148Sm[n 7]

62

86

147.9148227(26)

7(3)×1015 a

α

144Nd

0+

0.1124(10)

149Sm[n 8][n 10]

62

87

148.9171847(26)

觀測上穩定[n 11]

7/2-

0.1382(7)

150Sm

62

88

149.9172755(26)

觀測上穩定[n 12]

0+

0.0738(1)

151Sm[n 8][n 10]

62

89

150.9199324(26)

88.8(24) a

β−

151Eu

5/2-

151mSm

261.13(4) keV

1.4(1) µs

(11/2)-

152Sm[n 8]

62

90

151.9197324(27)

觀測上穩定[n 13]

0+

0.2675(16)

153Sm[n 8]

62

91

152.9220974(27)

46.284(4) h

β−

153Eu

3/2+

153mSm

98.37(10) keV

10.6(3) ms

IT

153Sm

11/2-

154Sm[n 8]

62

92

153.9222093(27)

觀測上穩定[n 14]

0+

0.2275(29)

155Sm

62

93

154.9246402(28)

22.3(2) min

β−

155Eu

3/2-

156Sm

62

94

155.925528(10)

9.4(2) h

β−

156Eu

0+

156mSm

1397.55(9) keV

185(7) ns

5-

157Sm

62

95

156.92836(5)

8.03(7) min

β−

157Eu

(3/2-)

158Sm

62

96

157.92999(8)

5.30(3) min

β−

158Eu

0+

159Sm

62

97

158.93321(11)

11.37(15) s

β−

159Eu

5/2-

160Sm

62

98

159.93514(21)#

9.6(3) s

β−

160Eu

0+

161Sm

62

99

160.93883(32)#

4.8(8) s

β−

161Eu

7/2+#

162Sm

62

100

161.94122(54)#

2.4(5) s

β−

162Eu

0+

163Sm

62

101

162.94536(75)#

1# s

β−

163Eu

1/2-#

164Sm

62

102

163.94828(86)#

500# ms

β−

164Eu

0+

165Sm

62

103

164.95298(97)#

200# ms

β−

165Eu

5/2-#

^ 1.0 1.1 1.2 1.3 畫上#號的數據代表沒有經過實驗的証明,僅為理論推測。

^ 2.0 2.1 2.2 2.3 用括號括起來的數據代表不確定性。

^ 半衰期超过5亿年的同位素以粗體表示。

^ 穩定的衰變產物以粗體表示。

^ 半衰期超过5亿年的衰变产物以粗斜体表示。

^ Believed to undergo β+β+ decay to 144Nd

^ 7.0 7.1 7.2 Primordial radioisotope

^ 8.0 8.1 8.2 8.3 8.4 8.5 Fission product

^ Used in Samarium-neodymium dating

^ 10.0 10.1 Neutron poison in reactors

^ Believed to undergo α decay to 145Nd with a half-life over 2×1015 years

^ Believed to undergo α decay to 146Nd

^ Believed to undergo α decay to 148Nd

^ Believed to undergo β−β− decay to 154Gd with a half-life over 2.3×1018 years

同位素列表

钷的同位素

釤的同位素

銪的同位素

参考文獻

编辑

^ 1.0 1.1 Chiera, Nadine M.; Sprung, Peter; Amelin, Yuri; Dressler, Rugard; Schumann, Dorothea; Talip, Zeynep. The 146Sm half-life re-measured: consolidating the chronometer for events in the early Solar System. Scientific Reports. 2024-08-01, 14 (1). doi:10.1038/s41598-024-64104-6.

^ 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.

^ Samir Maji; et al. Separation of samarium and neodymium: a prerequisite for getting signals from nuclear synthesis. Analyst. 2006, 131 (12): 1332–1334. Bibcode:2006Ana...131.1332M. PMID 17124541. doi:10.1039/b608157f.

^ 4.0 4.1 Kinoshita, N.; Paul, M.; Kashiv, Y.; Collon, P.; Deibel, C. M.; DiGiovine, B.; Greene, J. P.; Henderson, D. J.; Jiang, C. L.; Marley, S. T.; Nakanishi, T.; Pardo, R. C.; Rehm, K. E.; Robertson, D.; Scott, R.; Schmitt, C.; Tang, X. D.; Vondrasek, R.; Yokoyama, A. A Shorter 146Sm Half-Life Measured and Implications for 146Sm-142Nd Chronology in the Solar System. Science. 30 March 2012, 335 (6076): 1614–1617. Bibcode:2012Sci...335.1614K. ISSN 0036-8075. PMID 22461609. S2CID 206538240. arXiv:1109.4805 . doi:10.1126/science.1215510 (英语). (已撤稿,见doi:10.1126/science.adh7739)

^ Kinoshita, N.; Paul, M.; Kashiv, Y.; Collon, P.; Deibel, C. M.; DiGiovine, B.; Greene, J. P.; Jiang, C. L.; Marley, S. T.; Pardo, R. C.; Rehm, K. E.; Robertson, D.; Scott, R.; Schmitt, C.; Tang, X. D.; Vondrasek, R.; Yokoyama, A. Retraction. Science. 30 March 2023, 379 (6639): 1307. Bibcode:2023Sci...379.1307K. PMID 36996231. S2CID 236990856. doi:10.1126/science.adh7739 . Joelving, Frederik. One small error for a physicist, one giant blunder for planetary science. Retraction Watch. 30 March 2023 [30 March 2023]. (原始内容存档于2023-06-28).

^ He, M.; Shen, H.; Shi, G.; Yin, X.; Tian, W.; Jiang, S. Half-life of 151Sm remeasured. Physical Review C. 2009, 80 (6): 064305. Bibcode:2009PhRvC..80f4305H. doi:10.1103/PhysRevC.80.064305.

^ 存档副本. [2015-09-20]. (原始内容存档于2017-02-19).

Isotope masses from Ame2003 Atomic Mass Evaluation by G. Audi, A.H. Wapstra, C. Thibault, J. Blachot and O. Bersillon in Nuclear Physics A729 (2003).

Isotopic compositions and standard atomic masses from Atomic weights of the elements. Review 2000 (IUPAC Technical Report) (页面存档备份,存于互联网档案馆). Pure Appl. Chem. Vol. 75, No. 6, pp. 683-800, (2003) and Atomic Weights Revised (2005) (页面存档备份,存于互联网档案馆).

Half-life, spin, and isomer data selected from these sources. Editing notes on this article's talk page.

Audi, Bersillon, Blachot, Wapstra. The Nubase2003 evaluation of nuclear and decay properties (页面存档备份,存于互联网档案馆), Nuc. Phys. A 729, pp. 3-128 (2003).

National Nuclear Data Center, Brookhaven National Laboratory. Information extracted from the NuDat 2.1 database (页面存档备份,存于互联网档案馆) (retrieved Sept. 2005).

David R. Lide (ed.), Norman E. Holden in CRC Handbook of Chemistry and Physics, 85th Edition, online version. CRC Press. Boca Raton, Florida (2005). Section 11, Table of the Isotopes.

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