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Isotopes of rubidium
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Isotopes of rubidium
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Isotopes of rubidium

Isotopes of rubidium (37Rb)
Main isotopes[1] Decay
Isotope abun­dance half-life (t1/2) mode pro­duct
82Rb synth 1.2575 m β+ 82Kr
83Rb synth 86.2 d ε 83Kr
84Rb synth 32.82 d β+ 84Kr
β 84Sr
85Rb 72.2% stable
86Rb synth 18.645 d β 86Sr
ε 86Kr
87Rb 27.8% 4.97×1010 y β 87Sr
Standard atomic weight Ar°(Rb)

Rubidium (37Rb) has 35 known isotopes, from 72Rb to 106Rb, with naturally occurring rubidium composed of two: stable 85Rb (72.2%) and radioactive 87Rb (27.8%). The primordial radionuclide 87Rb has a half-life of 4.97×1010 years, beta decaying to stable 87Sr. It is, as the element is, widespread on Earth as rubidium readily substitutes for potassium in all minerals. The decay of 87Rb has been used extensively in dating rocks; see rubidium–strontium dating for a more detailed discussion.

Other than 87Rb, the longest-lived radioisotopes are 83Rb with a half-life of 86.2 days, 84Rb with a half-life of 32.82 days, and 86Rb with a half-life of 18.645 days. All other radioisotopes have half-lives less than a day, most less than 20 minutes. Of the isomeric states the most stable is 82mRb at 6.472 hours.

The ground state of 82Rb has a much shorter half-life of 1.2575 minutes. It is used medically in some cardiac positron emission tomography scans to assess myocardial perfusion. It is synthesized through the longer-lived 82Sr, made in a cyclotron, though a generator. It may be administered as the chloride.

List of isotopes

[edit]


Nuclide
[n 1]
Z N Isotopic mass (Da)[4]
[n 2][n 3]
Half-life[1]
[n 4][n 5]
Decay
mode
[1]
[n 6]
Daughter
isotope

[n 7][n 8]
Spin and
parity[1]
[n 9][n 5]
Natural abundance (mole fraction)
Excitation energy[n 5] Normal proportion[1] Range of variation
72Rb 37 35 71.95885(54)# 103(22) ns p 71Kr 1+#
73Rb 37 36 72.950605(44) <81 ns p 72Kr 3/2−#
74Rb 37 37 73.9442659(32) 64.78(3) ms β+ 74Kr 0+
75Rb 37 38 74.9385732(13) 19.0(12) s β+ 75Kr 3/2−
76Rb 37 39 75.9350730(10) 36.5(6) s β+ 76Kr 1−
β+, α (3.8×10−7%) 72Se
76mRb 316.93(8) keV 3.050(7) μs IT 76Rb (4+)
77Rb 37 40 76.9304016(14) 3.78(4) min β+ 77Kr 3/2−
78Rb 37 41 77.9281419(35) 17.66(3) min β+ 78Kr 0+
78m1Rb 46.84(14) keV 910(40) ns IT 78Rb (1−)
78m2Rb 111.19(22) keV 5.74(3) min β+ (91%) 78Kr 4−
IT (9%) 78Rb
79Rb 37 42 78.9239901(21) 22.9(5) min β+ 79Kr 5/2+
80Rb 37 43 79.9225164(20) 33.4(7) s β+ 80Kr 1+
80mRb 493.9(5) keV 1.63(4) μs IT 80Rb (6+)
81Rb 37 44 80.9189939(53) 4.572(4) h β+ 81Kr 3/2−
81mRb 86.31(7) keV 30.5(3) min IT (97.6%) 81Rb 9/2+
β+ (2.4%) 81Kr
82Rb 37 45 81.9182090(32) 1.2575(2) min β+ 82Kr 1+
82mRb 69.0(15) keV 6.472(6) h β+ 82Kr 5−
83Rb 37 46 82.9151142(25) 86.2(1) d EC 83Kr 5/2−
83mRb 42.0780(20) keV 7.8(7) ms IT 83Rb 9/2+
84Rb 37 47 83.9143752(24) 32.82(7) d β+ (96.1%) 84Kr 2−
β (3.9%) 84Sr
84mRb 463.59(8) keV 20.26(4) min IT 84Rb 6−
85Rb[n 10] 37 48 84.9117897360(54) Stable 5/2− 0.7217(2)
85mRb 514.0065(22) keV 1.015(1) μs IT 85Rb 9/2+
86Rb 37 49 85.91116744(21) 18.645(8) d β (99.9948%) 86Sr 2−
EC (0.0052%) 86Kr
86mRb 556.05(18) keV 1.017(3) min IT 86Rb 6−
87Rb[n 10][n 11][n 12] 37 50 86.909180529(6) 4.97(3)×1010 y β 87Sr 3/2− 0.2783(2)
88Rb 37 51 87.91131559(17) 17.78(3) min β 88Sr 2−
88mRb 1373.8(3) keV 123(13) ns IT 88Rb (7+)
89Rb 37 52 88.9122781(58) 15.32(10) min β 89Sr 3/2−
90Rb 37 53 89.9147976(69) 158(5) s β 90Sr 0−
90mRb 106.90(3) keV 258(4) s β (97.4%) 90Sr 3−
IT (2.6%) 90 Rb
91Rb 37 54 90.9165373(84) 58.2(3) s β 91Sr 3/2−
92Rb 37 55 91.9197285(66) 4.48(3) s β (99.99%) 92Sr 0−
β, n (0.0107%) 91Sr
93Rb 37 56 92.9220393(84) 5.84(2) s β (98.61%) 93Sr 5/2−
β, n (1.39%) 92Sr
93mRb 4423.1(15) keV 111(11) ns IT 93Rb (27/2−)
94Rb 37 57 93.9263948(22) 2.702(5) s β (89.7%) 94Sr 3−
β, n (10.3%) 93Sr
94m1Rb 104.2(2) keV 130(15) ns IT 94Rb (0−)
94m2Rb 2074.9(14) keV 107(16) ns IT 94Rb (10−)
95Rb 37 58 94.929264(22) 377.7(8) ms β (91.3%) 95Sr 5/2−
β, n (8.7%) 94Sr
95mRb 835.0(6) keV <500 ns IT 95Rb 9/2+#
96Rb 37 59 95.9341334(36) 201.5(9) ms β (86.3%) 96Sr 2−
β, n (13.7%) 95Sr
96m1Rb[n 13] 0(200)# keV 200# ms
[>1 ms]
1(+#)
96m2Rb 1134.6(11) keV 1.80(4) μs IT 96Rb (10−)
97Rb 37 60 96.9371771(21) 169.1(6) ms β (74.5%) 97Sr 3/2+
β, n (25.5%) 96Sr
97mRb 76.6(2) keV 5.7(6) μs IT 97Rb (1/2,3/2)−
98Rb 37 61 97.941632(17) 115(6) ms β(85.65%) 98Sr (0−)
β, n (14.3%) 97Sr
β, 2n (0.054%) 96Sr
98m1Rb 73(26) keV 96(3) ms β 98Sr (3+)
98m2Rb 178.5(4) keV 358(7) ns IT 98Rb (2−)
99Rb 37 62 98.9451192(43) 54(4) ms β (82.7%) 99Sr (3/2+)
β, n (17.3%) 98Sr
100Rb 37 63 99.950332(14) 51.3(16) ms β (94.3%) 100Sr 4−#
β, n (5.6%) 99Sr
β, 2n (0.15%) 98Sr
101Rb 37 64 100.954302(22) 31.8(33) ms β (72%) 101Sr 3/2+#
β, n (28%) 100Sr
102Rb 37 65 101.960008(89) 37(4) ms β, n (65%) 101Sr (4+)
β (35%) 102Sr
103Rb 37 66 102.96440(43)# 26(11) ms β 103Sr 3/2+#
104Rb 37 67 103.97053(54)# 35# ms
[>550 ns]
105Rb[5] 37 68
106Rb[5] 37 69
This table header & footer:
  1. ^ mRb – Excited nuclear isomer.
  2. ^ ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  3. ^ # – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  4. ^ Bold half-life – nearly stable, half-life longer than age of universe.
  5. ^ a b c # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  6. ^ Modes of decay:
    EC: Electron capture


    IT: Isomeric transition
    n: Neutron emission
    p: Proton emission
  7. ^ Bold italics symbol as daughter – Daughter product is nearly stable.
  8. ^ Bold symbol as daughter – Daughter product is stable.
  9. ^ ( ) spin value – Indicates spin with weak assignment arguments.
  10. ^ a b Fission product
  11. ^ Primordial radionuclide
  12. ^ Used in rubidium–strontium dating
  13. ^ Order of ground state and isomer is uncertain.

Rubidium-87

[edit]

Rubidium-87 is one of two natural isotopes of rubidium, with an abundance of 27.835%, and a half-life of 4.97×1010 years, with beta decay to strontium-87, a stable isotope.

During fractional crystallization of igneous rock, Sr tends to become concentrated in plagioclase, leaving Rb in the liquid phase. Hence, the Rb/Sr ratio in residual magma may increase over time, resulting in rocks with increasing Rb/Sr ratios with increasing differentiation. The highest ratios (10 or higher) occur in pegmatites. The age of a mineral, if it has not been subsequently altered, is determined by the parent and daughter abundances, the half-life, and the original content of the daughter, here strontium; the 87Sr/86Sr ratio helps in its calculation. See rubidium-strontium dating for further detail.

Rubidium-87 was the first and the most popular atom for making Bose–Einstein condensates in dilute atomic gases. Even though rubidium-85 is more abundant, rubidium-87 has a positive scattering length, which means it is mutually repulsive, at low temperatures. This prevents a collapse of all but the smallest condensates. It is also easy to evaporatively cool, with a consistent strong mutual scattering. There is also a strong supply of cheap uncoated diode lasers typically used in CD writers, which can operate at the correct wavelength.

See also

[edit]

Daughter products other than rubidium

References

[edit]
  1. ^ a b c d e Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3) 030001. doi:10.1088/1674-1137/abddae.
  2. ^ "Standard Atomic Weights: Rubidium". CIAAW. 1969.
  3. ^ Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04). "Standard atomic weights of the elements 2021 (IUPAC Technical Report)". Pure and Applied Chemistry. doi:10.1515/pac-2019-0603. ISSN 1365-3075.
  4. ^ Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*". Chinese Physics C. 45 (3) 030003. doi:10.1088/1674-1137/abddaf.
  5. ^ a b Sumikama, T.; et al. (2021). "Observation of new neutron-rich isotopes in the vicinity of 110Zr". Physical Review C. 103 (1): 014614. Bibcode:2021PhRvC.103a4614S. doi:10.1103/PhysRevC.103.014614. hdl:10261/260248. S2CID 234019083.{{cite journal}}: CS1 maint: article number as page number (link)