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Isotopes of rubidium

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Isotopes ofrubidium (37Rb)
Main isotopes[1]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
82Rbsynth1.2575 mβ+82Kr
83Rbsynth86.2 dε83Kr
84Rbsynth32.82 dβ+84Kr
β84Sr
85Rb72.2%stable
86Rbsynth18.645 dβ86Sr
ε86Kr
87Rb27.8%4.97×1010 yβ87Sr
Standard atomic weightAr°(Rb)

Rubidium (37Rb) has 35 knownisotopes, from72Rb to106Rb, with naturally occurring rubidium composed of two: stable85Rb (72.2%) andradioactive87Rb (27.8%). Theprimordial radionuclide87Rb has ahalf-life of4.97×1010 years,beta decaying to stable87Sr. It is, as the element is, widespread on Earth as rubidium readily substitutes forpotassium in allminerals. The decay of87Rb has been used extensively indating rocks; seerubidium–strontium dating for a more detailed discussion.

Other than87Rb, the longest-livedradioisotopes are83Rb with a half-life of 86.2 days,84Rb with a half-life of 32.82 days, and86Rb 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 is82mRb at 6.472 hours.

The ground state of82Rb has a much shorterhalf-life of 1.2575 minutes. It is used medically in somecardiacpositron emission tomography scans to assessmyocardial perfusion. It is synthesized through the longer-lived82Sr, made in a cyclotron, though agenerator. It may be administered as thechloride.

List of isotopes

[edit]


Nuclide
[n 1]
ZNIsotopic 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
72Rb373571.95885(54)#103(22) nsp71Kr1+#
73Rb373672.950605(44)<81 nsp72Kr3/2−#
74Rb373773.9442659(32)64.78(3) msβ+74Kr0+
75Rb373874.9385732(13)19.0(12) sβ+75Kr3/2−
76Rb373975.9350730(10)36.5(6) sβ+76Kr1−
β+,α (3.8×10−7%)72Se
76mRb316.93(8) keV3.050(7) μsIT76Rb(4+)
77Rb374076.9304016(14)3.78(4) minβ+77Kr3/2−
78Rb374177.9281419(35)17.66(3) minβ+78Kr0+
78m1Rb46.84(14) keV910(40) nsIT78Rb(1−)
78m2Rb111.19(22) keV5.74(3) minβ+ (91%)78Kr4−
IT (9%)78Rb
79Rb374278.9239901(21)22.9(5) minβ+79Kr5/2+
80Rb374379.9225164(20)33.4(7) sβ+80Kr1+
80mRb493.9(5) keV1.63(4) μsIT80Rb(6+)
81Rb374480.9189939(53)4.572(4) hβ+81Kr3/2−
81mRb86.31(7) keV30.5(3) minIT (97.6%)81Rb9/2+
β+ (2.4%)81Kr
82Rb374581.9182090(32)1.2575(2) minβ+82Kr1+
82mRb69.0(15) keV6.472(6) hβ+82Kr5−
83Rb374682.9151142(25)86.2(1) dEC83Kr5/2−
83mRb42.0780(20) keV7.8(7) msIT83Rb9/2+
84Rb374783.9143752(24)32.82(7) dβ+ (96.1%)84Kr2−
β (3.9%)84Sr
84mRb463.59(8) keV20.26(4) minIT84Rb6−
85Rb[n 10]374884.9117897360(54)Stable5/2−0.7217(2)
85mRb514.0065(22) keV1.015(1) μsIT85Rb9/2+
86Rb374985.91116744(21)18.645(8) dβ (99.9948%)86Sr2−
EC (0.0052%)86Kr
86mRb556.05(18) keV1.017(3) minIT86Rb6−
87Rb[n 10][n 11][n 12]375086.909180529(6)4.97(3)×1010 yβ87Sr3/2−0.2783(2)
88Rb375187.91131559(17)17.78(3) minβ88Sr2−
88mRb1373.8(3) keV123(13) nsIT88Rb(7+)
89Rb375288.9122781(58)15.32(10) minβ89Sr3/2−
90Rb375389.9147976(69)158(5) sβ90Sr0−
90mRb106.90(3) keV258(4) sβ (97.4%)90Sr3−
IT (2.6%)90 Rb
91Rb375490.9165373(84)58.2(3) sβ91Sr3/2−
92Rb375591.9197285(66)4.48(3) sβ (99.99%)92Sr0−
β,n (0.0107%)91Sr
93Rb375692.9220393(84)5.84(2) sβ (98.61%)93Sr5/2−
β, n (1.39%)92Sr
93mRb4423.1(15) keV111(11) nsIT93Rb(27/2−)
94Rb375793.9263948(22)2.702(5) sβ (89.7%)94Sr3−
β, n (10.3%)93Sr
94m1Rb104.2(2) keV130(15) nsIT94Rb(0−)
94m2Rb2074.9(14) keV107(16) nsIT94Rb(10−)
95Rb375894.929264(22)377.7(8) msβ (91.3%)95Sr5/2−
β, n (8.7%)94Sr
95mRb835.0(6) keV<500 nsIT95Rb9/2+#
96Rb375995.9341334(36)201.5(9) msβ (86.3%)96Sr2−
β, n (13.7%)95Sr
96m1Rb[n 13]0(200)# keV200# ms
[>1 ms]
1(+#)
96m2Rb1134.6(11) keV1.80(4) μsIT96Rb(10−)
97Rb376096.9371771(21)169.1(6) msβ (74.5%)97Sr3/2+
β, n (25.5%)96Sr
97mRb76.6(2) keV5.7(6) μsIT97Rb(1/2,3/2)−
98Rb376197.941632(17)115(6) msβ(85.65%)98Sr(0−)
β, n (14.3%)97Sr
β, 2n (0.054%)96Sr
98m1Rb73(26) keV96(3) msβ98Sr(3+)
98m2Rb178.5(4) keV358(7) nsIT98Rb(2−)
99Rb376298.9451192(43)54(4) msβ (82.7%)99Sr(3/2+)
β, n (17.3%)98Sr
100Rb376399.950332(14)51.3(16) msβ (94.3%)100Sr4−#
β, n (5.6%)99Sr
β, 2n (0.15%)98Sr
101Rb3764100.954302(22)31.8(33) msβ (72%)101Sr3/2+#
β, n (28%)100Sr
102Rb3765101.960008(89)37(4) msβ, n (65%)101Sr(4+)
β (35%)102Sr
103Rb3766102.96440(43)#26(11) msβ103Sr3/2+#
104Rb3767103.97053(54)#35# ms
[>550 ns]
105Rb[5]3768
106Rb[5]3769
This table header & footer:
  1. ^mRb – Excitednuclear 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 thanage of universe.
  5. ^abc# – 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. ^abFission product
  11. ^Primordialradionuclide
  12. ^Used inrubidium–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 of4.97×1010 years, withbeta decay tostrontium-87, a stable isotope.

During fractional crystallization ofigneous 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; the87Sr/86Sr ratio helps in its calculation. Seerubidium-strontium dating for further detail.

Rubidium-87 was the first and the most popular atom for makingBose–Einstein condensates in diluteatomic gases. Even thoughrubidium-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 uncoateddiode lasers typically used inCD writers, which can operate at the correct wavelength.

See also

[edit]

Daughter products other than rubidium

References

[edit]
  1. ^abcdeKondev, 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. ^abSumikama, 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.
Group12 3456789101112131415161718
PeriodHydrogen and
alkali metals
Alkaline
earth metals
Pnicto­gensChal­co­gensHalo­gensNoble gases
12
345678910
1112131415161718
192021222324252627282930313233343536
373839404142434445464748495051525354
55561 asterisk71727374757677787980818283848586
87881 asterisk103104105106107108109110111112113114115116117118
119120
1 asterisk5758596061626364656667686970 
1 asterisk8990919293949596979899100101102
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