Isotopes of yttrium

Last updated
Isotopes of yttrium  (39Y)
Main isotopes Decay
abun­dance half-life (t1/2) mode pro­duct
87Y synth 3.4 d ε 87Sr
γ
88Ysynth106.6 dε 88Sr
γ
89Y100% stable
90Y synth2.7 d β 90Zr
γ
91Ysynth58.5 dβ 91Zr
γ
Standard atomic weight Ar°(Y)

Natural yttrium (39Y) is composed of a single isotope yttrium-89. The most stable radioisotopes are 88Y, which has a half-life of 106.6 days, and 91Y, with a half-life of 58.51 days. All the other isotopes have half-lives of less than a day, except 87Y, which has a half-life of 79.8 hours, and 90Y, with 64 hours. The dominant decay mode below the stable 89Y is electron capture and the dominant mode after it is beta emission. Thirty-five unstable isotopes have been characterized.

90Y exists in equilibrium with its parent isotope strontium-90, which is a product of nuclear fission.

List of isotopes

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

[n 5]
Daughter
isotope

[n 6] [n 7]
Spin and
parity
[n 8] [n 4]
Natural abundance (mole fraction)
Excitation energy [n 4] Normal proportionRange of variation
76Y393775.95845(54)#500# ns [>170 ns]
77Y393876.94965(7)#63(17) ms p (>99.9%)76Sr5/2+#
β+ (<.1%)77Sr
78Y393977.94361(43)#54(5) msβ+78Sr(0+)
78mY0(500)# keV5.8(5) s5+#
79Y394078.93735(48)14.8(6) sβ+ (>99.9%)79Sr(5/2+)#
β+, p (<.1%)78Rb
80Y394179.93428(19)30.1(5) sβ+80Sr4−
80m1Y228.5(1) keV4.8(3) s(1−)
80m2Y312.6(9) keV4.7(3) µs(2+)
81Y394280.92913(7)70.4(10) sβ+81Sr(5/2+)
82Y394381.92679(11)8.30(20) sβ+82Sr1+
82m1Y402.63(14) keV268(25) ns4−
82m2Y507.50(13) keV147(7) ns6+
83Y394482.92235(5)7.08(6) minβ+83Sr9/2+
83mY61.98(11) keV2.85(2) minβ+ (60%)83Sr(3/2−)
IT (40%)83Y
84Y394583.92039(10)39.5(8) minβ+84Sr1+
84mY−80(190) keV4.6(2) sβ+84Sr(5−)
85Y394684.916433(20)2.68(5) hβ+85Sr(1/2)−
85m1Y19.8(5) keV4.86(13) hβ+ (99.998%)85Sr9/2+
IT (.002%)85Y
85m2Y266.30(20) keV178(6) ns5/2−
86Y394785.914886(15)14.74(2) hβ+86Sr4−
86m1Y218.30(20) keV48(1) minIT (99.31%)86Y(8+)
β+ (.69%)86Sr
86m2Y302.2(5) keV125(6) ns(7−)
87Y394886.9108757(17)79.8(3) hβ+87Sr1/2−
87mY380.82(7) keV13.37(3) hIT (98.43%)87Y9/2+
β+ (1.56%)87Sr
88Y394987.9095011(20)106.616(13) dβ+88Sr4−
88m1Y674.55(4) keV13.9(2) msIT88Y(8)+
88m2Y392.86(9) keV300(3) µs1+
89Y [n 9] 395088.9058483(27)Stable1/2−1.0000
89mY908.97(3) keV15.663(5) sIT89Y9/2+
90Y [n 9] 395189.9071519(27)64.053(20) hβ90Zr2−
90mY681.67(10) keV3.19(6) hIT (99.99%)90Y7+
β (.0018%)90Zr
91Y [n 9] 395290.907305(3)58.51(6) dβ91Zr1/2−
91mY555.58(5) keV49.71(4) minIT (98.5%)91Y9/2+
β (1.5%)91Zr
92Y395391.908949(10)3.54(1) hβ92Zr2−
93Y395492.909583(11)10.18(8) hβ93Zr1/2−
93mY758.719(21) keV820(40) msIT93Y7/2+
94Y395593.911595(8)18.7(1) minβ94Zr2−
95Y395694.912821(8)10.3(1) minβ95Zr1/2−
96Y395795.915891(25)5.34(5) sβ96Zr0−
96mY1140(30) keV9.6(2) sβ96Zr(8)+
97Y395896.918134(13)3.75(3) sβ (99.942%)97Zr(1/2−)
β, n (.058%)96Zr
97m1Y667.51(23) keV1.17(3) sβ (99.3%)97Zr(9/2)+
IT (.7%)97Y
β, n (.08%)96Zr
97m2Y3523.3(4) keV142(8) ms(27/2−)
98Y395997.922203(26)0.548(2) sβ (99.669%)98Zr(0)−
β, n (.331%)97Zr
98m1Y170.74(6) keV620(80) ns(2)−
98m2Y410(30) keV2.0(2) sβ (86.6%)98Zr(5+,4−)
IT (10%)98Y
β, n (3.4%)97Zr
98m3Y496.19(15) keV7.6(4) µs(2−)
98m4Y1181.1(4) keV0.83(10) µs(8−)
99Y396098.924636(26)1.470(7) sβ (98.1%)99Zr(5/2+)
β, n (1.9%)98Zr
99mY2141.65(19) keV8.6(8) µs(17/2+)
100Y396199.92776(8)735(7) msβ (98.98%)100Zr1−,2−
β, n (1.02%)99Zr
100mY200(200)# keV940(30) msβ100Zr(3,4,5)(+#)
101Y3962100.93031(10)426(20) msβ (98.06%)101Zr(5/2+)
β, n (1.94%)100Zr
102Y3963101.93356(9)0.30(1) sβ (95.1%)102Zr
β, n (4.9%)101Zr
102mY200(200)# keV360(40) msβ (94%)102Zrhigh
β, n (6%)101Zr
103Y3964102.93673(32)#224(19) msβ (91.7%)103Zr5/2+#
β, n (8.3%)102Zr
104Y3965103.94105(43)#180(60) msβ104Zr
105Y3966104.94487(54)#60# ms [>300 ns]β105Zr5/2+#
106Y3967105.94979(75)#50# ms [>300 ns]β106Zr
107Y3968106.95414(54)#30# ms [>300 ns]5/2+#
108Y [3] 3969107.95948(86)#20# ms [>300 ns]
109Y [3] 3970
110Y [4] 3971
111Y [4] 3972
This table header & footer:
  1. mY  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. 1 2 3 #  Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  5. Modes of decay:
    IT: Isomeric transition
    n: Neutron emission
    p: Proton emission
  6. Bold italics symbol as daughter  Daughter product is nearly stable.
  7. Bold symbol as daughter  Daughter product is stable.
  8. () spin value  Indicates spin with weak assignment arguments.
  9. 1 2 3 Fission product

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References

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  2. 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.
  3. 1 2 Ohnishi, Tetsuya; Kubo, Toshiyuki; Kusaka, Kensuke; et al. (2010). "Identification of 45 New Neutron-Rich Isotopes Produced by In-Flight Fission of a 238U Beam at 345 MeV/nucleon". J. Phys. Soc. Jpn. 79 (7). Physical Society of Japan: 073201. arXiv: 1006.0305 . Bibcode:2010JPSJ...79g3201T. doi: 10.1143/JPSJ.79.073201 .
  4. 1 2 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.