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Isotopes of rhenium

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(Redirected fromRhenium-185)

Isotopes ofrhenium (75Re)
Main isotopes[1]Decay
abun­dancehalf-life(t1/2)modepro­duct
185Re37.4%stable
186Resynth3.7185 dβ186Os
ε186W
186mResynth2×105 yIT186Re
β186Os
187Re62.6%4.12×1010 yβ187Os
Standard atomic weightAr°(Re)

Naturally occurringrhenium (75Re) is 37.4%185Re, which isstable (although it ispredicted to decay), and 62.6%187Re, which isunstable but has a very longhalf-life (4.12×1010 years).[4] Among elements with a known stable isotope, onlyindium andtellurium similarly occur with a stable isotope in lower abundance than the long-lived radioactive isotope.

There are 36 other unstable isotopes recognized, the longest-lived of which are183Re with a half-life of 70 days,184Re with a half-life of 38 days,186Re with a half-life of 3.7186 days,182Re with a half-life of 64.0 hours, and189Re with a half-life of 24.3 hours. There are also numerousisomers, the longest-lived of which are186mRe with a half-life of 200,000 years and184mRe with a half-life of 177.25 days.[5] All others have half-lives less than a day.

List of isotopes

[edit]


Nuclide
[n 1]
ZNIsotopic mass(Da)
[n 2][n 3]
Half-life
[n 4][n 5]
Decay
mode

[n 6]
Daughter
isotope

[n 7][n 8]
Spin and
parity
[n 9][n 5]
Natural abundance(mole fraction)
Excitation energy[n 5]Normal proportionRange of variation
159Re[6]758421(4) μsp (92.5%)158W(11/2−)
α (7.5%)155Ta
160Re[7]7585159.98212(43)#611(7) μsp (89%)159W(2−)
α (11%)156Ta
160mRe[8]185(21)# keV2.8(1) μsIT160Re(9+)
161Re7586160.97759(22)0.37(4) msp160W1/2+
161mRe123.8(13) keV15.6(9) msα157Ta11/2−
162Re7587161.97600(22)#107(13) msα (94%)158Ta(2−)
β+ (6%)162W
162mRe173(10) keV77(9) msα (91%)158Ta(9+)
β+ (9%)162W
163Re7588162.972081(21)390(70) msβ+ (68%)163W(1/2+)
α (32%)159Ta
163mRe115(4) keV214(5) msα (66%)159Ta(11/2−)
β+ (34%)163W
164Re7589163.97032(17)#0.53(23) sα (58%)160Tahigh
β+ (42%)164W
164mRe120(120)# keV530(230) ms(2#)−
165Re7590164.967089(30)1# sβ+165W1/2+#
α161Ta
165mRe47(26) keV2.1(3) sβ+ (87%)165W11/2−#
α (13%)161Ta
166Re7591165.96581(9)#2# sβ+166W2−#
α162Ta
167Re7592166.96260(6)#3.4(4) sα163Ta9/2−#
β+167W
167mRe130(40)# keV5.9(3) sβ+ (99.3%)167W1/2+#
α (.7%)163Ta
168Re7593167.96157(3)4.4(1) sβ+ (99.99%)168W(5+, 6+, 7+)
α (.005%)164Ta
168mRenon-exist6.6(15) s
169Re7594168.95879(3)8.1(5) sβ+ (99.99%)169W9/2−#
α (.005%)165Ta
169mRe145(29) keV15.1(15) sβ+ (99.8%)169W1/2+#
α (.2%)164Ta
170Re7595169.958220(28)9.2(2) sβ+ (99.99%)170W(5+)
α (.01%)166Ta
171Re7596170.95572(3)15.2(4) sβ+171W(9/2−)
172Re7597171.95542(6)15(3) sβ+172W(5)
172mRe0(100)# keV55(5) sβ+172W(2)
173Re7598172.95324(3)1.98(26) minβ+173W(5/2−)
174Re7599173.95312(3)2.40(4) minβ+174W
175Re75100174.95138(3)5.89(5) minβ+175W(5/2−)
176Re75101175.95162(3)5.3(3) minβ+176W3+
177Re75102176.95033(3)14(1) minβ+177W5/2−
177mRe84.71(10) keV50(10) μs5/2+
178Re75103177.95099(3)13.2(2) minβ+178W(3+)
179Re75104178.949988(26)19.5(1) minβ+179W(5/2)+
179m1Re65.39(9) keV95(25) μs(5/2−)
179m2Re1684.59(14)+Y keV>0.4 μs(23/2+)
180Re75105179.950789(23)2.44(6) minβ+180W(1)−
181Re75106180.950068(14)19.9(7) hβ+181W5/2+
182Re75107181.95121(11)64.0(5) hβ+182W7+
182m1Re60(100) keV12.7(2) hβ+182W2+
182m2Re235.736(10)+X keV585(21) ns2−
182m3Re461.3(1)+X keV0.78(9) μs(4−)
183Re75108182.950820(9)70.0(14) dEC183W5/2+
183mRe1907.6(3) keV1.04(4) msIT183Re(25/2+)
184Re75109183.952521(5)35.4(7) d[5]β+184W3(−)
184mRe188.01(4) keV177.25(7) d[5]IT (75.4%)184Re8(+)
β+ (24.6%)184W
185Re75110184.9529550(13)Observationally Stable[n 10]5/2+0.3740(2)
185mRe2124(2) keV123(23) ns(21/2)
186Re75111185.9549861(13)3.7186(5) dβ (93.1%)186Os1−
EC (6.9%)186W
186mRe149(7) keV2.0(5)×105 yIT[n 11]186Re(8+)
187Re[n 12][n 13]75112186.9557531(15)4.12(2)×1010 y[n 14]β[n 15]187Os5/2+0.6260(2)
188Re75113187.9581144(15)17.0040(22) hβ188Os1−
188mRe172.069(9) keV18.59(4) minIT188Re(6)−
189Re75114188.959229(9)24.3(4) hβ189Os5/2+
190Re75115189.96182(16)3.1(3) minβ190Os(2)−
190mRe210(50) keV3.2(2) hβ (54.4%)190Os(6−)
IT (45.6%)190Re
191Re75116190.963125(11)9.8(5) minβ191Os(3/2+, 1/2+)
192Re75117191.96596(21)#16(1) sβ192Os
193Re75118192.96747(21)#30# s [>300 ns]5/2+#
194Re75119193.97042(32)#2# s [>300 ns]
This table header & footer:
  1. ^mRe – 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


    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. ^Believed to undergo α decay to181Ta
  11. ^Theoretically capable of β decay to186Os[1][9]
  12. ^primordialradionuclide
  13. ^Used inrhenium–osmium dating
  14. ^Can undergoBound-state β decay with a half-life of 32.9 years when fullyionized
  15. ^Theorized to also undergo α decay to183Ta

Rhenium-186

[edit]
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This sectionneeds expansion with: Usage in medicine, ATC=V10. You can help byadding to it.(October 2019)

Rhenium-186 is a beta emitter andradiopharmaceutical that is used to treatglioblastoma,[10] is used intheranostic medicine[11] and has been reported to be used in synoviorthesis.[12]

References

[edit]
  1. ^abKondev, 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: Rhenium".CIAAW. 1973.
  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. ^Bosch, F.; Faestermann, T.; Friese, J.; et al. (1996). "Observation of bound-stateβ decay of fully ionized187Re:187Re-187Os Cosmochronometry".Physical Review Letters.77 (26):5190–5193.Bibcode:1996PhRvL..77.5190B.doi:10.1103/PhysRevLett.77.5190.PMID 10062738.
  5. ^abcJaniak, Ł.; Gierlik, M.; R. Prokopowicz, G. Madejowski; Wronka, S.; Rzadkiewicz, J.; Carroll, J. J.; Chiara, C. J. (2022). "Half-life of the 188-keV isomer of184Re".Physical Review C.106 (44303): 044303.Bibcode:2022PhRvC.106d4303J.doi:10.1103/PhysRevC.106.044303.S2CID 252792730.
  6. ^Page, R. D.; Bianco, L.; Darby, I. G.; Uusitalo, J.; Joss, D. T.; Grahn, T.; Herzberg, R.-D.; Pakarinen, J.; Thomson, J.; Eeckhaudt, S.; Greenlees, P. T.; Jones, P. M.; Julin, R.; Juutinen, S.; Ketelhut, S.; Leino, M.; Leppänen, A.-P.; Nyman, M.; Rahkila, P.; Sarén, J.; Scholey, C.; Steer, A.; Hornillos, M. B. Gómez; Al-Khalili, J. S.; Cannon, A. J.; Stevenson, P. D.; Ertürk, S.; Gall, B.; Hadinia, B.; Venhart, M.; Simpson, J. (26 June 2007)."α decay of Re 159 and proton emission from Ta 155".Physical Review C.75 (6): 061302.Bibcode:2007PhRvC..75f1302P.doi:10.1103/PhysRevC.75.061302.ISSN 0556-2813. Retrieved12 June 2023.
  7. ^Darby, I. G.; Page, R. D.; Joss, D. T.; Bianco, L.; Grahn, T.; Judson, D. S.; Simpson, J.; Eeckhaudt, S.; Greenlees, P. T.; Jones, P. M.; Julin, R.; Juutinen, S.; Ketelhut, S.; Leino, M.; Leppänen, A.-P.; Nyman, M.; Rahkila, P.; Sarén, J.; Scholey, C.; Steer, A. N.; Uusitalo, J.; Venhart, M.; Ertürk, S.; Gall, B.; Hadinia, B. (20 June 2011)."Precision measurements of proton emission from the ground states of Ta 156 and Re 160".Physical Review C.83 (6): 064320.Bibcode:2011PhRvC..83f4320D.doi:10.1103/PhysRevC.83.064320.ISSN 0556-2813. Retrieved21 June 2023.
  8. ^Darby, I. G.; Page, R. D.; Joss, D. T.; Simpson, J.; Bianco, L.; Cooper, R. J.; Eeckhaudt, S.; Ertürk, S.; Gall, B.; Grahn, T.; Greenlees, P. T.; Hadinia, B.; Jones, P. M.; Judson, D. S.; Julin, R.; Juutinen, S.; Ketelhut, S.; Leino, M.; Leppänen, A. -P.; Nyman, M.; Rahkila, P.; Sarén, J.; Scholey, C.; Steer, A. N.; Uusitalo, J.; Venhart, M. (10 January 2011)."Decay of the high-spin isomer in 160Re: Changing single-particle structure beyond the proton drip line".Physics Letters B.695 (1):78–81.Bibcode:2011PhLB..695...78D.doi:10.1016/j.physletb.2010.10.052.ISSN 0370-2693.
  9. ^https://www.nndc.bnl.gov/ensnds/186/Re/adopted.pdf, NNDC Chart of Nuclides, Adopted Levels for186Re.
  10. ^"Rhenium-186 liposomes as convection-enhanced nanoparticle brachytherapy for treatment of glioblastoma".academic.oup.com. Retrieved2024-12-07.
  11. ^Mastren, Tara; Radchenko, Valery; Bach, Hong T.; Balkin, Ethan R.; Birnbaum, Eva R.; Brugh, Mark; Engle, Jonathan W.; Gott, Matthew D.; Guthrie, James; Hennkens, Heather M.; John, Kevin D.; Ketring, Alan R.; Kuchuk, Marina; Maassen, Joel R.; Naranjo, Cleo M.; Nortier, F. Meiring; Phelps, Tim E.; Jurisson, Silvia S.; Wilbur, D. Scott; Fassbender, Michael E. (2017)."Bulk production and evaluation of high specific activity 186gRe for cancer therapy using enriched 186WO3 targets in a proton beam".Nuclear Medicine and Biology.49. Elsevier BV:24–29.doi:10.1016/j.nucmedbio.2017.02.006.ISSN 0969-8051.
  12. ^"Radiosynoviorthese (RSO) mit Rhenium-186 (Re-186)-Sulfid"(PDF). Retrieved2024-12-07.
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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