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Isotopes of rhenium

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(Redirected fromRhenium-188)

Isotopes ofrhenium (75Re)
Main isotopes[1]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
183Resynth70 dε183W
184Resynth35.4 dβ+184W
184mResynth177.25 dIT184Re
β+184W
185Re37.4%stable
186Resynth3.7185 dβ186Os
ε186W
186mResynth2×105 yIT186Re
187Re62.6%4.16×1010 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 (4.16×1010 years). 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 35.4 days,186Re with a half-life of 3.7185 days,182Re with a half-life of 64.2 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.[4] All others have half-lives less than a day.

List of isotopes

[edit]


Nuclide
[n 1]
ZNIsotopic mass(Da)[5]
[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
159Re7584158.98411(33)#40# μs1/2+#
159mRe210(50)# keV20(4) μsp (92.5%)158W(11/2−)
α (7.5%)155Ta
160Re7585159.98188(32)#611(7) μsp (89%)159W(4−)
α (11%)156Ta
160mRe177(15) keV2.8(1) μsIT160Re(9+)
161Re7586160.97762(16)440(1) μsp160W1/2+
161mRe123.7(13) keV14.7(3) msα (93.0%)157Ta11/2−
p (7.0%)160W
162Re7587161.97590(22)#107(13) msα (94%)158Ta(2)−
β+ (6%)162W
162mRe175(9) keV77(9) msα (91%)158Ta(9)+
β+ (9%)162W
163Re7588162.972085(20)390(70) msβ+ (68%)163W1/2+
α (32%)159Ta
163mRe120(5) keV214(5) msα (66%)159Ta11/2−
β+ (34%)163W
164Re7589163.970507(59)719(89) sα (?%)160Ta(2)−
β+ (?%)164W
164mRe[n 10]−50(250) keV890(130) msβ+ (97%)164W(9,10)+
α (3%)160Ta
165Re7590164.967086(25)1.6(6) sβ+ (86%)165W(1/2+)
α (14%)161Ta
165mRe[n 10]28(22) keV1.74(6) sβ+ (87%)165W(11/2−)
α (13%)161Ta
166Re7591165.965821(95)2.25(21) sβ+166W(7+)
α162Ta
167Re7592166.962604(43)#3.4(4) sα (?%)163Ta9/2−
β+ (?%)167W
167mRe131(13)# keV5.9(3) sβ+ (?%)167W1/2+
α (?%)163Ta
168Re7593167.961573(33)4.4(1) sβ+168W(7+)
α (0.005%)164Ta
169Re7594168.958766(12)8.1(5) sβ+169W(9/2−)
α (0.005%)165Ta
169mRe175(13) keV15.1(15) sβ+ (?%)169W(1/2+,3/2+)
α (?%)164Ta
170Re7595169.958235(12)>1# sβ+170W(8−,9−)#
170m1Re73(17) keV9.2(2) sβ+170W(5+)
170m2Re210.1(1) keV130(10) nsIT170Re(6,7,8,9)
171Re7596170.955716(30)15.2(4) sβ+171W(9/2−)
172Re7597171.955376(38)55(5) sβ+172W(2+)
172mRe[n 10]110(50)# keV15(3) sβ+172W(7+)
173Re7598172.953243(30)2.0(3) minβ+173W(5/2−)
174Re7599173.953115(30)2.40(4) minβ+174W3+#
174mRe100(50)# keV1# min
[>1 μs]
7+#
175Re75100174.951381(30)5.89(5) minβ+175W5/2−#
176Re75101175.951623(30)5.3(3) minβ+176W(3+)
177Re75102176.950328(30)14(1) minβ+177W5/2−
177mRe84.70(10) keV50(10) μsIT177Re5/2+
178Re75103177.950989(30)13.2(2) minβ+178W(3+)
179Re75104178.949990(26)19.5(1) minβ+179W5/2+
179m1Re65.35(9) keV95(25) μsIT179Re(5/2−)
179m2Re1822(50)# keV408(12) nsIT179Re(23/2+)
179m3Re5408.0(5) keV466(15) μsIT179Re(47/2+,49/2+)
180Re75105179.950792(23)2.46(3) minβ+180W(1)−
180m1Re90(30)# keV>1# μsIT180Re(4+,5+)
180m2Re3561(30)# keV9.0(7) μsIT180Re21−
181Re75106180.950062(13)19.9(7) hβ+181W5/2+
181m1Re262.91(11) keV156.7(19) nsIT181Re9/2−
181m2Re1656.37(14) keV250(10) nsIT181Re21/2−
181m3Re1880.57(16) keV11.5(9) μsIT181Re25/2+
181m4Re3869.40(18) keV1.2(2) μsIT181Re(35/2−)
182Re75107181.95121(11)64.2(5) hβ+182W7+
182m1Re[n 10]60(100) keV14.14(45) hβ+182W2+
182m2Re296(100) keV585(30) nsIT182Re(2)−
182m3Re521(100) keV0.78(9) μsIT182Re(4−)
183Re75108182.9508213(86)70.0(14) dEC183W5/2+
183mRe1907.21(15) keV1.04(4) msIT183Re25/2+
184Re75109183.9525281(46)35.4(7) dβ+184W3−
184mRe188.0463(17) keV177.25(7) d[4]IT (74.5%)184Re8+
β+ (25.5%)184W
185Re75110184.95295832(88)Observationally stable[n 11]5/2+0.3740(5)
185mRe2124.1(4) keV200(4) nsIT185Re25/2+
186Re75111185.95498917(88)3.7185(5) dβ (92.53%)186Os1−
EC (7.47%)186W
186mRe148.2(5) keV~2.0×105 yIT[n 12]186Re(8+)
187Re[n 13][n 14]75112186.95575222(79)4.16(2)×1010 y[n 15]β[n 16]187Os5/2+0.6260(5)
187m1Re206.2473(10) keV555.3(17) nsIT187Re9/2−
187m2Re1682.0(6) keV354(62) nsIT187Re21/2+
188Re75113187.95811366(79)17.005(3) hβ188Os1−
188mRe172.0848(24) keV18.59(4) minIT188Re6−
189Re75114188.9592278(88)24.3(4) hβ189Os5/2+
189mRe1770.9(6) keV223(14) μsIT189Re29/2+
190Re75115189.9618001(52)3.0(2) minβ190Os(2)−
190mRe204(10) keV3.1(2) hβ (54.4%)190Os(6−)
IT (45.6%)190Re
191Re75116190.963123(11)9.8(5) minβ191Os(3/2+)
191mRe1601.5(4) keV50.6(35) μsIT191Re25/2−
192Re75117191.966088(76)15.4(5) sβ192Os(0−)
192m1Re159(1) keV88(8) μsIT192Re
192m2Re267(10) keV<500 ms
193Re75118192.967545(42)3# min
[>300 ns]
5/2+#
193mRe146.0(2) keV69(6) μsIT193Re(9/2−)
194Re75119193.97074(22)#5(1) sβ194Os1−#
194m1Re150(50)# keV45(18) μsIT194Re4−#
194m2Re285(40) keV25(8) sβ194Os11−#
194m3Re833(33) keV100(10) sβ194Os
195Re75120194.97256(32)#5(1) sβ195Os5/2+#
196Re75121195.97600(32)#2.4(15) sβ196Os
196mRe120(40)# keV3.6(6) μsIT196Re
197Re75122196.97815(32)#400# ms
[>300 ns]
5/2+#
198Re75123197.98176(43)#1# s
[>300 ns]
199Re75124198.98419(43)#250# ms
[>300 ns]
5/2+#
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:
    α:Alpha decay
    β+:Positron emission
    EC:Electron capture
    β:Beta decay
    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. ^abcdOrder of ground state and isomer is uncertain.
  11. ^Believed to undergo α decay to181Ta
  12. ^Theoretically capable of β decay to186Os[6]
  13. ^primordialradionuclide
  14. ^Used inrhenium–osmium dating
  15. ^Instead undergoesBound-state β decay with a half-life of 32.9 years when fullyionized[7]
  16. ^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,[8] is used intheranostic medicine[9] and has been reported to be used in synoviorthesis.[10]

See also

[edit]

Daughter products other than rhenium

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: 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. ^abJaniak, 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.
  5. ^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.
  6. ^Seegmiller, D. W.; Lindner, M.; Meyer, R. A. (24 April 1972)."186Re: Nuclear structure and an isomer of half-life 2×105 y".Nuclear Physics A.185 (1):94–112.doi:10.1016/0375-9474(72)90553-2. See Section 4.2 "Search for β-decay from the isomeric level".
  7. ^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.
  8. ^"Rhenium-186 liposomes as convection-enhanced nanoparticle brachytherapy for treatment of glioblastoma".academic.oup.com. Retrieved2024-12-07.
  9. ^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.
  10. ^"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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