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Isotopes of manganese

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Isotopes ofmanganese (25Mn)
Main isotopes[1]Decay
abun­dancehalf-life(t1/2)modepro­duct
52Mnsynth5.591 dβ+52Cr
53Mntrace3.7×106 yε53Cr
54Mnsynth312.081 dε54Cr
β54Fe
β+54Cr
55Mn100%stable
Standard atomic weightAr°(Mn)

Naturally occurringmanganese (25Mn) is composed of one stableisotope,55Mn. Twenty-sevenradioisotopes have been characterized, with the most stable being53Mn with ahalf-life of 3.7 million years,54Mn with a half-life of 312.3 days, and52Mn with a half-life of 5.591 days. All of the remainingradioactive isotopes have half-lives that are less than 3 hours and the majority of these have half-lives that are less than a minute. This element also has sevenmeta states.

Manganese is part of theiron group of elements, which are thought to be synthesized in largestars shortly beforesupernova explosions.53Mn decays to53Cr with ahalf-life of 3.7 million years. Because of its relatively short half-life,53Mn occurs only in tiny amounts due to the action ofcosmic rays oniron in rocks.[4] Manganese isotopic contents are typically combined withchromium isotopic contents and have found application inisotope geology andradiometric dating. Mn−Cr isotopic ratios reinforce the evidence from26Al and107Pd for the early history of theSolar System. Variations in53Cr/52Cr and Mn/Cr ratios from severalmeteorites indicate an initial53Mn/55Mn ratio that suggests Mn−Cr isotopic systematics must result from in-situ decay of53Mn in differentiated planetary bodies. Hence53Mn provides additional evidence fornucleosynthetic processes immediately before coalescence of theSolar System.

The isotopes of manganese range from46Mn to73Mn. The primarydecay mode before the most abundant stable isotope,55Mn, iselectron capture and the primary mode after isbeta decay.

List of isotopes

[edit]


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

[n 4]
Daughter
isotope

[n 5]
Spin and
parity
[n 6][n 7]
Isotopic
abundance
Excitation energy[n 7]
46Mn252145.986669(93)36.2(4) msβ+,p (57.0%)45V(4+)
β+ (25%)46Cr
β+, 2p (18%)44Ti
β+,α?42Ti
47Mn252246.975774(34)88.0(13) msβ+47Cr5/2−#
β+, p? (<1.7%)46V
48Mn252347.9685488(72)158.1(22) msβ+ (99.72%)48Cr4+
β+, p (0.28%)47V
β+, α (6×10−4%)44Ti
49Mn252448.9596134(24)382(7) msβ+49Cr5/2−
50Mn252549.95423816(12)283.21(7) msβ+50Cr0+
50mMn225.31(7) keV1.75(3) minβ+50Cr5+
51Mn252650.94820877(33)45.81(21) minβ+51Cr5/2−
52Mn252751.94555909(14)5.591(3) dβ+52Cr6+
52mMn377.749(5) keV21.1(2) minβ+ (98.22%)52Cr2+
IT (1.78%)52Mn
53Mn252852.94128750(37)3.7(4)×106 yEC53Cr7/2−trace
54Mn252953.9403558(11)312.081(32) dEC54Cr3+
β (9.3×10−5%)54Fe
β+ (1.28×10−7%)54Cr
55Mn253054.93804304(28)Stable5/2−1.0000
56Mn253155.93890282(31)2.5789(1) hβ56Fe3+
57Mn253256.9382859(16)85.4(18) sβ57Fe5/2−
58Mn253357.9400666(29)3.0(1) sβ58Fe1+
58mMn71.77(5) keV65.4(5) sβ58Fe4+
IT?58Mn
59Mn253458.9403911(25)4.59(5) sβ59Fe5/2−
60Mn253559.9431366(25)280(20) msβ60Fe1+
60mMn271.90(10) keV1.77(2) sβ (88.5%)60Fe4+
IT (11.5%)60Mn
61Mn253660.9444525(25)709(8) msβ61Fe5/2−
β,n?60Fe
62Mn253761.9479074(70)92(13) msβ62Fe1+
β, n?61Fe
62mMn[n 8]343(6) keV671(5) msβ62Fe4+
β, n?61Fe
IT?61Mn
63Mn253862.9496647(40)275(4) msβ63Fe5/2−
β, n?62Fe
64Mn253963.9538494(38)88.8(24) msβ (97.3%)64Fe1+
β, n (2.7%)63Fe
64mMn174.1(5) keV439(31) μsIT64Mn(4+)
65Mn254064.9560197(40)91.9(7) msβ (92.1%)65Fe(5/2−)
β, n (7.9%)64Fe
66Mn254165.960547(12)63.8(9) msβ (92.6%)66Fe(1+)
β, n (7.4%)65Fe
β, 2n?64Fe
66mMn464.5(4) keV780(40) μsIT66Mn(5−)
β?66Fe
67Mn254266.96395(22)#46.7(23) msβ (90%)67Fe5/2−#
β, n (10%)66Fe
β, 2n?65Fe
68Mn254367.96895(32)#33.7(15) msβ (82%)68Fe(3)
β, n (18%)67Fe
β, 2n?66Fe
69Mn254468.97278(43)#22.1(16) msβ (60%)69Fe5/2−#
β, n (40%)68Fe
β, 2n?67Fe
70Mn254569.97805(54)#19.9(17) msβ70Fe(4,5)
β, n?69Fe
β, 2n?68Fe
71Mn254670.98216(54)#16# ms
[>400 ns]
β?71Fe5/2-#
β, n?70Fe
β, 2n?69Fe
72Mn254771.98801(64)#12# ms
[>620 ns]
β?72Fe
β, n?71Fe
β, 2n?70Fe
73Mn254872.99281(64)#12# ms
[>410 ns]
β?73Fe5/2−#
This table header & footer:
  1. ^mMn – 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. ^Modes of decay:
    EC:Electron capture


    IT:Isomeric transition
    n:Neutron emission
    p:Proton emission
  5. ^Bold symbol as daughter – Daughter product is stable.
  6. ^( ) spin value – Indicates spin with weak assignment arguments.
  7. ^ab# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  8. ^Order of ground state and isomer is uncertain.

References

[edit]
  1. ^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: Manganese".CIAAW. 2017.
  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. ^J. Schaefer; et al. (2006). "Terrestrial manganese-53 — A new monitor of Earth surface processes".Earth and Planetary Science Letters.251 (3–4):334–345.Bibcode:2006E&PSL.251..334S.doi:10.1016/j.epsl.2006.09.016.
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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