Manganese-56
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Naturally occurring
manganese Manganese is a chemical element; it has Symbol (chemistry), symbol Mn and atomic number 25. It is a hard, brittle, silvery metal, often found in minerals in combination with iron. Manganese was first isolated in the 1770s. It is a transition m ...
(25Mn) is composed of one stable
isotope Isotopes are distinct nuclear species (or ''nuclides'') of the same chemical element. They have the same atomic number (number of protons in their Atomic nucleus, nuclei) and position in the periodic table (and hence belong to the same chemica ...
, 55Mn. Twenty-seven
radioisotope A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess numbers of either neutrons or protons, giving it excess nuclear energy, and making it unstable. This excess energy can be used in one of three ...
s have been characterized, with the most stable being 53Mn with a
half-life Half-life is a mathematical and scientific description of exponential or gradual decay. Half-life, half life or halflife may also refer to: Film * Half-Life (film), ''Half-Life'' (film), a 2008 independent film by Jennifer Phang * ''Half Life: ...
of 3.7 million years, 54Mn with a half-life of 312.3 days, and 52Mn with a half-life of 5.591 days. All of the remaining
radioactive Radioactive decay (also known as nuclear decay, radioactivity, radioactive disintegration, or nuclear disintegration) is the process by which an unstable atomic nucleus loses energy by radiation. A material containing unstable nuclei is conside ...
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 seven
meta state A nuclear isomer is a metastable state of an atomic nucleus, in which one or more nucleons (protons or neutrons) occupy excited state levels (higher energy levels). "Metastable" describes nuclei whose excited states have half-lives of 10−9 s ...
s. Manganese is part of the
iron group In chemistry and physics, the iron group refers to elements that are in some way related to iron; mostly in period (row) 4 of the periodic table. The term has different meanings in different contexts. In chemistry, the term is largely obsolete, ...
of elements, which are thought to be synthesized in large
star A star is a luminous spheroid of plasma (physics), plasma held together by Self-gravitation, self-gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night sk ...
s shortly before
supernova A supernova (: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova occurs during the last stellar evolution, evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion ...
explosions. 53Mn decays to 53 Cr with a
half-life Half-life is a mathematical and scientific description of exponential or gradual decay. Half-life, half life or halflife may also refer to: Film * Half-Life (film), ''Half-Life'' (film), a 2008 independent film by Jennifer Phang * ''Half Life: ...
of 3.7 million years. Because of its relatively short half-life, 53Mn occurs only in tiny amounts due to the action of
cosmic rays Cosmic rays or astroparticles are high-energy particles or clusters of particles (primarily represented by protons or atomic nuclei) that move through space at nearly the speed of light. They originate from the Sun, from outside of the Solar ...
on
iron Iron is a chemical element; it has symbol Fe () and atomic number 26. It is a metal that belongs to the first transition series and group 8 of the periodic table. It is, by mass, the most common element on Earth, forming much of Earth's o ...
in rocks. Manganese isotopic contents are typically combined with
chromium Chromium is a chemical element; it has Symbol (chemistry), symbol Cr and atomic number 24. It is the first element in Group 6 element, group 6. It is a steely-grey, Luster (mineralogy), lustrous, hard, and brittle transition metal. Chromium ...
isotopic contents and have found application in
isotope geology Isotope geochemistry is an aspect of geology based upon the study of natural variations in the relative abundances of isotopes of various elements. Variations in isotopic abundance are measured by isotope-ratio mass spectrometry, and can reveal ...
and
radiometric dating Radiometric dating, radioactive dating or radioisotope dating is a technique which is used to Chronological dating, date materials such as Rock (geology), rocks or carbon, in which trace radioactive impurity, impurities were selectively incorporat ...
. Mn−Cr isotopic ratios reinforce the evidence from 26Al and 107Pd for the early history of the
Solar System The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Sola ...
. Variations in 53Cr/52Cr and Mn/Cr ratios from several
meteorite A meteorite is a rock (geology), rock that originated in outer space and has fallen to the surface of a planet or Natural satellite, moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical ...
s indicate an initial 53Mn/55Mn ratio that suggests Mn−Cr isotopic systematics must result from in-situ decay of 53Mn in differentiated planetary bodies. Hence 53Mn provides additional evidence for
nucleosynthetic Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons (protons and neutrons) and nuclei. According to current theories, the first nuclei were formed a few minutes after the Big Bang, through nuclear reactions ...
processes immediately before coalescence of the
Solar System The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Sola ...
. The isotopes of manganese range from 46Mn to 73Mn. The primary
decay mode Radioactive decay (also known as nuclear decay, radioactivity, radioactive disintegration, or nuclear disintegration) is the process by which an unstable atomic nucleus loses energy by radiation. A material containing unstable nuclei is conside ...
before the most abundant stable isotope, 55Mn, is
electron capture Electron capture (K-electron capture, also K-capture, or L-electron capture, L-capture) is a process in which the proton-rich nucleus of an electrically neutral atom absorbs an inner atomic electron, usually from the K or L electron shells. Th ...
and the primary mode after is
beta decay In nuclear physics, beta decay (β-decay) is a type of radioactive decay in which an atomic nucleus emits a beta particle (fast energetic electron or positron), transforming into an isobar of that nuclide. For example, beta decay of a neutron ...
.


List of isotopes

, -id=Manganese-46 , rowspan=4, 46Mn , rowspan=4 style="text-align:right" , 25 , rowspan=4 style="text-align:right" , 21 , rowspan=4, 45.986669(93) , rowspan=4, 36.2(4) ms , β+, p (57.0%) , 45V , rowspan=4, (4+) , rowspan=4, , - , β+ (25%) , 46Cr , - , β+, 2p (18%) , 44Ti , - , β+, α? , 42Ti , -id=Manganese-47 , rowspan=2, 47Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 22 , rowspan=2, 46.975774(34) , rowspan=2, 88.0(13) ms , β+ , 47Cr , rowspan=2, 5/2−# , rowspan=2, , - , β+, p? (<1.7%) , 46V , -id=Manganese-48 , rowspan=3, 48Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 23 , rowspan=3, 47.9685488(72) , rowspan=3, 158.1(22) ms , β+ (99.72%) , 48Cr , rowspan=3, 4+ , rowspan=3, , - , β+, p (0.28%) , 47V , - , β+, α (6×10−4%) , 44Ti , -id=Manganese-49 , 49Mn , style="text-align:right" , 25 , style="text-align:right" , 24 , 48.9596134(24) , 382(7) ms , β+ , 49Cr , 5/2− , , -id=Manganese-50 , 50Mn , style="text-align:right" , 25 , style="text-align:right" , 25 , 49.95423816(12) , 283.21(7) ms , β+ , 50Cr , 0+ , , -id=Manganese-50m , style="text-indent:1em" , 50mMn , colspan="3" style="text-indent:2em" , 225.31(7) keV , 1.75(3) min , β+ , 50Cr , 5+ , , -id=Manganese-51 , 51Mn , style="text-align:right" , 25 , style="text-align:right" , 26 , 50.94820877(33) , 45.81(21) min , β+ , 51Cr , 5/2− , , -id=Manganese-52 , 52Mn , style="text-align:right" , 25 , style="text-align:right" , 27 , 51.94555909(14) , 5.591(3) d , β+ , 52Cr , 6+ , , -id=Manganese-52m , rowspan=2 style="text-indent:1em" , 52mMn , rowspan=2 colspan="3" style="text-indent:2em" , 377.749(5) keV , rowspan=2, 21.1(2) min , β+ (98.22%) , 52Cr , rowspan=2, 2+ , rowspan=2, , - , IT (1.78%) , 52Mn , -id=Manganese-53 , 53Mn , style="text-align:right" , 25 , style="text-align:right" , 28 , 52.94128750(37) , 3.7(4)×106 y , EC , 53Cr , 7/2− ,
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, -id=Manganese-54 , rowspan=3, 54Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 29 , rowspan=3, 53.9403558(11) , rowspan=3, 312.081(32) d , EC , 54Cr , rowspan=3, 3+ , rowspan=3, , - , β (9.3×10−5%) , 54Fe , - , β+ (1.28×10−7%) , 54Cr , -id=Manganese-55 , 55Mn , style="text-align:right" , 25 , style="text-align:right" , 30 , 54.93804304(28) , colspan=3 align=center, Stable , 5/2− , 1.0000 , -id=Manganese-56 , 56Mn , style="text-align:right" , 25 , style="text-align:right" , 31 , 55.93890282(31) , 2.5789(1) h , β , 56Fe , 3+ , , -id=Manganese-57 , 57Mn , style="text-align:right" , 25 , style="text-align:right" , 32 , 56.9382859(16) , 85.4(18) s , β , 57Fe , 5/2− , , -id=Manganese-58 , 58Mn , style="text-align:right" , 25 , style="text-align:right" , 33 , 57.9400666(29) , 3.0(1) s , β , 58Fe , 1+ , , -id=Manganese-58m , rowspan=2 style="text-indent:1em" , 58mMn , rowspan=2 colspan="3" style="text-indent:2em" , 71.77(5) keV , rowspan=2, 65.4(5) s , β , 58Fe , rowspan=2, 4+ , rowspan=2, , - , IT? , 58Mn , -id=Manganese-59 , 59Mn , style="text-align:right" , 25 , style="text-align:right" , 34 , 58.9403911(25) , 4.59(5) s , β , 59Fe , 5/2− , , -id=Manganese-60 , 60Mn , style="text-align:right" , 25 , style="text-align:right" , 35 , 59.9431366(25) , 280(20) ms , β , 60Fe , 1+ , , -id=Manganese-60m , rowspan=2 style="text-indent:1em" , 60mMn , rowspan=2 colspan="3" style="text-indent:2em" , 271.90(10) keV , rowspan=2, 1.77(2) s , β (88.5%) , 60Fe , rowspan=2, 4+ , rowspan=2, , - , IT (11.5%) , 60Mn , -id=Manganese-61 , rowspan=2, 61Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 36 , rowspan=2, 60.9444525(25) , rowspan=2, 709(8) ms , β , 61Fe , rowspan=2, 5/2− , rowspan=2, , - , β, n? , 60Fe , -id=Manganese-62 , rowspan=2, 62Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 37 , rowspan=2, 61.9479074(70) , rowspan=2, 92(13) ms , β , 62Fe , rowspan=2, 1+ , rowspan=2, , - , β, n? , 61Fe , -id=Manganese-62m , rowspan=3 style="text-indent:1em" , 62mMnOrder of ground state and isomer is uncertain. , rowspan=3 colspan="3" style="text-indent:2em" , 343(6) keV , rowspan=3, 671(5) ms , β , 62Fe , rowspan=3, 4+ , rowspan=3, , - , β, n? , 61Fe , - , IT? , 62Mn , -id=Manganese-63 , rowspan=2, 63Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 38 , rowspan=2, 62.9496647(40) , rowspan=2, 275(4) ms , β , 63Fe , rowspan=2, 5/2− , rowspan=2, , - , β, n? , 62Fe , -id=Manganese-64 , rowspan=2, 64Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 39 , rowspan=2, 63.9538494(38) , rowspan=2, 88.8(24) ms , β (97.3%) , 64Fe , rowspan=2, 1+ , rowspan=2, , - , β, n (2.7%) , 63Fe , -id=Manganese-64m , style="text-indent:1em" , 64mMn , colspan="3" style="text-indent:2em" , 174.1(5) keV , 439(31) μs , IT , 64Mn , (4+) , , -id=Manganese-65 , rowspan=2, 65Mn , rowspan=2 style="text-align:right" , 25 , rowspan=2 style="text-align:right" , 40 , rowspan=2, 64.9560197(40) , rowspan=2, 91.9(7) ms , β (92.1%) , 65Fe , rowspan=2, (5/2−) , rowspan=2, , - , β, n (7.9%) , 64Fe , -id=Manganese-66 , rowspan=3, 66Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 41 , rowspan=3, 65.960547(12) , rowspan=3, 63.8(9) ms , β (92.6%) , 66Fe , rowspan=3, (1+) , rowspan=3, , - , β, n (7.4%) , 65Fe , - , β, 2n? , 64Fe , -id=Manganese-66m , rowspan=2 style="text-indent:1em" , 66mMn , rowspan=2 colspan="3" style="text-indent:2em" , 464.5(4) keV , rowspan=2, 780(40) μs , IT , 66Mn , rowspan=2, (5−) , rowspan=2, , - , β? , 66Fe , -id=Manganese-67 , rowspan=3, 67Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 42 , rowspan=3, 66.96395(22)# , rowspan=3, 46.7(23) ms , β (90%) , 67Fe , rowspan=3, 5/2−# , rowspan=3, , - , β, n (10%) , 66Fe , - , β, 2n? , 65Fe , -id=Manganese-68 , rowspan=3, 68Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 43 , rowspan=3, 67.96895(32)# , rowspan=3, 33.7(15) ms , β (82%) , 68Fe , rowspan=3, (3) , rowspan=3, , - , β, n (18%) , 67Fe , - , β, 2n? , 66Fe , -id=Manganese-69 , rowspan=3, 69Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 44 , rowspan=3, 68.97278(43)# , rowspan=3, 22.1(16) ms , β (60%) , 69Fe , rowspan=3, 5/2−# , rowspan=3, , - , β, n (40%) , 68Fe , - , β, 2n? , 67Fe , -id=Manganese-70 , rowspan=3, 70Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 45 , rowspan=3, 69.97805(54)# , rowspan=3, 19.9(17) ms , β , 70Fe , rowspan=3, (4,5) , rowspan=3, , - , β, n? , 69Fe , - , β, 2n? , 68Fe , -id=Manganese-71 , rowspan=3, 71Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 46 , rowspan=3, 70.98216(54)# , rowspan=3, 16# ms
400 ns, β? , 71Fe , rowspan=3, 5/2-# , rowspan=3, , - , β, n? , 70Fe , - , β, 2n? , 69Fe , -id=Manganese-72 , rowspan=3, 72Mn , rowspan=3 style="text-align:right" , 25 , rowspan=3 style="text-align:right" , 47 , rowspan=3, 71.98801(64)# , rowspan=3, 12# ms
620 ns, β? , 72Fe , rowspan=3, , rowspan=3, , - , β, n? , 71Fe , - , β, 2n? , 70Fe , -id=Manganese-73 , 73Mn , style="text-align:right" , 25 , style="text-align:right" , 48 , 72.99281(64)# , 12# ms
410 ns, β? , 73Fe , 5/2−# ,


See also

Daughter products other than manganese *
Isotopes of iron Natural iron (Fe) consists of four stable isotopes: 5.845% Fe (possibly radioactive with half-life > years), 91.754% Fe, 2.119% Fe and 0.286% Fe. There are 28 known radioisotopes and 8 nuclear isomers, the most stable of which are Fe (half-life 2 ...
* Isotopes of chromium * Isotopes of vanadium *
Isotopes of titanium Naturally occurring titanium (22Ti) is composed of five stable isotopes; 46Ti, 47Ti, 48Ti, 49Ti and 50Ti with 48Ti being the most abundant (73.8% natural abundance). Twenty-one radioisotopes have been characterized, with the most stable being 44T ...


References

* Isotope masses from: ** * Half-life, spin, and isomer data selected from the following sources. ** ** ** {{Navbox element isotopes Manganese
Manganese Manganese is a chemical element; it has Symbol (chemistry), symbol Mn and atomic number 25. It is a hard, brittle, silvery metal, often found in minerals in combination with iron. Manganese was first isolated in the 1770s. It is a transition m ...