Calcium Isotopes
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Calcium Calcium is a chemical element with the symbol Ca and atomic number 20. As an alkaline earth metal, calcium is a reactive metal that forms a dark oxide-nitride layer when exposed to air. Its physical and chemical properties are most similar to ...
(20Ca) has 26 known isotopes, ranging from 35Ca to 60Ca. There are five stable isotopes (40Ca, 42Ca, 43Ca, 44Ca and 46Ca), plus one isotope ( 48Ca) with such a long
half-life Half-life (symbol ) is the time required for a quantity (of substance) to reduce to half of its initial value. The term is commonly used in nuclear physics to describe how quickly unstable atoms undergo radioactive decay or how long stable ato ...
that for all practical purposes it can be considered stable. The most abundant isotope, 40Ca, as well as the rare 46Ca, are theoretically unstable on energetic grounds, but their decay has not been observed. Calcium also has a
cosmogenic isotope Cosmogenic nuclides (or cosmogenic isotopes) are rare nuclides (isotopes) created when a high-energy cosmic ray interacts with the nucleus of an ''in situ'' Solar System atom, causing nucleons (protons and neutrons) to be expelled from the atom ...
,
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 consid ...
41Ca, which has a
half-life Half-life (symbol ) is the time required for a quantity (of substance) to reduce to half of its initial value. The term is commonly used in nuclear physics to describe how quickly unstable atoms undergo radioactive decay or how long stable ato ...
of 99,400 years. Unlike
cosmogenic isotope Cosmogenic nuclides (or cosmogenic isotopes) are rare nuclides (isotopes) created when a high-energy cosmic ray interacts with the nucleus of an ''in situ'' Solar System atom, causing nucleons (protons and neutrons) to be expelled from the atom ...
s that are produced in the
atmosphere An atmosphere () is a layer of gas or layers of gases that envelop a planet, and is held in place by the gravity of the planetary body. A planet retains an atmosphere when the gravity is great and the temperature of the atmosphere is low. A s ...
, 41Ca is produced by
neutron activation Neutron activation is the process in which neutron radiation induces radioactivity in materials, and occurs when atomic nuclei capture free neutrons, becoming heavier and entering excited states. The excited nucleus decays immediately by emittin ...
of 40Ca. Most of its production is in the upper metre of the soil column, where the cosmogenic neutron flux is still sufficiently strong. 41Ca has received much attention in stellar studies because it decays to 41K, a critical indicator of solar system anomalies. The most stable artificial radioisotopes are 45Ca with a half-life of 163 days and 47Ca with a half-life of 4.5 days. All other calcium isotopes have half-lives measured in minutes or less. 40Ca comprises about 97% of naturally occurring calcium. 40Ca is also one of the daughter products of 40K decay, along with 40Ar. While K–Ar dating has been used extensively in the geological sciences, the prevalence of 40Ca in nature has impeded its use in dating. Techniques using
mass spectrometry Mass spectrometry (MS) is an analytical technique that is used to measure the mass-to-charge ratio of ions. The results are presented as a ''mass spectrum'', a plot of intensity as a function of the mass-to-charge ratio. Mass spectrometry is use ...
and a double spike isotope dilution have been used for K–Ca age dating.


List of isotopes

, - , rowspan=2, 35Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 15 , rowspan=2, 35.00514(21)# , rowspan=2, 25.7(2) ms , β+, p (95.9%) , 34Ar , rowspan=2, 1/2+# , rowspan=2, , rowspan=2, , - , β+, 2p (4.1%) , 33Cl , - , rowspan=2, 36Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 16 , rowspan=2, 35.99307(4) , rowspan=2, 101.2(15) ms , β+, p (51.2%) , 35Ar , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β+ (48.8%) , 36K , - , rowspan=2, 37Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 17 , rowspan=2, 36.9858979(7) , rowspan=2, 181.1(10) ms , β+, p (82.1%) , 36Ar , rowspan=2, 3/2+# , rowspan=2, , rowspan=2, , - , β+ (17.9%) , 37K , - , 38Ca , style="text-align:right" , 20 , style="text-align:right" , 18 , 37.97631923(21) , 443.70(25) ms , β+ , 38K , 0+ , , , - , 39Ca , style="text-align:right" , 20 , style="text-align:right" , 19 , 38.9707108(6) , 860.3(8) ms , β+ , 39K , 3/2+ , , , - , 40CaHeaviest nuclide with equal numbers of protons and neutrons with no observed decay , style="text-align:right" , 20 , style="text-align:right" , 20 , 39.962590866(22) , colspan=3 align=center, Observationally StableBelieved to undergo
double electron capture Double electron capture is a decay mode of an atomic nucleus. For a nuclide (''A'', ''Z'') with a number of nucleons ''A'' and atomic number ''Z'', double electron capture is only possible if the mass of the nuclide (''A'', ''Z''−2) is lower. I ...
to 40Ar with a half-life no less than 5.9×1021 y
, 0+ , 0.96941(156) , 0.96933–0.96947 , - , 41Ca , style="text-align:right" , 20 , style="text-align:right" , 21 , 40.96227792(15) , 9.94(15)×104 y , EC , 41K , 7/2− , Trace Cosmogenic nuclide , , - , 42Ca , style="text-align:right" , 20 , style="text-align:right" , 22 , 41.95861783(16) , colspan=3 align=center, Stable , 0+ , 0.00647(23) , 0.00646–0.00648 , - , 43Ca , style="text-align:right" , 20 , style="text-align:right" , 23 , 42.95876643(24) , colspan=3 align=center, Stable , 7/2− , 0.00135(10) , 0.00135–0.00135 , - , 44Ca , style="text-align:right" , 20 , style="text-align:right" , 24 , 43.9554815(3) , colspan=3 align=center, Stable , 0+ , 0.02086(110) , 0.02082–0.02092 , - , 45Ca , style="text-align:right" , 20 , style="text-align:right" , 25 , 44.9561863(4) , 162.61(9) d , β , 45Sc , 7/2− , , , - , 46Ca , style="text-align:right" , 20 , style="text-align:right" , 26 , 45.9536880(24) , colspan=3 align=center, Observationally StableBelieved to undergo ββ decay to 46Ti with a half-life no less than 2.8×1015 y , 0+ , 4(3)×10−5 , 4×10−5–4×10−5 , - , 47Ca , style="text-align:right" , 20 , style="text-align:right" , 27 , 46.9545414(24) , 4.536(3) d , β , 47Sc , 7/2− , , , - , 48Ca Primordial
radionuclide A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess nuclear energy, making it unstable. This excess energy can be used in one of three ways: emitted from the nucleus as gamma radiation; transfer ...
, style="text-align:right" , 20 , style="text-align:right" , 28 , 47.95252290(10) , (6.4)×1019 y, , ββLightest nuclide known to undergo double beta decay , 48Ti , 0+ , 0.00187(21) , 0.00186–0.00188 , - , 49Ca , style="text-align:right" , 20 , style="text-align:right" , 29 , 48.95562288(22) , 8.718(6) min , β , 49Sc , 3/2− , , , - , 50Ca , style="text-align:right" , 20 , style="text-align:right" , 30 , 49.9574992(17) , 13.9(6) s , β , 50Sc , 0+ , , , - , 51Ca , style="text-align:right" , 20 , style="text-align:right" , 31 , 50.9609957(6) , 10.0(8) s , β , 51Sc , (3/2−) , , , - , rowspan=2, 52Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 32 , rowspan=2, 51.9632136(7) , rowspan=2, 4.6(3) s , β (98%) , 52Sc , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β, n (2%) , 51Sc , - , rowspan=2, 53Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 33 , rowspan=2, 52.96845(5) , rowspan=2, 461(90) ms , β (60%) , 53Sc , rowspan=2, 3/2−# , rowspan=2, , rowspan=2, , - , β, n (40%) , 52Sc , - , rowspan=2, 54Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 34 , rowspan=2, 53.97299(5) , rowspan=2, 90(6) ms , β (93%) , 54Sc , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β, n (7%) , 53Sc , - , 55Ca , style="text-align:right" , 20 , style="text-align:right" , 35 , 54.98030(32)# , 22(2) ms , β , 55Sc , 5/2−# , , , - , 56Ca , style="text-align:right" , 20 , style="text-align:right" , 36 , 55.98508(43)# , 11(2) ms , β , 56Sc , 0+ , , , - , rowspan=2, 57Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 37 , rowspan=2, 56.99262(43)# , rowspan=2, 5# ms , β , 57Sc , rowspan=2, 5/2−# , rowspan=2, , rowspan=2, , - , β, n , 56Sc , - , rowspan=2, 58Ca , rowspan=2 style="text-align:right" , 20 , rowspan=2 style="text-align:right" , 38 , rowspan=2, 57.99794(54)# , rowspan=2, 3# ms , β , 58Sc , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β, n , 57Sc , - , 59Ca , style="text-align:right" , 20 , style="text-align:right" , 39 , , , β , 59Sc , , , , - , 60Ca , style="text-align:right" , 20 , style="text-align:right" , 40 , , , β , 60Sc , 0+ , ,


References


Further reading

* C. Michael Hogan. 2010
''Calcium''. ed. A. Jorgenson and C. Cleveland. ''Encyclopedia of Earth'', National Council for Science and the Environment, Washington, D.C.


External links


National Isotope Development Center Official website
{{Authority control Calcium
Calcium Calcium is a chemical element with the symbol Ca and atomic number 20. As an alkaline earth metal, calcium is a reactive metal that forms a dark oxide-nitride layer when exposed to air. Its physical and chemical properties are most similar to ...