| ||||||||||||||||||||||||||||||
Standard atomic weight Ar°(K) | ||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Potassium (
19K) has 25 known isotopes from 34
K to 57
K as well as 31
K, as well as an unconfirmed report of 59
K. [3] Three of those isotopes occur naturally: the two stable forms 39
K (93.3%) and 41
K (6.7%), and a very long-lived radioisotope 40
K (0.012%)
Naturally occurring radioactive 40
K decays with a half-life of 1.248×109 years. 89% of those decays are to stable 40
Ca by beta decay, whilst 11% are to 40
Ar by either electron capture or positron emission. This latter decay branch has produced an isotopic abundance of argon on Earth which differs greatly from that seen in gas giants and stellar spectra. 40
K has the longest known half-life for any positron-emitter nuclide. The long half-life of this primordial radioisotope is caused by a highly spin-forbidden transition: 40
K has a nuclear spin of 4, while both of its decay daughters are even–even isotopes with spins of 0.
40
K occurs in natural potassium in sufficient quantity that large bags of potassium chloride commercial salt substitutes can be used as a radioactive source for classroom demonstrations.[ citation needed ]40
K is the largest source of natural radioactivity in healthy animals and humans, greater even than 14
C. In a human body of 70 kg mass, about 4,400 nuclei of 40
K decay per second. [4]
The decay of 40
K to 40
Ar is used in potassium-argon dating of rocks. Minerals are dated by measurement of the concentration of potassium and the amount of radiogenic 40
Ar that has accumulated. Typically, the method assumes that the rocks contained no argon at the time of formation and all subsequent radiogenic argon (i.e., 40
Ar) was retained.[ citation needed ]40
K has also been extensively used as a radioactive tracer in studies of weathering.[ citation needed ]
All other potassium isotopes have half-lives under a day, most under a minute. The least stable is 31
K, a three-proton emitter discovered in 2019; its half-life was measured to be shorter than 10 picoseconds. [5] [6]
Stable potassium isotopes have been used for several nutrient cycling studies since potassium is a macronutrient required for life. [7]
Nuclide [n 1] | Z | N | Isotopic mass (Da) [8] [n 2] [n 3] | Half-life [9] [n 4] | Decay mode [9] | Daughter isotope [n 5] | Spin and parity [9] [n 6] [n 4] | Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy [n 4] | Normal proportion [9] | Range of variation | |||||||||||||||||
31 K [5] [6] | 19 | 12 | 31.03678(32)# | <10 ps | 3p | 28S | 3/2+# | ||||||||||||
34K [10] | 19 | 15 | 33.998404(18) | p | 33Ar | ||||||||||||||
35K | 19 | 16 | 34.98800541(55) | 175.2(19) ms | β+ (99.63%) | 35Ar | 3/2+ | ||||||||||||
β+, p (0.37%) | 34Cl | ||||||||||||||||||
36K | 19 | 17 | 35.98130189(35) | 341(3) ms | β+ (99.95%) | 36Ar | 2+ | ||||||||||||
β+, p (0.048%) | 35Cl | ||||||||||||||||||
β+, α (0.0034%) | 32S | ||||||||||||||||||
37K | 19 | 18 | 36.97337589(10) | 1.23651(94) s | β+ | 37Ar | 3/2+ | ||||||||||||
38K | 19 | 19 | 37.96908111(21) | 7.651(19) min | β+ | 38Ar | 3+ | ||||||||||||
38m1K | 130.15(4) keV | 924.35(12) ms | β+ (99.97%) | 38Ar | 0+ | ||||||||||||||
IT (0.0330%) | 38K | ||||||||||||||||||
38m2K | 3458.10(17) keV | 21.95(11) μs | IT | 38K | (7)+ | ||||||||||||||
39K | 19 | 20 | 38.9637064848(49) | Stable | 3/2+ | 0.932581(44) | |||||||||||||
40K [n 7] [n 8] | 19 | 21 | 39.963998165(60) | 1.248(3)×109 y | β− (89.28%) | 40Ca | 4− | 1.17(1)×10−4 | |||||||||||
EC (10.72%) | 40Ar | ||||||||||||||||||
β+ (0.001%) [11] | |||||||||||||||||||
40mK | 1643.638(11) keV | 336(12) ns | IT | 40K | 0+ | ||||||||||||||
41K | 19 | 22 | 40.9618252561(40) | Stable | 3/2+ | 0.067302(44) | |||||||||||||
42K | 19 | 23 | 41.96240231(11) | 12.355(7) h | β− | 42Ca | 2− | Trace [n 9] | |||||||||||
43K | 19 | 24 | 42.96073470(44) | 22.3(1) h | β− | 43Ca | 3/2+ | ||||||||||||
43mK | 738.30(6) keV | 200(5) ns | IT | 43K | 7/2− | ||||||||||||||
44K | 19 | 25 | 43.96158698(45) | 22.13(19) min | β− | 44Ca | 2− | ||||||||||||
45K | 19 | 26 | 44.96069149(56) | 17.8(6) min | β− | 45Ca | 3/2+ | ||||||||||||
46K | 19 | 27 | 45.96198158(78) | 96.30(8) s | β− | 46Ca | 2− | ||||||||||||
47K | 19 | 28 | 46.9616616(15) | 17.38(3) s | β− | 47Ca | 1/2+ | ||||||||||||
48K | 19 | 29 | 47.96534118(83) | 6.83(14) s | β− (98.86%) | 48Ca | 1− | ||||||||||||
β−, n (1.14%) | 47Ca | ||||||||||||||||||
49K | 19 | 30 | 48.96821075(86) | 1.26(5) s | β−, n (86%) | 48Ca | 1/2+ | ||||||||||||
β− (14%) | 49Ca | ||||||||||||||||||
50K | 19 | 31 | 49.9723800(83) | 472(4) ms | β− (71.4%) | 50Ca | 0− | ||||||||||||
β−, n (28.6%) | 49Ca | ||||||||||||||||||
β−, 2n? | 48Ca | ||||||||||||||||||
50mK | 172.0(4) keV | 125(40) ns | IT | 50K | (2−) | ||||||||||||||
51K | 19 | 32 | 50.975828(14) | 365(5) ms | β−, n (65%) | 50Ca | 3/2+ | ||||||||||||
β− (35%) | 51Ca | ||||||||||||||||||
β−, 2n? | 49Ca | ||||||||||||||||||
52K | 19 | 33 | 51.981602(36) | 110(4) ms | β−, n (72.2%) | 51Ca | 2−# | ||||||||||||
β− (25.5%) | 52Ca | ||||||||||||||||||
β−, 2n (2.3%) | 50Ca | ||||||||||||||||||
53K | 19 | 34 | 52.98680(12) | 30(5) ms | β−, n (64%) | 52Ca | 3/2+ | ||||||||||||
β− (26%) | 53Ca | ||||||||||||||||||
β−, 2n (10%) | 51Ca | ||||||||||||||||||
54K | 19 | 35 | 53.99447(43)# | 10(5) ms | β− | 54Ca | 2−# | ||||||||||||
β−, n? | 53Ca | ||||||||||||||||||
β−, 2n? | 52Ca | ||||||||||||||||||
55K | 19 | 36 | 55.00051(54)# | 10# ms [>620 ns] | β−? | 55Ca | 3/2+# | ||||||||||||
β−, n? | 54Ca | ||||||||||||||||||
β−, 2n? | 54Ca | ||||||||||||||||||
56K | 19 | 37 | 56.00857(64)# | 5# ms [>620 ns] | β−? | 56Ca | 2−# | ||||||||||||
β−, n? | 55Ca | ||||||||||||||||||
β−, 2n? | 54Ca | ||||||||||||||||||
57K | 19 | 38 | 57.01517(64)# | 2# ms [>400 ns] | β−? | 57Ca | 3/2+# | ||||||||||||
β−, n? | 56Ca | ||||||||||||||||||
β−, 2n? | 55Ca | ||||||||||||||||||
59K [3] [n 10] | 19 | 40 | 59.03086(86)# | 1# ms [>400 ns] | β−? | 59Ca | 3/2+# | ||||||||||||
β−, n? | 58Ca | ||||||||||||||||||
β−, 2n? | 57Ca | ||||||||||||||||||
This table header & footer: |
Fluorine (9F) has 19 known isotopes ranging from 13
F
to 31
F
and two isomers. Only fluorine-19 is stable and naturally occurring in more than trace quantities; therefore, fluorine is a monoisotopic and mononuclidic element.
Lead (82Pb) has four observationally stable isotopes: 204Pb, 206Pb, 207Pb, 208Pb. Lead-204 is entirely a primordial nuclide and is not a radiogenic nuclide. The three isotopes lead-206, lead-207, and lead-208 represent the ends of three decay chains: the uranium series, the actinium series, and the thorium series, respectively; a fourth decay chain, the neptunium series, terminates with the thallium isotope 205Tl. The three series terminating in lead represent the decay chain products of long-lived primordial 238U, 235U, and 232Th. Each isotope also occurs, to some extent, as primordial isotopes that were made in supernovae, rather than radiogenically as daughter products. The fixed ratio of lead-204 to the primordial amounts of the other lead isotopes may be used as the baseline to estimate the extra amounts of radiogenic lead present in rocks as a result of decay from uranium and thorium.
Bismuth (83Bi) has 41 known isotopes, ranging from 184Bi to 224Bi. Bismuth has no stable isotopes, but does have one very long-lived isotope; thus, the standard atomic weight can be given as 208.98040(1). Although bismuth-209 is now known to be radioactive, it has classically been considered to be a stable isotope because it has a half-life of approximately 2.01×1019 years, which is more than a billion times the age of the universe. Besides 209Bi, the most stable bismuth radioisotopes are 210mBi with a half-life of 3.04 million years, 208Bi with a half-life of 368,000 years and 207Bi, with a half-life of 32.9 years, none of which occurs in nature. All other isotopes have half-lives under 1 year, most under a day. Of naturally occurring radioisotopes, the most stable is radiogenic 210Bi with a half-life of 5.012 days. 210mBi is unusual for being a nuclear isomer with a half-life multiple orders of magnitude longer than that of the ground state.
There are seven stable isotopes of mercury (80Hg) with 202Hg being the most abundant (29.86%). The longest-lived radioisotopes are 194Hg with a half-life of 444 years, and 203Hg with a half-life of 46.612 days. Most of the remaining 40 radioisotopes have half-lives that are less than a day. 199Hg and 201Hg are the most often studied NMR-active nuclei, having spin quantum numbers of 1/2 and 3/2 respectively. All isotopes of mercury are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed. These isotopes are predicted to undergo either alpha decay or double beta decay.
There are two natural isotopes of iridium (77Ir), and 37 radioisotopes, the most stable radioisotope being 192Ir with a half-life of 73.83 days, and many nuclear isomers, the most stable of which is 192m2Ir with a half-life of 241 years. All other isomers have half-lives under a year, most under a day. All isotopes of iridium are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.
Natural tantalum (73Ta) consists of two stable isotopes: 181Ta (99.988%) and 180m
Ta
(0.012%).
Naturally occurring xenon (54Xe) consists of seven stable isotopes and two very long-lived isotopes. Double electron capture has been observed in 124Xe and double beta decay in 136Xe, which are among the longest measured half-lives of all nuclides. The isotopes 126Xe and 134Xe are also predicted to undergo double beta decay, but this process has never been observed in these isotopes, so they are considered to be stable. Beyond these stable forms, 32 artificial unstable isotopes and various isomers have been studied, the longest-lived of which is 127Xe with a half-life of 36.345 days. All other isotopes have half-lives less than 12 days, most less than 20 hours. The shortest-lived isotope, 108Xe, has a half-life of 58 μs, and is the heaviest known nuclide with equal numbers of protons and neutrons. Of known isomers, the longest-lived is 131mXe with a half-life of 11.934 days. 129Xe is produced by beta decay of 129I ; 131mXe, 133Xe, 133mXe, and 135Xe are some of the fission products of both 235U and 239Pu, so are used as indicators of nuclear explosions.
There are 39 known isotopes and 17 nuclear isomers of tellurium (52Te), with atomic masses that range from 104 to 142. These are listed in the table below.
The alkaline earth metal strontium (38Sr) has four stable, naturally occurring isotopes: 84Sr (0.56%), 86Sr (9.86%), 87Sr (7.0%) and 88Sr (82.58%). Its standard atomic weight is 87.62(1).
There are 34 known isotopes of krypton (36Kr) with atomic mass numbers from 69 through 102. Naturally occurring krypton is made of five stable isotopes and one which is slightly radioactive with an extremely long half-life, plus traces of radioisotopes that are produced by cosmic rays in the atmosphere.
Bromine (35Br) has two stable isotopes, 79Br and 81Br, and 35 known radioisotopes, the most stable of which is 77Br, with a half-life of 57.036 hours.
Germanium (32Ge) has five naturally occurring isotopes, 70Ge, 72Ge, 73Ge, 74Ge, and 76Ge. Of these, 76Ge is very slightly radioactive, decaying by double beta decay with a half-life of 1.78 × 1021 years (130 billion times the age of the universe).
Naturally occurring chromium (24Cr) is composed of four stable isotopes; 50Cr, 52Cr, 53Cr, and 54Cr with 52Cr being the most abundant (83.789% natural abundance). 50Cr is suspected of decaying by β+β+ to 50Ti with a half-life of (more than) 1.8×1017 years. Twenty-two radioisotopes, all of which are entirely synthetic, have been characterized, the most stable being 51Cr with a half-life of 27.7 days. All of the remaining radioactive isotopes have half-lives that are less than 24 hours and the majority of these have half-lives that are less than 1 minute. This element also has two meta states, 45mCr, the more stable one, and 59mCr, the least stable isotope or isomer.
Naturally occurring vanadium (23V) is composed of one stable isotope 51V and one radioactive isotope 50V with a half-life of 2.71×1017 years. 24 artificial radioisotopes have been characterized (in the range of mass number between 40 and 65) with the most stable being 49V with a half-life of 330 days, and 48V with a half-life of 15.9735 days. All of the remaining radioactive isotopes have half-lives shorter than an hour, the majority of them below 10 seconds, the least stable being 42V with a half-life shorter than 55 nanoseconds, with all of the isotopes lighter than it, and none of the heavier, have unknown half-lives. In 4 isotopes, metastable excited states were found (including 2 metastable states for 60V), which adds up to 5 meta states.
Calcium (20Ca) has 26 known isotopes, ranging from 35Ca to 60Ca. There are five stable isotopes, plus one isotope (48Ca) with such a long half-life that it is for all practical purposes 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, 41Ca, with half-life 99,400 years. Unlike cosmogenic isotopes that are produced in the air, 41Ca is produced by neutron activation of 40Ca. Most of its production is in the upper metre of the soil column, where the cosmogenic neutron flux is still strong enough. 41Ca has received much attention in stellar studies because it decays to 41K, a critical indicator of solar system anomalies. The most stable artificial isotopes are 45Ca with half-life 163 days and 47Ca with half-life 4.5 days. All other calcium isotopes have half-lives of minutes or less.
Argon (18Ar) has 26 known isotopes, from 29Ar to 54Ar, of which three are stable. On the Earth, 40Ar makes up 99.6% of natural argon. The longest-lived radioactive isotopes are 39Ar with a half-life of 268 years, 42Ar with a half-life of 32.9 years, and 37Ar with a half-life of 35.04 days. All other isotopes have half-lives of less than two hours, and most less than one minute.
Chlorine (17Cl) has 25 isotopes, ranging from 28Cl to 52Cl, and two isomers, 34mCl and 38mCl. There are two stable isotopes, 35Cl (75.8%) and 37Cl (24.2%), giving chlorine a standard atomic weight of 35.45. The longest-lived radioactive isotope is 36Cl, which has a half-life of 301,000 years. All other isotopes have half-lives under 1 hour, many less than one second. The shortest-lived are proton-unbound 29Cl and 30Cl, with half-lives less than 10 picoseconds and 30 nanoseconds, respectively; the half-life of 28Cl is unknown.
Aluminium or aluminum (13Al) has 23 known isotopes from 21Al to 43Al and 4 known isomers. Only 27Al (stable isotope) and 26Al (radioactive isotope, t1/2 = 7.2×105 y) occur naturally, however 27Al comprises nearly all natural aluminium. Other than 26Al, all radioisotopes have half-lives under 7 minutes, most under a second. The standard atomic weight is 26.9815385(7). 26Al is produced from argon in the atmosphere by spallation caused by cosmic-ray protons. Aluminium isotopes have found practical application in dating marine sediments, manganese nodules, glacial ice, quartz in rock exposures, and meteorites. The ratio of 26Al to 10Be has been used to study the role of sediment transport, deposition, and storage, as well as burial times, and erosion, on 105 to 106 year time scales. 26Al has also played a significant role in the study of meteorites.
There are 20 isotopes of sodium (11Na), ranging from 17
Na to 39
Na, and two isomers. 23
Na is the only stable isotope. It is considered a monoisotopic element and it has a standard atomic weight of 22.98976928(2). Sodium has two radioactive cosmogenic isotopes. With the exception of those two isotopes, all other isotopes have half-lives under a minute, most under a second. The shortest-lived is the unbound 18
Na, with a half-life of 1.3(4)×10−21 seconds.
Potassium-40 (40K) is a radioactive isotope of potassium which has a long half-life of 1.25 billion years. It makes up about 0.012% of the total amount of potassium found in nature.