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Standard atomic weight Ar°(Cl) | ||||||||||||||||||||||||||||
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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.
Nuclide [n 1] | Z | N | Isotopic mass (Da) [4] [n 2] [n 3] | Half-life [1] [n 4] | Decay mode [1] [n 5] | Daughter isotope [n 6] | Spin and parity [1] [n 7] [n 4] | Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy | Normal proportion [1] | Range of variation | |||||||||||||||||
28Cl [5] | 17 | 11 | 28.03035(54)# | p | 27S | 1+# | |||||||||||||
29Cl | 17 | 12 | 29.01505(20)# | 5.4(19) zs | p | 28S | (1/2+) | ||||||||||||
30Cl | 17 | 13 | 30.005018(26) | <50 ns [5] | p | 29S | 3+# | ||||||||||||
31Cl | 17 | 14 | 30.9924481(37) | 190(1) ms | β+ (97.6%) | 31S | 3/2+ | ||||||||||||
β+, p (2.4%) | 30P | ||||||||||||||||||
32Cl | 17 | 15 | 31.98568461(60) | 298(1) ms | β+ (99.92%) | 32S | 1+ | ||||||||||||
β+, α (0.054%) | 28Si | ||||||||||||||||||
β+, p (0.026%) | 31P | ||||||||||||||||||
33Cl | 17 | 16 | 32.97745199(42) | 2.5038(22) s | β+ | 33S | 3/2+ | ||||||||||||
34Cl | 17 | 17 | 33.973762490(52) | 1.5267(4) s | β+ | 34S | 0+ | ||||||||||||
34mCl | 146.360(27) keV | 31.99(3) min | β+ (55.4%) | 34S | 3+ | ||||||||||||||
IT (44.6%) | 34Cl | ||||||||||||||||||
35Cl | 17 | 18 | 34.968852694(38) | Stable | 3/2+ | 0.758(2) | |||||||||||||
36Cl [n 8] | 17 | 19 | 35.968306822(38) | 3.013(15)×105 y | β− (98.1%) | 36Ar | 2+ | 7×10−13 [6] [7] [n 9] | |||||||||||
β+ (1.9%) | 36S | ||||||||||||||||||
37Cl | 17 | 20 | 36.965902573(55) | Stable | 3/2+ | 0.242(2) | |||||||||||||
38Cl | 17 | 21 | 37.96801041(11) | 37.230(14) min | β− | 38Ar | 2− | ||||||||||||
38mCl | 671.365(8) keV | 715(3) ms | IT | 38Cl | 5− | ||||||||||||||
39Cl | 17 | 22 | 38.9680082(19) | 56.2(6) min | β− | 39Ar | 3/2+ | ||||||||||||
40Cl | 17 | 23 | 39.970415(34) | 1.35(3) min | β− | 40Ar | 2− | ||||||||||||
41Cl | 17 | 24 | 40.970685(74) | 38.4(8) s | β− | 41Ar | (1/2+) | ||||||||||||
42Cl | 17 | 25 | 41.973342(64) | 6.8(3) s | β− | 42Ar | (2−) | ||||||||||||
β−, n? | 41Ar | ||||||||||||||||||
43Cl | 17 | 26 | 42.974064(66) | 3.13(9) s | β− | 43Ar | (3/2+) | ||||||||||||
β−, n? | 42Ar | ||||||||||||||||||
44Cl | 17 | 27 | 43.978015(92) | 0.56(11) s | β− (>92%) | 44Ar | (2-) | ||||||||||||
β−, n? (<8%) | 43Ar | ||||||||||||||||||
45Cl | 17 | 28 | 44.98039(15) | 513(36) ms [8] | β− (76%) | 45Ar | (3/2+) | ||||||||||||
β−, n (24%) | 44Ar | ||||||||||||||||||
46Cl | 17 | 29 | 45.98525(10) | 232(2) ms | β−, n (60%) | 45Ar | 2-# | ||||||||||||
β− (40%) | 46Ar | ||||||||||||||||||
β−, 2n? | 44Ar | ||||||||||||||||||
47Cl | 17 | 30 | 46.98972(22)# | 101(5) ms | β− (>97%) | 47Ar | 3/2+# | ||||||||||||
β−, n? (<3%) | 46Ar | ||||||||||||||||||
β−, 2n? | 45Ar | ||||||||||||||||||
48Cl | 17 | 31 | 47.99541(54)# | 30# ms [>200 ns] | β−? | 48Ar | |||||||||||||
β−, n? | 47Ar | ||||||||||||||||||
β−, 2n? | 46Ar | ||||||||||||||||||
49Cl | 17 | 32 | 49.00079(43)# | 35# ms [>200 ns] | β−? | 49Ar | 3/2+# | ||||||||||||
β−, n? | 48Ar | ||||||||||||||||||
β−, 2n? | 47Ar | ||||||||||||||||||
50Cl | 17 | 33 | 50.00827(43)# | 10# ms [>620 ns] | β− | 50Ar | |||||||||||||
β−, n? | 49Ar | ||||||||||||||||||
β−, 2n? | 48Ar | ||||||||||||||||||
51Cl | 17 | 34 | 51.01534(75)# | 5# ms [>200 ns] | β−? | 51Ar | 3/2+# | ||||||||||||
β−, n? | 50Ar | ||||||||||||||||||
β−, 2n? | 49Ar | ||||||||||||||||||
52Cl | 17 | 35 | 52.02400(75)# | 2# ms [>400 ns] | β−? | 52Ar | |||||||||||||
β−, n? | 51Ar | ||||||||||||||||||
β−, 2n? | 50Ar | ||||||||||||||||||
This table header & footer: |
IT: | Isomeric transition |
n: | Neutron emission |
p: | Proton emission |
Trace amounts of radioactive 36Cl exist in the environment, in a ratio of about 7×10−13 to 1 with stable isotopes. 36Cl is produced in the atmosphere by spallation of 36 Ar by interactions with cosmic ray protons. In the subsurface environment, 36Cl is generated primarily as a result of neutron capture by 35Cl or muon capture by 40 Ca. 36Cl decays to either 36 S (1.9%) or to 36 Ar (98.1%), with a combined half-life of 308,000 years. The half-life of this hydrophilic nonreactive isotope makes it suitable for geologic dating in the range of 60,000 to 1 million years. Additionally, large amounts of 36Cl were produced by neutron irradiation of seawater during atmospheric detonations of nuclear weapons between 1952 and 1958. The residence time of 36Cl in the atmosphere is about 1 week. Thus, as an event marker of 1950s water in soil and ground water, 36Cl is also useful for dating waters less than 50 years before the present. 36Cl has seen use in other areas of the geological sciences, forecasts, and elements. In chloride-based molten salt reactors the production of 36
Cl by neutron capture is an inevitable consequence of using natural isotope mixtures of chlorine (i.e. Those containing 35
Cl). This produces a long lived radioactive product which has to be stored or disposed off. Isotope separation to produce pure 37
Cl can vastly reduce 36
Cl production, but a small amount might still be produced by (n,2n) reactions involving fast neutrons.
Stable chlorine-37 makes up about 24.23% of the naturally occurring chlorine on earth. Variation occurs as chloride mineral deposits have a slightly elevated chlorine-37 balance over the average found in sea water and halite deposits.[ citation needed ]
The mass number (symbol A, from the German word: Atomgewicht, "atomic weight"), also called atomic mass number or nucleon number, is the total number of protons and neutrons (together known as nucleons) in an atomic nucleus. It is approximately equal to the atomic (also known as isotopic) mass of the atom expressed in atomic mass units. Since protons and neutrons are both baryons, the mass number A is identical with the baryon number B of the nucleus (and also of the whole atom or ion). The mass number is different for each isotope of a given chemical element, and the difference between the mass number and the atomic number Z gives the number of neutrons (N) in the nucleus: N = A − Z.
Hydrogen (1H) has three naturally occurring isotopes: 1H, 2H, and 3H. 1H and 2H are stable, while 3H has a half-life of 12.32(2) years. Heavier isotopes also exist; all are synthetic and have a half-life of less than 1 zeptosecond (10−21 s). Of these, 5H is the least stable, while 7H is the most.
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.
Protactinium (91Pa) has no stable isotopes. The four naturally occurring isotopes allow a standard atomic weight to be given.
Naturally occurring erbium (68Er) is composed of six stable isotopes, with 166Er being the most abundant. Thirty-nine radioisotopes have been characterized with between 74 and 112 neutrons, or 142 to 180 nucleons, with the most stable being 169Er with a half-life of 9.4 days, 172Er with a half-life of 49.3 hours, 160Er with a half-life of 28.58 hours, 165Er with a half-life of 10.36 hours, and 171Er with a half-life of 7.516 hours. All of the remaining radioactive isotopes have half-lives that are less than 3.5 hours, and the majority of these have half-lives that are less than 4 minutes. This element also has numerous meta states, with the most stable being 167mEr.
Caesium (55Cs) has 41 known isotopes, the atomic masses of these isotopes range from 112 to 152. Only one isotope, 133Cs, is stable. The longest-lived radioisotopes are 135Cs with a half-life of 1.33 million years, 137
Cs
with a half-life of 30.1671 years and 134Cs with a half-life of 2.0652 years. All other isotopes have half-lives less than 2 weeks, most under an hour.
Tin (50Sn) is the element with the greatest number of stable isotopes. This is probably related to the fact that 50 is a "magic number" of protons. In addition, twenty-nine unstable tin isotopes are known, including tin-100 (100Sn) and tin-132 (132Sn), which are both "doubly magic". The longest-lived tin radioisotope is tin-126 (126Sn), with a half-life of 230,000 years. The other 28 radioisotopes have half-lives of less than a year.
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.
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 nickel (28Ni) is composed of five stable isotopes; 58
Ni
, 60
Ni
, 61
Ni
, 62
Ni
and 64
Ni
, with 58
Ni
being the most abundant. 26 radioisotopes have been characterised with the most stable being 59
Ni
with a half-life of 76,000 years, 63
Ni
with a half-life of 100.1 years, and 56
Ni
with a half-life of 6.077 days. All of the remaining radioactive isotopes have half-lives that are less than 60 hours and the majority of these have half-lives that are less than 30 seconds. This element also has 8 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.
Potassium has 25 known isotopes from 34
K to 57
K as well as 31
K, as well as an unconfirmed report of 59
K. 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%)
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.
Sulfur (16S) has 23 known isotopes with mass numbers ranging from 27 to 49, four of which are stable: 32S (95.02%), 33S (0.75%), 34S (4.21%), and 36S (0.02%). The preponderance of sulfur-32 is explained by its production from carbon-12 plus successive fusion capture of five helium-4 nuclei, in the so-called alpha process of exploding type II supernovas.
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.
Natural nitrogen (7N) consists of two stable isotopes: the vast majority (99.6%) of naturally occurring nitrogen is nitrogen-14, with the remainder being nitrogen-15. Thirteen radioisotopes are also known, with atomic masses ranging from 9 to 23, along with three nuclear isomers. All of these radioisotopes are short-lived, the longest-lived being nitrogen-13 with a half-life of 9.965(4) min. All of the others have half-lives below 7.15 seconds, with most of these being below 620 milliseconds. Most of the isotopes with atomic mass numbers below 14 decay to isotopes of carbon, while most of the isotopes with masses above 15 decay to isotopes of oxygen. The shortest-lived known isotope is nitrogen-10, with a half-life of 143(36) yoctoseconds, though the half-life of nitrogen-9 has not been measured exactly.
Beryllium (4Be) has 11 known isotopes and 3 known isomers, but only one of these isotopes is stable and a primordial nuclide. As such, beryllium is considered a monoisotopic element. It is also a mononuclidic element, because its other isotopes have such short half-lives that none are primordial and their abundance is very low. Beryllium is unique as being the only monoisotopic element with both an even number of protons and an odd number of neutrons. There are 25 other monoisotopic elements but all have odd atomic numbers, and even numbers of neutrons.
Chlorine-36 (36Cl) is an isotope of chlorine. Chlorine has two stable isotopes and one naturally occurring radioactive isotope, the cosmogenic isotope 36Cl. Its half-life is 301,300 ± 1,500 years. 36Cl decays primarily (98%) by beta-minus decay to 36Ar, and the balance to 36S.
Isotopes are distinct nuclear species of the same chemical element. They have the same atomic number and position in the periodic table, but different nucleon numbers due to different numbers of neutrons in their nuclei. While all isotopes of a given element have similar chemical properties, they have different atomic masses and physical properties.