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Seaborgium (106Sg) is a synthetic element and so has no stable isotopes. A standard atomic weight cannot be given. The first isotope to be synthesized was 263Sg in 1974. There are 13 known radioisotopes from 258Sg to 271Sg and 4 known isomers (259mSg, 261mSg, 263mSg, and 265mSg). The longest-lived isotope is 269Sg with a half-life of 14 minutes.
Nuclide [n 1] | Z | N | Isotopic mass (Da) [n 2] [n 3] | Half-life | Decay mode [n 4] | Daughter isotope | Spin and parity [n 5] | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy [n 5] | |||||||||||||||||||
258Sg [1] | 106 | 152 | 258.11298(44)# | 2.7(5) ms [2.6+0.6 −0.4 ms] | SF | (various) | 0+ | ||||||||||||
259Sg [5] | 106 | 153 | 259.11440(13)# | 402(56) ms | α | 255Rf | (11/2−) | ||||||||||||
β+ (<1%) | 259Db | ||||||||||||||||||
SF (rare) | (various) | ||||||||||||||||||
259mSg | 87 keV | 226(27) ms | α (97%) | 261Sg | (1/2+) | ||||||||||||||
SF (3%) | (various) | ||||||||||||||||||
β+ (<1%) | 259Db | ||||||||||||||||||
260Sg [1] | 106 | 154 | 260.114384(22) | 4.95(33) ms | SF (71%) | (various) | 0+ | ||||||||||||
α (29%) | 256Rf | ||||||||||||||||||
261Sg [1] | 106 | 155 | 261.115949(20) | 183(5) ms | α (98.1%) | 257Rf | (3/2+) | ||||||||||||
β+ (1.3%) | 261Db | ||||||||||||||||||
SF (0.6%) | (various) | ||||||||||||||||||
261mSg | 100(50)# keV | 9.3(1.8) µs [9.0+2.0 −1.5 μs] | IT | 261Sg | 7/2+# | ||||||||||||||
262Sg [1] | 106 | 156 | 262.11634(4) | 10.3(1.7) ms | SF (94%) | (various) | 0+ | ||||||||||||
α (6%) | 258Rf | ||||||||||||||||||
263Sg [1] | 106 | 157 | 263.11829(10)# | 940(140) ms | α (87%) | 259Rf | 9/2+# | ||||||||||||
SF (13%) | (various) | ||||||||||||||||||
263mSg | 51(19)# keV | 420(100) ms | α | 259Rf | 3/2+# | ||||||||||||||
264Sg | 106 | 158 | 264.11893(30)# | 37 ms | SF | (various) | 0+ | ||||||||||||
265Sg [6] | 106 | 159 | 265.12109(13)# | 8.5+2.6 −1.6 s | α | 261Rf | |||||||||||||
265mSg | 14.4+3.7 −2.5 s | α | 261mRf | ||||||||||||||||
266Sg [n 6] [1] | 106 | 160 | 266.12198(26)# | 390(110) ms | SF | (various) | 0+ | ||||||||||||
267Sg [n 7] [7] | 106 | 161 | 267.12436(30)# | 80+60 −20 s | SF (83%) | (various) | |||||||||||||
α (17%) | 263Rf | ||||||||||||||||||
268Sg [n 8] [2] | 106 | 162 | 268.12539(50)# | 13+17 −4 s | SF | (various) | 0+ | ||||||||||||
269Sg [n 9] | 106 | 163 | 269.12863(39)# | 14+10 −4 min [3] | α | 265Rf | |||||||||||||
271Sg [n 10] | 106 | 165 | 271.13393(63)# | 31+13 −7 s [4] | α (73%) | 267Rf | 3/2+# | ||||||||||||
SF (27%) | (various) | ||||||||||||||||||
This table header & footer: |
EC: | Electron capture |
SF: | Spontaneous fission |
Target | Projectile | CN | Attempt result |
---|---|---|---|
208Pb | 54Cr | 262Sg | Successful reaction |
207Pb | 54Cr | 261Sg | Successful reaction |
206Pb | 54Cr | 260Sg | Failure to date |
208Pb | 52Cr | 260Sg | Successful reaction |
209Bi | 51V | 260Sg | Successful reaction |
238U | 30Si | 268Sg | Successful reaction |
244Pu | 26Mg | 270Sg | Reaction yet to be attempted |
248Cm | 22Ne | 270Sg | Successful reaction |
249Cf | 18O | 267Sg | Successful reaction |
This section deals with the synthesis of nuclei of seaborgium by so-called "cold" fusion reactions. These are processes that create compound nuclei at low excitation energy (~10–20 MeV, hence "cold"), leading to a higher probability of survival from fission. The excited nucleus then decays to the ground state via the emission of one or two neutrons only.
The first attempt to synthesise seaborgium in cold fusion reactions was performed in September 1974 by a Soviet team led by G. N. Flerov at the Joint Institute for Nuclear Research at Dubna. They reported producing a 0.48 s spontaneous fission (SF) activity, which they assigned to the isotope 259Sg. Based on later evidence it was suggested that the team most likely measured the decay of 260Sg and its daughter 256Rf. The TWG concluded that, at the time, the results were insufficiently convincing. [8]
The Dubna team revisited this problem in 1983–1984 and were able to detect a 5 ms SF activity assigned directly to 260Sg. [8]
The team at GSI studied this reaction for the first time in 1985 using the improved method of correlation of genetic parent-daughter decays. They were able to detect 261Sg (x=1) and 260Sg and measured a partial 1n neutron evaporation excitation function. [9]
In December 2000, the reaction was studied by a team at GANIL, France; they were able to detect 10 atoms of 261Sg and 2 atoms of 260Sg to add to previous data on the reaction.
After a facility upgrade, the GSI team measured the 1n excitation function in 2003 using a metallic lead target. Of significance, in May 2003, the team successfully replaced the lead-208 target with more resistant lead(II) sulfide targets (PbS), which will allow more intense beams to be used in the future. They were able to measure the 1n,2n and 3n excitation functions and performed the first detailed alpha-gamma spectroscopy on the isotope 261Sg. They detected ~1600 atoms of the isotope and identified new alpha lines as well as measuring a more accurate half-life and new EC and SF branchings. Furthermore, they were able to detect the K X-rays from the daughter rutherfordium isotope for the first time. They were also able to provide improved data for 260Sg, including the tentative observation of an isomeric level. The study was continued in September 2005 and March 2006. The accumulated work on 261Sg was published in 2007. [10] Work in September 2005 also aimed to begin spectroscopic studies on 260Sg.
The team at the LBNL recently restudied this reaction in an effort to look at the spectroscopy of the isotope 261Sg. They were able to detect a new isomer, 261mSg, decaying by internal conversion into the ground state. In the same experiment, they were also able to confirm a K-isomer in the daughter 257Rf, namely 257m2Rf. [11]
The team at Dubna also studied this reaction in 1974 with identical results as for their first experiments with a lead-208 target. The SF activities were first assigned to 259Sg and later to 260Sg and/or 256Rf. Further work in 1983–1984 also detected a 5 ms SF activity assigned to the parent 260Sg. [8]
The GSI team studied this reaction for the first time in 1985 using the method of correlation of genetic parent-daughter decays. They were able to positively identify 259Sg as a product from the 2n neutron evaporation channel. [9]
The reaction was further used in March 2005 using PbS targets to begin a spectroscopic study of the even-even isotope 260Sg.
This reaction was studied in 1974 by the team at Dubna. It was used to assist them in their assignment of the observed SF activities in reactions using Pb-207 and Pb-208 targets. They were unable to detect any SF, indicating the formation of isotopes decaying primarily by alpha decay. [8]
The team at Dubna also studied this reaction in their series of cold fusion reactions performed in 1974. Once again they were unable to detect any SF activities. [8] The reaction was revisited in 2006 by the team at LBNL as part of their studies on the effect of the isospin of the projectile and hence the mass number of the compound nucleus on the yield of evaporation residues. They were able to identify 259Sg and 258Sg in their measurement of the 1n excitation function. [12]
The team at Dubna also studied this reaction in their series of cold fusion reactions performed in 1974. Once again they were unable to detect any SF activities. [8] In 1994, the synthesis of seaborgium was revisited using this reaction by the GSI team, in order to study the new even-even isotope 258Sg. Ten atoms of 258Sg were detected and decayed by spontaneous fission.
This section deals with the synthesis of nuclei of seaborgium by so-called "hot" fusion reactions. These are processes that create compound nuclei at high excitation energy (~40–50 MeV, hence "hot"), leading to a reduced probability of survival from fission and quasi-fission. The excited nucleus then decays to the ground state via the emission of 3–5 neutrons.
This reaction was first studied by Japanese scientists at the Japan Atomic Energy Research Institute (JAERI) in 1998. They detected a spontaneous fission activity, which they tentatively assigned to the new isotope 264Sg or 263Db, formed by EC of 263Sg. [13] In 2006, the teams at GSI and LBNL both studied this reaction using the method of correlation of genetic parent-daughter decays. The LBNL team measured an excitation function for the 4n,5n and 6n channels, whilst the GSI team were able to observe an additional 3n activity. [14] [15] [16] Both teams were able to identify the new isotope 264Sg, which decayed with a short lifetime by spontaneous fission.
In 1993, at Dubna, Yuri Lazarev and his team announced the discovery of long-lived 266Sg and 265Sg produced in the 4n and 5n channels of this nuclear reaction following the search for seaborgium isotopes suitable for a first chemical study. It was announced that 266Sg decayed by 8.57 MeV alpha-particle emission with a projected half-life of ~20 s, lending strong support to the stabilising effect of the Z = 108, N = 162 closed shells. [17] This reaction was studied further in 1997 by a team at GSI and the yield, decay mode and half-lives for 266Sg and 265Sg have been confirmed, although there are still some discrepancies. In the synthesis of 270Hs (see hassium), 266Sg was found to undergo exclusively SF with a short half-life (TSF = 360 ms). It is possible that this is the ground state, (266gSg) and that the other activity, produced directly, belongs to a high spin K-isomer, 266mSg, but further results are required to confirm this.
A recent re-evaluation of the decay characteristics of 265Sg and 266Sg has suggested that all decays to date in this reaction were in fact from 265Sg, which exists in two isomeric forms. The first, 265aSg has a principal alpha-line at 8.85 MeV and a calculated half-life of 8.9 s, while 265bSg has a decay energy of 8.70 MeV and a half-life of 16.2 s. Both isomeric levels are populated when produced directly. Data from the decay of 269Hs indicates that 265bSg is produced during the decay of 269Hs and that 265bSg decays into the shorter-lived 261gRf isotope. This contradicts the assignment of the long-lived alpha activity to 266Sg, instead suggesting that 266Sg undergoes fission in a short time.
Regardless of these assignments, the reaction has been successfully used in the recent attempts to study the chemistry of seaborgium (see below).
The synthesis of seaborgium was first realized in 1974 by the LBNL/LLNL team. [18] In their discovery experiment, they were able to apply the new method of correlation of genetic parent-daughter decays to identify the new isotope 263Sg. In 1975, the team at Oak Ridge were able to confirm the decay data but were unable to identify coincident X-rays in order to prove that seaborgium was produced. In 1979, the team at Dubna studied the reaction by detection of SF activities. In comparison with data from Berkeley, they calculated a 70% SF branching for 263Sg. The original synthesis and discovery reaction was confirmed in 1994 by a different team at LBNL. [19]
Isotopes of seaborgium have also been observed in the decay of heavier elements. Observations to date are summarised in the table below:
Evaporation Residue | Observed Sg isotope |
---|---|
291Lv, 287Fl, 283Cn | 271Sg |
285Fl | 269Sg |
276Ds, 272Hs | 268Sg |
271Hs | 267Sg |
270Hs | 266Sg |
277Cn, 273Ds, 269Hs | 265Sg |
271Ds, 267Ds | 263Sg |
270Ds | 262Sg |
269Ds, 265Hs | 261Sg |
264Hs | 260Sg |
Isotope | Year discovered | discovery reaction |
---|---|---|
258Sg | 1994 | 209Bi(51V,2n) |
259Sg | 1985 | 207Pb(54Cr,2n) |
260Sg | 1985 | 208Pb(54Cr,2n) |
261gSg | 1985 | 208Pb(54Cr,n) |
261mSg | 2009 | 208Pb(54Cr,n) |
262Sg | 2001 | 207Pb(64Ni,n) |
263Sgm | 1974 | 249Cf(18O,4n) [18] |
263Sgg | 1994 | 208Pb(64Ni,n) |
264Sg | 2006 | 238U(30Si,4n) |
265Sga, b | 1993 | 248Cm(22Ne,5n) |
266Sg | 2004 | 248Cm(26Mg,4n) |
267Sg | 2004 | 248Cm(26Mg,3n) |
268Sg | 2022 | 232Th(48Ca,4n) [2] |
269Sg | 2010 | 242Pu(48Ca,5n) |
270Sg | unknown | |
271Sg | 2003 | 242Pu(48Ca,3n) |
Initial work identified an 8.63 MeV alpha-decaying activity with a half-life of ~21 s and assigned to the ground state of 266Sg. Later work identified a nuclide decaying by 8.52 and 8.77 MeV alpha emission with a half-life of ~21 s, which is unusual for an even-even nuclide. Recent work on the synthesis of 270Hs identified 266Sg decaying by SF with a short 360 ms half-life. The recent work on 277Cn and 269Hs has provided new information on the decay of 265Sg and 261Rf. This work suggested that the initial 8.77 MeV activity should be reassigned to 265Sg. Therefore, the current information suggests that the SF activity is the ground state and the 8.52 MeV activity is a high spin K-isomer. Further work is required to confirm these assignments. A recent re-evaluation of the data has suggested that the 8.52 MeV activity should be associated with 265Sg and that 266Sg only undergoes fission.
The recent direct synthesis of 265Sg resulted in four alpha-lines at 8.94, 8.84, 8.76 and 8.69 MeV with a half-life of 7.4 seconds. The observation of the decay of 265Sg from the decay of 277Cn and 269Hs indicated that the 8.69 MeV line may be associated with an isomeric level with an associated half-life of ~ 20 s. It is plausible that this level is causing confusion between assignments of 266Sg and 265Sg since both can decay to fissioning rutherfordium isotopes.
A recent re-evaluation of the data has indicated that there are indeed two isomers, one with a principal decay energy of 8.85 MeV with a half-life of 8.9 s, and a second isomer that decays with energy 8.70 MeV with a half-life of 16.2 s.
The discovery synthesis of 263Sg resulted in an alpha-line at 9.06 MeV. [18] Observation of this nuclide by decay of 271gDs,271mDs and 267Hs has confirmed an isomer decaying by 9.25 MeV alpha emission. The 9.06 MeV decay was also confirmed. The 9.06 MeV activity has been assigned to the ground state isomer with an associated half-life of 0.3 s. The 9.25 MeV activity has been assigned to an isomeric level decaying with a half-life of 0.9 s.
Recent work on the synthesis of 271g,mDs was resulted in some confusing data regarding the decay of 267Hs. In one such decay, 267Hs decayed to 263Sg, which decayed by alpha emission with a half-life of ~ 6 s. This activity has not yet been positively assigned to an isomer and further research is required.
In the claimed synthesis of 293Og in 1999 the isotope 269Sg was identified as a daughter product. It decayed by 8.74 MeV alpha emission with a half-life of 22 s. The claim was retracted in 2001. This isotope was finally created in 2010.
The table below provides cross-sections and excitation energies for cold fusion reactions producing seaborgium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
Projectile | Target | CN | 1n | 2n | 3n |
---|---|---|---|---|---|
54Cr | 207Pb | 261Sg | |||
54Cr | 208Pb | 262Sg | 4.23 nb, 13.0 MeV | 500 pb | 10 pb |
51V | 209Bi | 260Sg | 38 pb, 21.5 MeV | ||
52Cr | 208Pb | 260Sg | 281 pb, 11.0 MeV |
The table below provides cross-sections and excitation energies for hot fusion reactions producing seaborgium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
Projectile | Target | CN | 3n | 4n | 5n | 6n |
---|---|---|---|---|---|---|
30Si | 238U | 268Sg | + | 9 pb, 40.0 | ~ 80 pb, 51.0 MeV | ~30 pb, 58.0 MeV |
22Ne | 248Cm | 270Sg | ~25 pb | ~250 pb | ||
18O | 249Cf | 267Sg | + |
Dubnium is a synthetic chemical element with the symbol Db and atomic number 105. It is highly radioactive: the most stable known isotope, dubnium-268, has a half-life of about 16 hours. This greatly limits extended research on the element.
Meitnerium is a synthetic chemical element with the symbol Mt and atomic number 109. It is an extremely radioactive synthetic element. The most stable known isotope, meitnerium-278, has a half-life of 4.5 seconds, although the unconfirmed meitnerium-282 may have a longer half-life of 67 seconds. The GSI Helmholtz Centre for Heavy Ion Research near Darmstadt, Germany, first created this element in 1982. It is named after Lise Meitner.
Nobelium is a synthetic chemical element with the symbol No and atomic number 102. It is named in honor of Alfred Nobel, the inventor of dynamite and benefactor of science. A radioactive metal, it is the tenth transuranic element and is the penultimate member of the actinide series. Like all elements with atomic number over 100, nobelium can only be produced in particle accelerators by bombarding lighter elements with charged particles. A total of twelve nobelium isotopes are known to exist; the most stable is 259No with a half-life of 58 minutes, but the shorter-lived 255No is most commonly used in chemistry because it can be produced on a larger scale.
Seaborgium is a synthetic chemical element with the symbol Sg and atomic number 106. It is named after the American nuclear chemist Glenn T. Seaborg. As a synthetic element, it can be created in a laboratory but is not found in nature. It is also radioactive; the most stable known isotope, 269Sg, has a half-life of approximately 14 minutes.
Livermorium is a synthetic chemical element with the symbol Lv and has an atomic number of 116. It is an extremely radioactive element that has only been created in a laboratory setting and has not been observed in nature. The element is named after the Lawrence Livermore National Laboratory in the United States, which collaborated with the Joint Institute for Nuclear Research (JINR) in Dubna, Russia, to discover livermorium during experiments conducted between 2000 and 2006. The name of the laboratory refers to the city of Livermore, California, where it is located, which in turn was named after the rancher and landowner Robert Livermore. The name was adopted by IUPAC on May 30, 2012. Four isotopes of livermorium are known, with mass numbers between 290 and 293 inclusive; the longest-lived among them is livermorium-293 with a half-life of about 60 milliseconds. A fifth possible isotope with mass number 294 has been reported but not yet confirmed.
Flerovium is a superheavy chemical element with symbol Fl and atomic number 114. It is an extremely radioactive synthetic element. It is named after the Flerov Laboratory of Nuclear Reactions of the Joint Institute for Nuclear Research in Dubna, Russia, where the element was discovered in 1999. The lab's name, in turn, honours Russian physicist Georgy Flyorov. IUPAC adopted the name on 30 May 2012. The name and symbol had previously been proposed for element 102 (nobelium), but was not accepted by IUPAC at that time.
Nihonium is a synthetic chemical element with the symbol Nh and atomic number 113. It is extremely radioactive; its most stable known isotope, nihonium-286, has a half-life of about 10 seconds. In the periodic table, nihonium is a transactinide element in the p-block. It is a member of period 7 and group 13.
Nobelium (102No) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 254No in 1966. There are thirteen known radioisotopes, which are 249No to 260No and 262No, and many isomers. The longest-lived isotope is 259No with a half-life of 58 minutes. The longest-lived isomer is 251m1No with a half-life of 1.02 seconds.
Lawrencium (103Lr) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 258Lr in 1961. There are fourteen known isotopes from 251Lr to 266Lr, and seven isomers. The longest-lived known isotope is 266Lr with a half-life of 11 hours.
Rutherfordium (104Rf) is a synthetic element and thus has no stable isotopes. A standard atomic weight cannot be given. The first isotope to be synthesized was either 259Rf in 1966 or 257Rf in 1969. There are 16 known radioisotopes from 253Rf to 270Rf and several isomers. The longest-lived isotope is 267Rf with a half-life of 48 minutes, and the longest-lived isomer is 263mRf with a half-life of 8 seconds.
Dubnium (105Db) is a synthetic element, thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 261Db in 1968. The 13 known radioisotopes are from 255Db to 270Db, and 1–3 isomers. The longest-lived known isotope is 268Db with a half-life of 16 hours.
Bohrium (107Bh) is an artificial element. Like all artificial elements, it has no stable isotopes, and a standard atomic weight cannot be given. The first isotope to be synthesized was 262Bh in 1981. There are 11 known isotopes ranging from 260Bh to 274Bh, and 1 isomer, 262mBh. The longest-lived isotope is 270Bh with a half-life of 2.4 minutes, although the unconfirmed 278Bh may have an even longer half-life of about 690 seconds.
Hassium (108Hs) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 265Hs in 1984. There are 13 known isotopes from 263Hs to 277Hs and 1–4 isomers. The most stable isotope of hassium cannot be determined based on existing data due to uncertainty that arises from the low number of measurements. The half-lives of 269Hs and 271Hs are about 12 seconds, whereas that of 270Hs is about 7.6 seconds. It is also possible that 277mHs is more stable than these, with its half-life likely being 130±100 seconds, but only one event of decay of this isotope has been registered as of 2016.
Meitnerium (109Mt) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 266Mt in 1982, and this is also the only isotope directly synthesized; all other isotopes are only known as decay products of heavier elements. There are eight known isotopes, from 266Mt to 278Mt. There may also be two isomers. The longest-lived of the known isotopes is 278Mt with a half-life of 8 seconds. The unconfirmed heavier 282Mt appears to have an even longer half-life of 67 seconds.
Darmstadtium (110Ds) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 269Ds in 1994. There are 11 known radioisotopes from 267Ds to 281Ds and 2 or 3 known isomers. The longest-lived isotope is 281Ds with a half-life of 14 seconds.
Roentgenium (111Rg) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 272Rg in 1994, which is also the only directly synthesized isotope; all others are decay products of heavier elements. There are seven known radioisotopes, having mass numbers of 272, 274, and 278–282. The longest-lived isotope is 282Rg with a half-life of about 2 minutes, although the unconfirmed 283Rg and 286Rg may have longer half-lives of about 5.1 minutes and 10.7 minutes respectively.
Copernicium (112Cn) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 277Cn in 1996. There are 6 known radioisotopes ; the longest-lived isotope is 285Cn with a half-life of 30 seconds.
Nihonium (113Nh) is a synthetic element. Being synthetic, a standard atomic weight cannot be given and like all artificial elements, it has no stable isotopes. The first isotope to be synthesized was 284Nh as a decay product of 288Mc in 2003. The first isotope to be directly synthesized was 278Nh in 2004. There are 6 known radioisotopes from 278Nh to 286Nh, along with the unconfirmed 287Nh and 290Nh. The longest-lived isotope is 286Nh with a half-life of 9.5 seconds.
Flerovium (114Fl) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 289Fl in 1999. Flerovium has seven known isotopes, and possibly 2 nuclear isomers. The longest-lived isotope is 289Fl with a half-life of 1.9 seconds, but the unconfirmed 290Fl may have a longer half-life of 19 seconds.
Moscovium (115Mc) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no known stable isotopes. The first isotope to be synthesized was 288Mc in 2004. There are five known radioisotopes from 286Mc to 290Mc. The longest-lived isotope is 290Mc with a half-life of 0.65 seconds.
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