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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 up to six isomers. The most stable known isotope is 271Hs, with a half-life of about 46 seconds, though this assignment is not definite due to uncertainty arising from a low number of measurements. The isotopes 269Hs and 270Hs respectively have half-lives of about 12 seconds and 7.6 seconds. It is also possible that the isomer 277mHs is more stable than these, with a reported half-life 130±100 seconds, but only one event of decay of this isotope has been registered as of 2016. [2] [3]
Nuclide [n 1] | Z | N | Isotopic mass (Da) [4] [n 2] [n 3] | Half-life | Decay mode [n 4] | Daughter isotope | Spin and parity [n 5] | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy | |||||||||||||||||||
263Hs | 108 | 155 | 263.12848(21)# | 760(40) μs | α | 259Sg | 3/2+# | ||||||||||||
264Hs [5] | 108 | 156 | 264.12836(3) | 0.7(3) ms | α (70%) | 260Sg | 0+ | ||||||||||||
SF (30%) | (various) | ||||||||||||||||||
265Hs [6] | 108 | 157 | 265.129792(26) | 1.96(16) ms | α | 261Sg | 9/2+# | ||||||||||||
265mHs | 229(22) keV | 360(150) μs | α | 261Sg | 3/2+# | ||||||||||||||
266Hs [n 6] [7] | 108 | 158 | 266.130049(29) | 2.97+0.78 −0.51 ms | α (76%) | 262Sg | 0+ | ||||||||||||
SF (24%) | (various) | ||||||||||||||||||
266mHs | 1100(70) keV | 280(220) ms [74+354 −34 ms] | α | 262Sg | 9-# | ||||||||||||||
267Hs | 108 | 159 | 267.13168(10)# | 55(11) ms | α | 263Sg | 5/2+# | ||||||||||||
267mHs [n 7] | 39(24) keV | 990(90) μs | α | 263Sg | |||||||||||||||
268Hs | 108 | 160 | 268.13201(32)# | 1.42(1.13) s [0.38+1.8 −0.17 s] | α | 264Sg | 0+ | ||||||||||||
269Hs | 108 | 161 | 269.13365(14)# | 13+10 −4 s [8] | α | 265Sg | 9/2+# | ||||||||||||
269mHs [8] | 20 keV# | 2.8+13.6 −1.3 s | α | 265mSg | 1/2# | ||||||||||||||
IT | 269Hs | ||||||||||||||||||
270Hs [9] | 108 | 162 | 270.13431(27)# | 7.6+4.9 −2.2 s | α | 266Sg | 0+ | ||||||||||||
SF (<50%) | (various) | ||||||||||||||||||
271Hs | 108 | 163 | 271.13708(30)# | 46+56 −16 s [8] | α | 267Sg | 11/2# | ||||||||||||
271mHs [8] | 20 keV# | 7.1+8.4 −2.5 s | α | 267mSg | 3/2# | ||||||||||||||
IT | 271Hs | ||||||||||||||||||
272Hs [n 8] [10] | 108 | 164 | 272.13849(55)# | 160+190 −60 ms | α | 268Sg | 0+ | ||||||||||||
273Hs [n 9] | 108 | 165 | 273.14146(40)# | 510+300 −140 ms [11] | α | 269Sg | 3/2+# | ||||||||||||
275Hs [n 10] [12] | 108 | 167 | 275.14653(64)# | 600+230 −130 ms | α | 271Sg | |||||||||||||
SF (<11%) | (various) | ||||||||||||||||||
277Hs [n 11] | 108 | 169 | 277.15177(48)# | 18+25 −7 ms [13] | SF | (various) | 3/2+# | ||||||||||||
277mHs [n 7] [n 11] [1] | 100(100) keV# | 130(100) s | SF | (various) | |||||||||||||||
This table header & footer: |
SF: | Spontaneous fission |
Target | Projectile | CN | Attempt result |
---|---|---|---|
136Xe | 136Xe | 272Hs | Failure to date |
198Pt | 70Zn | 268Hs | Failure to date [14] |
208Pb | 58Fe | 266Hs | Successful reaction |
207Pb | 58Fe | 265Hs | Successful reaction |
208Pb | 56Fe | 264Hs | Successful reaction |
207Pb | 56Fe | 263Hs | Reaction yet to be attempted |
206Pb | 58Fe | 264Hs | Successful reaction |
209Bi | 55Mn | 264Hs | Failure to date |
226Ra | 48Ca | 274Hs | Successful reaction |
232Th | 40Ar | 272Hs | Reaction yet to be attempted |
238U | 36S | 274Hs | Successful reaction |
238U | 34S | 272Hs | Successful reaction |
244Pu | 30Si | 274Hs | Reaction yet to be attempted |
248Cm | 26Mg | 274Hs | Successful reaction |
248Cm | 25Mg | 273Hs | Failure to date |
250Cm | 26Mg | 276Hs | Reaction yet to be attempted |
249Cf | 22Ne | 271Hs | Successful reaction |
Superheavy elements such as hassium are produced by bombarding lighter elements in particle accelerators that induce fusion reactions. Whereas most of the isotopes of hassium can be synthesized directly this way, some heavier ones have only been observed as decay products of elements with higher atomic numbers. [15]
Depending on the energies involved, the former are separated into "hot" and "cold". In hot fusion reactions, very light, high-energy projectiles are accelerated toward very heavy targets (actinides), giving rise to compound nuclei at high excitation energy (~40–50 MeV) that may either fission or evaporate several (3 to 5) neutrons. [16] In cold fusion reactions, the produced fused nuclei have a relatively low excitation energy (~10–20 MeV), which decreases the probability that these products will undergo fission reactions. As the fused nuclei cool to the ground state, they require emission of only one or two neutrons, and thus, allows for the generation of more neutron-rich products. [15] The latter is a distinct concept from that of where nuclear fusion claimed to be achieved at room temperature conditions (see cold fusion). [17]
Before the first successful synthesis of hassium in 1984 by the GSI team, scientists at the Joint Institute for Nuclear Research (JINR) in Dubna, Russia also tried to synthesize hassium by bombarding lead-208 with iron-58 in 1978. No hassium atoms were identified. They repeated the experiment in 1984 and were able to detect a spontaneous fission activity assigned to 260 Sg, the daughter of 264Hs. [18] Later that year, they tried the experiment again, and tried to chemically identify the decay products of hassium to provide support to their synthesis of element 108. They were able to detect several alpha decays of 253 Es and 253 Fm, decay products of 265Hs. [19]
In the official discovery of the element in 1984, the team at GSI studied the same reaction using the alpha decay genetic correlation method and were able to positively identify 3 atoms of 265Hs. [20] After an upgrade of their facilities in 1993, the team repeated the experiment in 1994 and detected 75 atoms of 265Hs and 2 atoms of 264Hs, during the measurement of a partial excitation function for the 1n neutron evaporation channel. [21] A further run of the reaction was conducted in late 1997 in which a further 20 atoms were detected. [22] This discovery experiment was successfully repeated in 2002 at RIKEN (10 atoms) and in 2003 at GANIL (7 atoms). The team at RIKEN further studied the reaction in 2008 in order to conduct the first spectroscopic studies of the even-even nucleus 264Hs. They were also able to detect a further 29 atoms of 265Hs.
The team at Dubna also conducted the analogous reaction with a lead-207 target instead of a lead-208 target in 1984:
They were able to detect the same spontaneous fission activity as observed in the reaction with a lead-208 target and once again assigned it to 260Sg, daughter of 264Hs. [19] The team at GSI first studied the reaction in 1986 using the method of genetic correlation of alpha decays and identified a single atom of 264Hs with a cross section of 3.2 pb. [23] The reaction was repeated in 1994 and the team were able to measure both alpha decay and spontaneous fission for 264Hs. This reaction was also studied in 2008 at RIKEN in order to conduct the first spectroscopic studies of the even-even nucleus 264Hs. The team detected 11 atoms of 264Hs.
In 2008, the team at RIKEN conducted the analogous reaction with a lead-206 target for the first time:
They were able to identify 8 atoms of the new isotope 263Hs. [24]
In 2008, the team at the Lawrence Berkeley National Laboratory (LBNL) studied the analogous reaction with iron-56 projectiles for the first time:
They were able to produce and identify six atoms of the new isotope 263Hs. [25] A few months later, the RIKEN team also published their results on the same reaction. [26]
Further attempts to synthesise nuclei of hassium were performed the team at Dubna in 1983 using the cold fusion reaction between a bismuth-209 target and manganese-55 projectiles:
They were able to detect a spontaneous fission activity assigned to 255 Rf, a product of the 263Hs decay chain. Identical results were measured in a repeat run in 1984. [19] In a subsequent experiment in 1983, they applied the method of chemical identification of a descendant to provide support to the synthesis of hassium. They were able to detect alpha decays from fermium isotopes, assigned as descendants of the decay of 262Hs. This reaction has not been tried since and 262Hs is currently unconfirmed. [19]
Under the leadership of Yuri Oganessian, the team at the Joint Institute for Nuclear Research studied the hot fusion reaction between calcium-48 projectiles and radium-226 targets in 1978:
However, results are not available in the literature. [19] The reaction was repeated at the JINR in June 2008 and 4 atoms of the isotope 270Hs were detected. [27] In January 2009, the team repeated the experiment and a further 2 atoms of 270Hs were detected. [28]
The team at Dubna studied the reaction between californium-249 targets and neon-22 projectiles in 1983 by detecting spontaneous fission activities:
Several short spontaneous fission activities were found, indicating the formation of nuclei of hassium. [19]
The hot fusion reaction between uranium-238 targets and projectiles of the rare and expensive isotope sulfur-36 was conducted at the GSI in April–May 2008:
Preliminary results show that a single atom of 270Hs was detected. This experiment confirmed the decay properties of the isotopes 270Hs and 266Sg. [29]
In March 1994, the team at Dubna led by the late Yuri Lazarev attempted the analogous reaction with sulfur-34 projectiles:
They announced the detection of 3 atoms of 267Hs from the 5n neutron evaporation channel. [30] The decay properties were confirmed by the team at GSI in their simultaneous study of darmstadtium. The reaction was repeated at the GSI in January–February 2009 in order to search for the new isotope 268Hs. The team, led by Prof. Nishio, detected a single atom each of both 268Hs and 267Hs. The new isotope 268Hs underwent alpha decay to the previously known isotope 264Sg.
Between May 2001 and August 2005, a GSI–PSI (Paul Scherrer Institute) collaboration studied the nuclear reaction between curium-248 targets and magnesium-26 projectiles:
The team studied the excitation function of the 3n, 4n, and 5n evaporation channels leading to the isotopes 269Hs, 270Hs, and 271Hs. [31] [32] The synthesis of the doubly magic isotope 270Hs was published in December 2006 by the team of scientists from the Technical University of Munich. [33] It was reported that this isotope decayed by emission of an alpha particle with an energy of 8.83 MeV and a half-life of ~22 s. This figure has since been revised to 3.6 s. [34]
Evaporation residue | Observed hassium isotope |
---|---|
267Ds | 263Hs [35] |
269Ds | 265Hs [36] |
270Ds | 266Hs [37] |
271Ds | 267Hs [38] |
277Cn, 273Ds | 269Hs [39] |
276Ds | 272Hs [10] |
285Fl, 281Cn, 277Ds | 273Hs [40] |
291Lv, 287Fl, 283Cn, 279Ds | 275Hs [41] |
293Lv, 289Fl, 285Cn, 281Ds | 277Hs [42] [43] [44] |
Hassium isotopes have been observed as decay products of darmstadtium. Darmstadtium currently has ten known isotopes, all but one of which have been shown to undergo alpha decays to become hassium nuclei with mass numbers between 263 and 277. Hassium isotopes with mass numbers 266, 272, 273, 275, and 277 to date have only been produced by decay of darmstadtium nuclei. Parent darmstadtium nuclei can be themselves decay products of copernicium, flerovium, or livermorium. [34] For example, in 2004, the Dubna team identified hassium-277 as a final product in the decay of livermorium-293 via an alpha decay sequence: [44]
An isotope assigned to 277Hs has been observed on one occasion decaying by SF with a long half-life of ~11 minutes. [45] The isotope is not observed in the decay of the ground state of 281Ds but is observed in the decay from a rare, as yet unconfirmed isomeric level, namely 281mDs. The half-life is very long for the ground state and it is possible that it belongs to an isomeric level in 277Hs. It has also been suggested that this activity actually comes from 278Bh, formed as the great-great-granddaughter of 290Fl through one electron capture to 290Nh and three further alpha decays. Furthermore, in 2009, the team at the GSI observed a small alpha decay branch for 281Ds producing the nuclide 277Hs decaying by SF in a short lifetime. The measured half-life is close to the expected value for ground state isomer, 277Hs. Further research is required to confirm the production of the isomer.
In 1999, American scientists at the University of California, Berkeley, announced that they had succeeded in synthesizing three atoms of 293118. [46] These parent nuclei were reported to have successively emitted three alpha particles to form hassium-273 nuclei, which were claimed to have undergone an alpha decay, emitting alpha particles with decay energies of 9.78 and 9.47 MeV and half-life 1.2 s, but their claim was retracted in 2001. [47] The isotope, however, was produced in 2010 by the same team. The new data matched the previous (fabricated) [48] data. [40]
According to macroscopic-microscopic (MM) theory, Z = 108 is a deformed proton magic number, in combination with the neutron shell at N = 162. This means that such nuclei are permanently deformed in their ground state but have high, narrow fission barriers to further deformation and hence relatively long SF partial half-lives. The SF half-lives in this region are typically reduced by a factor of 109 in comparison with those in the vicinity of the spherical doubly magic nucleus 298Fl, caused by an increase in the probability of barrier penetration by quantum tunnelling, due to the narrower fission barrier. In addition, N = 162 has been calculated as a deformed neutron magic number and hence the nucleus 270Hs has promise as a deformed doubly magic nucleus. Experimental data from the decay of Z = 110 isotopes 271Ds and 273Ds, provides strong evidence for the magic nature of the N = 162 sub-shell. The recent synthesis of 269Hs, 270Hs, and 271Hs also fully support the assignment of N = 162 as a magic closed shell. In particular, the low decay energy for 270Hs is in complete agreement with calculations. [49]
Evidence for the magicity of the Z = 108 proton shell can be deemed from two sources:
For SF, it is necessary to measure the half-lives for the isotonic nuclei 268Sg, 270Hs and 272Ds. Since fission of 270Hs has not been measured, detailed data of 268Sg fission is not yet available, [10] and 272Ds is still unknown, this method cannot be used to date to confirm the stabilizing nature of the Z = 108 shell. However, good evidence for the magicity of Z = 108 can be deemed from the large differences in the alpha decay energies measured for 270Hs, 271Ds and 273Ds. More conclusive evidence would come from the determination of the decay energy of the yet-unknown nuclide 272Ds.
An isotope assigned to 277Hs has been observed on one occasion decaying by spontaneous fission with a long half-life of ~11 minutes. [50] The isotope is not observed in the decay of the most common isomer of 281Ds but is observed in the decay from a rare, as yet unconfirmed isomeric level, namely 281mDs. The half-life is very long for the ground state and it is possible that it belongs to an isomeric level in 277Hs. Furthermore, in 2009, the team at the GSI observed a small alpha decay branch for 281Ds producing an isotope of 277Hs decaying by spontaneous fission with a short lifetime. The measured half-life is close to the expected value for ground state isomer, 277Hs. Further research is required to confirm the production of the isomer. [42] A more recent study suggests that this observed activity may actually be from 278Bh. [51]
The direct synthesis of 269Hs has resulted in the observation of three alpha particles with energies 9.21, 9.10, and 8.94 MeV emitted from 269Hs atoms. However, when this isotope is indirectly synthesized from the decay of 277Cn, only alpha particles with energy 9.21 MeV have been observed, indicating that this decay occurs from an isomeric level. Further research is required to confirm this. [31] [39]
267Hs is known to decay by alpha decay, emitting alpha particles with energies of 9.88, 9.83, and 9.75 MeV. It has a half-life of 52 ms. In the recent syntheses of 271Ds and 271mDs, additional activities have been observed. A 0.94 ms activity emitting alpha particles with energy 9.83 MeV has been observed in addition to longer lived ~0.8 s and ~6.0 s activities. Currently, none of these are assigned and confirmed and further research is required to positively identify them. [30]
The synthesis of 265Hs has also provided evidence for two isomeric levels. The ground state decays by emission of an alpha particle with energy 10.30 MeV and has a half-life of 2.0 ms. The isomeric state has 300 keV of excess energy and decays by the emission of an alpha particle with energy 10.57 MeV and has a half-life of 0.75 ms. [20]
Scientists at the GSI are planning to search for isomers of 270Hs using the reaction 226Ra(48Ca,4n) in 2010 using the new TASCA facility at the GSI. [52] In addition, they also hope to study the spectroscopy of 269Hs, 265Sg and 261Rf, using the reaction 248Cm(26Mg,5n) or 226Ra(48Ca,5n). This will allow them to determine the level structure in 265Sg and 261Rf and attempt to give spin and parity assignments to the various proposed isomers. [53]
The tables below provides cross-sections and excitation energies for nuclear reactions that produce isotopes of hassium directly. Data in bold represent maxima derived from excitation function measurements. + represents an observed exit channel.
Projectile | Target | CN | 1n | 2n | 3n |
---|---|---|---|---|---|
58Fe | 208Pb | 266Hs | 69 pb, 13.9 MeV | 4.5 pb | |
58Fe | 207Pb | 265Hs | 3.2 pb |
Projectile | Target | CN | 3n | 4n | 5n |
---|---|---|---|---|---|
48Ca | 226Ra | 274Hs | 9.0 pb | ||
36S | 238U | 274Hs | 0.8 pb | ||
34S | 238U | 272Hs | 2.5 pb, 50.0 MeV | ||
26Mg | 248Cm | 274Hs | 2.5 pb | 3.0 pb | 7.0 pb |
The below table contains various targets-projectile combinations for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.
DNS = Di-nuclear system ; σ = cross section
Target | Projectile | CN | Channel (product) | σ max | Model | Ref |
---|---|---|---|---|---|---|
136Xe | 136Xe | 272Hs | 1–4n (271–268Hs) | 10−6 pb | DNS | [54] |
238U | 34S | 272Hs | 4n (268Hs) | 10 pb | DNS | [54] |
238U | 36S | 274Hs | 4n (270Hs) | 42.97 pb | DNS | [55] |
244Pu | 30Si | 274Hs | 4n (270Hs) | 185.1 pb | DNS | [55] |
248Cm | 26Mg | 274Hs | 4n (270Hs) | 719.1 pb | DNS | [55] |
250Cm | 26Mg | 276Hs | 4n (272Hs) | 185.2 pb | DNS | [55] |
Hassium is a synthetic chemical element; it has symbol Hs and atomic number 108. It is highly radioactive: its most stable known isotopes have half-lives of approximately ten seconds. One of its isotopes, 270Hs, has magic numbers of protons and neutrons for deformed nuclei, giving it greater stability against spontaneous fission. Hassium is a superheavy element; it has been produced in a laboratory in very small quantities by fusing heavy nuclei with lighter ones. Natural occurrences of the element have been hypothesised but never found.
Meitnerium is a synthetic chemical element; it has symbol Mt and atomic number 109. It is named after Lise Meitner and 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.
Darmstadtium is a synthetic chemical element; it has symbol Ds and atomic number 110. It is extremely radioactive: the most stable known isotope, darmstadtium-281, has a half-life of approximately 14 seconds. Darmstadtium was first created in 1994 by the GSI Helmholtz Centre for Heavy Ion Research in the city of Darmstadt, Germany, after which it was named.
Roentgenium is a synthetic chemical element; it has symbol Rg and atomic number 111. It is extremely radioactive and can only be created in a laboratory. The most stable known isotope, roentgenium-282, has a half-life of 130 seconds, although the unconfirmed roentgenium-286 may have a longer half-life of about 10.7 minutes. Roentgenium was first created in 1994 by the GSI Helmholtz Centre for Heavy Ion Research near Darmstadt, Germany. It is named after the physicist Wilhelm Röntgen, who discovered X-rays. Only a few roentgenium atoms have ever been synthesized, and they have no practical application.
Livermorium is a synthetic chemical element; it has symbol Lv and atomic number 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. Six isotopes of livermorium are known, with mass numbers of 288–293 inclusive; the longest-lived among them is livermorium-293 with a half-life of about 80 milliseconds. A seventh possible isotope with mass number 294 has been reported but not yet confirmed.
In nuclear physics, the island of stability is a predicted set of isotopes of superheavy elements that may have considerably longer half-lives than known isotopes of these elements. It is predicted to appear as an "island" in the chart of nuclides, separated from known stable and long-lived primordial radionuclides. Its theoretical existence is attributed to stabilizing effects of predicted "magic numbers" of protons and neutrons in the superheavy mass region.
Copernicium is a synthetic chemical element; it has symbol Cn and atomic number 112. Its known isotopes are extremely radioactive, and have only been created in a laboratory. The most stable known isotope, copernicium-285, has a half-life of approximately 30 seconds. Copernicium was first created in 1996 by the GSI Helmholtz Centre for Heavy Ion Research near Darmstadt, Germany. It was named after the astronomer Nicolaus Copernicus on his 537th anniversary.
Flerovium is a synthetic chemical element; it has symbol Fl and atomic number 114. It is an extremely radioactive, superheavy element, 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; it has 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.
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.
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 thirteen known radioisotopes from 258Sg to 271Sg and five known isomers. The longest-lived isotopes are 267Sg with a half-life of 9.8 minutes and 269Sg with a half-life of 5 minutes. Due to a low number of measurements, and the consequent overlapping measurement uncertainties at the confidence level corresponding to one standard deviation, a definite assignment of the most stable isotope cannot be made.
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.
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. However, the unconfirmed 282Ds might have an even longer half-life of 67 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 seven 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 six known isotopes, along with the unconfirmed 290Fl, and possibly two nuclear isomers. The longest-lived isotope is 289Fl with a half-life of 1.9 seconds, but 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.
Livermorium (116Lv) is a synthetic element, and thus a standard atomic weight cannot be given. Like all artificial elements, it has no stable isotopes. The first isotope to be synthesized was 293Lv in 2000. There are six known radioisotopes, with mass numbers 288–293, as well as a few suggestive indications of a possible heavier isotope 294Lv. The longest-lived known isotope is 293Lv with a half-life of 53 ms.
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: CS1 maint: archived copy as title (link)Half-life, spin, and isomer data selected from: