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This article is part of [[Wikipedia:Wikiproject Isotopes]]. Please keep style and phrasings consistent across the set of pages. For later reference and improved reliability, data from all considered multiple sources is collected here. References are denoted by these letters:
*('''A''') G. Audi, O. Bersillon, J. Blachot, A.H. Wapstra. [http://amdc.in2p3.fr/web/nubase_en.html The Nubase2003 evaluation of nuclear and decay properties], Nuc. Phys. A 729, pp. 3-128 (2003). — Where this source indicates a speculative value, the # mark is also applied to values with weak assignment arguments from other sources, if grouped together. An asterisk after the A means that a comment of some importance may be available in the original.
*('''B''') National Nuclear Data Center, Brookhaven National Laboratory, information extracted from the [http://www.nndc.bnl.gov/nudat2/ NuDat 2.1 database]. (Retrieved Sept. 2005, from the code of the popup boxes).
*('''C''') David R. Lide (ed.), Norman E. Holden in ''CRC Handbook of Chemistry and Physics, 85th Edition'', online version. CRC Press. Boca Raton, Florida (2005). Section 11, Table of the Isotopes. — The CRC uses rounded numbers with implied uncertainties, where this concurs with the range of another source it is treated as exactly equal in this comparison.
*('''D''') More specific level data from reference B's ''Levels and Gammas database''.
*('''E''') Same as B but excitation energy replaced with that from D.

Z N refs symbol half-life spin excitation energy
100 142 AB |Fm-242 |0.8(2) ms |0+
100 142 C |Fm-242 |0.8 ms |
100 143 A |Fm-243 |210(60) ms |7/2-#
100 143 B |Fm-243 |0.18(+8-4) s |(7/2+)
100 143 C |Fm-243 |0.2 s |
100 144 ABC |Fm-244 |3.3(5) ms |0+
100 145 A |Fm-245 |4.2(13) s |1/2+#
100 145 BC |Fm-245 |4.2(13) s |
100 146 AB |Fm-246 |1.1(2) s |0+
100 146 C |Fm-246 |1.2 s |0+
100 147 A |Fm-247 |35(4) s |5/2+#
100 147 B |Fm-247 |29(1) s |(7/2+)
100 147 C |Fm-247 |35. s |
100 147 A* |Fm-247m |9.2(23) s | |non-exist
100 147 D |Fm-247m |9.2(23) s | |0+W keV
100 147 C |Fm-247m |9. s |
100 147 B |Fm-247m |4.3(4) s |(1/2+) |0 MeV
100 148 A |Fm-248 |36(3) s |0+
100 148 B |Fm-248 |36(2) s |0+
100 148 C |Fm-248 |34. s |0+
100 149 ABC |Fm-249 |2.6(7) min |(7/2+)#
100 150 ABC |Fm-250 |30(3) min |0+
100 150 A |Fm-250m |1.8(1) s |7,8# |1500(300)# keV
100 150 E |Fm-250m |1.8(1) s |0+ |0+X keV
100 150 C |Fm-250m |1.8 s |
100 151 ABC |Fm-251 |5.30(8) h |(9/2-)
100 151 AD |Fm-251m |15.2(23) µs |(5/2+) |191(2) keV
100 152 ABC |Fm-252 |25.39(4) h |0+
100 153 AB |Fm-253 |3.00(12) d |(1/2)+
100 153 C |Fm-253 |3.0 d |1/2+
100 154 ABC |Fm-254 |3.240(2) h |0+
100 155 ABC |Fm-255 |20.07(7) h |7/2+
100 156 ABC |Fm-256 |157.6(13) min |0+
100 157 ABC |Fm-257 |100.5(2) d |(9/2+)
100 158 A |Fm-258 |370(14) µs |0+
100 158 B |Fm-258 |370(43) µs |0+
100 158 C |Fm-258 |0.37 ms |
100 159 A |Fm-259 |1.5(3) s |3/2+#
100 159 BC |Fm-259 |1.5(3) s |
100 160 A* |Fm-260 |1# min |0+
100 160 B |Fm-260 |~4 ms |0+
100 160 C |Fm-260 |~4 ms |

[[User:Femto|Femto]] 11:38, 17 November 2005 (UTC)

===Talk===
----

== Mendelevium ==
== Mendelevium ==
{{archive top|[[WP:NOTAFORUM]]. Question already answered in the [[mendelevium]] article: no isotopes of fermium beta decay, and it's not our job to speculate on the hypothetical existence of one that does (which, by the way, is highly unlikely).}}
{{archive top|[[WP:NOTAFORUM]]. Question already answered in the [[mendelevium]] article: no isotopes of fermium beta decay, and it's not our job to speculate on the hypothetical existence of one that does (which, by the way, is highly unlikely).}}
Theoretically, is there an isotope of Fermium that decays into Mendelevium? So far, by extending the rn-process, I have gotten this far, but none decay into Mendelevium. Could maybe an extremely neutron-rich isotope decay into Mendelevium, and if so, what is it/could it be? [[User:32ieww|32ieww]] ([[User talk:32ieww|talk]]) 19:44, 11 February 2017 (UTC)
Theoretically, is there an isotope of Fermium that decays into Mendelevium? So far, by extending the rn-process, I have gotten this far, but none decay into Mendelevium. Could maybe an extremely neutron-rich isotope decay into Mendelevium, and if so, what is it/could it be? [[User:32ieww|32ieww]] ([[User talk:32ieww|talk]]) 19:44, 11 February 2017 (UTC)
{{archive bottom}}
{{archive bottom}}
:It's not ''that'' unlikely. [[:File:Superheavy decay modes predicted.png|Probably a lot would]]. The problem is that they're all probably heavier than 260, so there'd be no way to reach them at present. Or rather, there [[Peaceful nuclear explosion|is a way]], but it's banned by treaty. :) [[User:Double sharp|Double sharp]] ([[User talk:Double sharp|talk]]) 15:15, 8 May 2024 (UTC)

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== Spontaneous fission of <sup>242</sup>Fm ==

Should it be noted that <sup>242</sup>Fm is the lightest known nuclide to undergo purely spontaneous fission? [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 01:57, 23 October 2023 (UTC)

== Perhaps <sup>257</sup>Fm is the last beta-stable nuclide whose SF branch is not significant ==

After all, the only known heavier beta-stable nuclides are <sup>258</sup>Fm, <sup>260</sup>Fm, <sup>259</sup>Md, <sup>260</sup>No and <sup>262</sup>No, for all of which the only known decay mode is SF. [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 11:35, 28 November 2023 (UTC)

== Theoretical alpha half-life of <sup>258,259</sup>Fm ==

See [https://www.nndc.bnl.gov/ensnds/258/Fm/adopted.pdf here] for <sup>258</sup>Fm, and likewise for <sup>259</sup>Fm. Alpha decays for both isotopes are predicted to be very insignificant (alpha partial half-lives similar to longer than that of the most stable isotope of fermium <sup>257</sup>Fm). [[Special:Contributions/129.104.241.242|129.104.241.242]] ([[User talk:129.104.241.242|talk]]) 03:36, 5 May 2024 (UTC)

Latest revision as of 15:15, 8 May 2024

Mendelevium

[edit]

The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.


Theoretically, is there an isotope of Fermium that decays into Mendelevium? So far, by extending the rn-process, I have gotten this far, but none decay into Mendelevium. Could maybe an extremely neutron-rich isotope decay into Mendelevium, and if so, what is it/could it be? 32ieww (talk) 19:44, 11 February 2017 (UTC)[reply]

The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.
It's not that unlikely. Probably a lot would. The problem is that they're all probably heavier than 260, so there'd be no way to reach them at present. Or rather, there is a way, but it's banned by treaty. :) Double sharp (talk) 15:15, 8 May 2024 (UTC)[reply]
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Spontaneous fission of 242Fm

[edit]

Should it be noted that 242Fm is the lightest known nuclide to undergo purely spontaneous fission? 129.104.241.214 (talk) 01:57, 23 October 2023 (UTC)[reply]

Perhaps 257Fm is the last beta-stable nuclide whose SF branch is not significant

[edit]

After all, the only known heavier beta-stable nuclides are 258Fm, 260Fm, 259Md, 260No and 262No, for all of which the only known decay mode is SF. 129.104.241.214 (talk) 11:35, 28 November 2023 (UTC)[reply]

Theoretical alpha half-life of 258,259Fm

[edit]

See here for 258Fm, and likewise for 259Fm. Alpha decays for both isotopes are predicted to be very insignificant (alpha partial half-lives similar to longer than that of the most stable isotope of fermium 257Fm). 129.104.241.242 (talk) 03:36, 5 May 2024 (UTC)[reply]