Curium
Curium is a transuranic, radioactive chemical element with the symbol Cm and atomic number 96. This actinide element was named after eminent scientists Marie and Pierre Curie, both known for their research on radioactivity. Curium was first inte ...
(
96Cm) is an
artificial element with an atomic number of 96. Because it is an artificial element, a
standard atomic weight cannot be given, and it has no
stable isotopes. The first
isotope
Isotopes are two or more types of atoms that have the same atomic number (number of protons in their nuclei) and position in the periodic table (and hence belong to the same chemical element), and that differ in nucleon numbers (mass numbers) ...
synthesized was
242Cm in 1944, which has 146 neutrons.
There are 19 known
radioisotope
A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess nuclear energy, making it unstable. This excess energy can be used in one of three ways: emitted from the nucleus as gamma radiation; transferr ...
s ranging from
233Cm to
251Cm. There are also ten known
nuclear isomer
A nuclear isomer is a metastable state of an atomic nucleus, in which one or more nucleons (protons or neutrons) occupy excited state, higher energy levels than in the ground state of the same nucleus. "Metastable" describes nuclei whose excited ...
s. The longest-lived isotope is
247Cm, with
half-life
Half-life (symbol ) is the time required for a quantity (of substance) to reduce to half of its initial value. The term is commonly used in nuclear physics to describe how quickly unstable atoms undergo radioactive decay or how long stable ato ...
15.6 million years – orders of magnitude longer than that of any known isotope beyond curium, and long enough to study as a possible
extinct radionuclide
An extinct radionuclide is a radionuclide that was formed by nucleosynthesis before the formation of the Solar System, about 4.6 billion years ago, but has since decayed to virtually zero abundance and is no longer detectable as a primordial nuc ...
that would be produced by the
r-process
In nuclear astrophysics, the rapid neutron-capture process, also known as the ''r''-process, is a set of nuclear reactions that is responsible for the creation of approximately half of the atomic nuclei heavier than iron, the "heavy elements", ...
.
The longest-lived isomer is
246mCm with a half-life of 1.12 seconds.
List of isotopes
, -
, rowspan=2,
233Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 137
, rowspan=2, 233.05077(8)
, rowspan=2, 27(10) s
,
β+ (80%)
,
233Am
, rowspan=2, 3/2+#
, -
,
α (20%)
,
229Pu
, -
, rowspan=3,
234Cm
, rowspan=3 style="text-align:right" , 96
, rowspan=3 style="text-align:right" , 138
, rowspan=3, 234.05016(2)
, rowspan=3, 52(9) s
, β
+ (71%)
,
234Am
, rowspan=3, 0+
, -
, α (27%)
,
230Pu
, -
, SF (2%)
, (various)
, -
, rowspan=2,
235Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 139
, rowspan=2, 235.05143(22)#
, rowspan=2, 300(+250−100) s
, β
+
,
235Am
, rowspan=2, 5/2+#
, -
, α
,
231Pu
, -
, rowspan=2,
236Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 140
, rowspan=2, 236.05141(22)#
, rowspan=2, 6.8(0.8) min
, β
+ (82%)
,
236Am
, rowspan=2, 0+
, -
, α (18%)
,
232Pu
, -
, rowspan=2,
237Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 141
, rowspan=2, 237.05290(22)#
, rowspan=2, 20# min
, β
+
,
237Am
, rowspan=2, 5/2+#
, -
, α
,
233Pu
, -
, rowspan=2,
238Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 142
, rowspan=2, 238.05303(4)
, rowspan=2, 2.4(1) h
,
EC (90%)
,
238Am
, rowspan=2, 0+
, -
, α (10%)
,
234Pu
, -
, rowspan=2,
239Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 143
, rowspan=2, 239.05496(11)#
, rowspan=2, 2.5(0.4) h
, β
+ (99.9%)
,
239Am
, rowspan=2, (7/2−)
, -
, α (.1%)
,
235Pu
, -
, rowspan=3,
240Cm
, rowspan=3 style="text-align:right" , 96
, rowspan=3 style="text-align:right" , 144
, rowspan=3, 240.0555295(25)
, rowspan=3, 27(1) d
, α (99.5%)
,
236Pu
, rowspan=3, 0+
, -
, EC (.5%)
,
240Am
, -
,
SF (3.9×10
−6%)
, (various)
, -
, rowspan=2,
241Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 145
, rowspan=2, 241.0576530(23)
, rowspan=2, 32.8(2) d
, EC (99%)
,
241Am
, rowspan=2, 1/2+
, -
, α (1%)
,
237Pu
, -
, rowspan=4,
242Cm
[Most common isotopes]
, rowspan=4 style="text-align:right" , 96
, rowspan=4 style="text-align:right" , 146
, rowspan=4, 242.0588358(20)
, rowspan=4, 162.8(2) d
, α
,
238Pu
, rowspan=4, 0+
, -
, SF (6.33×10
−6%)
, (various)
, -
,
CD (10
−14%)
[Heaviest known nuclide to undergo cluster decay]
,
208Pb
34Si
, -
, β
+β
+ (rare)
,
242Pu
, -
, style="text-indent:1em" ,
242mCm
, colspan="3" style="text-indent:2em" , 2800(100) keV
, 180(70) ns
,
,
,
, -
, rowspan=3,
243Cm
, rowspan=3 style="text-align:right" , 96
, rowspan=3 style="text-align:right" , 147
, rowspan=3, 243.0613891(22)
, rowspan=3, 29.1(1) y
, α (99.71%)
,
239Pu
, rowspan=3, 5/2+
, -
, EC (.29%)
,
243Am
, -
, SF (5.3×10
−9%)
, (various)
, -
, style="text-indent:1em" ,
243mCm
, colspan="3" style="text-indent:2em" , 87.4(1) keV
, 1.08(3) μs
, IT
,
243Cm
, 1/2+
, -
, rowspan=2,
244Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 148
, rowspan=2, 244.0627526(20)
, rowspan=2, 18.10(2) y
, α
,
240Pu
, rowspan=2, 0+
, -
, SF (1.34×10
−4%)
, (various)
, -
, style="text-indent:1em" ,
244m1Cm
, colspan="3" style="text-indent:2em" , 1040.188(12) keV
, 34(2) ms
,
IT
,
244Cm
, 6+
, -
, style="text-indent:1em" ,
244m2Cm
, colspan="3" style="text-indent:2em" , 1100(900)# keV
, >500 ns
, SF
, (various)
,
, -
, rowspan=2,
245Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 149
, rowspan=2, 245.0654912(22)
, rowspan=2, 8.5(1)×10
3 y
, α
,
241Pu
, rowspan=2, 7/2+
, -
, SF (6.1×10
−7%)
, (various)
, -
, style="text-indent:1em" ,
245mCm
, colspan="3" style="text-indent:2em" , 355.92(10) keV
, 290(20) ns
, IT
,
245Cm
, 1/2+
, -
, rowspan=2,
246Cm
, rowspan=2 style="text-align:right" , 96
, rowspan=2 style="text-align:right" , 150
, rowspan=2, 246.0672237(22)
, rowspan=2, 4.76(4)×10
3 y
, α (99.97%)
,
242Pu
, rowspan=2, 0+
, -
, SF (.0261%)
, (various)
, -
, style="text-indent:1em" ,
246mCm
, colspan="3" style="text-indent:2em" , 1179.66(13) keV
, 1.12(0.24) s
, IT
,
246Cm
, 8-
, -
,
247Cm
, style="text-align:right" , 96
, style="text-align:right" , 151
, 247.070354(5)
, 1.56(5)×10
7 y
, α
,
243Pu
, 9/2−
, -
, style="text-indent:1em" ,
247m1Cm
, colspan="3" style="text-indent:2em" , 227.38(19) keV
, 26.3(0.3) μs
, IT
,
247Cm
, 5/2+
, -
, style="text-indent:1em" ,
247m2Cm
, colspan="3" style="text-indent:2em" , 404.90(3) keV
, 100.6(0.6) ns
, IT
,
247Cm
, 1/2+
, -
, rowspan=3,
248Cm
, rowspan=3 style="text-align:right" , 96
, rowspan=3 style="text-align:right" , 152
, rowspan=3, 248.072349(5)
, rowspan=3, 3.48(6)×10
5 y
, α (91.74%)
,
244Pu
, rowspan=3, 0+
, -
, SF (8.26%)
, (various)
, -
, β
−β
− (rare)
,
248Cf
, -
, style="text-indent:1em" ,
248mCm
, colspan="3" style="text-indent:2em" , 1458.1(1) keV
, 146(18) μs
, IT
,
248Cm
, (8-)
, -
,
249Cm
, style="text-align:right" , 96
, style="text-align:right" , 153
, 249.075953(5)
, 64.15(3) min
, β
−
,
249Bk
, 1/2(+)
, -
, style="text-indent:1em" ,
249mCm
, colspan="3" style="text-indent:2em" , 48.758(17) keV
, 23 μs
, α
,
245Pu
, (7/2+)
, -
, rowspan=3,
250Cm
, rowspan=3 style="text-align:right" , 96
, rowspan=3 style="text-align:right" , 154
, rowspan=3, 250.078357(12)
, rowspan=3, 8300# y
, SF (74%)
[The nuclide with the lowest ]atomic number
The atomic number or nuclear charge number (symbol ''Z'') of a chemical element is the charge number of an atomic nucleus. For ordinary nuclei, this is equal to the proton number (''n''p) or the number of protons found in the nucleus of every ...
known to undergo spontaneous fission
Spontaneous fission (SF) is a form of radioactive decay that is found only in very heavy chemical elements. The nuclear binding energy of the elements reaches its maximum at an atomic mass number of about 56 (e.g., iron-56); spontaneous breakdo ...
as the main decay mode
, (various)
, rowspan=3, 0+
, -
, α (18%)
,
246Pu
, -
, β
− (8%)
,
250Bk
, -
,
251Cm
, style="text-align:right" , 96
, style="text-align:right" , 155
, 251.082285(24)
, 16.8(2) min
, β
−
,
251Bk
, (1/2+)
Actinides vs fission products
References
* Isotope masses from:
**
* Isotopic compositions and standard atomic masses from:
**
**
* Half-life, spin, and isomer data selected from the following sources.
**
**
**
{{Navbox element isotopes
Curium
Curium
Curium is a transuranic, radioactive chemical element with the symbol Cm and atomic number 96. This actinide element was named after eminent scientists Marie and Pierre Curie, both known for their research on radioactivity. Curium was first inte ...