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Standard atomic weight Ar°(Cr) | ||||||||||||||||||||||||||||||||||||||
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Naturally occurring chromium (24Cr) is composed of four stable isotopes; 50Cr, 52Cr, 53Cr, and 54Cr with 52Cr being the most abundant (83.789% natural abundance). 50Cr is suspected of decaying by β+β+ to 50Ti with a half-life of (more than) 1.8×1017 years. Twenty-two radioisotopes, all of which are entirely synthetic, have been characterized, the most stable being 51Cr with a half-life of 27.7 days. All of the remaining radioactive isotopes have half-lives that are less than 24 hours and the majority of these have half-lives that are less than 1 minute. This element also has two meta states, 45mCr, the more stable one, and 59mCr, the least stable isotope or isomer.
53Cr is the radiogenic decay product of 53Mn. Chromium isotopic contents are typically combined with manganese isotopic contents and have found application in isotope geology. Mn-Cr isotope ratios reinforce the evidence from 26Al and 107Pd for the early history of the Solar System. Variations in 53Cr/52Cr and Mn/Cr ratios from several meteorites indicate an initial 53Mn/55Mn ratio that suggests Mn-Cr isotope systematics must result from in-situ decay of 53Mn in differentiated planetary bodies. Hence 53Cr provides additional evidence for nucleosynthetic processes immediately before coalescence of the Solar System. The same isotope is preferentially involved in certain leaching reactions, thereby allowing its abundance in seawater sediments to be used as a proxy for atmospheric oxygen concentrations.[4]
The isotopes of chromium range from 42Cr to 70Cr. The primary decay mode before the most abundant stable isotope, 52Cr, is electron capture and the primary mode after is beta decay.
List of isotopes
[edit]Nuclide [n 1] |
Z | N | Isotopic mass (Da) [n 2][n 3] |
Half-life [n 4] |
Decay mode [n 5] |
Daughter isotope [n 6] |
Spin and parity [n 7][n 4] |
Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy[n 4] | Normal proportion | Range of variation | |||||||||||||||||
42Cr | 24 | 18 | 42.00643(32)# | 14(3) ms [13(+4-2) ms] |
β+ (>99.9%) | 42V | 0+ | ||||||||||||
2p (<.1%) | 40Ti | ||||||||||||||||||
43Cr | 24 | 19 | 42.99771(24)# | 21.6(7) ms | β+ (71%) | 43V | (3/2+) | ||||||||||||
β+, p (23%) | 42Ti | ||||||||||||||||||
β+, 2p (6%) | 41Sc | ||||||||||||||||||
β+, α (<.1%) | 39Sc | ||||||||||||||||||
44Cr | 24 | 20 | 43.98555(5)# | 54(4) ms [53(+4-3) ms] |
β+ (93%) | 44V | 0+ | ||||||||||||
β+, p (7%) | 43Ti | ||||||||||||||||||
45Cr | 24 | 21 | 44.97964(54) | 50(6) ms | β+ (73%) | 45V | 7/2−# | ||||||||||||
β+, p (27%) | 44Ti | ||||||||||||||||||
45mCr | 50(100)# keV | 1# ms | IT | 45Cr | 3/2+# | ||||||||||||||
β+ | 45V | ||||||||||||||||||
46Cr | 24 | 22 | 45.968359(21) | 0.26(6) s | β+ | 46V | 0+ | ||||||||||||
47Cr | 24 | 23 | 46.962900(15) | 500(15) ms | β+ | 47V | 3/2− | ||||||||||||
48Cr | 24 | 24 | 47.954032(8) | 21.56(3) h | β+ | 48V | 0+ | ||||||||||||
49Cr | 24 | 25 | 48.9513357(26) | 42.3(1) min | β+ | 49V | 5/2− | ||||||||||||
50Cr | 24 | 26 | 49.9460442(11) | Observationally Stable[n 8] | 0+ | 0.04345(13) | 0.04294–0.04345 | ||||||||||||
51Cr | 24 | 27 | 50.9447674(11) | 27.7025(24) d | EC | 51V | 7/2− | ||||||||||||
52Cr | 24 | 28 | 51.9405075(8) | Stable | 0+ | 0.83789(18) | 0.83762–0.83790 | ||||||||||||
53Cr | 24 | 29 | 52.9406494(8) | Stable | 3/2− | 0.09501(17) | 0.09501–0.09553 | ||||||||||||
54Cr | 24 | 30 | 53.9388804(8) | Stable | 0+ | 0.02365(7) | 0.02365–0.02391 | ||||||||||||
55Cr | 24 | 31 | 54.9408397(8) | 3.497(3) min | β− | 55Mn | 3/2− | ||||||||||||
56Cr | 24 | 32 | 55.9406531(20) | 5.94(10) min | β− | 56Mn | 0+ | ||||||||||||
57Cr | 24 | 33 | 56.943613(2) | 21.1(10) s | β− | 57Mn | (3/2−) | ||||||||||||
58Cr | 24 | 34 | 57.94435(22) | 7.0(3) s | β− | 58Mn | 0+ | ||||||||||||
59Cr | 24 | 35 | 58.94859(26) | 460(50) ms | β− | 59Mn | 5/2−# | ||||||||||||
59mCr | 503.0(17) keV | 96(20) μs | (9/2+) | ||||||||||||||||
60Cr | 24 | 36 | 59.95008(23) | 560(60) ms | β− | 60Mn | 0+ | ||||||||||||
61Cr | 24 | 37 | 60.95472(27) | 261(15) ms | β− (>99.9%) | 61Mn | 5/2−# | ||||||||||||
β−, n (<.1%) | 60Mn | ||||||||||||||||||
62Cr | 24 | 38 | 61.95661(36) | 199(9) ms | β− (>99.9%) | 62Mn | 0+ | ||||||||||||
β−, n | 61Mn | ||||||||||||||||||
63Cr | 24 | 39 | 62.96186(32)# | 129(2) ms | β− | 63Mn | (1/2−)# | ||||||||||||
β−, n | 62Mn | ||||||||||||||||||
64Cr | 24 | 40 | 63.96441(43)# | 43(1) ms | β− | 64Mn | 0+ | ||||||||||||
65Cr | 24 | 41 | 64.97016(54)# | 27(3) ms | β− | 65Mn | (1/2−)# | ||||||||||||
66Cr | 24 | 42 | 65.97338(64)# | 10(6) ms | β− | 66Mn | 0+ | ||||||||||||
67Cr | 24 | 43 | 66.97955(75)# | 10# ms [>300 ns] |
β− | 67Mn | 1/2−# | ||||||||||||
68Cr[5] | 24 | 44 | 67.98316(54)# | 10# ms (>620 ns) |
β−?[n 9] | 68Mn | 0+ | ||||||||||||
β−, n?[n 9] | 67Mn | ||||||||||||||||||
β−, 2n?[n 9] | 66Mn | ||||||||||||||||||
69Cr[6] | 24 | 45 | 68.98966(54)# | 6# ms (>620 ns) |
β−?[n 9] | 69Mn | 7/2+# | ||||||||||||
β−, n?[n 9] | 68Mn | ||||||||||||||||||
β−, 2n?[n 9] | 67Mn | ||||||||||||||||||
70Cr[6] | 24 | 46 | 69.99395(64)# | 6# ms (>620 ns) |
β−?[n 9] | 70Mn | 0+ | ||||||||||||
β−, n?[n 9] | 69Mn | ||||||||||||||||||
β−, 2n?[n 9] | 68Mn | ||||||||||||||||||
This table header & footer: |
- ^ mCr – Excited nuclear isomer.
- ^ ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
- ^ # – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
- ^ a b c # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
- ^
Modes of decay:
EC: Electron capture IT: Isomeric transition
p: Proton emission - ^ Bold symbol as daughter – Daughter product is stable.
- ^ ( ) spin value – Indicates spin with weak assignment arguments.
- ^ Suspected of decaying by double electron capture to 50Ti with a half-life of no less than 1.3×1018 a
- ^ a b c d e f g h i Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide.
Chromium-51
[edit]Chromium-51 is a synthetic radioactive isotope of chromium having a half-life of 27.7 days and decaying by electron capture with emission of gamma rays (0.32 MeV); it is used to label red blood cells for measurement of mass or volume, survival time, and sequestration studies, for the diagnosis of gastrointestinal bleeding, and to label platelets to study their survival. It has a role as a radioactive label. Chromium Cr-51 has been used as a radioactive label for decades. It is used as a diagnostic radiopharmaceutical agent in nephrology to determine glomerular filtration rate, and in hematology to determine red blood cell volume or mass, study the red blood cell survival time and evaluate blood loss.[7]
External links
[edit]References
[edit]- ^ Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae.
- ^ "Standard Atomic Weights: Chromium". CIAAW. 1983.
- ^ Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04). "Standard atomic weights of the elements 2021 (IUPAC Technical Report)". Pure and Applied Chemistry. doi:10.1515/pac-2019-0603. ISSN 1365-3075.
- ^ R. Frei; C. Gaucher; S. W. Poulton; D. E. Canfield (2009). "Fluctuations in Precambrian atmospheric oxygenation recorded by chromium isotopes". Nature. 461 (7261): 250–3. Bibcode:2009Natur.461..250F. doi:10.1038/nature08266. PMID 19741707. S2CID 4373201.
- ^ Tarasov, O. B.; et al. (April 2009). "Evidence for a Change in the Nuclear Mass Surface with the Discovery of the Most Neutron-Rich Nuclei with 17 ≤ Z ≤ 25". Physical Review Letters. 102 (14): 142501. arXiv:0903.1975. Bibcode:2009PhRvL.102n2501T. doi:10.1103/PhysRevLett.102.142501. PMID 19392430. S2CID 42329617. Retrieved 3 January 2023.
- ^ a b Tarasov, O. B.; et al. (May 2013). "Production cross sections from 82 Se fragmentation as indications of shell effects in neutron-rich isotopes close to the drip-line". Physical Review C. 87 (5): 054612. arXiv:1303.7164. Bibcode:2013PhRvC..87e4612T. doi:10.1103/PhysRevC.87.054612.
- ^ "Chromium-51".
- Isotope masses from:
- Audi, Georges; Bersillon, Olivier; Blachot, Jean; Wapstra, Aaldert Hendrik (2003), "The NUBASE evaluation of nuclear and decay properties", Nuclear Physics A, 729: 3–128, Bibcode:2003NuPhA.729....3A, doi:10.1016/j.nuclphysa.2003.11.001
- Isotopic compositions and standard atomic masses from:
- de Laeter, John Robert; Böhlke, John Karl; De Bièvre, Paul; Hidaka, Hiroshi; Peiser, H. Steffen; Rosman, Kevin J. R.; Taylor, Philip D. P. (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry. 75 (6): 683–800. doi:10.1351/pac200375060683.
- Wieser, Michael E. (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure and Applied Chemistry. 78 (11): 2051–2066. doi:10.1351/pac200678112051.
- "News & Notices: Standard Atomic Weights Revised". International Union of Pure and Applied Chemistry. 19 October 2005.
- Half-life, spin, and isomer data selected from the following sources.
- Audi, Georges; Bersillon, Olivier; Blachot, Jean; Wapstra, Aaldert Hendrik (2003), "The NUBASE evaluation of nuclear and decay properties", Nuclear Physics A, 729: 3–128, Bibcode:2003NuPhA.729....3A, doi:10.1016/j.nuclphysa.2003.11.001
- National Nuclear Data Center. "NuDat 2.x database". Brookhaven National Laboratory.
- Holden, Norman E. (2004). "11. Table of the Isotopes". In Lide, David R. (ed.). CRC Handbook of Chemistry and Physics (85th ed.). Boca Raton, Florida: CRC Press. ISBN 978-0-8493-0485-9.
Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
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