Isotopes of krypton
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talk |
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There are 34 known
cosmic rays in the atmosphere
.
List of isotopes
Nuclide [n 1] |
Z | N | Isotopic mass (Da) [n 2][n 3] |
Half-life [n 4][n 5] |
Daughter isotope [n 7][n 8] |
Natural abundance (mole fraction) | |||||||||||||
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Excitation energy | Normal proportion | Range of variation | |||||||||||||||||
69Kr | 36 | 33 | 68.96518(43)# | 32(10) ms | β+ | 69Br | 5/2−# | ||||||||||||
70Kr | 36 | 34 | 69.95526(41)# | 52(17) ms | β+ | 70Br | 0+ | ||||||||||||
71Kr | 36 | 35 | 70.94963(70) | 100(3) ms | β+ (94.8%) | 71Br | (5/2)− | ||||||||||||
β+, p (5.2%) | 70Se | ||||||||||||||||||
72Kr | 36 | 36 | 71.942092(9) | 17.16(18) s | β+ | 72Br | 0+ | ||||||||||||
73Kr | 36 | 37 | 72.939289(7) | 28.6(6) s | β+ (99.32%) | 73Br | 3/2− | ||||||||||||
β+, p (.68%) | 72Se | ||||||||||||||||||
73mKr | 433.66(12) keV | 107(10) ns | (9/2+) | ||||||||||||||||
74Kr | 36 | 38 | 73.9330844(22) | 11.50(11) min | β+ | 74Br | 0+ | ||||||||||||
75Kr | 36 | 39 | 74.930946(9) | 4.29(17) min | β+ | 75Br | 5/2+ | ||||||||||||
76Kr | 36 | 40 | 75.925910(4) | 14.8(1) h | β+ | 76Br | 0+ | ||||||||||||
77Kr | 36 | 41 | 76.9246700(21) | 74.4(6) min | β+ | 77Br | 5/2+ | ||||||||||||
78Kr[n 10] | 36 | 42 | 77.9203648(12) | 9.2 +5.5 −2.6 ±1.3×1021 y[2] |
Double EC | 78Se | 0+ | 0.00355(3) | |||||||||||
79Kr | 36 | 43 | 78.920082(4) | 35.04(10) h | β+ | 79Br | 1/2− | ||||||||||||
79mKr | 129.77(5) keV | 50(3) s | 7/2+ | ||||||||||||||||
80Kr | 36 | 44 | 79.9163790(16) | Stable | 0+ | 0.02286(10) | |||||||||||||
81Kr[n 11] | 36 | 45 | 80.9165920(21) | 2.29(11)×105 y | EC | 81Br | 7/2+ | trace | |||||||||||
81mKr | 190.62(4) keV | 13.10(3) s | IT (99.975%)
|
81Kr | 1/2− | ||||||||||||||
EC (.025%) | 81Br | ||||||||||||||||||
82Kr | 36 | 46 | 81.9134836(19) | Stable | 0+ | 0.11593(31) | |||||||||||||
83Kr[n 12] | 36 | 47 | 82.914136(3) | Stable | 9/2+ | 0.11500(19) | |||||||||||||
83m1Kr | 9.4053(8) keV | 154.4(11) ns | 7/2+ | ||||||||||||||||
83m2Kr | 41.5569(10) keV | 1.83(2) h | IT | 83Kr | 1/2− | ||||||||||||||
84Kr[n 12] | 36 | 48 | 83.911507(3) | Stable | 0+ | 0.56987(15) | |||||||||||||
84mKr | 3236.02(18) keV | 1.89(4) µs | 8+ | ||||||||||||||||
85Kr[n 12] | 36 | 49 | 84.9125273(21) | 10.776(3) y | β− | 85Rb | 9/2+ | trace | |||||||||||
85m1Kr | 304.871(20) keV | 4.480(8) h | β− (78.6%) | 85Rb | 1/2− | ||||||||||||||
IT (21.4%) | 85Kr | ||||||||||||||||||
85m2Kr | 1991.8(13) keV | 1.6(7) µs [1.2(+10-4) µs] |
(17/2+) | ||||||||||||||||
86Kr[n 13][n 12] | 36 | 50 | 85.91061073(11) | Observationally Stable[n 14]
|
0+ | 0.17279(41) | |||||||||||||
87Kr | 36 | 51 | 86.91335486(29) | 76.3(5) min | β− | 87Rb | 5/2+ | ||||||||||||
88Kr | 36 | 52 | 87.914447(14) | 2.84(3) h | β− | 88Rb | 0+ | ||||||||||||
89Kr[n 12] | 36 | 53 | 88.91763(6) | 3.15(4) min | β− | 89Rb | 3/2(+#) | ||||||||||||
90Kr | 36 | 54 | 89.919517(20) | 32.32(9) s | β− | 90mRb | 0+ | ||||||||||||
91Kr | 36 | 55 | 90.92345(6) | 8.57(4) s | β− | 91Rb | 5/2(+) | ||||||||||||
92Kr[n 12] | 36 | 56 | 91.926156(13) | 1.840(8) s | β− (99.96%) | 92Rb | 0+ | ||||||||||||
β−, n (.033%) | 91Rb | ||||||||||||||||||
93Kr | 36 | 57 | 92.93127(11) | 1.286(10) s | β− (98.05%) | 93Rb | 1/2+ | ||||||||||||
β−, n (1.95%) | 92Rb | ||||||||||||||||||
94Kr | 36 | 58 | 93.93436(32)# | 210(4) ms | β− (94.3%) | 94Rb | 0+ | ||||||||||||
β−, n (5.7%) | 93Rb | ||||||||||||||||||
95Kr | 36 | 59 | 94.93984(43)# | 114(3) ms | β− | 95Rb | 1/2(+) | ||||||||||||
96Kr | 36 | 60 | 95.942998(62)[7] | 80(7) ms | β− | 96Rb | 0+ | ||||||||||||
97Kr | 36 | 61 | 96.94856(54)# | 63(4) ms | β− | 97Rb | 3/2+# | ||||||||||||
β−, n | 96Rb | ||||||||||||||||||
98Kr | 36 | 62 | 97.95191(64)# | 46(8) ms | 0+ | ||||||||||||||
99Kr | 36 | 63 | 98.95760(64)# | 40(11) ms | (3/2+)# | ||||||||||||||
100Kr | 36 | 64 | 99.96114(54)# | 10# ms [>300 ns] |
0+ | ||||||||||||||
101Kr | 36 | 65 | unknown | >635 ns | β−, 2n | 99Rb | unknown | ||||||||||||
β−, n | 100Rb | ||||||||||||||||||
β− | 101Rb | ||||||||||||||||||
102Kr[8] | 36 | 66 | 0+ | ||||||||||||||||
This table header & footer: |
- ^ mKr – 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).
- age of universe.
- ^ a b # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
- ^
Modes of decay:
n: Neutron emission - ^ Bold italics symbol as daughter – Daughter product is nearly stable.
- ^ Bold symbol as daughter – Daughter product is stable.
- ^ ( ) spin value – Indicates spin with weak assignment arguments.
- ^ Primordial radionuclide
- ^ Used to date groundwater
- ^ Fission product
- ^ Formerly used to define the meter
- ^ Believed to decay by β−β− to 86Sr
- The isotopic composition refers to that in air.
Notable isotopes
This section needs additional citations for verification. (May 2018) |
Krypton-81
This section needs expansion with: Usage in hydrogeology, ATC=V09. You can help by adding to it. (October 2019) |
Radioactive krypton-81 is the product of
spallation reactions with cosmic rays striking gases present in the Earth atmosphere, along with the six stable or nearly stable krypton isotopes.[9] Krypton-81 has a half-life
of about 229,000 years.
Krypton-81 is used for dating ancient (50,000- to 800,000-year-old)
aquitards with very low hydraulic conductivity.[10]
Krypton-85
Krypton-85 has a half-life of about 10.75 years. This isotope is produced by the
fuel rods from nuclear reactors.[citation needed
]
Atmospheric concentration
The atmospheric concentration of krypton-85 around the
To be more specific, those .Krypton-86
Krypton-86 was formerly used to define the meter from 1960 until 1983, when the definition of the meter was based on the wavelength of the 606 nm (orange) spectral line of a krypton-86 atom.[12]
Others
All other
radioisotopes of krypton have half-lives of less than one day, except for krypton-79, a positron emitter
with a half-life of about 35.0 hours.
References
- .
- ^ a b Patrignani, C.; et al. (. See p. 768
- ^ "Standard Atomic Weights: Krypton". CIAAW. 2001.
- ISSN 1365-3075.
- ^ "Chart of Nuclides". Brookhaven National Laboratory. Archived from the original on 2017-10-18. Retrieved 2011-11-21.
- S2CID 234019083.
- S2CID 220512482.
- S2CID 234019083.
- Bibcode:2004AMR....17..185L.
- ^
N. Thonnard; L. D. MeKay; T. C. Labotka (2001). Development of Laser-Based Resonance Ionization Techniques for 81-Kr and 85-Kr Measurements in the Geosciences (PDF) (Report). doi:10.2172/809813.
- U.S. Geological Survey. Archived from the originalon 2001-09-24. Retrieved 2007-03-20.
- .
Sources
- Isotope masses from:
- Audi, Georges; Bersillon, Olivier; Blachot, Jean;
- Isotopic compositions and standard atomic masses from:
- .
- Wieser, Michael E. (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". .
- "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;
- 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.). ISBN 978-0-8493-0485-9.
External links
- Brookhaven National Laboratory: Krypton-101 information Archived 2017-10-18 at the Wayback Machine