Isotopes of krypton

Isotopes of krypton (₃₆Kr)
β+	79Br
γ	–
ε	81Br
Standard atomic weight Ar°(Kr)
	83.798±0.002; 83.798±0.002 (abridged);
	view; talk; edit;

There are 34 known isotopes of krypton (₃₆Kr) with atomic mass numbers from 67 to 103. Naturally occurring krypton is made of five stable isotopes and one (⁷⁸
Kr
) which is slightly radioactive with an extremely long half-life, plus traces of radioisotopes that are produced by cosmic rays in the atmosphere.

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Nuclide ^{[n 1]}	Z	N	Isotopic mass (Da)^[5] ^{[n 2]}^{[n 3]}	Half-life^[1] ^{[n 4]}^{[n 5]}	Decay mode^[1] ^{[n 6]}	Daughter isotope ^{[n 7]}^{[n 8]}	Spin and parity^[1] ^{[n 9]}^{[n 5]}	Natural abundance (mole fraction)
Nuclide ^{[n 1]}	Excitation energy			Half-life^[1] ^{[n 4]}^{[n 5]}	Decay mode^[1] ^{[n 6]}	Daughter isotope ^{[n 7]}^{[n 8]}	Spin and parity^[1] ^{[n 9]}^{[n 5]}	Normal proportion^[1]	Range of variation
⁶⁷Kr	36	31	66.98331(46)#	7.4(29) ms	β⁺? (63%)	⁶⁷Br	3/2-#
⁶⁷Kr	36	31	66.98331(46)#	7.4(29) ms	2p (37%)	⁶⁵Se	3/2-#
⁶⁸Kr	36	32	67.97249(54)#	21.6(33) ms	β⁺, p (>90%)	⁶⁷Se	0+
					β⁺? (<10%)	⁶⁸Br
					p?	⁶⁷Br
⁶⁹Kr	36	33	68.96550(32)#	27.9(8) ms	β⁺, p (94%)	⁶⁸Se	(5/2−)
⁶⁹Kr	36	33	68.96550(32)#	27.9(8) ms	β⁺ (6%)	⁶⁹Br	(5/2−)
⁷⁰Kr	36	34	69.95588(22)#	45.00(14) ms	β⁺ (>98.7%)	⁷⁰Br	0+
⁷⁰Kr	36	34	69.95588(22)#	45.00(14) ms	β⁺, p (<1.3%)	⁶⁹Se	0+
⁷¹Kr	36	35	70.95027(14)	98.8(3) ms	β⁺ (97.9%)	⁷¹Br	(5/2)−
⁷¹Kr	36	35	70.95027(14)	98.8(3) ms	β⁺, p (2.1%)	⁷⁰Se	(5/2)−
⁷²Kr	36	36	71.9420924(86)	17.16(18) s	β⁺	⁷²Br	0+
⁷³Kr	36	37	72.9392892(71)	27.3(10) s	β⁺ (99.75%)	⁷³Br	(3/2)−
⁷³Kr	36	37	72.9392892(71)	27.3(10) s	β⁺, p (0.25%)	⁷²Se	(3/2)−
^73mKr	433.55(13) keV			107(10) ns	IT	⁷³Kr	(9/2+)
⁷⁴Kr	36	38	73.9330840(22)	11.50(11) min	β⁺	⁷⁴Br	0+
⁷⁵Kr	36	39	74.9309457(87)	4.60(7) min	β⁺	⁷⁵Br	5/2+
⁷⁶Kr	36	40	75.9259107(43)	14.8(1) h	β⁺	⁷⁶Br	0+
⁷⁷Kr	36	41	76.9246700(21)	72.6(9) min	β⁺	⁷⁷Br	5/2+
^77mKr	66.50(5) keV			118(12) ns	IT	⁷⁷Kr	3/2−
⁷⁸Kr^{[n 10]}	36	42	77.92036634(33)	9.2 ^+5.5 _−2.6 ±1.3×10²¹ y^[2]	Double EC	⁷⁸Se	0+	0.00355(3)
⁷⁹Kr	36	43	78.9200829(37)	35.04(10) h	β⁺	⁷⁹Br	1/2−
^79mKr	129.77(5) keV			50(3) s	IT	⁷⁹Kr	7/2+
⁸⁰Kr	36	44	79.91637794(75)	Stable			0+	0.02286(10)
⁸¹Kr^{[n 11]}	36	45	80.9165897(12)	2.29(11)×10⁵ y	EC	⁸¹Br	7/2+	6×10⁻¹³^[6]
^81mKr	190.64(4) keV			13.10(3) s	IT	⁸¹Kr	1/2−
^81mKr	190.64(4) keV			13.10(3) s	EC (0.0025%)	⁸¹Br	1/2−
⁸²Kr	36	46	81.9134811537(59)	Stable			0+	0.11593(31)
⁸³Kr^{[n 12]}	36	47	82.914126516(9)	Stable			9/2+	0.11500(19)
^83m1Kr	9.4053(8) keV			156.8(5) ns	IT	⁸³Kr	7/2+
^83m2Kr	41.5575(7) keV			1.830(13) h	IT	⁸³Kr	1/2−
⁸⁴Kr^{[n 12]}	36	48	83.9114977271(41)	Stable			0+	0.56987(15)
^84mKr	3236.07(18) keV			1.83(4) μs	IT	⁸⁴Kr	8+
⁸⁵Kr^{[n 12]}	36	49	84.9125273(21)	10.728(7) y	β⁻	⁸⁵Rb	9/2+	1×10⁻¹¹^[6]
^85m1Kr	304.871(20) keV			4.480(8) h	β⁻ (78.8%)	⁸⁵Rb	1/2−
^85m1Kr	304.871(20) keV			4.480(8) h	IT (21.2%)	⁸⁵Kr	1/2−
^85m2Kr	1991.8(2) keV			1.82(5) μs	IT	⁸⁵Kr	(17/2+)
⁸⁶Kr^{[n 13]}^{[n 12]}	36	50	85.9106106247(40)	Observationally Stable^{[n 14]}			0+	0.17279(41)
⁸⁷Kr	36	51	86.91335476(26)	76.3(5) min	β⁻	⁸⁷Rb	5/2+
⁸⁸Kr	36	52	87.9144479(28)	2.825(19) h	β⁻	⁸⁸Rb	0+
⁸⁹Kr^{[n 12]}	36	53	88.9178354(23)	3.15(4) min	β⁻	⁸⁹Rb	3/2+
⁹⁰Kr	36	54	89.9195279(20)	32.32(9) s	β⁻	^90mRb	0+
⁹¹Kr	36	55	90.9238063(24)	8.57(4) s	β⁻	⁹¹Rb	5/2+
⁹¹Kr	36	55	90.9238063(24)	8.57(4) s	β⁻, n?	⁹⁰Rb	5/2+
⁹²Kr^{[n 12]}	36	56	91.9261731(29)	1.840(8) s	β⁻ (99.97%)	⁹²Rb	0+
⁹²Kr^{[n 12]}	36	56	91.9261731(29)	1.840(8) s	β⁻, n (0.0332%)	⁹¹Rb	0+
⁹³Kr	36	57	92.9311472(27)	1.287(10) s	β⁻ (98.05%)	⁹³Rb	1/2+
⁹³Kr	36	57	92.9311472(27)	1.287(10) s	β⁻, n (1.95%)	⁹²Rb	1/2+
⁹⁴Kr	36	58	93.934140(13)	212(4) ms	β⁻ (98.89%)	⁹⁴Rb	0+
⁹⁴Kr	36	58	93.934140(13)	212(4) ms	β⁻, n (1.11%)	⁹³Rb	0+
⁹⁵Kr	36	59	94.939711(20)	114(3) ms	β⁻ (97.13%)	⁹⁵Rb	1/2+
					β⁻, n (2.87%)	⁹⁴Rb
					β⁻, 2n?	⁹³Rb
^95mKr	195.5(3) keV			1.582(22) μs	IT	⁸⁵Kr	(7/2+)
⁹⁶Kr	36	60	95.942998(62)^[7]	80(8) ms	β⁻ (96.3%)	⁹⁶Rb	0+
⁹⁶Kr	36	60	95.942998(62)^[7]	80(8) ms	β⁻, n (3.7%)	⁹⁵Rb	0+
⁹⁷Kr	36	61	96.94909(14)	62.2(32) ms	β⁻ (93.3%)	⁹⁷Rb	3/2+#
					β⁻, n (6.7%)	⁹⁶Rb
					β⁻, 2n?	⁹⁵Rb
⁹⁸Kr	36	62	97.95264(32)#	42.8(36) ms	β⁻ (93.0%)	⁹⁸Rb	0+
					β⁻, n (7.0%)	⁹⁷Rb
					β⁻, 2n?	⁹⁶Rb
⁹⁹Kr	36	63	98.95878(43)#	40(11) ms	β⁻ (89%)	⁹⁹Rb	5/2−#
					β⁻, n (11%)	⁹⁸Rb
					β⁻, 2n?	⁹⁷Rb
¹⁰⁰Kr	36	64	99.96300(43)#	12(8) ms	β⁻	¹⁰⁰Rb	0+
					β⁻, n?	⁹⁹Rb
					β⁻, 2n?	⁹⁸Rb
¹⁰¹Kr	36	65	100.96932(54)#	9# ms [>400 ns]	β⁻?	¹⁰¹Rb	5/2+#
					β⁻, n?	¹⁰⁰Rb
					β⁻, 2n?	⁹⁹Rb
¹⁰²Kr^[8]	36	66					0+
¹⁰³Kr^[9]	36	67
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[n 1]
^mKr – Excited nuclear isomer.
[n 2]
( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
[n 3]
# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
[n 4]
Bold half-life – nearly stable, half-life longer than age of universe.
[n 5]
# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
[n 6]
Modes of decay:

n: Neutron emission
[n 7]
Bold italics symbol as daughter – Daughter product is nearly stable.
[n 8]
Bold symbol as daughter – Daughter product is stable.
[n 9]
( ) spin value – Indicates spin with weak assignment arguments.
[N 10]
Primordial radionuclide
[N 11]
Used to date groundwater
[N 12]
Fission product
[N 13]
Formerly used to define the meter
[N 14]
Believed to decay by β⁻β⁻ to ⁸⁶Sr

The isotopic composition refers to that in air.

Krypton-81

Krypton-81 is useful in determining how old the water beneath the ground is.^[10] 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.^[11] 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) groundwater and to determine their residence time in deep aquifers. One of the main technical limitations of the method is that it requires the sampling of very large volumes of water: several hundred liters or a few cubic meters of water. This is particularly challenging for dating pore water in deep clay aquitards with very low hydraulic conductivity.^[12]

Krypton-85

Krypton-85 has a half-life of about 10.75 years. This isotope is produced by the nuclear fission of uranium and plutonium in nuclear weapons testing and in nuclear reactors, as well as by cosmic rays. An important goal of the Limited Nuclear Test Ban Treaty of 1963 was to eliminate the release of such radioisotopes into the atmosphere, and since 1963 much of that krypton-85 has had time to decay. However, it is almost inevitable that krypton-85 is released during the reprocessing of fuel rods from nuclear reactors.^[13]

Atmospheric concentration

The atmospheric concentration of krypton-85 around the North Pole is about 30 percent higher than that at the Amundsen–Scott South Pole Station because nearly all of the world's nuclear reactors and all of its major nuclear reprocessing plants are located in the northern hemisphere, and also well-north of the equator.^[14] To be more specific, those nuclear reprocessing plants with significant capacities are located in the United States, the United Kingdom, the French Republic, the Russian Federation, Mainland China (PRC), Japan, India, and Pakistan.

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.^[15]

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.

[1]
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.
[2]
Patrignani, C.; et al. (Particle Data Group) (2016). "Review of Particle Physics". Chinese Physics C. 40 (10): 100001. Bibcode:2016ChPhC..40j0001P. doi:10.1088/1674-1137/40/10/100001. See p. 768
[3]
"Standard Atomic Weights: Krypton". CIAAW. 2001.
[4]
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.
[5]
Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*". Chinese Physics C. 45 (3): 030003. doi:10.1088/1674-1137/abddaf.
[6]
Lu, Zheng-Tian (1 March 2013). "What trapped atoms reveal about global groundwater". Physics Today. 66 (3): 74–75. Bibcode:2013PhT....66c..74L. doi:10.1063/PT.3.1926. Retrieved 29 June 2024.
[7]
Smith, Matthew B.; Murböck, Tobias; Dunling, Eleanor; Jacobs, Andrew; Kootte, Brian; Lan, Yang; Leistenschneider, Erich; Lunney, David; Lykiardopoulou, Eleni Marina; Mukul, Ish; Paul, Stefan F.; Reiter, Moritz P.; Will, Christian; Dilling, Jens; Kwiatkowski, Anna A. (2020). "High-precision mass measurement of neutron-rich 96Kr". Hyperfine Interactions. 241 (1): 59. Bibcode:2020HyInt.241...59S. doi:10.1007/s10751-020-01722-2. S2CID 220512482.
[8]
Sumikama, T.; et al. (2021). "Observation of new neutron-rich isotopes in the vicinity of Zr110". Physical Review C. 103 (1): 014614. Bibcode:2021PhRvC.103a4614S. doi:10.1103/PhysRevC.103.014614. hdl:10261/260248. S2CID 234019083.
[9]
Shimizu, Y.; Kubo, T.; Sumikama, T.; Fukuda, N.; Takeda, H.; Suzuki, H.; Ahn, D. S.; Inabe, N.; Kusaka, K.; Ohtake, M.; Yanagisawa, Y.; Yoshida, K.; Ichikawa, Y.; Isobe, T.; Otsu, H.; Sato, H.; Sonoda, T.; Murai, D.; Iwasa, N.; Imai, N.; Hirayama, Y.; Jeong, S. C.; Kimura, S.; Miyatake, H.; Mukai, M.; Kim, D. G.; Kim, E.; Yagi, A. (8 April 2024). "Production of new neutron-rich isotopes near the N = 60 isotones Ge 92 and As 93 by in-flight fission of a 345 MeV/nucleon U 238 beam". Physical Review C. 109 (4): 044313. doi:10.1103/PhysRevC.109.044313.
[10]
Le-Yi Tu, Guo-Min Yang, Cun-Feng Cheng, Gu-Liang Liu, Xiang-Yang Zhang, and Shui-Ming Hu (2014). "Analysis of Krypton-85 and Krypton-81 in a Few Liters of Air". Analytical Chemistry. 86 (8): 4002–4007.{{cite journal}}: CS1 maint: multiple names: authors list (link)
[11]
Leya, I.; Gilabert, E.; Lavielle, B.; Wiechert, U.; Wieler, W. (2004). "Production rates for cosmogenic krypton and argon isotopes in H-chondrites with known ³⁶Cl-³⁶Ar ages" (PDF). Antarctic Meteorite Research. 17: 185–199. Bibcode:2004AMR....17..185L.
[12]
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). University of Tennessee, Institute for Rare Isotope Measurements. pp. 4–7. doi:10.2172/809813.
[13]
"Environmental Consequences Of Atmospheric Krypton-85" (PDF). p. 8. Retrieved 2024-12-08.
[14]
"Resources on Isotopes". U.S. Geological Survey. Archived from the original on 2001-09-24. Retrieved 2007-03-20.
[15]
Baird, K. M.; Howlett, L. E. (1963). "The International Length Standard". Applied Optics. 2 (5): 455–463. Bibcode:1963ApOpt...2..455B. doi:10.1364/AO.2.000455.

Sources

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.

Brookhaven National Laboratory: Krypton-101 information Archived 2017-10-18 at the Wayback Machine

[5] [n 1]
^mKr – Excited nuclear isomer.

[7] [n 2]
( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.

[TMS-8] [n 3]
# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).

[9] [n 4]
Bold half-life – nearly stable, half-life longer than age of universe.

[TNN-10] [n 5]
# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).

[11] [n 6]
Modes of decay:

n: Neutron emission

[12] [n 7]
Bold italics symbol as daughter – Daughter product is nearly stable.

[13] [n 8]
Bold symbol as daughter – Daughter product is stable.

[14] [n 9]
( ) spin value – Indicates spin with weak assignment arguments.

[15] [N 10]
Primordial radionuclide

[16] [N 11]
Used to date groundwater

[FP-18] [N 12]
Fission product

[19] [N 13]
Formerly used to define the meter

[20] [N 14]
Believed to decay by β⁻β⁻ to ⁸⁶Sr

[NUBASE2020-1] [1]
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.

[Patrignani2016-2] [2]
Patrignani, C.; et al. (Particle Data Group) (2016). "Review of Particle Physics". Chinese Physics C. 40 (10): 100001. Bibcode:2016ChPhC..40j0001P. doi:10.1088/1674-1137/40/10/100001. See p. 768

[3] [3]
"Standard Atomic Weights: Krypton". CIAAW. 2001.

[CIAAW2021-4] [4]
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.

[AME2020_II-6] [5]
Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*". Chinese Physics C. 45 (3): 030003. doi:10.1088/1674-1137/abddaf.

[zheng-tian-17] [6]
Lu, Zheng-Tian (1 March 2013). "What trapped atoms reveal about global groundwater". Physics Today. 66 (3): 74–75. Bibcode:2013PhT....66c..74L. doi:10.1063/PT.3.1926. Retrieved 29 June 2024.

[21] [7]
Smith, Matthew B.; Murböck, Tobias; Dunling, Eleanor; Jacobs, Andrew; Kootte, Brian; Lan, Yang; Leistenschneider, Erich; Lunney, David; Lykiardopoulou, Eleni Marina; Mukul, Ish; Paul, Stefan F.; Reiter, Moritz P.; Will, Christian; Dilling, Jens; Kwiatkowski, Anna A. (2020). "High-precision mass measurement of neutron-rich 96Kr". Hyperfine Interactions. 241 (1): 59. Bibcode:2020HyInt.241...59S. doi:10.1007/s10751-020-01722-2. S2CID 220512482.

[101Br-aps-22] [8]
Sumikama, T.; et al. (2021). "Observation of new neutron-rich isotopes in the vicinity of Zr110". Physical Review C. 103 (1): 014614. Bibcode:2021PhRvC.103a4614S. doi:10.1103/PhysRevC.103.014614. hdl:10261/260248. S2CID 234019083.

[23] [9]
Shimizu, Y.; Kubo, T.; Sumikama, T.; Fukuda, N.; Takeda, H.; Suzuki, H.; Ahn, D. S.; Inabe, N.; Kusaka, K.; Ohtake, M.; Yanagisawa, Y.; Yoshida, K.; Ichikawa, Y.; Isobe, T.; Otsu, H.; Sato, H.; Sonoda, T.; Murai, D.; Iwasa, N.; Imai, N.; Hirayama, Y.; Jeong, S. C.; Kimura, S.; Miyatake, H.; Mukai, M.; Kim, D. G.; Kim, E.; Yagi, A. (8 April 2024). "Production of new neutron-rich isotopes near the N = 60 isotones Ge 92 and As 93 by in-flight fission of a 345 MeV/nucleon U 238 beam". Physical Review C. 109 (4): 044313. doi:10.1103/PhysRevC.109.044313.

[24] [10]
Le-Yi Tu, Guo-Min Yang, Cun-Feng Cheng, Gu-Liang Liu, Xiang-Yang Zhang, and Shui-Ming Hu (2014). "Analysis of Krypton-85 and Krypton-81 in a Few Liters of Air". Analytical Chemistry. 86 (8): 4002–4007.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[cosmo-25] [11]
Leya, I.; Gilabert, E.; Lavielle, B.; Wiechert, U.; Wieler, W. (2004). "Production rates for cosmogenic krypton and argon isotopes in H-chondrites with known ³⁶Cl-³⁶Ar ages" (PDF). Antarctic Meteorite Research. 17: 185–199. Bibcode:2004AMR....17..185L.

[26] [12]
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). University of Tennessee, Institute for Rare Isotope Measurements. pp. 4–7. doi:10.2172/809813.

[27] [13]
"Environmental Consequences Of Atmospheric Krypton-85" (PDF). p. 8. Retrieved 2024-12-08.

[28] [14]
"Resources on Isotopes". U.S. Geological Survey. Archived from the original on 2001-09-24. Retrieved 2007-03-20.

[29] [15]
Baird, K. M.; Howlett, L. E. (1963). "The International Length Standard". Applied Optics. 2 (5): 455–463. Bibcode:1963ApOpt...2..455B. doi:10.1364/AO.2.000455.

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Isotopes of krypton

Krypton-81

Krypton-85

Atmospheric concentration

Krypton-86

Others

Sources

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Isotopes of krypton

Krypton-81

Krypton-85

Atmospheric concentration

Krypton-86

Others

Sources

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List of isotopes

Notable isotopes

References

External links