Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Neutrino detection  





2 Occurrence  





3 See also  





4 References  














Chlorine-37






Afrikaans
Čeština
Español
فارسی
Nederlands
Русский
Türkçe
Українська
 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


Chlorine-37, 37Cl
General
Symbol37Cl
Nameschlorine-37, 37Cl, Cl-37
Protons (Z)17
Neutrons (N)20
Nuclide data
Natural abundance24.23%
Isotope mass36.965903 Da
Isotopes of chlorine
Complete table of nuclides

Chlorine-37 (37
Cl
), is one of the stable isotopesofchlorine, the other being chlorine-35 (35
Cl
). Its nucleus contains 17 protons and 20 neutrons for a total of 37 nucleons. Chlorine-37 accounts for 24.23% of natural chlorine, chlorine-35 accounting for 75.77%, giving chlorine atoms in bulk an apparent atomic weight of 35.45(1) g/mol.[1]

Remarkably, solar neutrinos were discovered by an experiment (Homestake Experiment) using a radiochemical method based on chlorine-37 transmutation.[2]

Neutrino detection[edit]

One of the historically important radiochemical methods of solar neutrino detection is based on inverse electron capture triggered by the absorption of an electron neutrino.[3] Chlorine-37 transmutes into argon-37 via the reaction[4]

37
Cl
+
ν
e
37
Ar
+
e
.

Argon-37 then de-excites itself via electron capture (half-life = 35 d) into chlorine-37 via the reaction

37
Ar
+
e
37
Cl
+
ν
e
.

These last reactions involve Auger electrons of specific energies.[3][5] The detection of these electrons confirms that a neutrino event took place. Detection methods involve several hundred thousand liters of carbon tetrachloride (CCl4) or tetrachloroethylene (C2Cl4) stored in underground tanks.[2][3][6]

Occurrence[edit]

The representative terrestrial abundance of chlorine-37 is 24.22(4)% of chlorine atoms,[7] with a normal range of 24.14–24.36% of chlorine atoms. When measuring deviations in isotopic composition, the usual reference point is "Standard Mean Ocean Chloride" (SMOC), although a NIST Standard Reference Material (975a) also exists. SMOC is known to be around 24.219% chlorine-37 and to have an atomic weight of around 35.4525.[8]

There is a known variation in the isotopic abundance of chlorine-37. This heavier isotope tends to be more prevalent in chloride minerals than in aqueous solutions such as sea water, although the isotopic composition of organochlorine compounds can vary in either direction from the SMOC standard in the range of several parts per thousand.[8]

See also[edit]

References[edit]

  1. ^ Prohaska, Thomas; et al. (2022-05-25), "Standard atomic weights of the elements 2021 (IUPAC Technical Report)", Pure and Applied Chemistry, vol. 94, no. 5, pp. 573–600, doi:10.1515/pac-2019-0603, ISSN 0033-4545, retrieved 2024-06-07{{citation}}: CS1 maint: date and year (link)
  • ^ a b J.N. Bahcall (1969). "Neutrinos from the Sun". Scientific American. 221 (1): 28–37. Bibcode:1969SciAm.221a..28B. doi:10.1038/scientificamerican0769-28.
  • ^ a b c Sutton, Christine (1992). Spaceship Neutrino. Cambridge University Press. pp. 151–152. ISBN 978-0-521-36404-1. OCLC 25246163. chlorine-37 neutrino.
  • ^ F.H. Shu (1982). The Physical Universe: An Introduction to Astronomy. University Science Books. p. 122. ISBN 978-0-935702-05-7. chlorine 37 neutrino.
  • ^ A.H. Snell, F. Pleasonton (1955). "Spectrometry of the Neutrino Recoils of Argon-37". Physical Review. 100 (5): 1396–1403. Bibcode:1955PhRv..100.1396S. doi:10.1103/PhysRev.100.1396.
  • ^ A. Bhatnagar, W. Livingston (2005). Fundamental of Solar Astronomy. World Scientific. pp. 87–89. ISBN 978-981-238-244-3.
  • ^ Rosman, K. J. R.; Taylor, P. D. P. (1998), "Isotopic Compositions of the Elements 1997" (PDF), Pure and Applied Chemistry, 70 (1): 217–35, doi:10.1351/pac199870010217
  • ^ a b de Laeter, J. R.; et al. (2003), "Atomic Weights of the Elements: Review 2000", Pure and Applied Chemistry, 75 (6): 683–800, doi:10.1351/pac200375060683

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Chlorine-37&oldid=1233900783"

    Category: 
    Isotopes of chlorine
    Hidden categories: 
    CS1 maint: date and year
    Articles with short description
    Short description matches Wikidata
    Isotope content page
     



    This page was last edited on 11 July 2024, at 14:08 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki