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Whole number rule

From Wikipedia, the free encyclopedia
Rule of thumb in chemistry
Francis W. Aston received the 1922 Nobel Prize in Chemistry for his enunciation of the whole-number rule.

Inchemistry, thewhole number rule states that the masses of the isotopes arewhole number multiples of the mass of thehydrogen atom.[1] The rule is a modified version ofProut's hypothesis proposed in 1815, to the effect thatatomic weights are multiples of the weight of the hydrogen atom.[2] It is also known as theAston whole number rule[3] afterFrancis W. Aston who was awarded the Nobel Prize in Chemistry in 1922 "for his discovery, by means of hismass spectrograph, of isotopes, in a large number of non-radioactive elements, and for his enunciation of the whole-number rule".[4]

Law of definite proportions

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John Dalton's list of atomic weights and symbols

Thelaw of definite proportions was formulated byJoseph Proust around 1800[5] and states that all samples of a chemical compound will have the same elemental composition by mass. Theatomic theory ofJohn Dalton expanded this concept and explained matter as consisting of discreteatoms with one kind of atom for each element combined in fixed proportions to form compounds.[6]

Prout's hypothesis

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In 1815,William Prout reported on his observation that theatomic masses of the elements were whole multiples of the atomic mass ofhydrogen.[7][8] He then hypothesized that the hydrogen atom was the fundamental object and that the other elements were a combination of different numbers of hydrogen atoms.[9]

Aston's discovery of isotopes

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In 1920, Francis W. Aston demonstrated through the use of amass spectrometer that apparent deviations from Prout's hypothesis are predominantly due to the existence ofisotopes.[10] For example, Aston discovered that neon has two isotopes with masses very close to 20 and 22 as per the whole number rule, and proposed that the non-integer value 20.2 for the atomic weight of neon is due to the fact that natural neon is a mixture of about 90% neon-20 and 10% neon-22). A secondary cause of deviations is thebinding energy ormass defect of the individual isotopes.

Discovery of the neutron

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Main article:Discovery of the neutron
James Chadwick, discoverer of the neutron, with GeneralLeslie Groves, director of theManhattan Project.

During the 1920s, it was thought that the atomic nucleus was made of protons and electrons, which would account for the disparity between theatomic number of an atom and itsatomic mass.[11][12] In 1932,James Chadwick discovered an uncharged particle of approximately the mass as the proton, which he called theneutron.[13] The fact that the atomic nucleus is composed of protons and neutrons was rapidly accepted and Chadwick was awarded theNobel Prize in Physics in 1935 for his discovery.[14]

The modern form of the whole number rule is that theatomic mass of a given elementalisotope is approximately themass number (number of protons plus neutrons) times adalton (approximate mass of a proton, neutron, or hydrogen-1 atom). This rule predicts theatomic mass ofnuclides and isotopes with an error of at most 1%, with most of the error explained by the mass deficit caused bynuclear binding energy.

References

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  1. ^Budzikiewicz H, Grigsby RD (2006). "Mass spectrometry and isotopes: a century of research and discussion".Mass Spectrometry Reviews.25 (1):146–57.Bibcode:2006MSRv...25..146B.doi:10.1002/mas.20061.PMID 16134128.
  2. ^Prout, William (1815)."On the relation between the specific gravities of bodies in their gaseous state and the weights of their atoms".Annals of Philosophy.6:321–330. Retrieved2007-09-08.
  3. ^Christopher G. Morris (1992).Academic Press Dictionary of Science and Technology. Gulf Professional Publishing. pp. 169–.ISBN 978-0-12-200400-1.
  4. ^"The Nobel Prize in Chemistry 1922".nobelprize.org. TheNobel Foundation. 1922. Retrieved2014-08-13.
  5. ^Proust, J.-L. (1799). Researches on copper,Ann. chim.,32:26-54.Excerpt, in Henry M. Leicester and Herbert S. Klickstein,A Source Book in Chemistry, 1400–1900, Cambridge, MA: Harvard, 1952. Accessed 2008-05-08.
  6. ^Dalton, J. (1808).A New System of Chemical Philosophy, volume 1, Manchester.Excerpt. Accessed 2008-05-08.
  7. ^William Prout (1815). On the relation between the specific gravities of bodies in their gaseous state and the weights of their atoms.Annals of Philosophy, 6: 321–330.Online reprint
  8. ^William Prout (1816). Correction of a mistake in the essay on the relation between the specific gravities of bodies in their gaseous state and the weights of their atoms.Annals of Philosophy, 7: 111–13.Online reprint
  9. ^Lederman, Leon (1993).The God Particle. Delta.ISBN 9780385312110.
  10. ^Aston, Francis W. (1920)."The constitution of atmospheric neon".Philosophical Magazine.39 (6):449–455.doi:10.1080/14786440408636058.
  11. ^Brown, Laurie M. (1978). "The idea of the neutrino".Physics Today.31 (9):23–28.Bibcode:1978PhT....31i..23B.doi:10.1063/1.2995181.
  12. ^Friedlander G., Kennedy J.W. and Miller J.M. (1964)Nuclear and Radiochemistry (2nd edition), Wiley, pp. 22–23 and 38–39
  13. ^Chadwick, James (1932)."Possible Existence of a Neutron".Nature.129 (3252): 312.Bibcode:1932Natur.129Q.312C.doi:10.1038/129312a0.
  14. ^"James Chadwick – Biography".The Nobel Foundation. Retrieved21 April 2013.

Further reading

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External links

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