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Difference between revisions of "Binding Energy"

(About Binding Energy of a Nucleus)
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*[[Binding Energy|Binding energy]] = [[Mass Defect|mass defect]] × [[Speed of Light|c²]].
 
*[[Binding Energy|Binding energy]] = [[Mass Defect|mass defect]] × [[Speed of Light|c²]].
 
*[[Binding Energy|Binding energy]] [[measure]]d  in [[MeV]].
 
*[[Binding Energy|Binding energy]] [[measure]]d  in [[MeV]].
*Indicates the stability of the [[Atomic Nucleus|nucleus]].
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*[[Binding Energy|Binding energy]] indicates the stability of the [[Atomic Nucleus|nucleus]] with a higher [[Binding Energy|binding energy]] indicates a more stable [[Atomic Nucleus|nucleus]].
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*[[Binding Energy|Binding energy]] represents the [[energy]] required to disassemble a [[Atomic Nucleus|nucleus]] into individual [[nucleon]]s.
 
*Higher [[Binding Energy Per Nucleon|'''binding energy''' per nucleon]] implies a more stable [[Atomic Nucleus|nucleus]].
 
*Higher [[Binding Energy Per Nucleon|'''binding energy''' per nucleon]] implies a more stable [[Atomic Nucleus|nucleus]].
 
*The curve of [[Binding Energy Per Nucleon|'''binding energy''' per nucleon]] versus [[mass]] number shows a peak at [[iron]] (Fe-56).
 
*The curve of [[Binding Energy Per Nucleon|'''binding energy''' per nucleon]] versus [[mass]] number shows a peak at [[iron]] (Fe-56).

Revision as of 12:52, 22 May 2024

Key Stage 5

Meaning

The binding energy of a nucleus is the work that must be done to separate a nucleus into its constituent neutrons and protons.

About Binding Energy of a Nucleus

Examples