(B) The carbon cycle (also known as the $CNO$ cycle) is a process of stellar nucleosynthesis in which stars on the main sequence fuse hydrogen into he

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Regenerated at the end of the cycle

(B) The carbon cycle (also known as the $CNO$ cycle) is a process of stellar nucleosynthesis in which stars on the main sequence fuse hydrogen into helium. In this cycle,carbon nuclei act as catalysts. They facilitate the fusion process but are not consumed in the net reaction. Therefore,the carbon nucleus is regenerated at the end of the cycle.

Class 12 Chemistry Nuclear Chemistry Nucleus (Stability and Reaction)

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In the carbon cycle,from which hot stars obtain their energy,the $_6C^{14}$ nucleus is

A
Completely converted into energy
B
Regenerated at the end of the cycle
C
Combined with oxygen to form carbon monoxide
D
Broken up into its constituents protons and neutrons

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Nuclear Chemistry

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Nucleus (Stability and Reaction)

In the radioactive decay,${}_{Z}^{A}X \to {}_{6}^{12}C + {}_{+1}^{0}e$,find the values of $A$ and $Z$.

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The nucleus $^{64}_{29}Cu$ accepts an orbital electron to yield:

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During the emission of a positron from a nucleus, the mass number of the daughter element remains the same but the atomic number

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Which of the following isotopes is likely to be most stable?

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If the mass defect of a nuclide is $3.32 \times 10^{-26} \ g$, its binding energy in $MeV$ is:

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In the carbon cycle,from which hot stars obtain their energy,the $_6C^{14}$ nucleus is

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In the radioactive decay,${}_{Z}^{A}X \to {}_{6}^{12}C + {}_{+1}^{0}e$,find the values of $A$ and $Z$.

The nucleus $^{64}_{29}Cu$ accepts an orbital electron to yield:

During the emission of a positron from a nucleus, the mass number of the daughter element remains the same but the atomic number

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If the mass defect of a nuclide is $3.32 \times 10^{-26} \ g$, its binding energy in $MeV$ is:

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