Difficulty: Medium
Correct Answer: Collision between fast neutrons and nitrogen nuclei present in the atmosphere
Explanation:
Introduction / Context:
Radiocarbon, or carbon 14, is a radioactive isotope of carbon that is very important in archaeology and geology because it is used for radiocarbon dating of organic materials. The presence of carbon 14 in the atmosphere is not permanent; it is continuously produced by nuclear reactions. The question asks you to identify the main process responsible for the formation of radiocarbon in the upper atmosphere. Understanding this process links concepts from cosmic rays, nuclear reactions, and environmental science.
Given Data / Assumptions:
Concept / Approach:
High energy cosmic rays from space strike the earth's atmosphere and produce cascades of secondary particles, including fast neutrons. These neutrons can collide with nitrogen 14 nuclei, which are abundant in the atmosphere. A typical reaction is nitrogen 14 plus a neutron giving carbon 14 and a proton. In equation form, N 14 + n gives C 14 + p. This nuclear reaction converts nitrogen into radiocarbon. The newly formed carbon 14 combines with oxygen to form carbon dioxide containing carbon 14, which then mixes into the global carbon cycle. Ultraviolet light mainly affects ozone and oxygen chemistry, not carbon 14 production. Lightning and general solar radiation do not produce radiocarbon in the primary and continuous way that neutron nitrogen collisions do.
Step-by-Step Solution:
Step 1: Recognise that cosmic rays generate high energy neutrons in the upper atmosphere.Step 2: Note that the atmosphere contains a large amount of nitrogen 14, which can interact with these neutrons.Step 3: The key nuclear reaction is N 14 plus a neutron gives C 14 plus a proton.Step 4: This reaction directly converts nitrogen nuclei into radiocarbon, carbon 14.Step 5: Therefore, radiocarbon is produced mainly by collisions between fast neutrons and nitrogen nuclei in the atmosphere.
Verification / Alternative check:
Standard descriptions of radiocarbon dating in physics and chemistry textbooks explicitly mention the neutron nitrogen reaction as the source of carbon 14. The rate of production depends on cosmic ray intensity and atmospheric composition, which explains variations in radiocarbon levels over time. Other processes involving ultraviolet light or lightning are important for different atmospheric phenomena, such as ozone formation or nitrogen oxides, but they are not identified as the main source of carbon 14. This agreement between multiple educational sources and the nuclear reaction pathway confirms the correctness of the chosen process.
Why Other Options Are Wrong:
Ultraviolet light from the sun mainly causes photodissociation of oxygen and ozone, leading to ozone layer chemistry, but does not create carbon 14, so option B is incorrect. Solar radiation acting directly on carbon dioxide does not change stable carbon isotopes into carbon 14 in any dominant way under normal atmospheric conditions, so option C is wrong. Lightning discharges can produce nitrogen oxides and other chemical species but are not the primary source of radiocarbon, so option D is also incorrect. Only option A correctly identifies the collision between fast neutrons and nitrogen nuclei as the main mechanism for radiocarbon production.
Common Pitfalls:
Students may be tempted to pick options that mention solar or ultraviolet radiation because they seem naturally connected to atmospheric processes. Another pitfall is to overestimate the role of lightning in nuclear reactions, even though its main effects are chemical rather than nuclear. To avoid such errors, remember that producing a different isotope usually requires nuclear processes, which are more likely to involve high energy particles like neutrons rather than ordinary photons or electric discharges. Associating radiocarbon production with cosmic ray neutrons and nitrogen 14 helps fix the correct concept in memory.
Final Answer:
Collision between fast neutrons and nitrogen nuclei present in the atmosphere
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