Difference between revisions of "Generalized Nucleosynthesis in a Massive Star"

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== What the nucleosynthesis model shows ==
 
== What the nucleosynthesis model shows ==
 
The model is drawn as a cross section of the star, with fusion shells layered like an onion: hydrogen fusing to helium in the outermost shell, then helium to carbon, carbon to oxygen, oxygen to silicon and silicon to iron, around a core of iron (Fe). A table beside it gives the duration of each stage: 7 × 10<sup>6</sup> years for hydrogen to helium, 7 × 10<sup>5</sup> years for helium to carbon, 600 years for carbon to oxygen, 6 months for oxygen to silicon, 1 day for silicon to iron and a quarter of a second for core collapse. Each stage is far shorter than the one before it.
 
The model is drawn as a cross section of the star, with fusion shells layered like an onion: hydrogen fusing to helium in the outermost shell, then helium to carbon, carbon to oxygen, oxygen to silicon and silicon to iron, around a core of iron (Fe). A table beside it gives the duration of each stage: 7 × 10<sup>6</sup> years for hydrogen to helium, 7 × 10<sup>5</sup> years for helium to carbon, 600 years for carbon to oxygen, 6 months for oxygen to silicon, 1 day for silicon to iron and a quarter of a second for core collapse. Each stage is far shorter than the one before it.
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== Regents Exam Questions ==
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Released Regents questions that cannot be answered without this table, listed by exam. Each link opens the question with its answer key; the standard is the one the question assesses. The exams through August 2026 were given with the earlier edition of the ESSRT, which has the same table.
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{| class="wikitable" style="width:100%; text-align:center"
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! style="padding: 0.5em 1.5em;" | Exam
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! style="padding: 0.5em 1.5em;" | Cluster
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! style="padding: 0.5em 1.5em;" | Question
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! style="padding: 0.5em 1.5em;" | Standard
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|-
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| style="background-color:white;" | [[June 2025 Earth and Space Science Exam|June 2025 Earth and Space Sciences Regents]]
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| style="background-color:white;" | [[Questions:Stars and the Big Bang|Stars and the Big Bang]]
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| style="background-color:white;" | [[Questions:Stars and the Big Bang#q2|Question 17]]
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| style="background-color:white;" | [[HS-ESS1-3]]
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|-
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| style="background-color:white;" | [[June 2026 Earth and Space Science Exam|June 2026 Earth and Space Sciences Regents]]
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| style="background-color:white;" | [[Questions:Stars and Stellar Evolution|Stars and Stellar Evolution]]
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| style="background-color:white;" | [[Questions:Stars and Stellar Evolution#q1|Question 5]]
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| style="background-color:white;" | [[HS-ESS1-3]]
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|}

Revision as of 17:10, 25 October 2026

⇱ All Earth and Space Sciences Reference Tables (ESSRT)
Portion of Electromagnetic Spectrum Related to Earth and Space Sciences →

The Generalized Nucleosynthesis in a Massive Star model from the Reference Tables for Earth and Space Sciences (ESSRT) shows the series of nuclear fusion stages that build heavier and heavier elements inside a massive star, and how long each stage lasts. It primarily supports HS-ESS1-3.

Generalized Nucleosynthesis in a Massive Star from the Earth and Space Sciences Reference Tables (ESSRT): cross section of a massive star with fusion shells from hydrogen to iron around an iron core, and a table of how long each stage lasts

What the nucleosynthesis model shows

The model is drawn as a cross section of the star, with fusion shells layered like an onion: hydrogen fusing to helium in the outermost shell, then helium to carbon, carbon to oxygen, oxygen to silicon and silicon to iron, around a core of iron (Fe). A table beside it gives the duration of each stage: 7 × 106 years for hydrogen to helium, 7 × 105 years for helium to carbon, 600 years for carbon to oxygen, 6 months for oxygen to silicon, 1 day for silicon to iron and a quarter of a second for core collapse. Each stage is far shorter than the one before it.

Regents Exam Questions

Released Regents questions that cannot be answered without this table, listed by exam. Each link opens the question with its answer key; the standard is the one the question assesses. The exams through August 2026 were given with the earlier edition of the ESSRT, which has the same table.

Exam Cluster Question Standard
June 2025 Earth and Space Sciences Regents Stars and the Big Bang Question 17 HS-ESS1-3
June 2026 Earth and Space Sciences Regents Stars and Stellar Evolution Question 5 HS-ESS1-3