Where Elements Come From
CONCEPTUALExplain stellar nucleosynthesis: the Big Bang produced mainly hydrogen and helium; main-sequence fusion builds elements up to iron; and supernovae produce elements heavier than iron and scatter them into space — meaning the atoms in our bodies were forged in ancient stars
Mastery Evidence
- States that the Big Bang produced primarily hydrogen and helium, and that all heavier elements were made later in stars
- Explains that nuclear fusion in main-sequence stars converts hydrogen to helium and can continue building heavier elements up to iron
- Explains why elements heavier than iron require supernova explosions to form, and describes how supernovae distribute these elements into interstellar space where they become the raw material for new stars, planets, and life
Assessment Prompt
“If [child] was told that the calcium in their bones and the iron in their blood were made inside ancient stars that exploded billions of years ago, could they explain the chain of events from the Big Bang to the formation of those atoms to how they ended up on Earth?”
Prerequisites2
- Life Cycle of StarshardAges 9—11
- Atoms, Elements & CompoundssoftAges 11—12
Show full prerequisite tree
- Life Cycle of Stars hard
Stellar nucleosynthesis depends on understanding the basics of a star's life cycle
- Why the Sun Looks Brightest soft
Understanding star brightness and distance helps contextualise different stages of star life
- The Sun is a star hard
Must know the Sun is a star before understanding why it appears brighter than other stars
- Why seasons change soft
Curriculum daylight/seasons observation supports exploratory Sun/Moon/stars identification
- Naming the Planets soft
Relating daylight length to time of year draws on orbit and solar system vocabulary
- Days, Weeks, Months & Years soft
Observing and describing seasonal changes requires basic date and time vocabulary (months, seasons, year)
- Ordering Events in Time hard
Understanding days/months/years builds on sequencing events chronologically
- Sun, Moon & Stars hard
Must know the Sun and stars before learning about planets and the solar system
- Why seasons change soft
Curriculum daylight/seasons observation supports exploratory Sun/Moon/stars identification
- Naming the Planets soft
Relating daylight length to time of year draws on orbit and solar system vocabulary
- Days, Weeks, Months & Years soft
Observing and describing seasonal changes requires basic date and time vocabulary (months, seasons, year)
- Ordering Events in Time hard
Understanding days/months/years builds on sequencing events chronologically
- Why seasons change soft
Curriculum daylight/seasons observation supports exploratory Sun/Moon/stars identification
- Naming the Planets soft
Relating daylight length to time of year draws on orbit and solar system vocabulary
- Days, Weeks, Months & Years soft
Observing and describing seasonal changes requires basic date and time vocabulary (months, seasons, year)
- Ordering Events in Time hard
Understanding days/months/years builds on sequencing events chronologically
- Sun, Moon & Stars hard
Must know the Sun and stars before learning about planets and the solar system
- Why seasons change soft
Curriculum daylight/seasons observation supports exploratory Sun/Moon/stars identification
- Naming the Planets soft
Relating daylight length to time of year draws on orbit and solar system vocabulary
- Days, Weeks, Months & Years soft
Observing and describing seasonal changes requires basic date and time vocabulary (months, seasons, year)
- Ordering Events in Time hard
Understanding days/months/years builds on sequencing events chronologically
- Atoms, Elements & Compounds soft
Stellar nucleosynthesis depends on understanding atoms, elements, and isotopes
- The Particle Model hard
Atoms and molecules are the particles referred to in the particle model — builds directly on it
- Drawing Particle Diagrams hard
Using the particle model to explain density, compressibility, and anomalous expansion requires fluent reading and drawing of particle diagrams
- Matter Is Made of Particles hard
KS3 particle model extends US KS2 introduction to matter as particles too small to see
- Drawing Particle Diagrams hard
Developing a model of matter as particles too small to see is built on the particle diagram representation
- Heating & Cooling Changes hard
Must observe state changes before explaining them with particle model
- States of Matter Vocabulary hard
Describing and measuring changes of state requires solid/liquid/gas vocabulary and the term 'change of state'
- Drawing Particle Diagrams hard
Observing and describing change of state requires reading particle diagrams showing how arrangement changes on heating or cooling
- Solids, Liquids & Gases hard
Must understand observable states of matter before modelling them with particles
- States of Matter Vocabulary hard
Comparing and grouping materials as solids, liquids, or gases requires the naming vocabulary for the three states
- Drawing Particle Diagrams hard
Comparing and grouping solids, liquids, and gases by properties is greatly aided by the particle diagram representation
- Heating & Cooling Changes hard
Must classify states of matter before understanding changes between states
- States of Matter Vocabulary hard
Describing and measuring changes of state requires solid/liquid/gas vocabulary and the term 'change of state'
- Drawing Particle Diagrams hard
Observing and describing change of state requires reading particle diagrams showing how arrangement changes on heating or cooling
- Grouping Materials hard
Must group materials by properties before classifying into three states of matter
- States of Matter Vocabulary soft
Describing physical properties of materials uses solid/liquid/gas vocabulary introduced in the states of matter LANGUAGE node
- Changing Shapes of Solids soft
Changing shapes of solids provides context for understanding solid properties
- Describing Material Properties hard
Must know material properties before investigating how shapes change
- States of Matter Vocabulary soft
Describing physical properties of materials uses solid/liquid/gas vocabulary introduced in the states of matter LANGUAGE node
- Solids, Liquids & Gases hard
KS3 particle model extends KS2 classification of solids, liquids and gases by observable properties
- States of Matter Vocabulary hard
Comparing and grouping materials as solids, liquids, or gases requires the naming vocabulary for the three states
- Drawing Particle Diagrams hard
Comparing and grouping solids, liquids, and gases by properties is greatly aided by the particle diagram representation
- Heating & Cooling Changes hard
Must classify states of matter before understanding changes between states
- States of Matter Vocabulary hard
Describing and measuring changes of state requires solid/liquid/gas vocabulary and the term 'change of state'
- Drawing Particle Diagrams hard
Observing and describing change of state requires reading particle diagrams showing how arrangement changes on heating or cooling
- Grouping Materials hard
Must group materials by properties before classifying into three states of matter
- States of Matter Vocabulary soft
Describing physical properties of materials uses solid/liquid/gas vocabulary introduced in the states of matter LANGUAGE node
- Changing Shapes of Solids soft
Changing shapes of solids provides context for understanding solid properties
- Describing Material Properties hard
Must know material properties before investigating how shapes change
- States of Matter Vocabulary soft
Describing physical properties of materials uses solid/liquid/gas vocabulary introduced in the states of matter LANGUAGE node
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