How Do We Know the Earth Is Round, Rotating & Orbiting the Sun? | CER Astronomy Lesson
Phenomena-Driven Earth & Space Science Investigation Using Claims, Evidence & Reasoning.
How do we really know that the Earth is round, rotating, and orbiting the sun?
This fully interactive Google Slides lesson takes students far beyond memorizing facts—they test scientific claims using real evidence and CER reasoning.
Students investigate three essential questions:
How do we know the Earth is not flat?
How do we know the Earth rotates?
How do we know the Earth revolves around the sun?
Through engaging “Think & Compare” activities, students explore real observational evidence including:
Ship-over-the-horizon observations
Lunar eclipses
Light-beam curvature tests
Constellation shifts
Foucault’s pendulum
The Coriolis effect
Stellar parallax
Students use CER frameworks to construct scientific explanations grounded in evidence—supporting NGSS science practices.
The lesson then transitions into the historical debate of Ptolemy vs. Copernicus, allowing students to compare geocentric and heliocentric models before analyzing Galileo’s role and researching his life, discoveries, and trial.
This lesson is perfect for Earth & space science, evidence-based reasoning, history of science units, or literacy-rich science instruction.
Includes:
✔ 18-slide interactive Google Slides lesson
✔ Multiple CER templates
✔ Historical model comparison organizer
✔ Built-in student investigations
✔ Editable teacher key
✔ Exit ticket
✔ Student-friendly research prompts
Perfect for:
▪ Middle School Earth Science
▪ 9th Grade Earth Science or Astronomy
▪ Scientific thinking / CER units
▪ Cross-curricular literacy instruction
Grade & Course Recommendations
Most appropriate:
Grades 6–9
Course applicability:
Earth & Space Science
Integrated Science
Physical Science (Earth motions segment)
Astronomy
Scientific Reasoning / CER units
STEM literacy
Cross-Curricular Connections & Extensions
Cross-Curricular Connections
ELA / Literacy:
CER writing
Historical research on Galileo
Analysis of scientific texts, claims, and argumentation
Meme interpretation and media-literacy prompts
History / Social Studies:
Renaissance science
Catholic Church and scientific conflict
Islamic Golden Age astronomy (noted in slides showing support from Muslim scholars in 900 AD)
Math:
Geometry of circles, shadows, and angles
Using patterns of motion as evidence
Introductory parallax geometry
Technology:
Research skills
Analysis of visual simulations
Possible Extensions
Model stellar parallax with classroom trigonometry
Build a Foucault pendulum simulation or use an online version
Have students debate Ptolemy vs. Copernicus from a historical perspective
Conduct a “myth vs. evidence” unit on scientific misconceptions
Use NASA’s Eyes or other astronomy visualization tools
Daily slide + literacy - based exit ticket included with purchase
Join the Lesson Laboratory and Teach for Tomorrow!
NGSS Alignment (PEs + SEPs + CCCs)
Performance Expectations
Middle School (Primary Alignment):
MS-ESS1-1: Develop and use a model of Earth-Sun-Moon motions to explain seasons, eclipses, and lunar phases.
MS-ESS1-2: Use data to determine scale properties of objects in the solar system.
MS-ESS1-3: Analyze and interpret data to determine scale properties of stars using brightness comparisons.
High School (Secondary Alignment):
HS-ESS1-2: Construct explanations for the motions of orbiting bodies.
HS-ESS1-4: Use mathematical models to predict stellar motion (applies to stellar parallax segment).
Science & Engineering Practices (SEPs)
Analyzing and Interpreting Data: Ship horizon, lunar eclipse, Foucault pendulum, parallax
Constructing Explanations (CER): Students produce claim-evidence-reasoning arguments
Developing and Using Models: Geocentric vs. heliocentric, Earth–Moon–Sun geometry
Engaging in Argument from Evidence: Multiple CER prompts require evidence-based reasoning
Obtaining, Evaluating, and Communicating Information: Galileo research slide
Crosscutting Concepts (CCCs)
Patterns: Constellation movement, eclipses, predictable planetary motion
Cause & Effect: Earth’s rotation → pendulum motion, Coriolis effect
Scale, Proportion, and Quantity: Parallax, planetary distances
Systems & System Models: Solar system as an interacting set of bodies
Stability & Change: Understanding historical model change (Ptolemy → Copernicus → Galileo)
Common Core Standards (ELA/Literacy)
Middle School
RST.6-8.1: Cite evidence to support analysis of scientific information
RST.6-8.7: Integrate visual information (graphs, diagrams, eclipse models)
WHST.6-8.1: Write arguments focused on discipline-specific content (CER)
WHST.6-8.7: Conduct short research projects (Galileo slide)
High School
RST.9-10.1: Cite specific textual evidence
RST.9-10.7: Translate quantitative/visual representations into words
WHST.9-10.2: Write explanatory texts (CER structure)
WHST.9-10.8: Gather information from authoritative sources (Galileo research)
Phenomena-Driven Earth & Space Science Investigation Using Claims, Evidence & Reasoning.
How do we really know that the Earth is round, rotating, and orbiting the sun?
This fully interactive Google Slides lesson takes students far beyond memorizing facts—they test scientific claims using real evidence and CER reasoning.
Students investigate three essential questions:
How do we know the Earth is not flat?
How do we know the Earth rotates?
How do we know the Earth revolves around the sun?
Through engaging “Think & Compare” activities, students explore real observational evidence including:
Ship-over-the-horizon observations
Lunar eclipses
Light-beam curvature tests
Constellation shifts
Foucault’s pendulum
The Coriolis effect
Stellar parallax
Students use CER frameworks to construct scientific explanations grounded in evidence—supporting NGSS science practices.
The lesson then transitions into the historical debate of Ptolemy vs. Copernicus, allowing students to compare geocentric and heliocentric models before analyzing Galileo’s role and researching his life, discoveries, and trial.
This lesson is perfect for Earth & space science, evidence-based reasoning, history of science units, or literacy-rich science instruction.
Includes:
✔ 18-slide interactive Google Slides lesson
✔ Multiple CER templates
✔ Historical model comparison organizer
✔ Built-in student investigations
✔ Editable teacher key
✔ Exit ticket
✔ Student-friendly research prompts
Perfect for:
▪ Middle School Earth Science
▪ 9th Grade Earth Science or Astronomy
▪ Scientific thinking / CER units
▪ Cross-curricular literacy instruction
Grade & Course Recommendations
Most appropriate:
Grades 6–9
Course applicability:
Earth & Space Science
Integrated Science
Physical Science (Earth motions segment)
Astronomy
Scientific Reasoning / CER units
STEM literacy
Cross-Curricular Connections & Extensions
Cross-Curricular Connections
ELA / Literacy:
CER writing
Historical research on Galileo
Analysis of scientific texts, claims, and argumentation
Meme interpretation and media-literacy prompts
History / Social Studies:
Renaissance science
Catholic Church and scientific conflict
Islamic Golden Age astronomy (noted in slides showing support from Muslim scholars in 900 AD)
Math:
Geometry of circles, shadows, and angles
Using patterns of motion as evidence
Introductory parallax geometry
Technology:
Research skills
Analysis of visual simulations
Possible Extensions
Model stellar parallax with classroom trigonometry
Build a Foucault pendulum simulation or use an online version
Have students debate Ptolemy vs. Copernicus from a historical perspective
Conduct a “myth vs. evidence” unit on scientific misconceptions
Use NASA’s Eyes or other astronomy visualization tools
Daily slide + literacy - based exit ticket included with purchase
Join the Lesson Laboratory and Teach for Tomorrow!
NGSS Alignment (PEs + SEPs + CCCs)
Performance Expectations
Middle School (Primary Alignment):
MS-ESS1-1: Develop and use a model of Earth-Sun-Moon motions to explain seasons, eclipses, and lunar phases.
MS-ESS1-2: Use data to determine scale properties of objects in the solar system.
MS-ESS1-3: Analyze and interpret data to determine scale properties of stars using brightness comparisons.
High School (Secondary Alignment):
HS-ESS1-2: Construct explanations for the motions of orbiting bodies.
HS-ESS1-4: Use mathematical models to predict stellar motion (applies to stellar parallax segment).
Science & Engineering Practices (SEPs)
Analyzing and Interpreting Data: Ship horizon, lunar eclipse, Foucault pendulum, parallax
Constructing Explanations (CER): Students produce claim-evidence-reasoning arguments
Developing and Using Models: Geocentric vs. heliocentric, Earth–Moon–Sun geometry
Engaging in Argument from Evidence: Multiple CER prompts require evidence-based reasoning
Obtaining, Evaluating, and Communicating Information: Galileo research slide
Crosscutting Concepts (CCCs)
Patterns: Constellation movement, eclipses, predictable planetary motion
Cause & Effect: Earth’s rotation → pendulum motion, Coriolis effect
Scale, Proportion, and Quantity: Parallax, planetary distances
Systems & System Models: Solar system as an interacting set of bodies
Stability & Change: Understanding historical model change (Ptolemy → Copernicus → Galileo)
Common Core Standards (ELA/Literacy)
Middle School
RST.6-8.1: Cite evidence to support analysis of scientific information
RST.6-8.7: Integrate visual information (graphs, diagrams, eclipse models)
WHST.6-8.1: Write arguments focused on discipline-specific content (CER)
WHST.6-8.7: Conduct short research projects (Galileo slide)
High School
RST.9-10.1: Cite specific textual evidence
RST.9-10.7: Translate quantitative/visual representations into words
WHST.9-10.2: Write explanatory texts (CER structure)
WHST.9-10.8: Gather information from authoritative sources (Galileo research)