Astro 101 Core Concepts
Build foundational astronomy reasoning by linking Earth-sky geometry, measurement, and light into one guided progression.
A broad starter journey covering the core ideas students need before branching into specialized topics.
Instructions
Move in order through required demos first. For each demo: 1) Write one prediction before touching controls. 2) Capture one key observable from the run. 3) State one inference and why the model supports it.
Journey steps
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Moon Phases: Light, Not Shadow
RequiredExplain changing lunar appearance from illumination geometry.
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Seasons: Why Tilt Matters
RequiredUse Sun-angle evidence to explain seasonal temperature patterns.
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Eclipse Geometry: Shadows in Space
RequiredPredict when eclipses can and cannot occur from alignment + tilt.
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Parallax Distance: Measuring the Stars
RequiredInfer stellar distance from geometric baselines and measured angle shifts.
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Telescope Resolution: Sharper Eyes
RequiredConnect aperture/wavelength choices to resolving power limits.
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Blackbody Radiation: Thermal Spectrum and Temperature
RequiredInfer temperature from spectrum shape and peak location.
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Electromagnetic Spectrum: Light Beyond Visible
OptionalPlace visible light inside the broader electromagnetic spectrum.
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Angular Size: The Sky’s Ruler
OptionalDistinguish apparent size from physical size using distance context.
Why this sequence?
Why this sequence?
The first three demos anchor sky geometry, the middle demos introduce distance and instruments, and the final light modules connect observables to physical inference. Together they form a complete Astro 101 reasoning arc.