Learn

Learning preferences

Make learning more comfortable. Changes apply immediately.

Enlarges page content, including diagrams and their labels. You can also use your browser’s zoom.

Choose the colours that are easiest for you to distinguish. Applies to lesson diagrams and lab plots. Labels, shapes, hatching and line patterns also distinguish meanings. Source photographs and raw image brightness stay unchanged; mask-only views are available for image overlays.

ExampleComparisonSample link

Saved in this browser on this device. Preferences are separate from progress backups.

SCIENCE · INVESTIGATE AND EXPLAIN

Separate an interior’s volume, mass and inertia

Bulk density alone does not reveal a unique planetary interior. Rock, metal, volatile material, temperature and pressure can produce overlapping mass–radius relations. Differentiation redistributes material when sufficiently mobile dense components sink and lighter components rise; a layered interior is an inference constrained by gravity, rotation, composition and thermal history, not a direct photograph of the core.

Learning outcome: Change core radius and mantle density separately. Retain all three fractions and the radial weighting of inertia; explain what additional measurement could discriminate two mass–radius-compatible interiors.

Starting recap

Keep interior, thermal, surface-history, orbital and detection assumptions distinct before drawing a planetary inference.

All lessons are open directly. Your saved experiments remain when you leave and return.

Try

For f=0.4 and mantle density 3, core volume fraction is 0.064, mean density 3.32 g/cm³ and core mass fraction 0.512/3.32≈0.154217. Normalized inertia is 0.4×3.0512/3.32≈0.367614, below a uniform sphere.

Open the experiment

Predict

Does a core occupying 40% of radius occupy 40% of volume or mass?

Experiment

Change core radius and mantle density separately. Retain all three fractions and the radial weighting of inertia; explain what additional measurement could discriminate two mass–radius-compatible interiors.

Separate core volume, mass and rotational inertia

Worked teaching model · synthetic values · Original incompressible two-layer sphere: core density 8 g/cm³, outer radius normalized 1, sharp spherical boundary. Core volume fraction f³; mean density rho_m+(8−rho_m)f³. Normalized inertia C/(MR²)=(2/5)[rho_m+(8−rho_m)f⁵]/mean density. No pressure/compression, measured core size or unique composition inference.

Reset keeps your prediction, captures and practice history.

A dense small core can hold a larger mass fraction than its volume fraction.

Bulk density and normalized inertia are distinct integrals over interior structure. Multiple compositions and density profiles can share a bulk density; pressure, temperature and gravity data must constrain a real inference.

Outer radius: 1Core radius: 0.4000000Core density: 8 g/cm³Mantle density: 3 g/cm³Cross-section geometry; volume and mass are separate ledger quantities
Original conditional model ledger
QuantityValueUnit
Core volume fraction0.06400000fraction
Bulk mean density3.320000g/cm³
Core mass fraction0.1542169fraction
Mantle mass fraction0.8457831fraction
Normalized axial moment of inertia0.3676145C/(MR²)

Original supplied models, not actual planet observations or a unique interior, atmosphere or discovery claim.

A dense small core can hold a larger mass fraction than its volume fraction.

Bulk density and normalized inertia are distinct integrals over interior structure. Multiple compositions and density profiles can share a bulk density; pressure, temperature and gravity data must constrain a real inference.

Captures preserve recipes and replay their calculated results. They are synthetic model evidence, not physical measurements.

Understand

1. Define the planetary evidence

Bulk density alone does not reveal a unique planetary interior. Rock, metal, volatile material, temperature and pressure can produce overlapping mass–radius relations. Differentiation redistributes material when sufficiently mobile dense components sink and lighter components rise; a layered interior is an inference constrained by gravity, rotation, composition and thermal history, not a direct photograph of the core.

2. Connect mechanism and inference

The original two-layer sphere has normalized outer radius one, core density 8 g/cm³ and mantle density ρm. If core radius fraction is f, its volume fraction is f³ and mean density is ρm+(8−ρm)f³. Core mass fraction is 8f³ divided by mean density. Radius fraction, volume fraction and mass fraction therefore cannot be interchanged.

Rotation supplies another weighting: material farther from the axis contributes more strongly to moment of inertia. Integrating spherical shells gives C/(MR²)=(2/5)[ρm+(8−ρm)f⁵]/[ρm+(8−ρm)f³]. A uniform sphere has ratio 0.4; concentrating mass inward lowers it under these assumptions. The fifth power in the numerator is not a typographical replacement for the third-power volume term.

Terrestrial planets are predominantly rock and metal, whereas gas and ice giants contain much larger volatile inventories and strongly compressed interiors. Small moons, asteroids and comets have different gravity and thermal histories. Our incompressible sharp-boundary sphere omits compression, gradients, irregular shape and rotation-induced distortion, so its fitted core fraction would not be a unique real composition.

3. Work the supplied case

For f=0.4 and mantle density 3, core volume fraction is 0.064, mean density 3.32 g/cm³ and core mass fraction 0.512/3.32≈0.154217. Normalized inertia is 0.4×3.0512/3.32≈0.367614, below a uniform sphere.

4. Predict and investigate

Does a core occupying 40% of radius occupy 40% of volume or mass?

Change core radius and mantle density separately. Retain all three fractions and the radial weighting of inertia; explain what additional measurement could discriminate two mass–radius-compatible interiors.

Apply the evidence to a changed case

Use f=0.6 and mantle density 3. Find volume fraction, mean density and core mass fraction.

Retain the evidence frame, calculations and assumptions before opening public feedback.

Compare a worked response

Volume fraction is 0.216; mean density is 4.08 g/cm³; core mass fraction is 1.728/4.08≈0.423529. None equals the radius fraction 0.6.

Source and boundaries

Primary source. Checked 31 October 2026. Original diagrams and supplied model records are not actual planetary observations. No direct solar viewing, instrument operation or physical experiment is requested.

Apply

Which fraction equals the core’s volume fraction in this spherical model?

Public practice checks a specific claim. It does not establish independent mastery.

Use f=0.6 and mantle density 3. Find volume fraction, mean density and core mass fraction.

Continue

Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.

Skipping retains experiments and awards no mastery.

Save a science backup or import one

Science work is stored locally in this browser, separately from mathematics and AI. It does not sync automatically. Use this science-only backup; this checkout's older all-subject export does not include science.

A legacy file is available only when the complete snapshot fits the 36 MB limit. For larger snapshots, prepare a complete file set below; never discard notebooks to make a smaller file.

Matching imported notebook drafts replace their current drafts. Omitted lessons and known first attempts remain. Export your current work first if you want to retain both drafts.

Complete file sets and course backups

A file set can hold more work than one science file. Keep its manifest and every part together. Each file is limited to 36 MB. This format needs this version of LearnAI or a compatible newer version; older versions can use only the legacy single-file backup above.

The set includes every saved science course and global continuation at this moment. Later edits need a new export. A conflicting tab exports its own visible work, which may differ from saved work in another tab.

0 file(s) selected. File order and filenames do not determine identity. Missing, changed or conflicting parts block the entire restore; no good part is applied by itself.

Science storage: loading. No account or remote computation is required.