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For K-12 Students · Milankovitch Cycles

Milankovitch Cycles for a carbon cycle

Built for k-12 students learning it in middle or high school. Watch the idea come alive with plain-language steps and everyday examples — perfect for projects and homework. Simulate a carbon cycle live below — adjust the inputs and watch it respond, right in your browser.

Milankovitch CyclesLive

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Three slow changes in Earth's orbit — the stretch of its ellipse (eccentricity), the tilt of its axis (obliquity), and the wobble of that axis (precession) — combine to modulate summer sunlight at high latitudes. That insolation rhythm paces the glacial-interglacial cycles recorded in ice and ocean cores.

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Data Inspector

Eccentricity~100 kyr
Obliquity~41 kyr
Precession~23 kyr

Insolation forcing

Reading this result: With obliquity weighted highest, a ~41 kyr beat dominates — the pattern that paced glacial cycles before ~1 million years ago, when axial tilt led the forcing.

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Frequently asked questions

Is this good for k-12 students?
Yes — this version of "Milankovitch Cycles for a carbon cycle" is framed for k-12 students learning it in middle or high school. Watch the idea come alive with plain-language steps and everyday examples — perfect for projects and homework.
Do I need to install anything?
No. It runs in any modern browser, free, with no account required.