Given a star and a transit signal, estimate the planet's size, orbit, and temperature, then verify the result by regenerating the observables in the browser.
If the planet blocks a fraction of the star's light, the simplest estimate treats the transit depth as the ratio of the blocked disk area to the stellar disk area.
For a planet whose mass is tiny compared with the star's, Kepler's third law links orbital period to semi-major axis.
A simple radiative-balance estimate combines the inverse-square falloff of stellar energy with blackbody re-radiation.
The page generates a stylized transit using the inferred depth and central-transit duration, then optionally adds mild noise.
The orbit panel is not to scale between different presets, but it uses the inferred star and orbit sizes consistently within the current scenario.
| Quantity | Input / estimate | Independent recomputation |
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