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Astrophysicshard

Exoplanetary Transit Photometry Reconstruction

Design a high-precision experimental apparatus to simulate a multi-planet transit system using a single modulated light source and varied occluding masks. You must develop a signal processing protocol to extract individual planetary radii and orbital periods from the noisy aggregate light curve data, accounting for limb-darkening effects and sampling jitter. Ensure the final model can distinguish between transit depth variations and system noise at a confidence level of 3-sigma.

Materials: LED light source, PWM controller, opaque cardstock, circular aperture cutters, photodiode sensor, Arduino or equivalent microcontroller, and a data-logging interface.

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Background: NASA/ESA Hubble