Finding a planet in starlight.
How can a planet hide in starlight?
How can a planet hide in starlight?
Fit the source, opaque planet and photometric detector.
When an opaque planet crosses a star, it removes some of the arriving light. For a uniform star and a central transit, the fractional drop is the planet-to-star area ratio. A grazing path blocks less area. The dip must stand out above measurement noise, and real observations need further checks to rule out other causes.
Uniform stellar disc, opaque circular planet and geometric circle overlap. Planet radius is in Earth radii; stellar radius in Solar radii, using REarth/RSun ≈ 0.0091577. Noise is an illustrative independent photometric uncertainty. No limb darkening, stellar variability or real detection classifier. The bench is an optical crossing simulator.
Detect a planet transit with signal at least five times the noise.
Find a transit dip above detector noise.