Formula and example
How it is calculated
Relative light loss ≈ (planet radius/star radius)²
Worked example
If the planet’s radius is one tenth of the star’s radius, the model gives a light loss of 1%, or 10,000 ppm.
Things to check
- Both radii must use the same length unit. A radius ratio is sufficient.
- The model assumes a full transit. Limb darkening, a grazing transit and additional light in the measurement field change the actual depth.