astronomylabFor teachers
Find a planet in a missing glimmer.

Transit Depth Formula & Exoplanet Transits

The transit method finds exoplanets from tiny dips in starlight. Learn the transit depth formula δ ≈ (Rp/R★)², with Jupiter- and Earth-sized examples.

Light curve · dip depth vertically enlarged

The idea behind it

A transiting planet hides a fraction of its star’s visible disk. Larger planets block more light. The light curve plots the remaining brightness as the planet moves across the star.

The relationship to remember

Central transit depth ≈ (planet radius / star radius)²

Planet/star radius = 0.1026. Central full-overlap depth would be 1.052%; the chosen path gives a maximum 1.052% dip.

Make your own discovery

Compare Earth-sized and Jupiter-sized presets. Notice how much harder it is to detect the smaller planet.

Open the Exoplanet Transit Simulator & Depth Calculator ↗

Key formulas

QuantityFormulaNote or example
Transit depthδ ≈ (Rp / R★)²Planet fully in front of a uniform star
Planet radius from depthRp ≈ R★ × √δInvert a measured dip
Earth–Sun radius ratioR⊕ / R☉ ≈ 0.00916So δ ≈ 0.0084%

Worked examples

Each row uses one of this lab’s presets and the same model as the interactive tool.

ExampleMaximum depthLight receivedRadius ratio
Jupiter-sized1.052%98.948%0.1026
Earth-sized0.0084%99.9916%0.0092
Grazing transit0.6448%99.3552%0.1026

What this model leaves out

An opaque circular planet, a uniformly bright star, and a straight path. Overlapping disk areas handle grazing transits. No limb darkening, starspots, noise, or orbital-speed effects.

Keep wondering

Check your understanding

Does every planet transit?

No. The orbit must be aligned so that the planet passes in front of the star from our viewpoint.

Can a transit reveal a planet’s mass?

A transit primarily constrains size relative to the star. Mass usually requires additional observations.

What is the transit depth formula?

For a planet fully in front of a uniformly bright star, the fractional drop in brightness is about the square of the planet-to-star radius ratio: δ ≈ (Rp/R★)². A 1% dip around a Sun-like star implies a planet about one tenth of the star’s radius — roughly Jupiter’s size.

Continue with the formula reference or test yourself in space practice.