Paritian

Science

Exoplanet Transit Calculator (Depth, Duration and Probability)

How much a planet dims its star as it crosses the disc, how long the crossing lasts and how likely a random observer is to see it, from the sizes, the orbital period and the star's mass.

Results

Transit depth (dip in starlight) 1.0560 %
Transit duration 2.93 h
Orbital distance 0.0451 AU
Chance that a random observer sees the transit 10.31 %
Radius ratio, planet ÷ star 0.10276
How it changes
Transit depth (dip in starlight)Radius of the planet 0.000 – 3.000. Transit depth (dip in starlight): 0 → 9.50415Transit depth (dip in starlight)02468100.0000.5001.0001.5002.0002.5003.000Radius of the planet

The dashed line marks the value you entered.

What this tool does

A transiting planet blocks a fraction of the starlight equal to the square of the radius ratio: a Jupiter in front of a Sun-like star dims it by about 1 %, an Earth by only 0.008 % — which is why finding Earth-sized worlds needs space telescopes. The orbital distance follows from Kepler's third law, and the transit lasts a few hours for a close-in planet. Only orbits seen almost edge-on cause transits: the geometric chance is roughly the stellar radius divided by the orbital distance, about 10 % for a hot Jupiter and 0.5 % for an Earth-like orbit.

Formula

depth = (R_p ÷ R_s)² · a³ = G M P² ÷ 4π² · T = (P ÷ π) asin[ (R_s ÷ a) √((1 + k)² − b²) ÷ sin i ]

Variables

SymbolMeaningUnit
rsRadius of the star (Sun = 1)—
rpRadius of the planet—
unPlanet radius is given in—
pdOrbital period of the planetd
smMass of the star (Sun = 1)—
ibImpact parameter (0 = across the middle of the star, 1 = grazing the edge)—
DPTransit depth (dip in starlight)%
DUTransit durationh
AOrbital distanceAU
PRChance that a random observer sees the transit%
KRadius ratio, planet ÷ star—

Worked example

  • Radius of the star (Sun = 1)1
  • Radius of the planet1
  • Planet radius is given in2
  • Orbital period of the planet3.5 d
  • Mass of the star (Sun = 1)1
  • Impact parameter (0 = across the middle of the star, 1 = grazing the edge)0.3
  • Transit depth (dip in starlight)1.0560 %
  • Transit duration2.93 h
  • Orbital distance0.0451 AU
  • Chance that a random observer sees the transit10.31 %
  • Radius ratio, planet ÷ star0.10276

Limitations

  • The formula assumes ideal conditions: no friction losses, no air resistance and no efficiency losses unless you enter them.
  • The result is an estimate based only on the values you type. Real situations often include factors this calculator does not know about.