Astronomy & space · lesson 3 of 4
Exoplanet transits and radial velocities
A planet crossing a star's visible disk can cause a periodic brightness dip. For an idealized small dark planet and uniform stellar disk, depth≈(Rp/Rstar)².
Learn the ideas
Prerequisites: Ratios, graphs and Newtonian orbits.
Transit method
A planet crossing a star's visible disk can cause a periodic brightness dip. For an idealized small dark planet and uniform stellar disk, depth≈(Rp/Rstar)².
Radial velocity
A star and planet orbit their common centre of mass. Periodic line-of-sight stellar velocity changes can be inferred from spectral shifts.
Selection
Neither method detects every planet equally well. Orbital orientation, noise, stellar activity and observational duration affect sensitivity.
Confirmation
A candidate signal needs checks against false positives. A transit alone is not proof of life or a complete atmospheric measurement.
Worked examples
In the idealized transit model, Rp/Rstar=0.1. Find fractional transit depth.
Square the radius ratio.
0.01
For idealized transit depth 0.0004, find Rp/Rstar.
Take the positive square root of the depth.
0.02
Check your understanding
8 questionsDecimals or fractions are accepted for numeric answers. Proofs and written responses use sample answers and require human marking. This is practice, not a protected examination.
Further reading and review references
These are reference links, not copied exercises, institutional endorsement or proof of independent review.