Expert-level exoplanet science covering detection methods, orbital dynamics, planetary atmospheres, habitability, and the search for biosignatures.
Transit: planet crosses star, flux decreases by Rp squared over Rs squared, period from timing. Radial velocity: Doppler shift of stellar lines, measures m sin i. Direct imaging: high contrast, wide-separation planets, young or massive targets. Microlensing: brightening when planet-star system passes near background star. Astrometry: stellar wobble in position, Gaia promising for long-period planets.
Transmission spectroscopy: during transit, starlight through atmosphere reveals absorption features. Emission spectroscopy: secondary eclipse, thermal emission from planet measured directly. Phase curves: full orbit photometry, day-night temperature contrast. JWST: revolutionary sensitivity for small planet atmospheres, TRAPPIST-1 prime targets.
Fulton gap: bimodal radius distribution at 1.5 to 2 Earth radii from photoevaporation. Hot Jupiters: close-in giant planets, migrated from outer disk. Super-Earths: 1 to 4 Earth radii, most common type found by Kepler. Occurrence rates: Kepler statistics, eta-Earth for solar-type stars.
Habitable zone: range of orbital distances for surface liquid water. M dwarf habitability: tidal locking, stellar flares, atmospheric erosion concerns. Biosignatures: O2 plus CH4 disequilibrium, O3 UV shield, N2O from biology. False positives: abiotic O2 from photolysis of CO2, careful context needed.
| Pitfall | Fix |
|---|---|
| Confusing equilibrium temperature with surface temperature | Greenhouse effect raises surface temperature significantly |
| Single biosignature as detection | Multiple independent lines of evidence needed |
| Ignoring stellar variability in transit analysis | Starspots can mimic or mask transit signals |
| Earth-centric habitability only | Other types of planets may support life |