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The 58 pages that link to Radial velocity method, each with the reason it gives.
Orbital periodRelated: The repeating stellar motion yields the companion's orbital period.
Hot JupiterRelated: A close giant planet often induces a detectable stellar wobble.
Super-EarthRelated: The star's wobble can reveal a super-Earth's minimum mass.
Alpha CentauriRelated: It revealed the gravitational signal used to discover Proxima Centauri b.
Red dwarfRelated: A planet can induce a detectable wobble in a low-mass red dwarf.
Gas giantRelated: It established the masses of many gas giants orbiting other stars.
OrbitRelated: A companion’s orbit produces measurable back-and-forth motion in its star.
StarRelated: A planet’s gravity makes its star move slightly toward and away from Earth.
Astronomical observationRelated: It detects a planet’s gravitational tug on its host star.
Planetary orbitRelated: The orbit sets the timing and amplitude of the star’s measured wobble.
Stellar orbitRelated: Spectral shifts can trace a star’s line-of-sight orbital motion.
TESSRelated: Radial-velocity follow-up can confirm TESS candidates and measure their masses.
Exoplanet detectionRelated: The star’s reflex motion supplies evidence independent of a transit.
Barnard's StarRelated: Astronomers use this method to search for planets tugging on Barnard's Star.
Jupiter massRelated: It often yields a planet’s minimum mass in Jupiter-mass units.
Giant planetRelated: A giant planet's gravitational pull can induce a measurable stellar wobble.
55 Cancri eRelated: The planet's initial detection came from the star's motion, not a direct image.
HD 189733 bRelated: Stellar motion helped characterize the planet’s orbit and mass.