Radial-velocity (RV) method detects an exoplanet via the Doppler shift of stellar absorption lines as the host star wobbles around the common barycentre under the planet's gravitational tug. Amplitude: K = (2π G / P)^{1/3} · (m_p sin i) /…
Radial-velocity (RV) method detects an exoplanet via the Doppler shift of stellar absorption lines as the host star wobbles around the common barycentre under the planet's gravitational tug. Amplitude: K = (2π G / P)^{1/3} · (m_p sin i) /…