When to Use Doppler Radial Velocity 3D Explorer - Best Sessions and Limits
Open the Doppler Radial Velocity 3D Explorer when you need the star-wobble detection method itself - 51 Pegasi b's ~4.23 day period, K ~55.7 m/s - and skip it when you only need the transit-dimming method or the general wavelength-shift mechanism.
A five-minute classroom demo
A five-minute classroom demo starts when you open Doppler Radial Velocity 3D Explorer, switch from 51 Pegasi b to the Jupiter-Sun preset, and pause so students see the wobble shrink from 55.7 m/s down to the ~13 m/s reflex Jupiter induces on the Sun.
Wobble-method literacy in Doppler Radial Velocity 3D Explorer
Wobble-method literacy in Doppler Radial Velocity 3D Explorer stays readable when you keep the facts panel open for the period and semi-amplitude K while watching the scrolling velocity strip trace approach and recession.
Sessions Doppler Radial Velocity 3D Explorer does not fit
Sessions Doppler Radial Velocity 3D Explorer does not fit are spectrograph or line-profile simulation, real astrometric wobble scale, or transit-dimming detection. Use Exoplanet Transit 3D or Redshift Doppler 3D instead. Walk the controls in the Doppler Radial Velocity 3D Explorer step-by-step guide.