Radial velocity is a method for finding planets around other stars by looking for the gravitational tug of those planets on their parent stars. NEID, shown here mounted on the 3.5-meter WIYN telescope at the Kitt Peak National Observatory, is a cutting edge-radial velocity instrument. (NSF’s National Optical-Infrared Astronomy Research Laboratory/KPNO/NSF/AURA)
Home Radial velocity is a method for finding planets around other stars by looking for the gravitational tug of those planets on their parent stars. NEID, shown here mounted on the 3.5-meter WIYN telescope at the Kitt Peak National Observatory, is a cutting edge-radial velocity instrument. (NSF’s National Optical-Infrared Astronomy Research Laboratory/KPNO/NSF/AURA) Radial velocity is a method for finding planets around other stars by looking for the gravitational tug of those planets on their parent stars. NEID, shown here mounted on the 3.5-meter WIYN telescope at the Kitt Peak National Observatory, is a cutting edge-radial velocity instrument. (NSF’s National Optical-Infrared Astronomy Research Laboratory/KPNO/NSF/AURA)