## What is the formula for radial velocity?

Since velocity is just change of position per unit time (in this case Vr = dr/dt) the change in phase between the two pulses gives us the radial velocity. Radial velocity is the component of wind velocity parallel to the direction of the radar beam either toward or away from the radar.

## What is the radial velocity curve?

The maximum radial velocity tells you how fast a star is moving in its orbit around the centre of mass. You can read that off the radial velocity curve – it’s the value at the top of the peak. If you know the mass of the star, combining this with the measured orbital speed allows you to work out the mass of the planet.

**How is radial velocity method used?**

The radial-velocity method for detecting exoplanets relies on the fact that a star does not remain completely stationary when it is orbited by a planet. The star moves, ever so slightly, in a small circle or ellipse, responding to the gravitational tug of its smaller companion.

### What is microlensing method?

Microlensing is a form of gravitational lensing in which the light from a background source is bent by the gravitational field of a foreground lens to create distorted, multiple and/or brightened images.

### How do you calculate radial velocity using redshift?

The radial velocity is the velocity towards the observer (negative), or from the observer away (positive). It is calculated from the shift z in percent of the speed of light and in meters per second. The formula is v = c * [(1+z)²-1] / [(1+z)²+1] with the speed of light c as 299792458 meters per second.

**What is a radial velocity spectrometer?**

Radial Velocity Spectrometer (RVS) The RVS provides the third component of the space velocity of each star down to about 17th magnitude. The instrument is a near-infrared (845–872 nm), medium-resolution (λ/Δλ ~ 11500), integral-field spectrograph dispersing all the light entering the field of view.