When measuring radial velocity ($V_r$), what spectral phenomenon indicates a star is moving toward the observer?

Answer

A shift toward the blue end of the spectrum, known as blueshift

The radial velocity component relies fundamentally on the Doppler effect applied to light emitted by the star. If a light source, like a star, is moving directly toward an observer, the wavelengths of the emitted light are compressed due to this relative motion. This compression shifts the observed spectral lines to higher frequencies, corresponding to the blue end of the visible light spectrum, a phenomenon explicitly termed blueshift. Conversely, movement away causes stretching, leading to redshift. Astronomers utilize this precise shift, comparing the observed absorption line positions to their known laboratory wavelengths, to calculate the exact speed of approach.

When measuring radial velocity ($V_r$), what spectral phenomenon indicates a star is moving toward the observer?
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