When the first exoplanet was identified via the radial velocity method, the Swiss team was able to detect a wobble in the star 51 Pegasi at a rate of 50 meters per second. The wobble is the star's movement back and forth caused by the gravitational pull of the planet, and in that first case …
Continue reading "Storming the One-Meter-Per-Second Barrier"
When the first exoplanet was identified via the radial velocity method, the Swiss team was able to detect a wobble in the star 51 Pegasi at a rate of 50 meters per second. The wobble is the star's movement back and forth caused by the gravitational pull of the planet, and in that first case …
Continue reading "Storming the One-Meter-Per-Second Barrier"
