Too tiny and distant to be seen directly, these planets are detected when their gravity affects the velocity of their parent star, causing the star to "wobble" in a regularly repeating pattern. Planet hunters have detected such wobbles as small as 1.0 m/second, equivalent to walking speed.
Lick astronomers monitor about 1,000 stars similar to the sun in luminosity, surface temperature, and evolutionary stage. Many Jupiter-size and Saturn-size planets have been discovered. As technology improves, smaller planets will be discovered more frequently. The ultimate goal of extrasolar planet search is to discover a solar system similar to our own with earth-like planets that may support life.
The fully-robotic Automated Planet Finder (APF) telescope searches robotically for extrasolar planets every night. The Shane telescope and the Hamilton spectrograph are also used to hunt for planets.
In the video below, watch Steve Vogt, Professor of Astronomy and Astrophysics at UC Santa Cruz, discuss how we discover habitable exoplanets with the Automated Planet Finder at Lick Observatory