Planet Search Continues With New Techniques
The announcement in January of the discovery of two more extrasolar planets brings the total to 17 since the first was reported in 1995. All have been detected and confirmed using the radial velocity method, in which astronomers measure the slight shift in the frequency of a star's light caused by the tug of gravity of its planets (see table below). Other detection methods are expected to bear fruit in 1999, including astronmetry, which measures a star's wobble caused by a planet; transit photometry, which looks for predictable variations in a star's brightness caused by a planet passing in front of it, and microlensing, in which a planet perturbs a star's gravitational field.
More information about extrasolar planets.
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